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The LOC14/05/2012 09:45
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Dr Martin Hirsch (IFIC/CSIC, Universidad Valencia)14/05/2012 10:00
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Pedro Machado (Universidade de São Paulo and CEA-Saclay)14/05/2012 10:40The lepton mixing angle theta 13, the only unknown angle in the standard three-flavor neutrino mixing scheme, is finally measured by recent reactor and accelerator experiments. We perform a combined analysis of the data coming from T2K, MINOS , Double Chooz, and Daya Bay, extracting a 6.2 sigma significance for nonzero theta 13. We also discuss near future expectations on the precision of the...Go to contribution page
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Dr Enrico Bertuzzo (IPHT-CEA Saclay)14/05/2012 11:30
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Dr Albert Villanova del Moral (LUPM Montpellier)14/05/2012 11:55
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Dr Akin Wingerter (LPSC)14/05/2012 12:20
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Dr Laurent Lellouch (CPT)14/05/2012 14:30
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Dr Nicolas Garron (university of Edinburgh)14/05/2012 15:10
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M. Antonin Portelli (Centre de Physique Théorique (CPT))14/05/2012 15:35
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Dr Gregory Vulvert (IFIC Valencia)14/05/2012 16:00Lattice QCD benefits nowadays from numerous progess thanks to algorithmic enhancements to push down the quark masses to reach the physical masses and to increase the lattice geometry to avoid finite volume effects. However using fermions which do not break the chiral symmetry both in valence and sea sector is still a challenge. An alternative is to consider mixed action simulations, where one...Go to contribution page
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Dirk Zerwas (LAL Orsay)14/05/2012 16:50
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Dr Abdelhak Djouadi (LPT Orsay)14/05/2012 17:30
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M. Guillaume Drieu La Rochelle (LAPTH)14/05/2012 17:55The BMSSM (Beyond the MSSM) framework is an effective theory approach that encapsulates a variety of extensions beyond the MSSM with which it shares the same field content. The lightest Higgs mass can be much heavier than in the MSSM without creating a tension with naturalness or requiring superheavy stops. The phenomenology of the Higgs sector is at the same time much richer. I discuss here...Go to contribution page
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Dr Malcolm Fairbairn (King's College London)15/05/2012 09:30I will (extremely) briefly review the evidence for dark matter and then the ongoing efforts to detect it using indirect and direct detection. I will talk about recent developments in indirect detection including a couple of potential signals from Fermi and some recent pessimistic predictions from N-body simulations. I will then review the ongoing search for dark matter via direct detection. ...Go to contribution page
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M. Quentin Le Boulc'h (LPSC)15/05/2012 10:10The relic density of Dark Matter in the Universe imposes today one of the most stringent constraints on new physics models such as the Minimal Supersymmetric Standard Model (MSSM). The most recent analysis of the WMAP collaboration has already reached an accuracy of 3%, and the upcoming results obtained with the Planck satellite will be even more precise. It is therefore mandatory for the...Go to contribution page
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Béranger DUMONT (LPSC Grenoble)15/05/2012 10:35
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M. Jonathan Da Silva (Laboratoire d'Annecy-Le-Vieux de Physique Théorique)15/05/2012 11:30In this talk I will present a study on the NUHM2 supersymmetric model where both the cosmic inflation and the observed dark matter abundance can be explained, with a Higgs boson mass in the range favoured by the latest LHC data. The two inflaton candidates LLe and udd are embedded within the MSSM therefore their decay naturally excites all the relevant degrees of freedom which thermalizes the...Go to contribution page
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Dr philippe brax (IPHT Saclay)15/05/2012 11:55I will describe how neutrinos could go faster than the speed of light in a dense environment if gravity were modified by a scalar field. I will show that the speed difference would almost always be unobservable for natural values of the couplings of scalars to matter.Go to contribution page
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Cedric Weiland (LPT Orsay)15/05/2012 12:20The inverse seesaw is a very appealing mechanism to generate neutrino masses since it provides natural neutrino Yukawa couplings ($Y_\nu \sim O(1)$) and a seesaw scale close to the electroweak one, thus within LHC reach. In a previous work (arXiv:1111.5836) where we embedded the inverse seesaw in a supersymmetric extension of the Standard Model (MSSM), we have highlighted that the...Go to contribution page
