Prof.
Leszek Roszkowski
(University of Sheffield and NCBJ)
03/04/2017, 10:00
Mr
Thomas Hambye
(Univ. of Brussels (ULB))
03/04/2017, 10:45
Prof.
Viatcheslav Mukhanov
(LMU - Munich)
03/04/2017, 12:00
Dr
Geraldine Servant
(CERN)
03/04/2017, 14:30
Mr
Simone Dresti
(Georg-August University Göttingen)
03/04/2017, 17:00
Mr
Ernany Rossi Schmitz
(University of Bonn)
03/04/2017, 17:30
Jeremy Bernon
(LPSC)
04/04/2017, 09:45
Prof.
Francesco Sannino
(CP3-Origins, SDU)
04/04/2017, 11:00
Wilfried Buchmuller
(DESY)
04/04/2017, 11:45
Dr
Pedro Schwaller
(CERN)
04/04/2017, 14:30
Prof.
Daniel Litim
(University of Sussex)
04/04/2017, 15:15
Mr
Jason Veatch
(Göttingen University)
04/04/2017, 16:30
Ursula Laa
(LPSC Grenoble)
04/04/2017, 17:00
Dr
Diogo Buarque Franzosi
(II Physics Institute, Goettingen U.)
04/04/2017, 17:30
Torsten Bringmann
(Hamburg University)
05/04/2017, 09:00
Dr
Felix Kahlhoefer
(DESY)
05/04/2017, 09:45
Dr
Riccardo Catena
(Institut fuer Theoretische Physik Goettingen)
05/04/2017, 11:45
Jakob Schwichtenberg
(Institute for Theoretical Particle Physics (TTP) at the Karlsruhe Institute of Technology (KIT))
05/04/2017, 14:00
Raghuveer Garani
(Physikalisches Institut, University Bonn)
05/04/2017, 14:30
Dr
Takashi Toma
(Technische Universität München)
05/04/2017, 15:00
Tobias Binder
(ITP, Goettingen University)
05/04/2017, 15:30
Dr
Takashi Toma
(Technische Universität München)
Many models of Higgs portal dark matter find themselves under pressure from increasingly tight direct detection constraints. In the framework of gauge field dark matter, we study how such bounds can be relaxed while retaining the thermal WIMP paradigm. When the hidden sector gauge symmetry is broken via the Higgs mechanism, the hidden sector generally contains unstable states which are lighter...
Mr
Jakob Schwichtenberg
(Institute for Theoretical Particle Physics (TTP) at the Karlsruhe Institute of Technology (KIT))
We discuss fermionic dark matter in non-supersymmetric $E_6$ Grand Unification. The fundamental representation of $E_6$ contains, in addition to the standard model fermions, exotic fermions and we argue that one of them is a viable, interesting dark matter candidate. Its stability is guaranteed by a remnant discrete symmetry that originates when the $E_6$ gauge symmetry is broken...
Raghuveer Garani
(Physikalisches Institut, University Bonn)
The annihilation of dark matter (DM) particles accumulated in the Sun could produce a flux of neutrinos, which is potentially detectable with neutrino detectors/telescopes and the DM elastic scattering cross section can be constrained. Although the process of DM
capture in astrophysical objects like the Sun is commonly assumed to be due to interactions only with nucleons, there are scenarios...
Mr
Ernany Rossi Schmitz
(University of Bonn)
In the framework of a 3−3−1 model with right-handed neutrinos and three scalar triplets we consider different spontaneous symmetry breaking patterns seeking for a non-linear realization of accidental symmetries of the model, which will produce physical Nambu-Goldstone (NG) bosons in the neutral scalar spectrum. We make a detailed study of the safety of the model concerning the NG boson...
Mr
Simone Dresti
(Georg-August University Göttingen)
In a Quantum Field Theory with a time-dependent background time-translational symmetry is broken. We therefore expect renormalization to lead to time-dependent loop corrections.
In my talk I will discuss the first order corrections to the power spectrum and the time-dependence that we observe.
Dr
Diogo Buarque Franzosi
(II Physics Institute, Goettingen U.)
Unitarity constraints on the scattering of longitudinal weak bosons can provide information about the spectra and effective description of Composite Higgs models. We use this information to construct realistic scenarios and study the potential of observing signals of strong vector boson scattering at the LHC and a 100 TeV collider.
