BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Prospects for SUSY discovery with MoEDAL DTSTART;VALUE=DATE-TIME:20181214T083000Z DTEND;VALUE=DATE-TIME:20181214T090000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10277@indico.ific.uv.es DESCRIPTION:Speakers: Vasiliki Mitsou (IFIC Valencia)\nWe present a study on searches for supersymmetric metastable particles at the MoEDAL detector . MoEDAL is sensitive to highly ionising objects such as magnetic monopole s or massive long-lived charged particles and we focus on the latter in th is talk. Requirements for triggering or reducing cosmic-ray and cavern bac kgrounds\, applied in ATLAS and CMS analyses\, are not necessary at MoEDAL \, due to its different detector concept\, requiring slow-moving particles \, and low background. Using Monte Carlo simulations\, we compare the sens itivities of MoEDAL versus ATLAS/CMS for various long-lived particles in s upersymmetric models\, and seek a scenario where MoEDAL can act in a compl ementary way to ATLAS and CMS.\n\nhttps://indico.ific.uv.es/event/3485/con tributions/10277/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10277/ END:VEVENT BEGIN:VEVENT SUMMARY:The International Linear Collider\, status and scientific case DTSTART;VALUE=DATE-TIME:20181213T100000Z DTEND;VALUE=DATE-TIME:20181213T103000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10280@indico.ific.uv.es DESCRIPTION:Speakers: Juan Antonio Fuster Verdu (IFIC (Instituto de Fisica Corpuscular))\nhttps://indico.ific.uv.es/event/3485/contributions/10280/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10280/ END:VEVENT BEGIN:VEVENT SUMMARY:A global fit of right-handed neutrinos with GAMBIT DTSTART;VALUE=DATE-TIME:20181213T113000Z DTEND;VALUE=DATE-TIME:20181213T120000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10262@indico.ific.uv.es DESCRIPTION:Speakers: Julia Harz (Technical University of Munich (TUM) )\n https://indico.ific.uv.es/event/3485/contributions/10262/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10262/ END:VEVENT BEGIN:VEVENT SUMMARY:Restricted texture in SS-I DTSTART;VALUE=DATE-TIME:20181212T113000Z DTEND;VALUE=DATE-TIME:20181212T120000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10257@indico.ific.uv.es DESCRIPTION:Speakers: Filipe Joaquim (CFTP\, IST)\nhttps://indico.ific.uv. es/event/3485/contributions/10257/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10257/ END:VEVENT BEGIN:VEVENT SUMMARY:Social dinner DTSTART;VALUE=DATE-TIME:20181213T200000Z DTEND;VALUE=DATE-TIME:20181213T230000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10288@indico.ific.uv.es DESCRIPTION:https://indico.ific.uv.es/event/3485/contributions/10288/ LOCATION:Pan Comido URL:https://indico.ific.uv.es/event/3485/contributions/10288/ END:VEVENT BEGIN:VEVENT SUMMARY:Welcome DTSTART;VALUE=DATE-TIME:20181212T075000Z DTEND;VALUE=DATE-TIME:20181212T080000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10287@indico.ific.uv.es DESCRIPTION:https://indico.ific.uv.es/event/3485/contributions/10287/ LOCATION:Casa de la Ciencia del CSIC URL:https://indico.ific.uv.es/event/3485/contributions/10287/ END:VEVENT BEGIN:VEVENT SUMMARY:Registration DTSTART;VALUE=DATE-TIME:20181212T073000Z DTEND;VALUE=DATE-TIME:20181212T075000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10286@indico.ific.uv.es DESCRIPTION:https://indico.ific.uv.es/event/3485/contributions/10286/ LOCATION:Casa de la Ciencia del CSIC URL:https://indico.ific.uv.es/event/3485/contributions/10286/ END:VEVENT BEGIN:VEVENT SUMMARY:The promising future of a robust cosmological neutrino mass measur ement DTSTART;VALUE=DATE-TIME:20181212T155000Z DTEND;VALUE=DATE-TIME:20181212T161000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10267@indico.ific.uv.es DESCRIPTION:Speakers: Maria Archidiacono (RWTH Aachen University)\nThe imp act of massive neutrinos on cosmological observables comes from a very pec uliar effect: light massive neutrinos behave as radiation before their non -relativistic transition\, while afterwards they gradually become a matter component. For that reason\, combination of high- and low- redshift probe s can provide very tight\, yet model dependent\, constraints on the neutri no mass sum. In this talk I will show how future galaxy surveys can potent ially pin down the neutrino mass sum.