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SUMMARY:On the smallness of the cosmological constant in SUGRA models with
  Planck scale SUSY breaking and degenerate vacua
DTSTART;VALUE=DATE-TIME:20140705T093000Z
DTEND;VALUE=DATE-TIME:20140705T100000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1568@indico.ific.uv.es
DESCRIPTION:Speakers: Roman Nevzorov (University of Adelaide)\nIn $N=1$ su
 pergravity (SUGRA)  supersymmetric (SUSY) and non-supersymmetric Minkowski
  vacua originating in the hidden \nsector can be degenerate. This allows f
 or consistent \nimplementation of the multiple point principle (MPP) \nass
 umption. We present no--scale inspired SUGRA model \nwhere the MPP assumpt
 ion is realised at the tree--level \nwithout extra fine-tuning. In the sup
 ersymmetric phase \nin flat Minkowski space SUSY may be broken dynamically
  \ninducing tiny vacuum energy density which can be assigned\, \nby virtue
  of MPP\, to all other phases including the one \nin which we live. We arg
 ue that the measured value of the cosmological constant\, as well as the s
 mall values of \nquartic Higgs self--coupling and the corresponding beta \
 nfunction at the Planck scale\, which can be obtained by extrapolating the
  Standard Model (SM) couplings to high \nenergies\, can originate from sup
 ergravity (SUGRA) models \nwith degenerate vacua. This scenario is realise
 d if \nthere are at least three exactly degenerate vacua. In the \nfirst v
 acuum\, associated with the physical one\, local \nsupersymmetry (SUSY) is
  broken near the Planck scale \nwhile the breakdown of the $SU(2)_W\\times
  U(1)_Y$ symmetry \ntakes place at the electroweak (EW) scale. In the seco
 nd \nvacuum local SUSY breaking is induced by gaugino condensation \nat a 
 scale which is just slightly lower than $\\Lambda_{QCD}$ \nin the physical
  vacuum. Finally\, in the third vacuum local \nSUSY and EW symmetry are br
 oken near the Planck scale.\n\nhttps://indico.ific.uv.es/event/2025/contri
 butions/1568/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1568/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Calculating repetitively.III:
DTSTART;VALUE=DATE-TIME:20140705T100000Z
DTEND;VALUE=DATE-TIME:20140705T103000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1437@indico.ific.uv.es
DESCRIPTION:Speakers: Gopinath Kamath (Indian Institute of Technology Madr
 as)\nThis talk has two highlights: a. The utility of the Dirac δ – func
 tion as an aid to repetitive integration in multiple integrals\, and b. An
  extension to 3 + 1 dimensional stationary curved space of a recent effort
  by the author in 2 + 1 dimensional stationary curved space to determine t
 he zeta function for the Lagrangian density for a real massive scalar fiel
 d using the Schwinger operator expansion\; this is a reworking to advantag
 e by the author of the Antonsen – Bormann idea that was originally propo
 sed by these latter authors for the computation of the heat kernel in curv
 ed space. The repetitive nature of the calculation in 2 + 1 dimensional cu
 rved space at all higher orders(≥3) in the gravitational constant G sugg
 ested the use of the Dirac delta-function and one of its integral represen
 tations – in that it is convenient to obtain answers\, so its utility is
  also checked in the 3 + 1 dimensional case.\n\nhttps://indico.ific.uv.es/
 event/2025/contributions/1437/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1437/
END:VEVENT
BEGIN:VEVENT
SUMMARY:A unified approach to nuclei: The BPS Skyrme Model
DTSTART;VALUE=DATE-TIME:20140705T130000Z
DTEND;VALUE=DATE-TIME:20140705T133000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1418@indico.ific.uv.es
