BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:social dinner details DTSTART;VALUE=DATE-TIME:20181030T223000Z DTEND;VALUE=DATE-TIME:20181030T225000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10063@indico.ific.uv.es DESCRIPTION:https://indico.ific.uv.es/event/3366/contributions/10063/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10063/ END:VEVENT BEGIN:VEVENT SUMMARY:Produccion de radioisotopos para medicina nuclear mediante tecnica s de aceleracion laser DTSTART;VALUE=DATE-TIME:20181029T174000Z DTEND;VALUE=DATE-TIME:20181029T180000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9984@indico.ific.uv.es DESCRIPTION:Speakers: Juan Peñas Nadales (Universidade de Santiago de Com postela)\nMuchas de las técnicas de imagen médica se basan en el uso d e radiación ionizante. En particular la tomografía por emisión de po sitrones (PET) permite obtener imágenes tridimensionales de calidad tras suministrarle al paciente un fármaco con un marcador emisor de positron es.\nActualmente\, la producción de isótopos radioactivos destinados a imagen y tratamientos médicos tiene lugar principalmente en aceleradore s de partículas convencionales. Recientemente se ha propuesto el empleo de láseres ultraintensos de femtosegundo los cuales\, a través de la i nteracción láser-plasma\, son capaces de acelerar partículas ligeras en un rango de energías suficiente como para generar estos isótopos m ediante reacciones nucleares.\nEl Laboratorio Láser de Aceleración y A plicaciones (L2A2) de la Universidad de Santiago de Compostela dispone de un láser de femtosegundo capaz de operar con una tasa de disparo de 10 H z\, con el que se pretende conseguir un haz de protones continuo de hasta 10 MeV. La focalización del láser sobre un blanco primario\, alcanzand o intensidades de en torno a 10^19 W/cm2\, permite por diversos mecanismos físicos la generación de un haz de partículas ligeras (protones\, d euterones\, etc) que\, al incidir sobre un blanco secundario\, dan lugar a la producción de isótopos radioactivos.\nEn esta charla presentaremos el dispositivo experimental instalado en el L2A2 para este fin describien do en particular los sistemas de focalización\, el blanco de aceleracio ́n y su control y los sensores de caracterización de los protones acele rados.\n\nhttps://indico.ific.uv.es/event/3366/contributions/9984/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9984/ END:VEVENT BEGIN:VEVENT SUMMARY:Electron Capture of 8B into highly excited states of 8Be DTSTART;VALUE=DATE-TIME:20181030T075000Z DTEND;VALUE=DATE-TIME:20181030T081000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9989@indico.ific.uv.es DESCRIPTION:Speakers: Sílvia Viñals Onsès (CSIC - IEM)\nIn this talk\, I will present the study of the decay of 8B into highly excited states of 8Be with the aim of determining the branching ratios. Our interest lies in the 2+ doublet at 16.6 and 16.9 MeV populated via β+ and electron captur e (EC) respectively and also the so far unobserved EC-delayed proton emiss ion via the 17.640 MeV state\, that has a theoretical branching ratio of 2 .3·10-8. The 2+ doublet is interesting due to the high isospin mixing [1] \, leading to dominant configurations as 7Li+p and 7Be+n respectively\nI w ill discuss the aims of the experiment\, the setup and I will give the res ults obtained so far in the analysis.\n[1] P. von Brentano\, Phys. Rep. 26 4 (1996) 57\n\nhttps://indico.ific.uv.es/event/3366/contributions/9989/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9989/ END:VEVENT BEGIN:VEVENT SUMMARY:Caracterización por técnicas IBA de blancos de reacciones nuclea res DTSTART;VALUE=DATE-TIME:20181029T140000Z DTEND;VALUE=DATE-TIME:20181029T142000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9987@indico.ific.uv.es DESCRIPTION:Speakers: Francisco Javier Ferrer (Centro Nacional de Acelerad ores)\nLa caracterización de los blancos utilizados en experimentos de f ísica nuclear resulta fundamental en la interpretación de los resultad os de éstos. Dos tipos de desviaciones respecto a los blancos diseñado s\, inhomogeneidades y presencia de impurezas\, pueden alterar la composic ión inicialmente planificada. Las técnicas IBA constituyen una herrami enta de caracterización idónea para medir los blancos que se utilizara ́n posteriormente (o que hayan sido usados) en experimentos de reacciones nucleares. Se presentarán diferentes ejemplos de caracterización de b lancos.\n\nhttps://indico.ific.uv.es/event/3366/contributions/9987/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9987/ END:VEVENT BEGIN:VEVENT SUMMARY:Recent studies at the three CNA Irradiation facilities and coming upgrade DTSTART;VALUE=DATE-TIME:20181030T085000Z DTEND;VALUE=DATE-TIME:20181030T091000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9991@indico.ific.uv.es DESCRIPTION:Speakers: PEDRO MARTÍN-HOLGADO (CNA - Centro Nacional de Acel eradores)\nIn this work we summarize some recent experiments carried out a t the three different irradiation facilities from the Centro Nacional de A celeradores\, using either gamma radiation from a Co-60 source\, or proton s and neutrons from the particle accelerators. In addition\, the main char acteristics of a new chamber which will be available at CNA in the near fu ture and specially designed to irradiate at elevated and cryogenic tempera tures will be shown and discussed.\n\nhttps://indico.ific.uv.es/event/3366 /contributions/9991/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9991/ END:VEVENT BEGIN:VEVENT SUMMARY:LASER-DRIVEN NEUTRONS FOR TIME-OF-FLIGHT EXPERIMENTS DTSTART;VALUE=DATE-TIME:20181030T091000Z DTEND;VALUE=DATE-TIME:20181030T093000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9981@indico.ific.uv.es DESCRIPTION:Speakers: María de los Ángeles Millán Callado (Centro Nacio nal de Aceleradores - Universidad de Sevilla)\nLos haces de neutrones puls ados suponen una valiosa herramienta en física nuclear\, con aplicaciones en un amplio abanico de campos [1-7]. Estos haces de neutrones\, producid os actualmente mediante aceleradores de partículas convencionales [8-11] \, se caracterizan mediante “tiempo de vuelo” (TOF\, por sus siglas en inglés)\, lo que nos permite conocer el espectro energético de nuestro haz de neutrones. El uso de esta técnica está limitado por la resoluc ión temporal que podamos obtener\, la intensidad de cada pulso\, y la fre cuencia con las que podamos producirlos.\nEn las últimas décadas\, el desarrollo de láseres de pulso ultracorto (femtosegundo) y alta potencia (> 1019 W/cm2) ha abierto la puerta a un gran número de nuevas aplicaci ones [12]. Gran parte de los recursos de investigación se han invertido en el estudio de la aceleración de haces de iones asistidos por láser\ , dirigiendo la mayoría de los esfuerzos en la optimización en la prod ucción de las distintas especies de partículas. El uso de estos haces en la producción de neutrones ha permitido alcanzar valores por pulso co mpetitivos respecto a las fuentes tradicionales [13-14] lo que podría co nvertir a este tipo de fuentes láser en una interesante alternativa para la comunidad de haces pulsados. Sin embargo\, hasta ahora\, estos neutron es no han sido utilizados para llevar a cabo ningún experimento de fís ica nuclear.\nEn este contexto\, nuestro grupo de investigación desde la Universidad de Sevilla\, y en colaboración con otros grupos de investig ación con amplia experiencia en producción\, detección y uso de hace s pulsados de neutrones en instalaciones convencionales\, se ha propuesto realizar una serie de experimentos con el objetivo de producir y caracteri zar haces de neutrones pulsados asistidos por láser\, optimizando las te ́cnicas de detección\, análisis y diagnóstico utilizadas actualment e en fuentes de neutrones convencionales para implementarlas en sistemas d e producción láser con el propósito de asentar la viabilidad de llev ar a cabo experimentos de física nuclear en este tipo de fuentes e ident ificar las ventajas y desventajas de este método de producción respect o a los sistemas convencionales.\nPara ello\, se pretende realizar experim entos en diferentes instalaciones láser tanto en España (L2A2 en Santi ago de Compostela y CLPU en Salamanca) como en Europa (CILEX en Paris y LE X Photonics en Munich).\nReferencias\n[1] Barbagallo M. et al.\, Phys. Rev . Lett. 117\, 152701 (2016). [2] Guerrero C. et al.\, Phys. Rev. C 85\, 04 4616 (2012).\n[3] Lederer C. et al.\, Phys. Rev. Lett. 110\, 022501 (2013) .\n[4] Lerendegui-Marco J.\, et al. Phys. Rev. C 97\, 024605 (2018). [5] M endoza E. et al.\, Phys. Rev. C 97\, 054616 (2018).\n[6] Praena\, J. et al .\, Nucl. Data Sheets. 120\, 205–207. (2014).\n[7] Sato\, H. et al.\, Nu cl. Instrum. and Meth A. 605(1-2)\, 36-39. (2009).\n[8] Bensussan A. and J . M.Salome. Nucl. Instrum. and Meth. 155(1-2)\, 11-23 (1978). [9] Guerrero \, C. et al. Eur. Phys. J. A. 49\, 27 (2013).\n[10] Lederer\, C. et al Phy s. Rev. C 85\, 055809 (2012).\n[11] Mastinu\, P. et al. Phys. Procedia\, 2 6\, 261-273 (2012).\n[12] Danson\, C. et al.\, High Power Laser Sci.\, 3. e3\, 1-14. (2015).\n[13] Pomerantz I. et al.\, Phys Rev Lett 113\, 184801 (2014).\n[14] Roth M. et al.\, Phys Rev Lett 110\, 044802. (2013).\n\nhttp s://indico.ific.uv.es/event/3366/contributions/9981/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9981/ END:VEVENT BEGIN:VEVENT SUMMARY:Condensation of tetraneutrons in the neutron star interiors DTSTART;VALUE=DATE-TIME:20181029T142000Z DTEND;VALUE=DATE-TIME:20181029T144000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9982@indico.ific.uv.es DESCRIPTION:Speakers: Oleksii Ivanytskyi (University of Salamanca)\nBased on recent experimental and theoretical hints on possible formation of a re sonant four-neutron system we study effects of appearance of such an aggre gates in neutron rich baryon matter inside neutron stars. For this purpose we employ a relativistic mean field approach which includes nucleons\, Δ -isobars as well as light nuclear clusters. Our analysis demonstrates that tetraneutrons existing as the Bose-Einstein condensate can appear even de spite their short lifetime and strong effects of the Pauli blocking. This significantly affects the equation of state of cold baryonic matter and ob servable characteristics of neutrons stars. Tetraneutron driven suppressio n of Δ-baryons is another important result of our study. The most promine nt manifestation of  the tetraneutron condensation in neutron stars is re lated  to suppression of the superconducting phase which can be concluded from analysis of the nucleon-nucleon pairing gap and density of pairs.