​\n\nhttps://indico.ific.uv.es/even t/3485/contributions/10267/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10267/ END:VEVENT BEGIN:VEVENT SUMMARY:Supersymmetry searches at the ATLAS experiment DTSTART;VALUE=DATE-TIME:20181214T113000Z DTEND;VALUE=DATE-TIME:20181214T120000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10285@indico.ific.uv.es DESCRIPTION:Speakers: Judita Mamuzic (IFIC/CSIC)\nSupersymmetry represents an important theory in physics Beyond the Standard Model which postulates a symmetry between fermions and bosons\, and introduces a new set of part icles at the electroweak scale. An overview of recent results in SUSY sear ches using strong\, electroweak\, third generation production\, R-parity v iolation models\, and long lived particles\, using 13 TeV Run 2 ATLAS data will be presented. Emphasis will be given to models related to neutrino p hysics\, such as the Bilinear R-parity violation (bRPV) model\, where the results of 8 TeV searches will be shown.\n\nhttps://indico.ific.uv.es/even t/3485/contributions/10285/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10285/ END:VEVENT BEGIN:VEVENT SUMMARY:The DUNE experiment DTSTART;VALUE=DATE-TIME:20181214T110000Z DTEND;VALUE=DATE-TIME:20181214T113000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10284@indico.ific.uv.es DESCRIPTION:Speakers: Anselmo Cervera (IFIC)\nDUNE is a next-generation ne utrino oscillation experiment whose main goal is to discover CP violation in the leptonic sector and measure the mass hierarchy in a single experime nt. It has a very rich scientific program that also includes proton decay searches\, supernovae burst neutrino detection and beyond standard model p hysics. In this talk the experiment and his current status will be describ ed as well as his physics potencial.\n\nhttps://indico.ific.uv.es/event/34 85/contributions/10284/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10284/ END:VEVENT BEGIN:VEVENT SUMMARY:Status of KM3NeT and results from ANTARES DTSTART;VALUE=DATE-TIME:20181214T103000Z DTEND;VALUE=DATE-TIME:20181214T110000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10283@indico.ific.uv.es DESCRIPTION:Speakers: Juande Zornoza (IFIC)\nI will review the most recent results of the ANTARES neutrino telescopes and describe the status and ph ysics program of its successor\, KM3NeT\, already in construction.\n\nhttp s://indico.ific.uv.es/event/3485/contributions/10283/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10283/ END:VEVENT BEGIN:VEVENT SUMMARY:Production of Magnetic Monopoles Via Photon Fusion and search resu lts from MoEDAL experiment DTSTART;VALUE=DATE-TIME:20181214T093000Z DTEND;VALUE=DATE-TIME:20181214T100000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10282@indico.ific.uv.es DESCRIPTION:Speakers: Arka Santra (Instituto de Fisica Corpuscular)\nIf th e Dirac magnetic monopoles exist\, they can be probed in the collider expe riments. In the previous searches\, only the Drell-Yan production mechanis m of magnetic monopoles was used to look for these particles. But the cros s-section of the photon-fusion production mechanism of the magnetic monopo les is higher than that of the Drell-Yan production mechanism at the LHC e nergy. I will discuss the photon-fusion production mechanism of spins 0\, 1⁄2 and 1 magnetic monopoles using MadGraph event generator. I will also compare the kinematic and angular distributions of magnetic monopoles hav ing those three spins. The comparison between Drell-Yan process and photon -fusion process will also be shown (from Baines et. al. arXiv:1808.08942 [ hep-ph]). I will discuss the monopole search results of MoEDAL experiment (from Physics Letters B\, 782\, (2018)\, https://doi.org/10.1016/j.physlet b.2018.05.069) where this experiment has set the strongest limits on monop oles of high magnetic charge.