DESCRIPTION:Speakers: Carlos Naya (Universidade de Santiago de Compostela 
 and Instituto Galego de Física de Altas Enerxías (IGFAE))\nIn this talk\
 , we will present a concrete model of a low energy effective field theory 
 of QCD\, the well-known Skyrme Model. Specifically\, we will work with the
  BPS submodel [1] in order to describe the binding energies of nuclei. Thi
 s BPS Skyrme model is charaterized by having a saturated bound for the ene
 rgy proportional to the baryon number of the nuclei. After presenting this
  classical result\, we will proceed with a semi-classical quantization of 
 the coordinates of spin and isospin. Then\, with the further inclusion of 
 the Coulomb interaction as well as a small explicit breaking of the isospi
 n symmetry\, we finally calculate the binding energies of nuclei\, where a
 n excellent agreement has been found for the nuclei with high baryon numbe
 r [2]\, [3].\n\n\nReferences\n\n[1] C. Adam\, J. Sanchez-Guillen\, A. Were
 szczynski\, Acta Phys. Pol. B 41\, (2010) 2717 .\n[2] C. Adam\, C. Naya\, 
 J. Sanchez-Guillen\, A. Wereszczynski\, Phys. Rev. Lett. 111 (2013) 232501
 .\n[3] C. Adam\, C. Naya\, J. Sanchez-Guillen\, A. Wereszczynski\, Phys. R
 ev. C 88 (2013) 054313.\n\nhttps://indico.ific.uv.es/event/2025/contributi
 ons/1418/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1418/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Lifshitz hyperscaling violating holography
DTSTART;VALUE=DATE-TIME:20140705T133000Z
DTEND;VALUE=DATE-TIME:20140705T140000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1371@indico.ific.uv.es
DESCRIPTION:Speakers: Ioannis Papadimitriou (Instituto de Fisica Teorica U
 AM/CSIC)\nHolographic techniques have been instrumental in understanding c
 ertain aspects of strongly correlated systems\, both in high energy and co
 ndensed matter physics. One of the most interesting applications of hologr
 aphy in the condensed matter setting is the study of quantum critical poin
 ts exhibiting Lifshitz or hyperscaling violating Lifshitz symmetry. Althou
 gh various aspects of the holographic dictionary for Lifshitz quantum crit
 ical points have been studied in special cases\, the general structure for
  arbitrary critical exponent z has not been fully understood\, while very 
 little is known for the hyperscaling violating case. \n\nWe develop a gene
 ral method for systematically constructing the holographic dictionary for 
 both Lifshitz and hyperscaling violating Lifshitz critical points with arb
 itrary Lorentz violating and hyperscaling violating parameters\, for a lar
 ge class of bulk actions admitting such backgrounds. This allows us to det
 ermine quite generically various physical properties of the dual quantum c
 ritical points\, such as the spectrum of operators\, the Ward identities\,
  and the Lifshitz confromal anomaly.\n\nhttps://indico.ific.uv.es/event/20
 25/contributions/1371/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1371/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Vacuum instability in holography
DTSTART;VALUE=DATE-TIME:20140705T103000Z
DTEND;VALUE=DATE-TIME:20140705T110000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1358@indico.ific.uv.es
DESCRIPTION:Speakers: Koji Hashimoto (Osaka university / RIKEN)\nWe analyz
 e vacuum instability of strongly coupled gauge theories in a constant\nele
 ctric ﬁeld using AdS/CFT correspondence. The model is the N = 2 1-ﬂavo
 r\nsupersymmetric large Nc QCD in the strong ’t Hooft coupling limit. We
  calculate the\nEuler-Heisenberg eﬀective Lagrangian L(E)\, which encode
 s the nonlinear response\nand the quantum decay rate of the vacuum in a ba
 ckground electric ﬁeld E\, from\nthe complex D-brane action in AdS/CFT. 