\n\ nhttps://indico.ific.uv.es/event/3366/contributions/9982/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9982/ END:VEVENT BEGIN:VEVENT SUMMARY:Evaluación de la resolución en energía y tiempo de SiPMs recien tes de SensL y Hamamatsu acoplados a LYSO\, CeGAGG\, PrLUAG y otros centel ladores DTSTART;VALUE=DATE-TIME:20181030T083000Z DTEND;VALUE=DATE-TIME:20181030T085000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9990@indico.ific.uv.es DESCRIPTION:Speakers: Miguel García Díez (Grupo de Física Nuclear (GFN) Universidad Complutense de Madrid)\nLos SiPMs ocupan un lugar importante en la detección de radiación para experimentos de física nuclear e i magen médica. Aparecen nuevos modelos cada pocos meses con característ icas mejoradas. Analizamos en este trabajo los últimos modelos de SiPM d e Hamamatsu y SensL que introducen mejoras en la PDE con respecto a los mo delos anteriores. Se han acoplado a varios cristales centelladores\, LYSO\ , PrLuAG\, CeGAG y CsI. El PrLUAG es un cristal notablemente más rápid o que el LYSO\, presenta su pico de emisión en los 310 nm\, lo que pone a prueba la sensibilidad espectral de los SiPMS en el extremo de su respue sta. El CEGAG presenta una gran emisión de fotones\, por lo que cabría esperar buena resolución energética por su parte.\nSe han probado dif erentes combinaciones y tamaños de cristales centelladores con cuatro Si PMs de Hamamatsu: S13360-3050CS\, S13360-66050CS\, S13360-6075Cs\, S14160- 6050HS\, y dos SiPMs de SensL: MicroES-SMA-30035TSV y MicroFJ-SMA-60035.\n Los resultados obtenidos muestran que\, la mejora en la PDE de los nuevos SiPMs\, se traduce en mejores resoluciones en energía\, 8% (CeGAGG)\, 10 % (LYSO) y 16% (PrLUAG)\, utilizando el modelo S13360-6075CS de Hamamatsu. En todos los casos el factor más limitante se ha encontrado la diferenc ia entre las secciones transversales de los cristales probados (10x10 mm2) y del SiPM (6x6 mm2). Los resultados con CsI (6x6mm2) son reveladores a e ste respecto. Con respecto a la resolución temporal\, para las combinaci ones favorables de SiPMs y cristales se han conseguido valores de resoluci ón en torno a 250 ps (FWHM\,CRT)\, en este caso los mejores resultados s e obtienen con SiPM de SensL.\n\nhttps://indico.ific.uv.es/event/3366/cont ributions/9990/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9990/ END:VEVENT BEGIN:VEVENT SUMMARY:The new pulsed neutron beam facility at CNA (Spain) DTSTART;VALUE=DATE-TIME:20181030T081000Z DTEND;VALUE=DATE-TIME:20181030T083000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9988@indico.ific.uv.es DESCRIPTION:Speakers: Miguel Macías Martínez (CNA (Centro Nacional de Ac eleradores)\, Univ. Sevilla)\nThe neutron research activities with the Tan dem Pelletron Accelerator at CNA in Seville (Spain) is based on the develo pment of neutron sources with different energy and angular distributions\, which could be generated by 7Li(p\,n) and D(D\,n) reactions. The neutron beam characterization is done using the Time of Flight technique (TOF). Th e TOF technique allows measuring neutron induced cross section as a functi on of the neutron energy\, which can be obtained from the flight time that a neutron spends to travel over known path. To implement TOF technique on e needs pulsed ion beams.\nIn order to provide pulsed beams\, CNA team and NEC staff are currently working on a chopping/bunching system installatio n and commissioning\, as well as the addition of new equipment to better m onitor and control the beam in a new neutron line. The beam chopper consis ts of a pair of electrically deflecting plates\, mounted in parallel to th e initial ion beam. One plate is normally polarized with dc voltage deflec ting the beam on an absorbing beam catcher. The second one is supplied wit h an electronic switch. Both work together producing an oscillation of the beam in the transverse direction\, thus creating a beam pulse. The bunchi ng unit\, being made up involving a pair of tubular electrodes\, is mounte d coaxially to the ion beam\, after the pulsing unit. The electrodes are s upplied with radiofrequency voltage phase locked to the different frequenc ies of the chopping system. The entrance and the exit gaps of the tubular bunching electrodes are used for the time compression of the beam pulse. T he other new devices are: a beam profile monitor (BPM)\, two magnetic stee rers\, two manual slits\, a Faraday cup\, and a Pick-Up.\nThe chopping/bun ching system has been designed to deal with a primary beam of protons or d euterium. The first tests with protons show a pulsed beam with a FWHM of t he order of ns and expected frequency.\nThese promising results will lead the way to various research lines in Seville\, among them are nuclear ener gy production\, radiation protection\, cancer therapy by neutron irradiati on\, radio- biological and nuclear structure research.\n\nhttps://indico.i fic.uv.es/event/3366/contributions/9988/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9988/ END:VEVENT BEGIN:VEVENT SUMMARY:Red de investigación en imagen médica. DTSTART;VALUE=DATE-TIME:20181030T092000Z DTEND;VALUE=DATE-TIME:20181030T093500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10032@indico.ific.uv.es DESCRIPTION:Speakers: Ricardo Graciani Diaz (Universitat de Barcelona\, In stitute of Cosmo Sciences\, ICCUB)\nhttps://indico.ific.uv.es/event/3366/c ontributions/10032/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10032/ END:VEVENT BEGIN:VEVENT SUMMARY:Multidetector data acquisition system (AliVATA) DTSTART;VALUE=DATE-TIME:20181030T090000Z DTEND;VALUE=DATE-TIME:20181030T091500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10031@indico.ific.uv.es DESCRIPTION:Speakers: Gabriela Llosa (IFIC-CSIC)\nhttps://indico.ific.uv.e s/event/3366/contributions/10031/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10031/ END:VEVENT BEGIN:VEVENT SUMMARY:Transient current Technique based on the two-photon-absorption pro cess for semiconductor devices characerization DTSTART;VALUE=DATE-TIME:20181030T084000Z DTEND;VALUE=DATE-TIME:20181030T085500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10030@indico.ific.uv.es DESCRIPTION:Speakers: Ivan Vila Alvarez (Instituto de Física de Cantabria (CSIC-UC))\nhttps://indico.ific.uv.es/event/3366/contributions/10030/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10030/ END:VEVENT BEGIN:VEVENT SUMMARY:Tomografía Muónica aplicada al mantenimiento preventivo de equip os industriales. DTSTART;VALUE=DATE-TIME:20181030T082000Z DTEND;VALUE=DATE-TIME:20181030T083500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10029@indico.ific.uv.es DESCRIPTION:Speakers: Pablo Martinez (Instituto de Fisica de Cantabria)\, Pablo Martinez Ruiz Del Arbol (ETH Zürich\, Switzerland)\nhttps://indico. ific.uv.es/event/3366/contributions/10029/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10029/ END:VEVENT BEGIN:VEVENT SUMMARY:Laser-plasma X-Ray source for high resolution imaging applications DTSTART;VALUE=DATE-TIME:20181029T154000Z DTEND;VALUE=DATE-TIME:20181029T155500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10028@indico.ific.uv.es DESCRIPTION:Speakers: Lucía Martín Blanco (Universidad de Santiago de Co mpostela)\nhttps://indico.ific.uv.es/event/3366/contributions/10028/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10028/ END:VEVENT BEGIN:VEVENT SUMMARY:Neutron beams at CNA for applications: the HiSPANoS facility DTSTART;VALUE=DATE-TIME:20181029T142000Z DTEND;VALUE=DATE-TIME:20181029T143500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10027@indico.ific.uv.es DESCRIPTION:Speakers: Carlos GUERRERO (CERN)\, Carlos Guerrero (Universida d de Sevilla)\, Carlos Guerrero (Universidad de Sevilla)\nhttps://indico.i fic.uv.es/event/3366/contributions/10027/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10027/ END:VEVENT BEGIN:VEVENT SUMMARY:Aplicaciones Médicas de la Línea externa del ciclotrón del Cent ro Nacional de Aceleradores DTSTART;VALUE=DATE-TIME:20181029T150000Z DTEND;VALUE=DATE-TIME:20181029T151500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10026@indico.ific.uv.es DESCRIPTION:Speakers: Mª Carmen Jiménez-Ramos (Centro Nacional de Aceler adores-Sevilla)\nhttps://indico.ific.uv.es/event/3366/contributions/10026/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10026/ END:VEVENT BEGIN:VEVENT SUMMARY:Commissioning of IFIC High Gradient RF Laboratory to test S-band a ccelerating structures for hadron-therapy accelerators DTSTART;VALUE=DATE-TIME:20181029T144000Z DTEND;VALUE=DATE-TIME:20181029T145500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10025@indico.ific.uv.es DESCRIPTION:Speakers: Marçà Boronat Arevalo (IFIC)\nhttps://indico.ific. uv.es/event/3366/contributions/10025/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10025/ END:VEVENT BEGIN:VEVENT SUMMARY:TRITIUM: Un detector de tritio para la central nuclear de Almaraz. DTSTART;VALUE=DATE-TIME:20181029T140000Z DTEND;VALUE=DATE-TIME:20181029T141500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10023@indico.ific.uv.es DESCRIPTION:Speakers: Marcos Martinez (Contrato temporal)\nhttps://indico. ific.uv.es/event/3366/contributions/10023/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10023/ END:VEVENT BEGIN:VEVENT SUMMARY:Verificación de Rango de Protones mediante el uso de contrastes DTSTART;VALUE=DATE-TIME:20181029T152000Z DTEND;VALUE=DATE-TIME:20181029T153500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10022@indico.ific.uv.es DESCRIPTION:Speakers: Víctor Valladolid Onecha ()\nhttps://indico.ific.uv .es/event/3366/contributions/10022/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10022/ END:VEVENT BEGIN:VEVENT SUMMARY:Tasas de producción de emisores beta+ para la verificación del r ango en protonterapia DTSTART;VALUE=DATE-TIME:20181029T180000Z DTEND;VALUE=DATE-TIME:20181029T182000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10013@indico.ific.uv.es DESCRIPTION:Speakers: Mª Teresa Rodríguez González (Universidad de Sevi lla)\nEn protonterapia\, la verificación de rango in vivo usando un esca ́ner PET se basa en la comparación entre la actividad medida y la activ idad estimada de emisores de positrones inducidos por el haz de protones e n los principales elementos del cuerpo humano: carbono\, oxígeno\, nitro ́geno\, calcio y fósforo. La exactitud con la que se conoce dicha estim ación depende de la exactitud de la simulación Monte Carlo correspondi ente\, que a su vez depende de la exactitud con la que se conocen las secc iones eficaces de interés [1]. Una revisión de los datos experimentale s disponibles en EXFOR [2\,3] muestra que para determinadas reacciones no existen datos en todo el rango de energías del haz de protones (hasta 25 0 MeV) y que\, además\, existen diferencias significativas entre las dis tintas medidas. Esto es particularmente serio para el caso de emisores β+ de vida media corta (\n\nhttps://indico.ific.uv.es/event/3366/contributio ns/10013/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10013/ END:VEVENT BEGIN:VEVENT SUMMARY:Nanopartículas de lantánidos para imagen multimodal DTSTART;VALUE=DATE-TIME:20181029T172000Z DTEND;VALUE=DATE-TIME:20181029T174000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10011@indico.ific.uv.es DESCRIPTION:Speakers: Laura Fernández Maza (Universidad de Sevilla)\nLas nanopartículas de lantánidos constituyen un prometedor grupo de agentes para imagen multimodal. Por sus propiedades fisicoquímicas podrían ser útiles en diferentes técnicas diagnósticas\; bioluminiscencia\, resonan cia magnética (MRI)\, tomografía computarizada (CT) y tomografía por em isión de positrones (PET). En el presente trabajo se marcaron nanopartíc ulas de trifluoruro de lantano con Flúor-18 para estudios de imagen por P ET/CT.