\n\nhttps://indico.ific.uv.es/event/3485/cont ributions/10282/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10282/ END:VEVENT BEGIN:VEVENT SUMMARY:Higgs portal DM at colliders DTSTART;VALUE=DATE-TIME:20181214T090000Z DTEND;VALUE=DATE-TIME:20181214T093000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10281@indico.ific.uv.es DESCRIPTION:Speakers: Abdelhak Djouadi (LPT Orsay)\nhttps://indico.ific.uv .es/event/3485/contributions/10281/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10281/ END:VEVENT BEGIN:VEVENT SUMMARY:Some aspects of Leptogenesis with discrete flavor symmetry DTSTART;VALUE=DATE-TIME:20181213T110000Z DTEND;VALUE=DATE-TIME:20181213T113000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10279@indico.ific.uv.es DESCRIPTION:Speakers: Anjan Giri (IIT Hyderabad)\nWe will briefly discuss about a scenario of Leptogenesis with the simple S_3 discrete flavor symme try. In order to explain the neutrino phenomenology we will incorporate Ty pe-I and II seesaw scenarios with additional right handed neutrinos and sc alar triplets. Thereafter\, we will attempt to explain the baryon asymmetr y and discuss the prospects.\n\nhttps://indico.ific.uv.es/event/3485/contr ibutions/10279/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10279/ END:VEVENT BEGIN:VEVENT SUMMARY:The origin of flavor mixing from dihedral groups and Dirac neutrin o masses DTSTART;VALUE=DATE-TIME:20181213T103000Z DTEND;VALUE=DATE-TIME:20181213T110000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10278@indico.ific.uv.es DESCRIPTION:Speakers: Gui-Jun Ding (University of Science and Technology o f China)\nhttps://indico.ific.uv.es/event/3485/contributions/10278/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10278/ END:VEVENT BEGIN:VEVENT SUMMARY:Spontaneous CP Violation and Controlled Scalar FCNC in a 2HDM DTSTART;VALUE=DATE-TIME:20181213T090000Z DTEND;VALUE=DATE-TIME:20181213T093000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10276@indico.ific.uv.es DESCRIPTION:Speakers: Miguel Nebot (U. of Valencia - IFIC)\nA 2HDM where a ll CP Violation originates from the vacuum state is presented. The model i ncludes Scalar Flavour Changing Neutral Couplings which are shown to be co ntrolled. The viability of the model is illustrated in a phenomenological analysis\, including beyond-SM observation prospects\n\nhttps://indico.ifi c.uv.es/event/3485/contributions/10276/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10276/ END:VEVENT BEGIN:VEVENT SUMMARY:CP violation from strings DTSTART;VALUE=DATE-TIME:20181213T083000Z DTEND;VALUE=DATE-TIME:20181213T090000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10275@indico.ific.uv.es DESCRIPTION:Speakers: Michael Ratz (UC Irvine)\nhttps://indico.ific.uv.es/ event/3485/contributions/10275/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10275/ END:VEVENT BEGIN:VEVENT SUMMARY:Discrete Family Symmetries and CP Violation DTSTART;VALUE=DATE-TIME:20181213T080000Z DTEND;VALUE=DATE-TIME:20181213T083000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10274@indico.ific.uv.es DESCRIPTION:Speakers: Mu-Chun Chen (UC Irvine)\nhttps://indico.ific.uv.es/ event/3485/contributions/10274/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10274/ END:VEVENT BEGIN:VEVENT SUMMARY:Search for Right-Handed Neutrinos from Dark Matter Annihilation wi th Fermi-LAT and H.E.S.S. Telescopes DTSTART;VALUE=DATE-TIME:20181214T150000Z DTEND;VALUE=DATE-TIME:20181214T152000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10273@indico.ific.uv.es DESCRIPTION:Speakers: Miguel Campos (King's College London)\nThe best stra tegy for indirect detection of dark matter depends entirely on its annihil ation processes. In this work we discuss a model independent probe for dar k matter annihilations into right-handed neutrinos in the GeV-TeV mass ran ge\, using dwarf spheroidal galaxies and the galactic center observations performed by Fermi-LAT and H.E.S.S.\, respectively. We exclude the thermal annihilation cross section for dark matter masses below 200 GeV.\n\nhttps ://indico.ific.uv.es/event/3485/contributions/10273/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10273/ END:VEVENT BEGIN:VEVENT SUMMARY:Impact of non-standard interactions at long baseline experiments DTSTART;VALUE=DATE-TIME:20181213T142000Z DTEND;VALUE=DATE-TIME:20181213T144000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10272@indico.ific.uv.es DESCRIPTION:Speakers: Poonam Mehta (Jawaharlal Nehru University)\nhttps:// indico.ific.uv.es/event/3485/contributions/10272/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10272/ END:VEVENT BEGIN:VEVENT SUMMARY:Cosmic neutrinos vs. galactic feedback DTSTART;VALUE=DATE-TIME:20181214T144000Z DTEND;VALUE=DATE-TIME:20181214T150000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10271@indico.ific.uv.es DESCRIPTION:Speakers: Gabriele Parimbelli (SISSA)\nMassive neutrinos and b aryon