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Dr Francois Gelis (IPhT)15/05/2012 14:30
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Dr Yacine Mehtar-Tani (IPhT)15/05/2012 15:10We study the perturbative evolution of a jet via multiple gluon emissions induced by the interactions between the jet constituents and a dense QCD medium like a quark-gluon plasma. We focus on the typical medium-induced gluon emissions, for which the gluon formation time is much smaller than the overall size of the medium. We show that the typical time between two subsequent emissions is...Go to contribution page
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M. Thomas Epelbaum (IPhT)15/05/2012 15:35The quark gluon plasma thermalization in heavy ion collisions is an open problem that gave rise to many works in recent years. One of the approaches developped to study this QCD non pertubative problem is a resummation scheme that amounts to averaging over classical fields with random initial conditions. Its numerical implementation is presented here in the case of a scalar field theory with a...Go to contribution page
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elisa meunier (LMPT)15/05/2012 16:00The maximal algebra of symmetries of the free Schrodinger equation is determined. This algebra is an infinite dimensional extension of the Schrodinger algebra (by higher symmetries which are not kinematical transformations), it is isomorphic to the Weyl algebra of quantum observables, and it may be interpreted as a non-relativistic higher-spin algebra. The associated infinite collection of...Go to contribution page
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Dr Emilian Dudas (Ecole Polytechnique)16/05/2012 09:30
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M. Tomas Jezo (LPSC)16/05/2012 10:10General SU(2)xSU(2)xU(1) models represent a well-motivated intermediate step towards the unification of the Standard Model gauge groups. Based on a recent global analysis of low-energy and LEP constraints of these models, we perform numerical scans of their various signals at the LHC. We show that total cross sections for lepton and third-generation quark pairs, while experimentally easily...Go to contribution page
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M. Alfredo Urbano (Department of Physics and INFN, University of Salento)16/05/2012 10:35
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Dr Christopher Smith (IPN Lyon)16/05/2012 11:30Baryon (B) and lepton (L) numbers are conserved in the standard model lagrangian, but generally not in new physics models. In this talk, we adopt an effective approach to analyze, in a model-independent way, the possible signatures of B and L violating interactions at the LHC. Then, we particularize the discussion to the minimal supersymmetric standard model, where such interactions may now be...Go to contribution page
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Dr Bruno Machet (CNRS)16/05/2012 11:55I show that the Standard Model of weak interactions cannot have less than two Higgs doublets as soon as they are considered (to transform) as $\bar q_i q_j$ and $\bar q_i \gamma_5 q_j$ bilinears. There are exactly two for one generation of quarks, which is the simple case under scrutiny here. All basic physical properties, not only of massive gauge bosons, but also of fermions and J=0 mesons...Go to contribution page
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Dr Emmanuel NEZRI (LAM CNRS)16/05/2012 12:20
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Dr Gavin Salam (LPTHE Jussieu)16/05/2012 14:30
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Dr Nejc Kosnik (Laboratoire de l'accelerateur lineaire)16/05/2012 15:10We discuss the advantages of combining the experimental bound on B(Bs->mu+ mu-) and the measured B(B->Kl+l-) to get the model independent constraints on physics beyond the Standard Model. Since the two decays give complementary information, one can study not only the absolute values of the Wilson coefficients that are zero in the Standard Model, but also their phases. We also emphasize the...Go to contribution page
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Dr David GREYNAT (Fisica Teorica - Uni. de Zaragoza)16/05/2012 15:35With the help of the Mellin-Barnes transform, we show how to simultaneously resum the expansion of any kind of non-analytic functions around 0, 1 and $ infinity$ in a systematic way. We exemplify the method for the perturbative vector, axial scalar and pseudo-scalar correlator at $\mathcal{O}(\alpha_s^{3})$. We show that the coefficients, $\Omega(n)$, of the Taylor expansion of the vacuum...Go to contribution page
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Konstantin Petrov (LAL)16/05/2012 16:00
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