\nSe obtuvo el [18F]fluoruro por bombardeo de un target líquido 18O (p\,n)18F en el ciclotrón del CNA. La actividad se transfirió a un módu lo de síntesis dentro una celda blindada de la Unidad de Radiofarmacia. L a reacción de marcaje tuvo lugar a temperatura ambiente. Antes de inyecta rlas al animal\, se analizaron las nanopartículas por radiocromatografía en capa fina\, para asegurar la pureza radioquímica. Los controles de pH y la estabilidad in vitro en plasma humano se llevaron a cabo en estudios anteriores. Se inyectaron 4 MBq de nanopartículas radiactivas por la ven a lateral de la cola de un ratón sano BALB/c y se realizó el estudio PET estático de 15 minutos seguido del estudio CT. El animal permaneció ane stesiado durante ambos estudios\, por lo que las imágenes funcionales PET pudieron superponerse a las imágenes anatómicas del CT.\n\nhttps://indi co.ific.uv.es/event/3366/contributions/10011/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10011/ END:VEVENT BEGIN:VEVENT SUMMARY:Determinación y caracterización de movimiento en escáner PET de animal despierto DTSTART;VALUE=DATE-TIME:20181029T164000Z DTEND;VALUE=DATE-TIME:20181029T170000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10009@indico.ific.uv.es DESCRIPTION:Speakers: Fernando Arias Valcayo (Universidad Complutense de M adrid)\nEn este trabajo se ha estudiado la técnica de seguimiento de mar cadores fiduciales emisores de positrones para detectar y corregir movimie nto en adquisiciones de tomografía por emisión de positrones (PET). El objetivo es poder realizar adquisiciones PET con animales despiertos. Est o evitaría el uso de anestesia y sus efectos en el funcionamiento normal del cerebro bajo estudio.\nSe han estudiado distintas métricas para det erminar el movimiento tanto en el espacio del sinograma como en el de la i magen retroproyectada. Se ha probado que varias de estas métricas\, basa das en la distribución no uniforme del escáner\, son capaces de detect ar instantes en los que el animal se encuentra quieto. El método del cen troide de líneas de respuestas ha sido el más rápido.\nMediante la g eneración de datos con trazado de rayos y simulaciones Montecarlo con Pe nelo-PET\, se ha estudiado cómo afectan factores como el ruido o la reso lución del escáner\, en la correcta localización de los marcadores. Con ello se pretende poder estimar la actividad óptima de las fuentes de pendiendo del estudio que se quiere realizar. Para la correcta localizacio ́n de las fuentes se ha utilizado un nuevo filtro\, que hemos denominado pseudo-FBP\, que mejora el contraste obtenido con la retroproyección est ándar\, sin aumentar mucho el tiempo de cálculo.\nPor último\, se ha caracterizado el movimiento de los cuatro marcadores colocados sobre una rata en una adquisición con FDG mediante el PET Super-Argus. Para ello s e ha usado el algoritmo Kabsch para determinar el movimiento de sólido r ígido de la imagen retroproyectada. El uso de las imágenes retroproyec tadas de cada instante de tiempo (en lugar de las imágenes reconstruidas que requieren entre uno y dos órdenes de magnitud más de tiempo de ca ́lculo) es un gran avance en este campo\, dado que abre las puertas a su uso en futuros estudios en vivo.\nEn resumen\, en este trabajo mostramos c ómo es posible estimar y caracterizar de manera rápida y eficiente el movimiento en PET mediante el uso de marcadores fiduciales emisores de pos itrones colocados sobre el animal en estudio.\n\nhttps://indico.ific.uv.es /event/3366/contributions/10009/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10009/ END:VEVENT BEGIN:VEVENT SUMMARY:Aplicaciones en Patrimonio Cultural en el CNA DTSTART;VALUE=DATE-TIME:20181029T162000Z DTEND;VALUE=DATE-TIME:20181029T164000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10008@indico.ific.uv.es DESCRIPTION:Speakers: Miguel Ángel Respaldiza (Universidad de Sevilla)\nE l uso de las técnicas nucleares de análisis ha experimentado un auge ext raordinario en las últimas décadas en el campo del Patrimonio Cultural. Hoy en día\, su uso en el estudio de objetos de interés para el Patrimon io se ha vuelto esencial. Desde los años 90\, el grupo de investigación en Física Nuclear Aplicada del Centro Nacional de Aceleradores ha realiza do un esfuerzo importante para desarrollar diferentes técnicas analítica s no destructivas para el estudio de objetos de arte y arqueológicos. Est os esfuerzos se centraron inicialmente en el uso de las técnicas IBA (Ion Beam Analysis) y\, últimamente\, en el desarrollo de equipos portátiles de fluorescencia de rayos X (XRF)\, incluidas las versiones con microhace s gracias a la implementación de lentes policapilares (μXRF y XRF confoc al).\n En esta comunicación se presentarán los diferentes métodos e ins trumentación desarrollados en los últimos años en el CNA\, e ilustrarem os con varias aplicaciones sus capacidades para el análisis de diferente s tipos de objetos: joyas\, monedas\, pinturas\, vidrios\, etc. Se mostrar án las ventajas y limitaciones de las diferentes técnicas y también se presentarán ejemplos de cómo la combinación de varios de estos métodos puede superar algunas de esas limitaciones.\n\nhttps://indico.ific.uv.es/ event/3366/contributions/10008/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10008/ END:VEVENT BEGIN:VEVENT SUMMARY:Neutron capture cross section measurement of 205Tl at the n_TOF fa cility (CERN) DTSTART;VALUE=DATE-TIME:20181029T144000Z DTEND;VALUE=DATE-TIME:20181029T150000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9983@indico.ific.uv.es DESCRIPTION:Speakers: Adrià Cassanovas ()\nTl-205 is most abundant stable isotope of thallium in the Earth. It is produced mainly during the slow ( s) process of nucleosynthesis by neutron capture. During some stages of th e s process\, and due to the high temperatures involved\, it becomes stabl e and decays to Pb-205. This isotope of lead is radioactive\, and it is pr oduced only by the s-process\, and therefore it is thought that it could b e used as a "clock" of the process. The Tl-205 abundance is strongly depen dent on its neutron capture rate\, and by means of the mechanism mentioned before\, so it is the abundance of Pb-205. Having considered this\, the A NT group of the UPC carried out the measurement of the capture cross secti on of Tl-205 in the n_TOF experiment at CERN this last summer\, aiming to improve both the accuracy and precision of the cross section for nucleosyn thesis calculations. In this talk\, besides explaining more in detail the astrophyisical motivations\, a description of the measurement process\, an d some preliminary results\, will be shown.\n\nhttps://indico.ific.uv.es/e vent/3366/contributions/9983/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9983/ END:VEVENT BEGIN:VEVENT SUMMARY:Shell closure at N=34 and the Si-48 nucleus. DTSTART;VALUE=DATE-TIME:20181030T093000Z DTEND;VALUE=DATE-TIME:20181030T095000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9985@indico.ific.uv.es DESCRIPTION:Speakers: Antonio M. Lallena Rojo Lallena (Universidad de Gran ada)\, Marta Anguiano (Universidad de Granada)\nBy using a non-relativisti c independent particle approach we investigate the mechanism promot- ing 3 4 as new magic number. We carried out Hartree-Fock plus Bardeen-Cooper-Sch rieffer and Quasi-particle Random Phase Approximation calculations by cons istently using the same finite- range interaction in all the three steps o f our approach. We used two Gogny-like interactions\, with and without ten sor terms. We find that the shell closure for N = 34 neutrons appears in i sotones with proton number smaller than 26. The smaller is the proton numb er\, the more evident is the shell closure at N = 34. An ideal nucleus to investigate this effect is 48Si \, as it has been recently suggested.\n\nh ttps://indico.ific.uv.es/event/3366/contributions/9985/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9985/ END:VEVENT BEGIN:VEVENT SUMMARY:Measurement of the Cm-244 and Cm-246 neutron-induced cross section s at the n_TOF facility DTSTART;VALUE=DATE-TIME:20181030T095000Z DTEND;VALUE=DATE-TIME:20181030T101000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9986@indico.ific.uv.es DESCRIPTION:Speakers: Victor Alcayne Aicua (CIEMAT (Spain))\nThe neutron c apture reactions in 244Cm and 246Cm isotopes open the path of the formatio n of heavier Cm isotopes and heavier elements such as Bk and Cf in a nucle ar reactor. In addition\, both isotopes are two of the minor actinides wit h a large contribution to the decay heat and to the neutron emission in ir radiated fuels proposed for the transmutation of the nuclear waste and fas t critical reactors. The available experimental data for both isotopes is very scarce due to the difficulties in performing the measurements: high i ntrinsic activity of the samples and the limited facilities capable of pro viding isotopically enriched samples. We measure the neutron capture cross section measurement with isotopically enriched samples of 244Cm and 246Cm provided by JAEA. The measurement covers the range from 1 eV to 250 eV. T he measure was done in to difference experimental areas with different det ectors: In Experimental Area 2 (EAR-2) with C6D6 and also in experimental Area 1 (EAR-1) with the Total Absorption Calorimeter.