feedback both suppress the matter power spectrum at small scales and are therefore expected to be degenerate with each other. I will show that this degeneracy is not perfect and can indeed be broken by performing tom ography on the cold dark matter and shear power spectra. Neutrino effects and non-linearities are included through fitting functions to N-body simul ations\, while for baryon feedback I employ the Baryon Correction Model\, whose parameters have well-established physical meaning. In the last part I also include the intrinsic alignment effect in weak lensing and show tha t not even this systematic will likely bias the measurement on neutrino ma ss.\n\nhttps://indico.ific.uv.es/event/3485/contributions/10271/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10271/ END:VEVENT BEGIN:VEVENT SUMMARY:Dynamical generation of fermion masses in a warped extra dimension DTSTART;VALUE=DATE-TIME:20181214T142000Z DTEND;VALUE=DATE-TIME:20181214T144000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10270@indico.ific.uv.es DESCRIPTION:Speakers: Javier Castellano (JGU Mainz)\nWe explore the possib ility of dynamically generating bulk fermion masses with an odd bulk scala r in warped extra dimensions. The odd bulk scalar acquires vacuum expectat ion value (VEV) along the extra-dimension and its Yukawa interactions with bulk fermions generate their bulk masses. The zero-mode localization of f ermions along the warped extra dimension naturally explain the observed fl avor structure and 4D fermion mass hierarchy of the SM fermions. We study the phenomenological implications of first KK mode of the scalar field and its interaction with SM Higgs\, which is localized at the IR brane.\n\nht tps://indico.ific.uv.es/event/3485/contributions/10270/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10270/ END:VEVENT BEGIN:VEVENT SUMMARY:Are the neutrinos driving the SM to the Swampland? DTSTART;VALUE=DATE-TIME:20181214T140000Z DTEND;VALUE=DATE-TIME:20181214T142000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10269@indico.ific.uv.es DESCRIPTION:Speakers: Víctor Martín Lozano (Bonn University -- BCTP )\n It is known that not every effective field theory could be embedded in qua ntum gravity\, but only those which are consistent with the QG conjectures . Does these constraints have an impact in low energy physics? Recently\, Ooguri and Vafa argued using a strong approach of the Weak Gravity Conject ure that non-supersymmetric stable AdS vacua are incompatible with quantum gravity. It is also known that compactifying the Standard Model to 3 or 2 dimensions can give rise to AdS vacua. Using the fact that those vacua mu st be absent\, several constraints are set on the SM and BSM particles\, o btaining a lower bound on the cosmological constant in terms of the masses of the neutrinos. Moving forward one can translate those into an upper bo und for the EW scale around the TeV range.\n\nhttps://indico.ific.uv.es/ev ent/3485/contributions/10269/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10269/ END:VEVENT BEGIN:VEVENT SUMMARY:A general framework for modeling the small scale power in non-stan dard cosmologies DTSTART;VALUE=DATE-TIME:20181213T161000Z DTEND;VALUE=DATE-TIME:20181213T163000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10268@indico.ific.uv.es DESCRIPTION:Speakers: Riccardo Murgia (SISSA\, Trieste)\nStructure formati on at small cosmological scales provides an important frontier for Dark Ma tter (DM) research. Scenarios with small DM particle masses\, large moment a or hidden interactions tend to suppress the gravitational clustering at small scales\, inducing a cut-off in the matter power spectrum P(k) on suc h small scales. So far\, many non-cold DM (nCDM) candidates have been prop osed in order to give a better description of the structure formation and distribution at small scales\, with respect to the standard cold DM (CDM) model. The details of the small-scale power suppression\, usually describe d by the so-called transfer function T^2(k)=P_nCDM(k)/P_CDM(k)\, depend on the DM particle nature\, allowing for a direct link between DM models and astrophysical observations. However\, most of the constraints currently a vailable refer to a very specific shape of transfer function T(k)\, corres ponding to thermal warm DM\, i.e. candidates with a Fermi-Dirac momentum d