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Rector de la UC (Universidad de Cantabria)6/27/16, 3:00 PM
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Simona Murgia (University of California at Irvine)6/27/16, 3:15 PM
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Nestor Mirabal (NASA/Goddard Space Flight Center)6/27/16, 4:05 PMIndirect searches
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Monica Vazquez Acosta (Instituto de Astrofísica de Canarias)6/27/16, 4:30 PMIndirect searches
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Alejandro Ibarra (Technische Universität München)6/27/16, 5:35 PM
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Simon Kast (Karlsruhe Institut of Technology)6/27/16, 6:25 PMIndirect searches
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James Taylor (University of Waterloo)6/27/16, 6:50 PMIndirect searches
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Kristian Hahn (Northwestern University)6/28/16, 8:50 AM
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Christophe Clement (Stockholm)6/28/16, 9:40 AMCollider Searches
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Nadir Daci (Vrije Universiteit Brussel)6/28/16, 10:05 AMCollider Searches
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Pablo Martinez de Arbol (ETH Zurich)6/28/16, 10:30 AMCollider Searches
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Thomas Jacques (SISSA)6/28/16, 11:20 AM
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Martino Borsato (Universidad de Santiago de Compostela)6/28/16, 12:10 PMCollider Searches
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Arturo Sanchez Pineda (Universita' di Napoli)6/28/16, 12:35 PMCollider Searches
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Daniele Trocino (Northeastern Univ.)6/28/16, 1:00 PMCollider Searches
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Ning Zhou (Tsinghua University, Beijing, China.)6/28/16, 3:00 PM
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Gennaro Corcella (INFN-LNF)6/28/16, 3:50 PMIndirect searches
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Sven Heinemeyer (IFCA/IFT (CSIC))6/28/16, 4:15 PMCollider Searches
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David Cerdeño (Institute for Particle Physics Phenomenology (Durham university))6/28/16, 5:05 PM
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Keith Olive (University of Minnesota)6/28/16, 5:55 PM
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Aldo Ianni (Canfranc)6/29/16, 8:50 AM
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Maria Bossa (Gran Sasso Science Institute)6/29/16, 9:40 AMDirect Searches
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Susana Cebrian6/29/16, 10:05 AMDirect Searches
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Nahuel Ferreiro Iachellini (Max Planck Institute for Physics)6/29/16, 10:30 AMDirect Searches
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Laura Baudis (university of zurich)6/29/16, 11:20 AM
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Lukas BŸtikofer (University of Bern)6/29/16, 12:10 PMDirect Searches
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Payam Pakarha (ZUrich University)6/29/16, 12:35 PMDirect Searches
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Scotto Lavina Luca (Subatech, CNRS/IN2P3)6/29/16, 1:00 PMDirect Searches
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Javier Tiffenberg (Fermilab)6/29/16, 3:00 PMDirect Searches
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Theopisti Dafni (Universidad de Zaragoza)6/29/16, 3:50 PMDirect Searches
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Matteo Cadeddu (Cagliari University and INFN)6/29/16, 4:15 PMDirect Searches
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Juan Jose Hernandez-Rey (Instituto de Física Corpuscular (IFIC))6/29/16, 5:05 PM
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Benoit Farnaey6/30/16, 8:50 AM
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Go Ogiya (Max Planck Institute for Extraterrestrial Physics)6/30/16, 9:40 AMAstrophysics Evidence/Cosmology
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Vladimir Avila (Instituto de Astronom’a, UNAM)6/30/16, 10:05 AMAstrophysics Evidence/Cosmology
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Jose Onorbe (Max Planck Institute FŸr Astronomie)6/30/16, 10:30 AMAstrophysics Evidence/Cosmology
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Celine Boehm (Institute for Particle Physics Phenomenology-Durham University)6/30/16, 11:20 AM
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Jose Maria Diego (IFCA)6/30/16, 12:10 PMAstrophysics Evidence/Cosmology
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Tomoaki Ishiyama (Chiba University)6/30/16, 12:35 PMAstrophysics Evidence/Cosmology
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M Angeles Perez-Garcia (University of Salamanca , Spain)6/30/16, 1:00 PMAstrophysics Evidence/Cosmology
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Xavier Barcons (Instituto de Fisica de Cantabria(IFCA))6/30/16, 3:00 PMAstrophysics Evidence/Cosmology
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Richard Galvez (Vanderbilt University)6/30/16, 3:35 PMAstrophysics Evidence/Cosmology
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Francisco S.N. Lobo (Institute of Astrophysics and Space Sciences, University of Lisbon)6/30/16, 4:00 PMAstrophysics Evidence/Cosmology
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Sebastian Trujillo-Gomez (University of Zurich)6/30/16, 4:25 PMAstrophysics Evidence/Cosmology
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Thomas Hambye (Université Libre de Bruxelles)7/1/16, 8:50 AM
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Matti Heikinheimo (Helsinki Institute of Physics)7/1/16, 9:40 AMIndirect searches
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Andrea Vittino (TUM Munich)7/1/16, 10:05 AMIndirect searches
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Maxim Laletin (University of Liege)7/1/16, 10:30 AM