\n\nhttps://indico.if ic.uv.es/event/3366/contributions/9986/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9986/ END:VEVENT BEGIN:VEVENT SUMMARY:Dark matter and the scale of new physics DTSTART;VALUE=DATE-TIME:20181029T140000Z DTEND;VALUE=DATE-TIME:20181029T142000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9912@indico.ific.uv.es DESCRIPTION:Speakers: Clara Murgui (IFIC)\nWe discuss the possibility of f inding an upper bound on the seesaw scale using the cosmological bound on the cold dark matter relic density. We investigate a simple relation betwe en the origin of neutrino masses and the properties of a dark matter candi date in a simple theory where the new symmetry breaking scale defines the seesaw scale. Imposing the cosmological bounds\, we find an upper bound of order multi-TeV on the lepton number violation scale. We investigate the predictions for direct and indirect detection dark matter experiments and the possible signatures at the Large Hadron Collider.\n\nhttps://indico.if ic.uv.es/event/3366/contributions/9912/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9912/ END:VEVENT BEGIN:VEVENT SUMMARY:Asamblea FNUC DTSTART;VALUE=DATE-TIME:20181029T150000Z DTEND;VALUE=DATE-TIME:20181029T160000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9992@indico.ific.uv.es DESCRIPTION:Speakers: Luis Fraile (Universidad Complutense de Madrid)\nhtt ps://indico.ific.uv.es/event/3366/contributions/9992/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9992/ END:VEVENT BEGIN:VEVENT SUMMARY:Fermion mass matrix models DTSTART;VALUE=DATE-TIME:20181029T172200Z DTEND;VALUE=DATE-TIME:20181029T174000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10014@indico.ific.uv.es DESCRIPTION:Speakers: julien alcaide de wandeleer (uv)\nhttps://indico.ifi c.uv.es/event/3366/contributions/10014/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10014/ END:VEVENT BEGIN:VEVENT SUMMARY:Complex Wilson coefficients in the analysis of B-anomalies DTSTART;VALUE=DATE-TIME:20181029T154800Z DTEND;VALUE=DATE-TIME:20181029T160600Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9856@indico.ific.uv.es DESCRIPTION:Speakers: Jorge Alda Gallo (Universidad de Zaragoza)\nhttps:// indico.ific.uv.es/event/3366/contributions/9856/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9856/ END:VEVENT BEGIN:VEVENT SUMMARY:Are we overlooking Lepton Flavour Universal New Physics in b -> s l l DTSTART;VALUE=DATE-TIME:20181029T153000Z DTEND;VALUE=DATE-TIME:20181029T154800Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9857@indico.ific.uv.es DESCRIPTION:Speakers: Pere Masjuan (IFAE-UAB)\nhttps://indico.ific.uv.es/e vent/3366/contributions/9857/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9857/ END:VEVENT BEGIN:VEVENT SUMMARY:Leptoquarks\, in view of recent excitements DTSTART;VALUE=DATE-TIME:20181029T141800Z DTEND;VALUE=DATE-TIME:20181029T143600Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9852@indico.ific.uv.es DESCRIPTION:Speakers: Rusa Mandal (IFIC\, Valencia University)\nhttps://in dico.ific.uv.es/event/3366/contributions/9852/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9852/ END:VEVENT BEGIN:VEVENT SUMMARY:New developments for ambient neutron dosimetry in continuous and p ulsed fields DTSTART;VALUE=DATE-TIME:20181029T170000Z DTEND;VALUE=DATE-TIME:20181029T172000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-10010@indico.ific.uv.es DESCRIPTION:Speakers: Ariel Tarifeño Saldivia (IFIC (CSIC-Univ. Valencia) )\nNeutrons are intentionally used or incidentally created in various scen arios. Depending on the neutron energy\, this kind of radiation can domina te the total dose received. Thus\, the detection of neutrons\, for radiati on protection purposes\, is an important issue in areas such as basic rese arch\, nuclear power plants\, healthcare\, industrial applications\, defen se and homeland security. The commercially available detectors for area mo nitoring are based on polyethylene moderated proportional counters [KNO10] . They were designed in the late nineties\, according to the ICRP74 recomm endations [ICRP74]\, in order to measure the ambient to dose equivalent H* (10).\nFor continuous neutron fields\, commercial surveys fits well the re commended response up to 10 or 20 MeV [IAEA2001]. At higher energies\, the response of most of the commercial dosimeters present underestimations of the ambient dose (H*(10)). This is a major concern in modern medical appl ications\, such as proton therapy\, where secondary neutrons are produced with energies spanning from 60 up to 250 MeV[AGO98\, FAR15\, MAR16].\nFor pulsed fields\, i. e. when the neutron intensity presents large variations in short periods of time\, there are currently several concerns about the reliability of commercial neutron dosimeters [KLE06\, CAR14]. This is a m ajor issue for the radiation protection in the new particle accelerator te chnologies\, for example synchrotrons and medical linacs\, where beam loss es produce short bursts of secondary neutron radiation\; or pulsed neutron facilities for basic research and applications\, such as spallation and f usion sources\, high intensity lasers\, among others.\nAt UPC\, provided t he experience gained by our group in the design of complex neutron detecto rs for research in nuclear physics\, we have started a project for the des ign of improved ambient neutron dosimeters. The new designs are intended f or application in pulsed fields and proton therapy. The status and future of the project is presented.\n\nhttps://indico.ific.uv.es/event/3366/contr ibutions/10010/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/10010/ END:VEVENT BEGIN:VEVENT SUMMARY:Perspectives for multimessenger astrophysics after the discovery o f GWs DTSTART;VALUE=DATE-TIME:20181031T115500Z DTEND;VALUE=DATE-TIME:20181031T122500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9958@indico.ific.uv.es DESCRIPTION:Speakers: Maurizio Spurio (Univ Bologna and INFN)\nhttps://ind ico.ific.uv.es/event/3366/contributions/9958/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9958/ END:VEVENT BEGIN:VEVENT SUMMARY:Flavour anomalies in B decays DTSTART;VALUE=DATE-TIME:20181031T112000Z DTEND;VALUE=DATE-TIME:20181031T115000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9957@indico.ific.uv.es DESCRIPTION:Speakers: Arantza Oyanguren (IFIC\, CSIC-Univ Valencia)\nhttps ://indico.ific.uv.es/event/3366/contributions/9957/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9957/ END:VEVENT BEGIN:VEVENT SUMMARY:Exploring the Nuclear Landscape DTSTART;VALUE=DATE-TIME:20181031T104500Z DTEND;VALUE=DATE-TIME:20181031T111500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9956@indico.ific.uv.es DESCRIPTION:Speakers: Alfredo Poves (IFT\, UAM-CSIC)\nhttps://indico.ific. uv.es/event/3366/contributions/9956/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9956/ END:VEVENT BEGIN:VEVENT SUMMARY:Outlook in BSM physics DTSTART;VALUE=DATE-TIME:20181031T094500Z DTEND;VALUE=DATE-TIME:20181031T101500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9955@indico.ific.uv.es DESCRIPTION:Speakers: Verónica Sanz (Univ Sussex)\nhttps://indico.ific.uv .es/event/3366/contributions/9955/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9955/ END:VEVENT BEGIN:VEVENT SUMMARY:Recent SM results at LHC: EWK+top+Higgs DTSTART;VALUE=DATE-TIME:20181031T091000Z DTEND;VALUE=DATE-TIME:20181031T094000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9954@indico.ific.uv.es DESCRIPTION:Speakers: Javier Brochero (IFICA\, U Cantabria-CSIC)\nhttps:// indico.ific.uv.es/event/3366/contributions/9954/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9954/ END:VEVENT BEGIN:VEVENT SUMMARY:The Long Range Plan of NuPECC: the roadmap of Nuclear Physics in E urope DTSTART;VALUE=DATE-TIME:20181031T083500Z DTEND;VALUE=DATE-TIME:20181031T090500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9953@indico.ific.uv.es DESCRIPTION:Speakers: Angela Bracco (Univ Milano and INFN )\nhttps://indic o.ific.uv.es/event/3366/contributions/9953/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9953/ END:VEVENT BEGIN:VEVENT SUMMARY:BSM (ATLAS and CMS) DTSTART;VALUE=DATE-TIME:20181031T080000Z DTEND;VALUE=DATE-TIME:20181031T083000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9952@indico.ific.uv.es DESCRIPTION:Speakers: Judita Mamuzic (IFIC\, CSIC-Univ Valencia)\nhttps:// indico.ific.uv.es/event/3366/contributions/9952/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9952/ END:VEVENT BEGIN:VEVENT SUMMARY:Axions and other dark matter candidates DTSTART;VALUE=DATE-TIME:20181030T170500Z DTEND;VALUE=DATE-TIME:20181030T173500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9959@indico.ific.uv.es DESCRIPTION:Speakers: Javier Redondo (Univ Zaragoza)\nhttps://indico.ific. uv.es/event/3366/contributions/9959/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9959/ END:VEVENT BEGIN:VEVENT SUMMARY:Future colliders DTSTART;VALUE=DATE-TIME:20181030T163000Z DTEND;VALUE=DATE-TIME:20181030T170000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9951@indico.ific.uv.es DESCRIPTION:Speakers: Jorgen D'Hondt (Vrije Univ Brussel)\nhttps://indico. ific.uv.es/event/3366/contributions/9951/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9951/ END:VEVENT BEGIN:VEVENT SUMMARY:Gamma-ray observations and status of CTA DTSTART;VALUE=DATE-TIME:20181030T153000Z DTEND;VALUE=DATE-TIME:20181030T160000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9950@indico.ific.uv.es DESCRIPTION:Speakers: Manel Martínez (IFAE Barcelona)\nhttps://indico.ifi c.uv.es/event/3366/contributions/9950/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9950/ END:VEVENT BEGIN:VEVENT SUMMARY:Unveling the interior of neutron stars with R3B/FAIR experiment DTSTART;VALUE=DATE-TIME:20181030T145500Z DTEND;VALUE=DATE-TIME:20181030T152500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9949@indico.ific.uv.es DESCRIPTION:Speakers: Dolores Cortina (Univ Santiago de Compostela)\nhttps ://indico.ific.uv.es/event/3366/contributions/9949/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9949/ END:VEVENT BEGIN:VEVENT SUMMARY:Status and prospects of the LHCb experiment DTSTART;VALUE=DATE-TIME:20181030T142000Z DTEND;VALUE=DATE-TIME:20181030T145000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9948@indico.ific.uv.es DESCRIPTION:Speakers: Xavier Vilasís-Cardona (Univ Ramon Llull)\nhttps:// indico.ific.uv.es/event/3366/contributions/9948/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9948/ END:VEVENT BEGIN:VEVENT SUMMARY:Constraints on the SM Higgs from the WGC DTSTART;VALUE=DATE-TIME:20181029T164000Z DTEND;VALUE=DATE-TIME:20181029T170000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9919@indico.ific.uv.es DESCRIPTION:Speakers: Eduardo Gonzalo (IFT)\nIt has been recently argued t hat the presence of any non-SUSY AdS stable vacua implies that a theory ca nnot be consistently coupled to gravity (Ooguri-Vafa conjecture). The appl ication of this conjecture to the SM and its compactifications to two or t hree dimensions has lead to interesting predictions on low energy physics. One of these predictions is an upper bound on the Higgs vev\, determined by the cosmological constant\, that appears when trying to avoid the forma tion of an AdS minima around the neutrino scale. We will show that\, when the number of quark/lepton generations is bigger or equal than three\, the Higgs vev is also bounded from below by $\\Lambda_{\\text{QCD}}$. These b ounds force the EW and QCD scale to be relatively close. They also imply t hat the Higgs vev is stable against quantum corrections\, leading to a rea ssessment of the SM hierarchy problem.