Dr
Vasiliki Mitsou
(IFIC - CSIC / Valencia Univ.)
15/05/2017, 16:30
Dr
Diego Martinez Santos
(GAIN and Universidade de Santiago de Compostela)
15/05/2017, 16:50
Poster
We perform a fit of various SUSY models (with a WIMP DM candidate) to experimental data from LHC searches, astrophysical data, low-energy and flavor observables.
Based on this analysis we give predictions for the propects of Direct Detection experiments, ongoing LHC searches and future colider searches.
We stress the complementarity of the various searches to determine the nature of DM.
Oliver Keith Baker
(Yale University)
15/05/2017, 17:10
Presentation
This Dark Sector search in the ATLAS collaboration
uses Higgs boson exotic decays as a possible portal
to such new phenomena. Use is made of the Standard Model
(SM) decay to four leptons:
H-->ZZ*-->4l
The current analysis is sensitive to the possible existence
of "Dark Sector" or "Hidden Sector" vector boson ("Zd") or
pseudoscalar boson ("a") that is beyond the SM:
...
Prof.
Richard Creswick
(University of South Carolina)
15/05/2017, 17:55
Axions can be emitted in the M1 transition of Fe-57 in the Sun. The width of the 14.4 keV axion spectrum is Doppler broadened to about 5 eV (FWHM). The angular size of the region of the Sun responsible for axion production subtends an angle of approximately 0.05 deg., which means the Sun is a nearly monochromatic point source of 14.4 keV axions and ideally suited for coherent Bragg conversion...
Dr
John Blanchard
(Helmholtz-Institut Mainz)
15/05/2017, 18:15
The Cosmic Axion Spin Precession Experiment (CASPEr) uses nuclear magnetic resonance (NMR) techniques to search for spin precession induced by ultralight axion dark matter. I will discuss recent experimental progress, including a new experimental mode based on zero- to ultralow-field (ZULF) NMR.