istribution. Nonetheless\, most of the viable dark matter candidates are n ot characterised by a thermal momentum distribution. In this talk\, I will present a general analytical fitting formula for the transfer function T( k)\, which is able to reproduce a large variety of shapes in the suppressi on of the power spectrum. I will show that it covers the parameter space o f the most popular nCDM scenarios\, such as sterile neutrinos\, mixed (col d + warm) models\, ultralight scalar DM and other models suggested by effe ctive field theory of structure formation. Finally\, I will discuss the fi rst astrophysical constraints on its free parameters\, obtained through a comprehensive analysis of the Lyman-alpha forest data and easily translata ble to bounds on the fundamental nCDM properties.\n\nhttps://indico.ific.u v.es/event/3485/contributions/10268/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10268/ END:VEVENT BEGIN:VEVENT SUMMARY:The Cold Dark Matter axion and Axion Stars DTSTART;VALUE=DATE-TIME:20181213T155000Z DTEND;VALUE=DATE-TIME:20181213T161000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10266@indico.ific.uv.es DESCRIPTION:Speakers: Luca Visinelli (Uppsala University)\nhttps://indico. ific.uv.es/event/3485/contributions/10266/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10266/ END:VEVENT BEGIN:VEVENT SUMMARY:Cuckoo's Eggs in Neutron Stars: Can LIGO Hear Chirps from the Dark Sector? DTSTART;VALUE=DATE-TIME:20181213T153000Z DTEND;VALUE=DATE-TIME:20181213T155000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10265@indico.ific.uv.es DESCRIPTION:Speakers: Ranjan Laha (Johannes Gutenberg University Mainz)\nW e explore in detail the possibility that gravitational wave signals from b inary inspirals are affected by a new force that couples only to dark matt er particles. We discuss the impact of both the new force acting between t he binary partners as well as radiation of the force carrier. We identify numerous constraints on any such scenario\, ultimately concluding that obs ervable effects on the dynamics of binary inspirals due to such a force ar e not possible if the dark matter is accrued during ordinary stellar evolu tion. Constraints arise from the requirement that the astronomical body be able to collect and bind at small enough radius an adequate number of dar k matter particles\, from the requirement that the particles thus collecte d remain bound to neutron stars in the presence of another neutron star\, and from the requirement that the theory allows old neutron stars to exist and retain their charge. Thus\, we show that any deviation from the predi ctions of general relativity observed in binary inspirals must be due eith er to the material properties of the inspiraling objects themselves\, such as a tidal deformability\, to a true fifth force coupled to baryons\, or to a non-standard production mechanism for the dark matter cores of neutro n stars. Viable scenarios of the latter type include production of dark ma tter in exotic neutron decays\, or the formation of compact dark matter ob jects in the early Universe that later seed star formation or are captured by stars.\n\nhttps://indico.ific.uv.es/event/3485/contributions/10265/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10265/ END:VEVENT BEGIN:VEVENT SUMMARY:Constraining invisible neutrino decay with atmospheric neutrinos DTSTART;VALUE=DATE-TIME:20181213T144000Z DTEND;VALUE=DATE-TIME:20181213T150000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10264@indico.ific.uv.es DESCRIPTION:Speakers: Tarak Thakore (IFIC)\nhttps://indico.ific.uv.es/even t/3485/contributions/10264/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10264/ END:VEVENT BEGIN:VEVENT SUMMARY:New physics in coherent neutrino scattering DTSTART;VALUE=DATE-TIME:20181213T140000Z DTEND;VALUE=DATE-TIME:20181213T142000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10263@indico.ific.uv.es DESCRIPTION:Speakers: Xunjie Xu (Max-Planck-Institut für Kernphysik)\nIn this talk\, I am going to review the recent progress of coherent neutrino- nucleus scattering experiments and summarize the constraints on various BS M physics\, including NSI\, SPVAT interactions\, sterile neutrinos\, light mediators\, neutrino magnetic moments\, dark matter\, etc.