\n\nhttps://indico.ific.uv.es/event/ 3366/contributions/9919/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9919/ END:VEVENT BEGIN:VEVENT SUMMARY:Quasi-local energy and compactification DTSTART;VALUE=DATE-TIME:20181029T162000Z DTEND;VALUE=DATE-TIME:20181029T164000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9918@indico.ific.uv.es DESCRIPTION:Speakers: Raquel Santos (IFT)\nBased on the quasi-local energy definition of Brown and York\, we compute the integral of the trace of th e extrinsic curvature over a codimension-2 hypersurface. In particular\, w e study the difference between the uncompactified Minkowski spacetime and the toroidal Kaluza-Klein compactification. For the latter\, we find that this quantity interpolates between zero and the value for the uncompactifi ed spacetime\, as the size of the compact dimension increases. Thus\, the quasi-local energy is able to discriminate between the two spacetimes.\n\n https://indico.ific.uv.es/event/3366/contributions/9918/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9918/ END:VEVENT BEGIN:VEVENT SUMMARY:Grand Unified Theories: Double SU(4) DTSTART;VALUE=DATE-TIME:20181029T154000Z DTEND;VALUE=DATE-TIME:20181029T160000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9917@indico.ific.uv.es DESCRIPTION:Speakers: Pablo Diez Valle (UCM)\nThe Standard Model of partic les physics (SM)\, which describes the strong\, weak and electromagnetic interactions\, has shown to be very successful. However\, there are clear indications that the SM is not the ultimate theory of elementary particl e interactions since it has troubles to explain some phenomena such as th e neutrino masses. It is known that some of these problems could be resolv ed considering a gauge theory with invariance under a larger group than t he SM gauge group. Thereby the Standard Model would be the low-energy lim it of this new gauge theory. We call them Grand Uni ed theories (GUTs). M ost of GUTs have important implications in Cosmology\, for example an exp lication for the baryon asymmetry of the universe\, new dark matter candi dates\, an approach to the earliest universe energies... We will introduc e Grand Uni cation and we will discuss its role in Cosmology. Furthermore \, we shall present an uni fied model based on gauge group SU(4)_CxSU(4)_ RL.\n\nhttps://indico.ific.uv.es/event/3366/contributions/9917/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9917/ END:VEVENT BEGIN:VEVENT SUMMARY:AdS-Phobia: confronting the SM and SUSY with the WGC DTSTART;VALUE=DATE-TIME:20181029T152000Z DTEND;VALUE=DATE-TIME:20181029T154000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9916@indico.ific.uv.es DESCRIPTION:Speakers: Alvaro Herraez (IFT)\nAfter recalling that the sharp ened version of the WGC proposed by Ooguri and Vafa implies that any stabl e non-SUSY AdS vacuum is in the swampland\, we will present several conseq uences that this may have for the SM and some of its extensions. First\, w e will argue why it is interesting to consider compatifications of the SM to 2D on $T^2/Z_N$. From these we can conclude that the SM is not robust against the appearance of AdS vacua in 2D and hence would be\, by itself\, inconsistent with quantum gravity. However\, if the SM is embedded at som e scale into a supersymmetric version\, these AdS vacua present in the non -SUSY case disappear or become unstable\, suggesting that the WGC favors s upersymmetry. Finally\, we present different scenarios in which embedding the orbifold action into different gauge symmetries can lead to additional constraints.\n\nhttps://indico.ific.uv.es/event/3366/contributions/9916/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9916/ END:VEVENT BEGIN:VEVENT SUMMARY:Determination of the lightest hybrid meson pole DTSTART;VALUE=DATE-TIME:20181029T144000Z DTEND;VALUE=DATE-TIME:20181029T150000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9914@indico.ific.uv.es DESCRIPTION:Speakers: Arkaitz Rodas (UCM)\nMapping gluonic states in the light sector is a challenge\,\nand has led to controversies in the past. I n particular\, the experiments have reported two different states with exo tic signature\, \\pi_1(1400) and \\pi_1(1600)\, which couple separately \n to \\eta \\pi and \\eta' \\pi. This picture is not compatible with the Lat tice QCD estimates for hybrid states\, nor with most phenomenological mode ls.\nWe consider the most recent partial wave analysis of the \\eta pi sys tem performed by COMPASS. We fit it with a coupled-channel amplitude which enforces the unitarity and analyticity of the S-matrix. We provide\na rob ust extraction of a single exotic \\pi_1 resonant pole\, with mass and wid th 1564 +- 24 +- 86 MeV and 492 +- 54 +- 102 MeV\, which couples to both \ \eta(') pi channels. We find no evidence for a second exotic state. We als o provide the resonant parameters of the a_2(1320) and a'_2(1700).\n\nhttp s://indico.ific.uv.es/event/3366/contributions/9914/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9914/ END:VEVENT BEGIN:VEVENT SUMMARY:Alpha-prime corrected black holes DTSTART;VALUE=DATE-TIME:20181029T142000Z DTEND;VALUE=DATE-TIME:20181029T144000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9913@indico.ific.uv.es DESCRIPTION:Speakers: Alejandro Ruiperez (IFT)\nI will talk about a family of alpha'-corrected solutions of the Heterotic Superstring effective acti on describing four-dimensional black holes which are sourced by five brane s\, strings and Kaluza-Klein monopoles. I will then focus!\non small black holes\, discussing if higher-curvature corrections can render the horizon regular or not.!\n\nhttps://indico.ific.uv.es/event/3366/contributions/99 13/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9913/ END:VEVENT BEGIN:VEVENT SUMMARY:Discussion on the future of the "red LHC" DTSTART;VALUE=DATE-TIME:20181030T092000Z DTEND;VALUE=DATE-TIME:20181030T100000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9911@indico.ific.uv.es DESCRIPTION:Speakers: All ()\nhttps://indico.ific.uv.es/event/3366/contrib utions/9911/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9911/ END:VEVENT BEGIN:VEVENT SUMMARY:Cross section measurents for ttbar and searches for stops at 13TeV in CMS DTSTART;VALUE=DATE-TIME:20181030T090000Z DTEND;VALUE=DATE-TIME:20181030T092000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9910@indico.ific.uv.es DESCRIPTION:Speakers: Luca Scodellaro (IFCA)\nhttps://indico.ific.uv.es/ev ent/3366/contributions/9910/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9910/ END:VEVENT BEGIN:VEVENT SUMMARY:Search for electroweak superpartners in events with multi-leptons DTSTART;VALUE=DATE-TIME:20181030T084000Z DTEND;VALUE=DATE-TIME:20181030T090000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9909@indico.ific.uv.es DESCRIPTION:Speakers: Iñaki Lara Pérez (Universidad Autónoma de Madrid- IFT)\nhttps://indico.ific.uv.es/event/3366/contributions/9909/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9909/ END:VEVENT BEGIN:VEVENT SUMMARY:Searches for vector-like quarks with the ATLAS detector DTSTART;VALUE=DATE-TIME:20181030T082000Z DTEND;VALUE=DATE-TIME:20181030T084000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9908@indico.ific.uv.es DESCRIPTION:Speakers: Tal van Daalen (IFAE)\nhttps://indico.ific.uv.es/eve nt/3366/contributions/9908/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9908/ END:VEVENT BEGIN:VEVENT SUMMARY:LHC bounds on coloured scalars: the Manohar-Wise model DTSTART;VALUE=DATE-TIME:20181030T080000Z DTEND;VALUE=DATE-TIME:20181030T082000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9907@indico.ific.uv.es DESCRIPTION:Speakers: Víctor Miralles Aznar (IFIC-UV)\nhttps://indico.ifi c.uv.es/event/3366/contributions/9907/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9907/ END:VEVENT BEGIN:VEVENT SUMMARY:LHCb VeLo Upgrade DTSTART;VALUE=DATE-TIME:20181029T181000Z DTEND;VALUE=DATE-TIME:20181029T183000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9906@indico.ific.uv.es DESCRIPTION:Speakers: Antonio Fernández Prieto (Universidade de Santiago de Compostela)\nhttps://indico.ific.uv.es/event/3366/contributions/9906/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9906/ END:VEVENT BEGIN:VEVENT SUMMARY:LHCb SciFi and CALO Upgrade DTSTART;VALUE=DATE-TIME:20181029T175000Z DTEND;VALUE=DATE-TIME:20181029T181000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9905@indico.ific.uv.es DESCRIPTION:Speakers: Jose Mazorras (IFIC)\nhttps://indico.ific.uv.es/even t/3366/contributions/9905/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9905/ END:VEVENT BEGIN:VEVENT SUMMARY:Pixel upgrade for Phase2 in CMS DTSTART;VALUE=DATE-TIME:20181029T173000Z DTEND;VALUE=DATE-TIME:20181029T175000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9904@indico.ific.uv.es DESCRIPTION:Speakers: Ivan Vila Alvarez (Instituto de Física de Cantabria (CSIC-UC))\nhttps://indico.ific.uv.es/event/3366/contributions/9904/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9904/ END:VEVENT BEGIN:VEVENT SUMMARY:Upgrade activities of the CMS Drift Tubes detector DTSTART;VALUE=DATE-TIME:20181029T171000Z DTEND;VALUE=DATE-TIME:20181029T173000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9903@indico.ific.uv.es DESCRIPTION:Speakers: Barbara Alvarez Gonzalez (Universidad de Oviedo)\nht tps://indico.ific.uv.es/event/3366/contributions/9903/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9903/ END:VEVENT BEGIN:VEVENT SUMMARY:ATLAS Inner Tracker upgrade DTSTART;VALUE=DATE-TIME:20181029T165000Z