Simona Murgia
(University of California at Irvine)
6/27/16, 3:15 PM
Nestor Mirabal
(NASA/Goddard Space Flight Center)
6/27/16, 4:05 PM
Indirect searches
Monica Vazquez Acosta
(Instituto de Astrofísica de Canarias)
6/27/16, 4:30 PM
Indirect searches
Alejandro Ibarra
(Technische Universität München)
6/27/16, 5:35 PM
Simon Kast
(Karlsruhe Institut of Technology)
6/27/16, 6:25 PM
Indirect searches
James Taylor
(University of Waterloo)
6/27/16, 6:50 PM
Indirect searches
Kristian Hahn
(Northwestern University)
6/28/16, 8:50 AM
Christophe Clement
(Stockholm)
6/28/16, 9:40 AM
Collider Searches
Nadir Daci
(Vrije Universiteit Brussel)
6/28/16, 10:05 AM
Collider Searches
Pablo Martinez de Arbol
(ETH Zurich)
6/28/16, 10:30 AM
Collider Searches
Martino Borsato
(Universidad de Santiago de Compostela)
6/28/16, 12:10 PM
Collider Searches
Arturo Sanchez Pineda
(Universita' di Napoli)
6/28/16, 12:35 PM
Collider Searches
Daniele Trocino
(Northeastern Univ.)
6/28/16, 1:00 PM
Collider Searches
Ning Zhou
(Tsinghua University, Beijing, China.)
6/28/16, 3:00 PM
Gennaro Corcella
(INFN-LNF)
6/28/16, 3:50 PM
Indirect searches
Sven Heinemeyer
(IFCA/IFT (CSIC))
6/28/16, 4:15 PM
Collider Searches
David Cerdeño
(Institute for Particle Physics Phenomenology (Durham university))
6/28/16, 5:05 PM
Maria Bossa
(Gran Sasso Science Institute)
6/29/16, 9:40 AM
Direct Searches
Susana Cebrian
6/29/16, 10:05 AM
Direct Searches
Nahuel Ferreiro Iachellini
(Max Planck Institute for Physics)
6/29/16, 10:30 AM
Direct Searches
Laura Baudis
(university of zurich)
6/29/16, 11:20 AM
Lukas BŸtikofer
(University of Bern)
6/29/16, 12:10 PM
Direct Searches
Payam Pakarha
(ZUrich University)
6/29/16, 12:35 PM
Direct Searches
Scotto Lavina Luca
(Subatech, CNRS/IN2P3)
6/29/16, 1:00 PM
Direct Searches
Javier Tiffenberg
(Fermilab)
6/29/16, 3:00 PM
Direct Searches
Theopisti Dafni
(Universidad de Zaragoza)
6/29/16, 3:50 PM
Direct Searches
Matteo Cadeddu
(Cagliari University and INFN)
6/29/16, 4:15 PM
Direct Searches
Juan Jose Hernandez-Rey
(Instituto de Física Corpuscular (IFIC))
6/29/16, 5:05 PM
Go Ogiya
(Max Planck Institute for Extraterrestrial Physics)
6/30/16, 9:40 AM
Astrophysics Evidence/Cosmology
Vladimir Avila
(Instituto de Astronom’a, UNAM)
6/30/16, 10:05 AM
Astrophysics Evidence/Cosmology
Jose Onorbe
(Max Planck Institute FŸr Astronomie)
6/30/16, 10:30 AM
Astrophysics Evidence/Cosmology
Celine Boehm
(Institute for Particle Physics Phenomenology-Durham University)
6/30/16, 11:20 AM
Jose Maria Diego
(IFCA)
6/30/16, 12:10 PM
Astrophysics Evidence/Cosmology
Tomoaki Ishiyama
(Chiba University)
6/30/16, 12:35 PM
Astrophysics Evidence/Cosmology
M Angeles Perez-Garcia
(University of Salamanca , Spain)
6/30/16, 1:00 PM
Astrophysics Evidence/Cosmology
Xavier Barcons
(Instituto de Fisica de Cantabria(IFCA))
6/30/16, 3:00 PM
Astrophysics Evidence/Cosmology
Richard Galvez
(Vanderbilt University)
6/30/16, 3:35 PM
Astrophysics Evidence/Cosmology
Francisco S.N. Lobo
(Institute of Astrophysics and Space Sciences, University of Lisbon)
6/30/16, 4:00 PM
Astrophysics Evidence/Cosmology
Sebastian Trujillo-Gomez
(University of Zurich)
6/30/16, 4:25 PM
Astrophysics Evidence/Cosmology
Thomas Hambye
(Université Libre de Bruxelles)
7/1/16, 8:50 AM
Matti Heikinheimo
(Helsinki Institute of Physics)
7/1/16, 9:40 AM
Indirect searches
Andrea Vittino
(TUM Munich)
7/1/16, 10:05 AM
Indirect searches
Maxim Laletin
(University of Liege)
7/1/16, 10:30 AM
Igor Irastorza
(Universidad de Zaragoza)
7/1/16, 11:20 AM
81.
SHIP Collaboration: a new Facility at CERN/SPS with dedicated detectors to probe the dark sector
Behzad Hossein
(infn Cagliari)
7/1/16, 12:10 PM
Indirect searches
Alberto Casas
(IFT (Instituto de Fisica))
7/1/16, 12:40 PM
Abir Sarkar
(Raman Research Institute)
Indirect searches
Neutrino 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...
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...
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...
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...
thomas hambye
(Université Libre de Bruxelles)
Indirect searches
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...
Indirect searches
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...
Keith Olive
(University of Minnesota)
Direct Searches
The 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...
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...
Collider Searches