\n\nhttps://ind ico.ific.uv.es/event/3485/contributions/10263/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10263/ END:VEVENT BEGIN:VEVENT SUMMARY:How to weaken the cosmological neutrino mass bound DTSTART;VALUE=DATE-TIME:20181212T163000Z DTEND;VALUE=DATE-TIME:20181212T165000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10261@indico.ific.uv.es DESCRIPTION:Speakers: Isabel Oldengott (University of Valencia)\nhttps://i ndico.ific.uv.es/event/3485/contributions/10261/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10261/ END:VEVENT BEGIN:VEVENT SUMMARY:Flavour symmetry as the origin of the axion DTSTART;VALUE=DATE-TIME:20181212T161000Z DTEND;VALUE=DATE-TIME:20181212T163000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10260@indico.ific.uv.es DESCRIPTION:Speakers: Fredrik Björkeroth (INFN Frascati)\nMotivated by re cent interest in the connection between axions and flavour\, we investigat e a generic\, generation-dependent U(1) quark flavour symmetry\, with emph asis on achieving maximal reduction in the number of free Yukawa parameter s. We find that there are only two inequivalent Yukawa textures\, each one giving rise to six physically distinct models. The U(1) symmetries that g enerate these textures all have a QCD anomaly\, and hence are PQ symmetrie s. The resultant axion has flavour-violating couplings to quarks\, and in some cases the coupling to nucleons can be suppressed\, rendering the axio n nucleophobic.\n\nhttps://indico.ific.uv.es/event/3485/contributions/1026 0/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10260/ END:VEVENT BEGIN:VEVENT SUMMARY:Majoron Dark Matter and Constraints on the Majoron-Neutrino Coupli ng DTSTART;VALUE=DATE-TIME:20181212T153000Z DTEND;VALUE=DATE-TIME:20181212T155000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10259@indico.ific.uv.es DESCRIPTION:Speakers: Tim Brune (TU Dortmund)\nWe revisit a singlet Majoro n model in which neutrino masses arise from the spontaneous violation of l epton number. If the Majoron obtains a mass of order MeV\, it can play the role of dark matter. We discuss constraints on the couplings of the massi ve Majoron to neutrinos from supernova data and from neutrinoless double b eta decay with Majoron emission. The combination of both constraints exclu des a large range of Majoron-Neutrino couplings in the mass range of inter erest for Majoron dark matter.\n\nhttps://indico.ific.uv.es/event/3485/con tributions/10259/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10259/ END:VEVENT BEGIN:VEVENT SUMMARY:Neutrino Phenomenology from A5 x CP DTSTART;VALUE=DATE-TIME:20181212T144000Z DTEND;VALUE=DATE-TIME:20181212T150000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10258@indico.ific.uv.es DESCRIPTION:Speakers: María Luisa López Ibáñez (Universidad de Valenci a)\nWe analyse the phenomenological implication for lepton masses and mixi ng implied by the breaking of the discrete symmetries A5 x CP into the sub groups Z2 x CP in the neutrino sector and Z5 in the charged lepton sector with and without supersymmetry.\n\nhttps://indico.ific.uv.es/event/3485/co ntributions/10258/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10258/ END:VEVENT BEGIN:VEVENT SUMMARY:Master Majorana neutrino mass parametrization DTSTART;VALUE=DATE-TIME:20181212T142000Z DTEND;VALUE=DATE-TIME:20181212T144000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10256@indico.ific.uv.es DESCRIPTION:Speakers: Isabel Cordero Carrión (University of Valencia)\nAf ter discussing the general form of a Majorana neutrino mass matrix we will introduce a master parametrization for the Yukawa matrices in agreement w ith neutrino oscillation data. This parametrization extends previous resul ts in the literature and can be used for any model that induces Majorana n eutrino masses with the seesaw mechanism. The application of the master pa rametrization will be illustrated with several examples.\n\nhttps://indico .ific.uv.es/event/3485/contributions/10256/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10256/ END:VEVENT BEGIN:VEVENT SUMMARY:Non-renormalizable interactions of the Standard Model fields DTSTART;VALUE=DATE-TIME:20181212T140000Z DTEND;VALUE=DATE-TIME:20181212T142000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10255@indico.ific.uv.es DESCRIPTION:Speakers: Renato Fonseca (IFIC - Valencia)\nThe Standard Model fields can interact through non-renormalizable operators\, the simplest o f which is the one mentioned by Weinberg\, with dimension 5. The list of a ll such operators up to dimension 6 is known and\, since the last few year s\, so is the number of all effective interactions up to dimension 15. How ever\, counting operators and listing them explicitly are different things . In this presentation I will talk about the challenges associated to writ ing down the Standard Model non-renormalizable interactions beyond dimensi on 6.