 We ﬁnd that the decay rate given by\nImL(E) becomes nonzero above a crit
 ical electric ﬁeld set by the conﬁning force\nbetween quarks. A large 
 E expansion of Im L(E) is found to coincide with that\nof the Schwinger e
 ﬀects in QED\, replacing its electron mass by the conﬁning force.\n\nh
 ttps://indico.ific.uv.es/event/2025/contributions/1358/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1358/
END:VEVENT
BEGIN:VEVENT
SUMMARY:N=2 SUGRA BPS Multi-center solutions\, quadratic prepotentials and
  Freudenthal transformations
DTSTART;VALUE=DATE-TIME:20140705T110000Z
DTEND;VALUE=DATE-TIME:20140705T113000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1253@indico.ific.uv.es
DESCRIPTION:Speakers: torrente-lujan emilio (universidad de murcia)\nWe pr
 esent a detailed  description of $N=2$ stationary \nBPS multicenter black 
 hole solutions for quadratic prepotentials\nwith an arbitrary number of ce
 nters and scalar fields\nmaking a systematic  use of the algebraic propert
 ies of the matrix of second derivatives of the prepotential\,  $\\mathcal{
 S}$\, which in this case is a scalar-independent matrix. In particular we 
 obtain bounds on the physical parameters of the multicenter solution such 
 as horizon areas and ADM mass. We discuss the possibility and convenience 
 of setting up a basis of the symplectic vector space built from charge \ne
 igenvectors of the $\\ssigma$\, the set of vectors \n$(\\Ppm q_a)$ with $\
 \Ppm$ $\\ssigma$-eigenspace projectors.\n\nThe anti-involution matrix $\\m
 athcal{S}$ can be understood \nas a  Freudenthal duality $\\tilde{x}=\\ssi
 gma x$.\nWe show that this duality can be generalized to\n``Freudenthal tr
 ansformations'' \n$$x\\to \\lambda\\exp(\\theta \\ssigma) x= a x+b\\tilde{
 x}$$\nunder which the horizon area\, ADM mass and intercenter \ndistances 
 scale up leaving constant the scalars at the fixed points.\nIn the special
  case $\\lambda=1$\, ``$\\ssigma$-rotations''\, \nthe transformations leav
 e invariant the solution.\nThe standard Freudenthal duality can be written
  as\n $\\tilde x= \\exp\\left(\\frac{\\pi}{2} \\ssigma\\right) x .$\nWe ar
 gue that these generalized transformations  leave\ninvariant not only the 
 quadratic prepotential theories\n but also the general stringy extremal qu
 artic form $\\Delta_4$\,\n$\\Delta_4(x)= \\Delta_4(\\cos\\theta x+\\sin\\t
 heta\\tilde{x})$\nand therefore its entropy at lowest order.\n\nhttps://in
 dico.ific.uv.es/event/2025/contributions/1253/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1253/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Spontaneous Breaking of Scale Invariance in U(N) Chern-Simons Gaug
 e Theories in Three  Dimensions
DTSTART;VALUE=DATE-TIME:20140705T140000Z
DTEND;VALUE=DATE-TIME:20140705T143000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1108@indico.ific.uv.es
DESCRIPTION:Speakers: William Bardeen (Fermilab)\nI demonstrate the existe
 nce of a massive phase in a conformally invariant U(N) \nChern-Simons gaug
 e theory in D=3 with matter fields in the fundamental representation.  The
 se \nmodels have attracted recent attention as being dual\, in the conform
 al phase\, to theories of \nhigher spin gravity on AdS_4.  Using the ‘t 
 Hooft large N expansion\, exact solutions are \nobtained for scalar curren
 t correlators in the massive phase where the conformal symmetry \nis spont
 aneously broken.  A massless dilaton appears as a composite state\, and it
 s \nproperties are discussed.  Solutions exist for matter fields that are 
 either bosons or fermions.\n\nhttps://indico.ific.uv.es/event/2025/contrib
 utions/1108/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1108/
END:VEVENT
BEGIN:VEVENT
SUMMARY:A scenario for critical scalar field collapse in AdS_3
DTSTART;VALUE=DATE-TIME:20140705T143000Z
DTEND;VALUE=DATE-TIME:20140705T150000Z
DTSTAMP;VALUE=DATE-TIME:20260419T050833Z
UID:indico-contribution-122-1071@indico.ific.uv.es
DESCRIPTION:Speakers: Alessandro Fabbri (Centro Fermi / Univ. Bologna / IF
 IC (CSIC))\nWe present a family of exact solutions\, depending on two para
 meters\nalpha and b (related to the scalar field strength)\, to the three-
 dimensional Einstein-scalar field equations with negative cosmological con
 stant.\nFor b = 0 these solutions reduce to the static BTZ family of vacuu
 m\nsolutions\, with mass M =-alpha. For nonvanishing b\, the solutions bec
 ome\ndynamical and develop a strong spacelike central singularity. \nThe a
 lpha  0 agrees qualitatively with that observed in numerical simulations o
 f subcritical collapse. \nWe analyze the linear perturbations of the thres
 hold solution\,\nalpha = 0\, in the Lambda = 0 approximation\, and find th
 at it has only one unstable growing mode\, which qualifies it as a candida
 te critical solution for scalar field collapse.\n\nhttps://indico.ific.uv.
 es/event/2025/contributions/1071/
LOCATION: Sala 8+9
URL:https://indico.ific.uv.es/event/2025/contributions/1071/
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