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Igor Irastorza (Universidad de Zaragoza)7/1/16, 11:20 AM
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81. SHIP Collaboration: a new Facility at CERN/SPS with dedicated detectors to probe the dark sectorBehzad Hossein (infn Cagliari)7/1/16, 12:10 PMIndirect searches
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Alberto Casas (IFT (Instituto de Fisica))7/1/16, 12:40 PM
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Abir Sarkar (Raman Research Institute)Indirect searchesNeutrino oscillation models predict extra mass eigenstates beyond 3 standard model neutrino mass eigenstates. Sterile neutrino models, based on short baseline experiments provide $\Delta m_{41}^2=1.75 \rm eV ^2$. But a few eV mass neutrino dark matter is ruled out by several cosmological datasets. In this work, we couple neutrino with a hidden sector whose temperature is different from the...Go to contribution page
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Pradyumn Kumar Sahoo (BITS-Pilani, Hyderabad Campus)An anisotropic Bianchi type-III universe is investigated in presence of perfect fluid within the framework of f(R; T) gravity where R is the Ricci scalar and T is the trace of the energy momentum tensor, for the choice of functional f(R; T) = R + 2f(T) and f(R; T) = f1(R) + f2(T). We have shown that the field equations are solvable for any arbitrary function of a scale factor. To get a...Go to contribution page
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Sebastian Wild (TU Munich)We examine the dark matter interpretation of the modulation signal reported by the DAMA experiment from the perspective of effective field theories displaying Galilean invariance. We consider the most general effective coupling leading to the elastic scattering of a dark matter particle with a nucleon, and by employing a novel statistical approach for comparing direct detection data in this...Go to contribution page
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Sebastian IngenhŸtt (Technische UniversitŠt MŸnchen)We consider scenarios where the dark matter becomes unstable due to a non-minimal coupling to gravity. We show that the dark matter can decay into Standard Model particles with a lifetime which is potentially accessible to gamma-ray or neutrino telescopes. We determine the decay branching fractions in some simple scenarios and we set limits on the size of the dark matter non-minimal coupling...Go to contribution page
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Eung Jin Chun (Korea Institute for Advanced Study)We update indirect constraints on Electro-Weak Dark Matter (EWDM) considering the Sommerfeld?Ramsauer?Townsend (SRT) effect for its annihilations into a pair of standard model gauge bosons assuming that EWDM accounts for the observed dark matter (DM) relic density for a given DM mass and mass gaps among the multiplet components. For the radiative or smaller mass splitting, the hypercharged...Go to contribution page
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thomas hambye (Université Libre de Bruxelles)Indirect searches
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Dmytro Iakubovskyi (Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine)A number of observational studies claim detection or non-detection of the extra line in X-ray spectra of various cosmic objects dominated by dark matter -- gravitationally interacting substance that constitutes the major fraction of non-relativistic matter in the Universe. In this talk I summarize the results of these studies and especially the status of the detection of new emission line at...Go to contribution page
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Direct Searches
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Indirect searches
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Ship collaboratio Ship Collaboration (CERN)SHIP is a new general purpose fixed target facility, whose Technical Proposal has been recently reviewed by the CERN SPS Committee, who recommended that the experiment proceeds further to a Comprehensive Design phase. In its initial phase, the 400GeV proton beam extracted from the SPS will be dumped on a heavy target with the aim of integrating $2\times 10^{20}$ pot in 5 years. A dedicated...Go to contribution page
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Keith Olive (University of Minnesota)Direct SearchesThe absence of low energy supersymmetry in run I data at the LHC has pushed the nominal scale for supersymmetry beyond a TeV. While this is consistent with the discovery of the Higgs boson at $\approx$ 125 GeV, simple models with scalar and gaugino mass universality are being pushed into corners of parameter space. Non-supersymmetric grand unified theories such as SO(10) may also provide a...Go to contribution page
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Aldo Ianni (Laboratorio Subterraneo de Canfranc)
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Anna Saburova (Sternberg Astronomical institute of Moscow State University)We examined the reliability of estimates of pseudoisothermal, Burkert and NFW dark halo parameters for best fit models. To do it we constructed the chi^2 maps for the grid of the dark halo parameters for a sample of 14 disc galaxies with high quality rotation curves from THINGS. We showed that in a half of considered galaxies the best fit mass-modelling results are questionable. The...Go to contribution page
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Collider Searches
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shahram khosravi (Texas A&M University)Spacetimematter is a five dimensional geometry where matter is baked into geometry as a new dimension. Every event point of spacetimematter follows the uncertainty principle, which limits the accuracy of the measurement of its space, time, and matter coordinates turning it into a Space-Time-Matter (STM) geometrical quantum with space, time, and matter edges. State functions of STMs curve...Go to contribution page
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