DTEND;VALUE=DATE-TIME:20181029T171000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9902@indico.ific.uv.es DESCRIPTION:Speakers: Daniele Madaffari (IFIC - Valencia)\nhttps://indico. ific.uv.es/event/3366/contributions/9902/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9902/ END:VEVENT BEGIN:VEVENT SUMMARY:Measurements of cross sections for inclusive photon and photon+jet production at 13 TeV and prospects for HL/HE-LHC DTSTART;VALUE=DATE-TIME:20181029T163000Z DTEND;VALUE=DATE-TIME:20181029T165000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9901@indico.ific.uv.es DESCRIPTION:Speakers: Daniel Camarero Munoz (Universidad Autonoma de Madri d (ES))\nhttps://indico.ific.uv.es/event/3366/contributions/9901/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9901/ END:VEVENT BEGIN:VEVENT SUMMARY:Highlights of heavy ion physics at LHCb DTSTART;VALUE=DATE-TIME:20181029T154000Z DTEND;VALUE=DATE-TIME:20181029T160000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9900@indico.ific.uv.es DESCRIPTION:Speakers: Óscar Boente (University of Santiago de Compostela) \nhttps://indico.ific.uv.es/event/3366/contributions/9900/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9900/ END:VEVENT BEGIN:VEVENT SUMMARY:Measuring transverse momentum distributions with jets DTSTART;VALUE=DATE-TIME:20181029T152000Z DTEND;VALUE=DATE-TIME:20181029T154000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9899@indico.ific.uv.es DESCRIPTION:Speakers: Daniel Gutierrez Reyes (UCM)\nhttps://indico.ific.uv .es/event/3366/contributions/9899/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9899/ END:VEVENT BEGIN:VEVENT SUMMARY:Evidence for associated production of a Higgs boson with a top qua rk pair in multi-lepton final states DTSTART;VALUE=DATE-TIME:20181029T150000Z DTEND;VALUE=DATE-TIME:20181029T152000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9898@indico.ific.uv.es DESCRIPTION:Speakers: Carlos Francisco Erice (Universidad de Oviedo)\nhttp s://indico.ific.uv.es/event/3366/contributions/9898/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9898/ END:VEVENT BEGIN:VEVENT SUMMARY:Cross-section measurement of Higgs boson decaying to a pair of tau leptons with the ATLAS detector DTSTART;VALUE=DATE-TIME:20181029T144000Z DTEND;VALUE=DATE-TIME:20181029T150000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9897@indico.ific.uv.es DESCRIPTION:Speakers: Sergi Rodriguez Bosca (IFIC (CSIC/UV))\nhttps://indi co.ific.uv.es/event/3366/contributions/9897/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9897/ END:VEVENT BEGIN:VEVENT SUMMARY:Testing B physics anomalies at ATLAS/CMS DTSTART;VALUE=DATE-TIME:20181029T142000Z DTEND;VALUE=DATE-TIME:20181029T144000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9896@indico.ific.uv.es DESCRIPTION:Speakers: Pablo Martin (IFT (UAM-CSIC))\nhttps://indico.ific.u v.es/event/3366/contributions/9896/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9896/ END:VEVENT BEGIN:VEVENT SUMMARY:Review of raditive B meson decays in LHCb DTSTART;VALUE=DATE-TIME:20181029T140000Z DTEND;VALUE=DATE-TIME:20181029T142000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9895@indico.ific.uv.es DESCRIPTION:Speakers: Samuel Coquereau (Universitat de Barcelona)\nhttps:/ /indico.ific.uv.es/event/3366/contributions/9895/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9895/ END:VEVENT BEGIN:VEVENT SUMMARY:Overview and prospects of phi_s measurements DTSTART;VALUE=DATE-TIME:20181030T095000Z DTEND;VALUE=DATE-TIME:20181030T101000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9869@indico.ific.uv.es DESCRIPTION:Speakers: Veronika Chobanova (University of Santiago de Compos tela)\nhttps://indico.ific.uv.es/event/3366/contributions/9869/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9869/ END:VEVENT BEGIN:VEVENT SUMMARY:Electromagnetic dipole moments of Heavy Baryons with bent crystals at the LHC DTSTART;VALUE=DATE-TIME:20181030T093000Z DTEND;VALUE=DATE-TIME:20181030T095000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9868@indico.ific.uv.es DESCRIPTION:Speakers: Joan Ruiz Vidal (IFIC - University of Valencia and C SIC)\nhttps://indico.ific.uv.es/event/3366/contributions/9868/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9868/ END:VEVENT BEGIN:VEVENT SUMMARY:Pseudoscalar pole contribution to the hadronic light-by-light piec e of (g-2)_\\mu DTSTART;VALUE=DATE-TIME:20181030T091000Z DTEND;VALUE=DATE-TIME:20181030T093000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9867@indico.ific.uv.es DESCRIPTION:Speakers: Adolfo Guevara (Universidad Complutense de Madrid)\n https://indico.ific.uv.es/event/3366/contributions/9867/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9867/ END:VEVENT BEGIN:VEVENT SUMMARY:Amplitude analysis of B and charm decays DTSTART;VALUE=DATE-TIME:20181030T085000Z DTEND;VALUE=DATE-TIME:20181030T091000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9866@indico.ific.uv.es DESCRIPTION:Speakers: Jeremy Dalseno (University of Santiago de Compostela )\nhttps://indico.ific.uv.es/event/3366/contributions/9866/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9866/ END:VEVENT BEGIN:VEVENT SUMMARY:Vacuum Induced CP Violation in a Two Higgs Doublet Model with Cont rolled Scalar FCNC DTSTART;VALUE=DATE-TIME:20181030T083000Z DTEND;VALUE=DATE-TIME:20181030T085000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9865@indico.ific.uv.es DESCRIPTION:Speakers: Miguel Nebot Gómez (U. of Valencia - IFIC)\nhttps:/ /indico.ific.uv.es/event/3366/contributions/9865/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9865/ END:VEVENT BEGIN:VEVENT SUMMARY:CP violation with charmless Vector-Vector decays DTSTART;VALUE=DATE-TIME:20181030T081000Z DTEND;VALUE=DATE-TIME:20181030T083000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9864@indico.ific.uv.es DESCRIPTION:Speakers: Cibrán Santamarina Ríos (Universidade de Santiago de Compostela)\nhttps://indico.ific.uv.es/event/3366/contributions/9864/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9864/ END:VEVENT BEGIN:VEVENT SUMMARY:Strange decays at LHCb DTSTART;VALUE=DATE-TIME:20181030T075000Z DTEND;VALUE=DATE-TIME:20181030T081000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9863@indico.ific.uv.es DESCRIPTION:Speakers: Miguel Ramos Pernas (LHCb experiment)\nhttps://indi co.ific.uv.es/event/3366/contributions/9863/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9863/ END:VEVENT BEGIN:VEVENT SUMMARY:K --> pi pi in the Standard Model: status and prospects DTSTART;VALUE=DATE-TIME:20181030T073000Z DTEND;VALUE=DATE-TIME:20181030T075000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9862@indico.ific.uv.es DESCRIPTION:Speakers: Hector Gisbert Mullor (IFIC)\nhttps://indico.ific.uv .es/event/3366/contributions/9862/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9862/ END:VEVENT BEGIN:VEVENT SUMMARY:Challenge of tracking long-lived particles at LHCb DTSTART;VALUE=DATE-TIME:20181029T174000Z DTEND;VALUE=DATE-TIME:20181029T175800Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9861@indico.ific.uv.es DESCRIPTION:Speakers: Louis Henry (IFIC)\nhttps://indico.ific.uv.es/event/ 3366/contributions/9861/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9861/ END:VEVENT BEGIN:VEVENT SUMMARY:Flavour Conservation in Two Higgs Doublet Models DTSTART;VALUE=DATE-TIME:20181029T170400Z DTEND;VALUE=DATE-TIME:20181029T172200Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9860@indico.ific.uv.es DESCRIPTION:Speakers: Fernando Cornet-Gomez (IFIC (UV &\; CSIC))\nhttps ://indico.ific.uv.es/event/3366/contributions/9860/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9860/ END:VEVENT BEGIN:VEVENT SUMMARY:Global fits in the Aligned Two-Higgs Doublet model DTSTART;VALUE=DATE-TIME:20181029T164600Z DTEND;VALUE=DATE-TIME:20181029T170400Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9859@indico.ific.uv.es DESCRIPTION:Speakers: Ana Peñuelas Martínez (IFIC-UV)\nhttps://indico.if ic.uv.es/event/3366/contributions/9859/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9859/ END:VEVENT BEGIN:VEVENT SUMMARY:Photon polarization from b-baryon decays DTSTART;VALUE=DATE-TIME:20181029T162800Z DTEND;VALUE=DATE-TIME:20181029T164600Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9858@indico.ific.uv.es DESCRIPTION:Speakers: Luis Miguel García (IFIC)\nhttps://indico.ific.uv.e s/event/3366/contributions/9858/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9858/ END:VEVENT BEGIN:VEVENT SUMMARY:Photon Polarization from Bs->phigamma decays DTSTART;VALUE=DATE-TIME:20181029T151200Z DTEND;VALUE=DATE-TIME:20181029T153000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9855@indico.ific.uv.es DESCRIPTION:Speakers: Clara Remon Alepuz (PhD Student)\nhttps://indico.ifi c.uv.es/event/3366/contributions/9855/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9855/ END:VEVENT BEGIN:VEVENT SUMMARY:LFU tests in the angular observables of B -> D* l nu DTSTART;VALUE=DATE-TIME:20181029T145400Z DTEND;VALUE=DATE-TIME:20181029T151200Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9854@indico.ific.uv.es DESCRIPTION:Speakers: Marco Fedele ()\nhttps://indico.ific.uv.es/event/336 6/contributions/9854/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9854/ END:VEVENT BEGIN:VEVENT SUMMARY:Lepton Flavour Universality tests using semitauonic decays at LHCb DTSTART;VALUE=DATE-TIME:20181029T143600Z DTEND;VALUE=DATE-TIME:20181029T145400Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9853@indico.ific.uv.es DESCRIPTION:Speakers: Beatriz Garcia Plana (U. Santiago)\nhttps://indico.i fic.uv.es/event/3366/contributions/9853/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9853/ END:VEVENT BEGIN:VEVENT SUMMARY:Status and prospects of rare B decays DTSTART;VALUE=DATE-TIME:20181029T140000Z DTEND;VALUE=DATE-TIME:20181029T141800Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9851@indico.ific.uv.es DESCRIPTION:Speakers: Carlos Sanchez Mayordomo (IFIC - Universitat de Val ència)\nhttps://indico.ific.uv.es/event/3366/contributions/9851/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9851/ END:VEVENT BEGIN:VEVENT SUMMARY:Neutrinos DTSTART;VALUE=DATE-TIME:20181030T134500Z DTEND;VALUE=DATE-TIME:20181030T141500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9946@indico.ific.uv.es DESCRIPTION:Speakers: Pilar Hernández (IFIC\, CSIC-Univ Valencia)\nhttps: //indico.ific.uv.es/event/3366/contributions/9946/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9946/ END:VEVENT BEGIN:VEVENT SUMMARY:Charla equipo gestor programa FPN y discusión estrategia europea DTSTART;VALUE=DATE-TIME:20181030T103000Z DTEND;VALUE=DATE-TIME:20181030T122500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9947@indico.ific.uv.es DESCRIPTION:Speakers: Javier Cuevas (Universidad de Oviedo)\nhttps://indic o.ific.uv.es/event/3366/contributions/9947/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9947/ END:VEVENT BEGIN:VEVENT SUMMARY:Radiative corrections in Dalitz decays of $\\pi^0$\, $\\eta$ and $ \\eta^\\prime$ mesons DTSTART;VALUE=DATE-TIME:20181029T150000Z DTEND;VALUE=DATE-TIME:20181029T152000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9915@indico.ific.uv.es DESCRIPTION:Speakers: Tomas Husek (IFIC)\nWe briefly summarize current exp erimental and theoretical results on the two important processes of the lo w-energy hadron physics involving neutral pions: the Dalitz decay of $\\pi ^0$ and the rare decay $\\pi^0\\to e^+e^-$. As novel results we present th e complete set of radiative corrections to the Dalitz decays $\\eta^{(\\pr ime)}\\to\\ell^+\\ell^-\\gamma$ beyond the soft-photon approximation\, i.e .