TY - JOUR
T1 - Recommendations of the LHC Dark Matter Working Group
T2 - Comparing LHC searches for dark matter mediators in visible and invisible decay channels and calculations of the thermal relic density
AU - Albert, Andreas
AU - Backović, Mihailo
AU - Boveia, Antonio
AU - Buchmueller, Oliver
AU - Busoni, Giorgio
AU - De Roeck, Albert
AU - Doglioni, Caterina
AU - DuPree, Tristan
AU - Fairbairn, Malcolm
AU - Genest, Marie Hélène
AU - Gori, Stefania
AU - Gustavino, Giuliano
AU - Hahn, Kristian
AU - Haisch, Ulrich
AU - Harris, Philip C.
AU - Hayden, Dan
AU - Ippolito, Valerio
AU - John, Isabelle
AU - Kahlhoefer, Felix
AU - Kulkarni, Suchita
AU - Landsberg, Greg
AU - Lowette, Steven
AU - Mawatari, Kentarou
AU - Riotto, Antonio
AU - Shepherd, William
AU - Tait, Tim M.P.
AU - Tolley, Emma
AU - Tunney, Patrick
AU - Zaldivar, Bryan
AU - Zinser, Markus
PY - 2019
Y1 - 2019
N2 - Weakly-coupled TeV-scale particles may mediate the interactions between normal matter and dark matter. If so, the LHC would produce dark matter through these mediators, leading to the familiar “mono-X” search signatures, but the mediators would also produce signals without missing momentum via the same vertices involved in their production. This document from the LHC Dark Matter Working Group suggests how to compare searches for these two types of signals in case of vector and axial-vector mediators, based on a workshop that took place on September 19/20, 2016 and subsequent discussions. These suggestions include how to extend the spin-1 mediated simplified models already in widespread use to include lepton couplings. This document also provides analytic calculations of the relic density in the simplified models and reports an issue that arose when ATLAS and CMS first began to use preliminary numerical calculations of the dark matter relic density in these models.
AB - Weakly-coupled TeV-scale particles may mediate the interactions between normal matter and dark matter. If so, the LHC would produce dark matter through these mediators, leading to the familiar “mono-X” search signatures, but the mediators would also produce signals without missing momentum via the same vertices involved in their production. This document from the LHC Dark Matter Working Group suggests how to compare searches for these two types of signals in case of vector and axial-vector mediators, based on a workshop that took place on September 19/20, 2016 and subsequent discussions. These suggestions include how to extend the spin-1 mediated simplified models already in widespread use to include lepton couplings. This document also provides analytic calculations of the relic density in the simplified models and reports an issue that arose when ATLAS and CMS first began to use preliminary numerical calculations of the dark matter relic density in these models.
U2 - 10.1016/j.dark.2019.100377
DO - 10.1016/j.dark.2019.100377
M3 - Article
AN - SCOPUS:85072870487
SN - 2212-6864
VL - 26
JO - Physics of the Dark Universe
JF - Physics of the Dark Universe
M1 - 100377
ER -