\n\nhttps://indico.ific.uv.es/event/3485/contributions/10255/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10255/ END:VEVENT BEGIN:VEVENT SUMMARY:Dark Matter - when 3-body final states dominate 2-body DTSTART;VALUE=DATE-TIME:20181212T110000Z DTEND;VALUE=DATE-TIME:20181212T113000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10254@indico.ific.uv.es DESCRIPTION:Speakers: Thomas Weiler (Vanderbilt University)\nAn overview o f Dark Mattter suppressions and enhancements will be presented.\n\nhttps:/ /indico.ific.uv.es/event/3485/contributions/10254/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10254/ END:VEVENT BEGIN:VEVENT SUMMARY:Exploring dark matter\, neutrino mass and R_K* anomalies in L_\\mu - L_\\tau model DTSTART;VALUE=DATE-TIME:20181212T103000Z DTEND;VALUE=DATE-TIME:20181212T110000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10253@indico.ific.uv.es DESCRIPTION:Speakers: Rukmani Mohanta (University of Hyderabad)\nWe invest igate Majorana dark matter in a new variant of $U(1)_{L_\\mu-L_\\tau}$ gau ge extension of Standard Model\, where the scalar sector is enriched with an inert doublet and a $(\\bar{3}\,1\,1/3)$ scalar leptoquark. We compute the WIMP-nucleon cross section in leptoquark portal and the relic density mediated by inert doublet components\, leptoquark and the new $Z^\\prime$ boson. We constrain the parameter space consistent with PLANCK limit on re lic density\, PICO-60 and LUX bounds on spin-dependent direct detection cr oss section. Furthermore\, we constrain the new couplings from the present experimental data from flavour sector such as $Br (\\tau \\to \\mu \\nu_\ \tau \\bar \\nu_\\mu)$\, $B_s-\\bar{B_s}$ mixing etc\, which occur at one- loop level in the presence of $Z^\\prime$ and leptoquark. Using the allowe d parameter space\, we estimate the lepton non-universality parameters $R_ K^*$ and $R_\\phi$. We also briefly discuss about the neutrino mass genera tion at one-loop level.\n\nhttps://indico.ific.uv.es/event/3485/contributi ons/10253/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10253/ END:VEVENT BEGIN:VEVENT SUMMARY:Invisible axion DM and GUTs DTSTART;VALUE=DATE-TIME:20181212T100000Z DTEND;VALUE=DATE-TIME:20181212T103000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10252@indico.ific.uv.es DESCRIPTION:Speakers: Jihn E. Kim (Kyung Hee University)\nInspired from GU Ts and string compactification\, I will discuss the oscillating axion ener gy\, flavors with CKM matrix.\n\nhttps://indico.ific.uv.es/event/3485/cont ributions/10252/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10252/ END:VEVENT BEGIN:VEVENT SUMMARY:Constraints on neutrino physics from CMB observations DTSTART;VALUE=DATE-TIME:20181212T090000Z DTEND;VALUE=DATE-TIME:20181212T093000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10251@indico.ific.uv.es DESCRIPTION:Speakers: Massimiliano Lattanzi (Universita' di Ferrara)\nhttp s://indico.ific.uv.es/event/3485/contributions/10251/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10251/ END:VEVENT BEGIN:VEVENT SUMMARY:Nu physics in direct dark matter detection DTSTART;VALUE=DATE-TIME:20181212T083000Z DTEND;VALUE=DATE-TIME:20181212T090000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10250@indico.ific.uv.es DESCRIPTION:Speakers: David G. Cerdeño (IPPP\, Durham University)\nhttps: //indico.ific.uv.es/event/3485/contributions/10250/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10250/ END:VEVENT BEGIN:VEVENT SUMMARY:Dirac neutrinos and Dark Matter DTSTART;VALUE=DATE-TIME:20181212T080000Z DTEND;VALUE=DATE-TIME:20181212T083000Z DTSTAMP;VALUE=DATE-TIME:20260912T222212Z UID:indico-contribution-3485-10249@indico.ific.uv.es DESCRIPTION:Speakers: Ernest Ma (University of California\, Riverside)\nht tps://indico.ific.uv.es/event/3485/contributions/10249/ LOCATION: URL:https://indico.ific.uv.es/event/3485/contributions/10249/ END:VEVENT END:VCALENDAR