\\ over the whole range of the Dalitz plot and with no restrictions on th e energy of a radiative photon. The corrections inevitably depend on the $ \\eta^{(\\prime)}\\to\\gamma^*\\gamma^{(*)}$ transition form factors. For the singly-virtual transition form factor appearing e.g.\\ in the bremsstr ahlung correction\, recent dispersive calculations are used. For the one-p hoton-irreducible contribution at the one-loop level (for the doubly-virtu al form factor)\, we use a vector-meson-dominance-inspired model while tak ing into account the $\\eta$-$\\eta^\\prime$ mixing.\n\nhttps://indico.ifi c.uv.es/event/3366/contributions/9915/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9915/ END:VEVENT BEGIN:VEVENT SUMMARY:Confronting SUSY GUT with Dark Matter\, Sparticle Spectroscopy and Muon(g-2) DTSTART;VALUE=DATE-TIME:20181030T084500Z DTEND;VALUE=DATE-TIME:20181030T090500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9849@indico.ific.uv.es DESCRIPTION:Speakers: Mario E. Gómez (Univ Huelva)\nhttps://indico.ific.u v.es/event/3366/contributions/9849/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9849/ END:VEVENT BEGIN:VEVENT SUMMARY:Latest results from the NEXT experiment DTSTART;VALUE=DATE-TIME:20181029T162000Z DTEND;VALUE=DATE-TIME:20181029T164500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9933@indico.ific.uv.es DESCRIPTION:Speakers: Brais Palmeiro (USC & IFIC (CSIC-UV) )\nhttps://indi co.ific.uv.es/event/3366/contributions/9933/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9933/ END:VEVENT BEGIN:VEVENT SUMMARY:Hadron physics for neutrino oscillation experiments DTSTART;VALUE=DATE-TIME:20181029T151000Z DTEND;VALUE=DATE-TIME:20181029T153500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9881@indico.ific.uv.es DESCRIPTION:Speakers: Luis Álvarez Ruso (IFIC\, CSIC-Univ Valencia)\nhttp s://indico.ific.uv.es/event/3366/contributions/9881/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9881/ END:VEVENT BEGIN:VEVENT SUMMARY:Results from T2K DTSTART;VALUE=DATE-TIME:20181029T145000Z DTEND;VALUE=DATE-TIME:20181029T151000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9930@indico.ific.uv.es DESCRIPTION:Speakers: Alexander Izmaylov (IFIC\, CSIC-Univ Valencia)\nhttp s://indico.ific.uv.es/event/3366/contributions/9930/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9930/ END:VEVENT BEGIN:VEVENT SUMMARY:Searches for Dark Matter with the ANTARES/KM3Net neutrino telescop es DTSTART;VALUE=DATE-TIME:20181029T182500Z DTEND;VALUE=DATE-TIME:20181029T184000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9945@indico.ific.uv.es DESCRIPTION:Speakers: Sara Rebecca Gozzini (IFIC\, CSIC-Univ Valencia)\nht tps://indico.ific.uv.es/event/3366/contributions/9945/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9945/ END:VEVENT BEGIN:VEVENT SUMMARY:Oscillation Physics with KM3NeT-ORCA DTSTART;VALUE=DATE-TIME:20181029T184000Z DTEND;VALUE=DATE-TIME:20181029T185500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9936@indico.ific.uv.es DESCRIPTION:Speakers: Tarak Thakore (IFIC\, CSIC-Univ Valencia)\nhttps://i ndico.ific.uv.es/event/3366/contributions/9936/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9936/ END:VEVENT BEGIN:VEVENT SUMMARY:Searches for point-like sources with the ANTARES neutrino telescop e DTSTART;VALUE=DATE-TIME:20181029T181000Z DTEND;VALUE=DATE-TIME:20181029T182500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9814@indico.ific.uv.es DESCRIPTION:Speakers: Giulia Illuminati (IFIC\, CSIC-Univ Valencia)\nhttps ://indico.ific.uv.es/event/3366/contributions/9814/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9814/ END:VEVENT BEGIN:VEVENT SUMMARY:The Earth as seen by neutrinos: an update DTSTART;VALUE=DATE-TIME:20181029T174500Z DTEND;VALUE=DATE-TIME:20181029T181000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9836@indico.ific.uv.es DESCRIPTION:Speakers: Andrea Donini (IFIC\, CSIC-Univ Valencia)\nhttps://i ndico.ific.uv.es/event/3366/contributions/9836/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9836/ END:VEVENT BEGIN:VEVENT SUMMARY:protoDUNE-SP DTSTART;VALUE=DATE-TIME:20181029T172500Z DTEND;VALUE=DATE-TIME:20181029T174500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9931@indico.ific.uv.es DESCRIPTION:Speakers: Pablo Fernández (IFIC\, CSIC-Univ Valencia)\nhttps: //indico.ific.uv.es/event/3366/contributions/9931/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9931/ END:VEVENT BEGIN:VEVENT SUMMARY:protoDUNE dual-phase DTSTART;VALUE=DATE-TIME:20181029T170500Z DTEND;VALUE=DATE-TIME:20181029T172500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9932@indico.ific.uv.es DESCRIPTION:Speakers: Ana Gallego (CIEMAT)\nhttps://indico.ific.uv.es/even t/3366/contributions/9932/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9932/ END:VEVENT BEGIN:VEVENT SUMMARY:Light sterile neutrinos: the 2018 status DTSTART;VALUE=DATE-TIME:20181029T164500Z DTEND;VALUE=DATE-TIME:20181029T170500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9815@indico.ific.uv.es DESCRIPTION:Speakers: Stefano Gariazzo (IFIC\, CSIC-Univ Valencia)\nhttps: //indico.ific.uv.es/event/3366/contributions/9815/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9815/ END:VEVENT BEGIN:VEVENT SUMMARY:Discusión general de la red RENATA DTSTART;VALUE=DATE-TIME:20181030T093000Z DTEND;VALUE=DATE-TIME:20181030T100000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9937@indico.ific.uv.es DESCRIPTION:Speakers: Sergio Pastor (IFIC\, CSIC-Univ Valencia)\nhttps://i ndico.ific.uv.es/event/3366/contributions/9937/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9937/ END:VEVENT BEGIN:VEVENT SUMMARY:Recent Results from AMS-02 on the International Space Station DTSTART;VALUE=DATE-TIME:20181030T090500Z DTEND;VALUE=DATE-TIME:20181030T093000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9935@indico.ific.uv.es DESCRIPTION:Speakers: Miguel Molero (CIEMAT)\nhttps://indico.ific.uv.es/ev ent/3366/contributions/9935/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9935/ END:VEVENT BEGIN:VEVENT SUMMARY:Testing dark matter with dense stars DTSTART;VALUE=DATE-TIME:20181030T082500Z DTEND;VALUE=DATE-TIME:20181030T084500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9848@indico.ific.uv.es DESCRIPTION:Speakers: M. Ángeles Pérez-García (Univ Salamanca)\nhttps:/ /indico.ific.uv.es/event/3366/contributions/9848/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9848/ END:VEVENT BEGIN:VEVENT SUMMARY:Status of ANAIS DTSTART;VALUE=DATE-TIME:20181030T080000Z DTEND;VALUE=DATE-TIME:20181030T082500Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9934@indico.ific.uv.es DESCRIPTION:Speakers: María Martínez (Univ Zaragoza)\nhttps://indico.ifi c.uv.es/event/3366/contributions/9934/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9934/ END:VEVENT BEGIN:VEVENT SUMMARY:Status of three-neutrino mixing DTSTART;VALUE=DATE-TIME:20181029T153500Z DTEND;VALUE=DATE-TIME:20181029T160000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9816@indico.ific.uv.es DESCRIPTION:Speakers: Christoph A. Ternes (IFIC\, CSIC-Univ Valencia)\nhtt ps://indico.ific.uv.es/event/3366/contributions/9816/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9816/ END:VEVENT BEGIN:VEVENT SUMMARY:Double Chooz results DTSTART;VALUE=DATE-TIME:20181029T143000Z DTEND;VALUE=DATE-TIME:20181029T145000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9850@indico.ific.uv.es DESCRIPTION:Speakers: Diana Navas-Nicolás (CIEMAT)\nhttps://indico.ific.u v.es/event/3366/contributions/9850/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9850/ END:VEVENT BEGIN:VEVENT SUMMARY:Coffee break DTSTART;VALUE=DATE-TIME:20181029T160000Z DTEND;VALUE=DATE-TIME:20181029T162000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9468@indico.ific.uv.es DESCRIPTION:https://indico.ific.uv.es/event/3366/contributions/9468/ LOCATION: URL:https://indico.ific.uv.es/event/3366/contributions/9468/ END:VEVENT BEGIN:VEVENT SUMMARY:Type IIA flux vacua with D6-branes DTSTART;VALUE=DATE-TIME:20181030T094000Z DTEND;VALUE=DATE-TIME:20181030T100000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9929@indico.ific.uv.es DESCRIPTION:Speakers: Dagoberto Escobar (IFT)\nWe consider Type IIA compac tifications on Calabi-Yau orientifolds\nwith non-trivial background fluxes and mobile D6-branes.  In this context\, we investigate whether some kno wn examples of stable type IIA vacua are kept in the presence of open stri ng degrees of freedom.\n\nhttps://indico.ific.uv.es/event/3366/contributio ns/9929/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9929/ END:VEVENT BEGIN:VEVENT SUMMARY:Standard model fermion corrections to the Chiral Electroweak Lagra ngian at one-loop level DTSTART;VALUE=DATE-TIME:20181030T092000Z DTEND;VALUE=DATE-TIME:20181030T094000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9928@indico.ific.uv.es DESCRIPTION:Speakers: Carlos Quezada (UCM)\nWe consider an effective non-l inear Electroweak Chiral Lagrangian  containing three would-be Goldstone bosons: w^a which transform non-linearly as a triplet under SU(2)_L  X SU (2)_R and a Higgs singlet h plus its couplings to fermions via Yukawa inte ractions. This low energy model is valid for the range M_h\,M_W\,M_Z \n\nh ttps://indico.ific.uv.es/event/3366/contributions/9928/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9928/ END:VEVENT BEGIN:VEVENT SUMMARY:Testable Axion-Like Particles In The Minimal Linear sigma-Model DTSTART;VALUE=DATE-TIME:20181030T090000Z DTEND;VALUE=DATE-TIME:20181030T092000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9927@indico.ific.uv.es DESCRIPTION:Speakers: Javier Alonso-Gonzalez (IFT)\nAxion and axion-like p article models are typically affected by a strong fine-tuning problem in c onceiving the electroweak and the Peccei-Quinn breaking scales. Within the context of the Minimal Linear ${\\sigma}$ Model\, axion-like particle c onstructions are identified where this hierarchy problem is solved\, accou nting for a TeV Peccei-Quinn breaking scale and a pseudoscalar particle wi th a mass larger than 10 MeV. Potential signatures at the LHC are discusse d. \n\nThe talk would be bases on "J. Alonso-González\, L. Merlo\, F. Po bbe\, S. Rigolin and O. Sumensari\, >\, arXiv:1807.08643 [hep-ph]”.\n\n https://indico.ific.uv.es/event/3366/contributions/9927/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9927/ END:VEVENT BEGIN:VEVENT SUMMARY:Hierarchies in SU(2)_L x SU(2)_R x U(1)_X effective potential mode ls DTSTART;VALUE=DATE-TIME:20181030T084000Z DTEND;VALUE=DATE-TIME:20181030T090000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9926@indico.ific.uv.es DESCRIPTION:Speakers: Clara Alvarez Luna (UCM)\nIn the present work we stu dy a model with an SU(2)_L x SU(2)_R x U(1)_X$ symmetry\, with two scalar doublets. We start from a massless lagrangian\, but by using the Coleman-W einberg mechanism we obtain masses for both the gauge bosons and the scala rs. We also calculate the renormalized effective potential\, depending on the masses and couplings of the model. With this formalism we obtain two s ets of gauge bosons\, corresponding to the L and R sectors\, in addition t o the two scalars. We analyse the mass ratio of these sectors in order to obtain a hyerarchy between them. With an appropriate choice of parameters we can have the L particles in the SM range\, while the R particles have m uch higher masses.\n\nhttps://indico.ific.uv.es/event/3366/contributions/9 926/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9926/ END:VEVENT BEGIN:VEVENT SUMMARY:Fermionic Perturbations in Hybrid Loop Quantum Cosmology DTSTART;VALUE=DATE-TIME:20181030T082000Z DTEND;VALUE=DATE-TIME:20181030T084000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9925@indico.ific.uv.es DESCRIPTION:Speakers: Santiago Prado Loy (IEM)\nIn this seminar\, we apply the formalism known as hybrid loop quantum cosmology to the physically in teresting case of fermionic cosmological perturbations. Within this formal ism\, we study the possible splitting procedures between the cosmological geometry and the perturbations\, leading to different Hamiltonian dynamics . The geometry is quantized by methods inspired in loop quantum gravity\, whereas the perturbations are quantized by usual techniques of quantum fie ld theory in curved spacetimes. We then discuss the freedom available to d efine creation and annihilation operators for the fermionic degrees of fre edom and determine the sufficient and necessary conditions that this defin ition must satisfy in order to provide a quantum theory with good properti es in the matter sector.\n\nhttps://indico.ific.uv.es/event/3366/contribut ions/9925/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9925/ END:VEVENT BEGIN:VEVENT SUMMARY:Spontaneous proton decay and the origin of Peccei-Quinn symmetry DTSTART;VALUE=DATE-TIME:20181030T080000Z DTEND;VALUE=DATE-TIME:20181030T082000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9924@indico.ific.uv.es DESCRIPTION:Speakers: Mario Reig (IFIC)\nWe propose a new interpretation o f Peccei-Quinn symmetry within the Standard Model\, identifying it with th e axial B+L symmetry i.e. U(1)PQ≡U(1)γ5(B+L). This new interpretation r etains all the attractive features of Peccei-Quinn solution to strong CP p roblem but in addition also leads to several other new and interesting con sequences. Owing to the identification U(1)PQ≡U(1)γ5(B+L) the axion als o behaves like Majoron inducing small seesaw masses for neutrinos after sp ontaneous symmetry breaking. Another novel feature of this identification is the phenomenon of spontaneous (and also chiral) proton decay with its d ecay rate associated with the axion decay constant. Low energy processes w hich can be used to test this interpretation are pointed out.\n\nhttps://i ndico.ific.uv.es/event/3366/contributions/9924/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9924/ END:VEVENT BEGIN:VEVENT SUMMARY:Supertranslations: redundancies of horizon data\, and global symme tries at null infinity DTSTART;VALUE=DATE-TIME:20181029T180000Z DTEND;VALUE=DATE-TIME:20181029T182000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9923@indico.ific.uv.es DESCRIPTION:Speakers: Guillermo Milans (IFT)\nWe characterise the geometri cal nature of smooth supertranslations\ndefined on a generic non-expanding horizon (NEH) embedded in vacuum. To this\nend we consider the constraint s imposed by the vacuum Einstein’s equations on the\nNEH structure\, and discuss the transformation properties of their solutions under\nsupertran slations. We present a freely specifiable data set which is both necessary \nand sufficient to reconstruct the full horizon geometry\, and is compose d of objects\nwhich are invariant under supertranslations. We conclude tha t smooth supertranslations\ndo not transform the geometry of the NEH\, and that they should be regarded\nas pure gauge. Our results apply both to st ationary\, and non-stationary states of a\nNEH\, the later ones being able to describe radiative processes taking place on the\nhorizon. As a consis tency check we repeat the analysis for BMS supertranslations\ndefined on n ull infinity\, I. Using the same framework as for the NEH we recover the\n well known result that BMS supertranslations act non-trivially on the free data on\nI. The full analysis is done in exact\, non-linear\, general rel ativity.\n\nhttps://indico.ific.uv.es/event/3366/contributions/9923/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9923/ END:VEVENT BEGIN:VEVENT SUMMARY:Constraints on anharmonic corrections of fuzzy dark matter DTSTART;VALUE=DATE-TIME:20181029T174000Z DTEND;VALUE=DATE-TIME:20181029T180000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9922@indico.ific.uv.es DESCRIPTION:Speakers: Hector Villarrubia-Rojo (UCM)\nThe cold dark matter (CDM) scenario has proved successful in cosmology.\nHowever\, we lack a fu ndamental understanding of its microscopic nature. Moreover\, the\napparen t disagreement between CDM predictions and subgalactic-structure observati ons\nhas prompted the debate about its behaviour at small scales. These pr oblems could be\nalleviated if the dark matter is composed of ultralight f ields m ∼ 10 −22 eV\, usually known\nas fuzzy dark matter (FDM). Some specific models\, with axion-like potentials\, have been\nthoroughly studi ed and are collectively referred to as ultralight axions (ULAs) or axion-l ike\nparticles (ALPs). In this work we consider anharmonic corrections to the mass term coming from a repulsive quartic self-interaction. Whenever t his anharmonic term dominates\, the field behaves as radiation instead of cold matter\, modifying the time of matter-radiation equality. Additionall y\, even for high masses\, i.e. masses that reproduce the cold mat-\nter b ehaviour\, the presence of anharmonic terms introduce a cut-off in the mat ter power\nspectrum through its contribution to the sound speed. We analyz e the model and derive\nconstraints using a modified version of class and comparing with CMB and large-scale\nstructure data.\n\nhttps://indico.ific .uv.es/event/3366/contributions/9922/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9922/ END:VEVENT BEGIN:VEVENT SUMMARY:RG-2 flow\, mass and entropy DTSTART;VALUE=DATE-TIME:20181029T172000Z DTEND;VALUE=DATE-TIME:20181029T174000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9921@indico.ific.uv.es DESCRIPTION:Speakers: Oscar Lasso (IFT)\nThe RG-2 flow is the two-loop app roximation for the world-sheet non \nlinear sigma model renormalization gr oup flow. The first truncation of \nthe flow is the well known Ricci flow\ , at two loops higher order \ncurvature terms appear\, changing almost com pletely the behaviour of \nthe evolution equation. In this talk we study t he RG-2 flow in the \ncontext of general relativity. Considering a time sy mmetric foliation \nof an asymptotically flat spacetime we show that the a rea A of a \nclosed two dimensional surface S is monotonous under the RG-2 flow\, \nrefining and extending the previous results already known for th e \nRicci flow\, we also discuss about the possibility of extending the \n result to all loops. We show that the inequality relating the area of \nth e surface S and the Hawking mass already found for the Ricci flow is \nsti ll satisfied when we make evolve the area under the new flow.\n\nhttps://i ndico.ific.uv.es/event/3366/contributions/9921/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9921/ END:VEVENT BEGIN:VEVENT SUMMARY:Higher-order corrections in the Higgs sector of the MnuSSM DTSTART;VALUE=DATE-TIME:20181029T170000Z DTEND;VALUE=DATE-TIME:20181029T172000Z DTSTAMP;VALUE=DATE-TIME:20260712T150907Z UID:indico-contribution-3366-9920@indico.ific.uv.es DESCRIPTION:Speakers: Thomas Biekotter (IFT)\nThe MnuSSM is a simple super symmetric extension of the Standard Model (SM) capable of predicting neutr ino physics in agreement with experiment. In this paper we perform the com plete one-loop renormalization of the neutral scalar sector of the MnuSSM with one and three generations of right-handed neutrinos in a mixed on-she ll/DR scheme. The renormalization procedure is discussed in detail\, empha sizing conceptual differences to the minimal (MSSM) and next-to-minimal (N MSSM) supersymmetric standard model regarding the field renormalization an d the treatment of non-flavor-diagonal soft mass parameters\, which have t heir origin in the breaking of R-parity. We calculate the full one-loop co rrections to the neutral scalar masses of the MnuSSM. The one-loop contrib utions are supplemented by available MSSM higher-order corrections. We obt ain numerical results for a SM-like Higgs boson mass consistent with exper imental bounds. Corrections genuine for the MnuSSM are discussed in exampl e scenarios. Finally we show that the MnuSSM can accomodate a Higgs boson that could explain an excess of diphoton events at ∼96GeV\, as reported by CMS\, as well as the 2σ excess of bb events observed at LEP at a simil ar mass scale.\n\nhttps://indico.ific.uv.es/event/3366/contributions/9920/ LOCATION:Hospedería Fonseca y hotel Abba Fonseca (Salamanca) URL:https://indico.ific.uv.es/event/3366/contributions/9920/ END:VEVENT END:VCALENDAR