Comprehensive exploration of t-channel simplified models of dark matter

被引:5
|
作者
Arina, Chiara [1 ]
Fuks, Benjamin [2 ,3 ]
Heisig, Jan [4 ,5 ]
Kraemer, Michael [4 ]
Mantani, Luca [6 ]
Panizzi, Luca [7 ,8 ,9 ]
机构
[1] Catholic Univ Louvain, Ctr Cosmol Particle Phys & Phenomenol CP3, B-1348 Louvain La Neuve, Belgium
[2] Sorbonne Univ, Lab Phys Theor & Hautes Energies LPTHE, UMR 7589, 4 Pl Jussieu, F-75252 Paris 05, France
[3] CNRS, 4 Pl Jussieu, F-75252 Paris 05, France
[4] Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol, D-52056 Aachen, Germany
[5] Univ Virginia, Dept Phys, Charlottesville, VA 22904 USA
[6] Univ Cambridge, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England
[7] Univ Calabria, Dipartimento Fis, I-87036 Cosenza, Italy
[8] INFN Cosenza, I-87036 Cosenza, Cosenza, Italy
[9] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, England
关键词
SEARCH;
D O I
10.1103/PhysRevD.108.115007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyze six classes of t-channel dark matter simplified models in which the Standard Model field content is extended by a colored mediator and a dark matter state. The two new states are enforced to be odd under a new parity, while all Standard Model fields are taken even so that dark matter stability is guaranteed. We study several possibilities for the spin of the new particles and the self-conjugate property of the dark matter, and we focus on model configurations in which the dark matter couples to the right-handed up quark for simplicity. We investigate how the parameter spaces of the six models can be constrained by current and future cosmological, astrophysical and collider searches, and we highlight the strong complementary between those probes. Our results demonstrate that scenarios featuring a complex (non self-conjugate) dark matter field are excluded by cosmology and astrophysics alone, the only possibility to avoid these bounds being to invoke very weak couplings and mechanisms such as conversion -driven freeze-out. For models with self-conjugate dark matter, mediator and dark matter masses are pushed deep into the TeV regime, with the lower limits on the mediator mass reaching 3 to 4 TeV and those on the dark matter mass 1 to 2 TeV. In large parts of the parameter space these strong bounds are driven by same -sign mediator pair production, a channel so far not considered in the experimental analyses embedding t-channel dark matter model interpretations.
引用
收藏
页数:20
相关论文
共 50 条
  • [31] Simplified models for displaced dark matter signatures
    Buchmueller, Oliver
    De Roeck, Albert
    Hahn, Kristian
    McCullough, Matthew
    Schwaller, Pedro
    Sung, Kevin
    Yu, Tien-Tien
    JOURNAL OF HIGH ENERGY PHYSICS, 2017, (09):
  • [32] Simplified models for dark matter interacting with quarks
    Anthony DiFranzo
    Keiko I. Nagao
    Arvind Rajaraman
    Tim M.P. Tait
    Journal of High Energy Physics, 2013
  • [33] Simplified models for dark matter interacting with quarks
    DiFranzo, Anthony
    Nagao, Keiko I.
    Rajaraman, Arvind
    Tait, Tim M. P.
    JOURNAL OF HIGH ENERGY PHYSICS, 2013, (11):
  • [34] Simplified models for dark matter searches at the LHC
    Abdallah, Jalal
    Araujo, Henrique
    Arbey, Alexandre
    Ashkenazi, Adi
    Belyaev, Alexander
    Berger, Joshua
    Boehm, Celine
    Boveia, Antonio
    Brennan, Amelia
    Brooke, Jim
    Buchmueller, Oliver
    Buckley, Matthew
    Busoni, Giorgio
    Calibbi, Lorenzo
    Chauhan, Sushil
    Daci, Nadir
    Davies, Gavin
    De Bruyn, Isabelle
    De Jong, Paul
    De Roeck, Albert
    de Vries, Kees
    Del Re, Daniele
    De Simone, Andrea
    Di Simone, Andrea
    Doglioni, Caterina
    Dolan, Matthew
    Dreiner, Herbi K.
    Ellis, John
    Eno, Sarah
    Etzion, Erez
    Fairbairn, Malcolm
    Feldstein, Brian
    Flaecher, Henning
    Feng, Eric
    Fox, Patrick
    Genest, Marie-Helene
    Gouskos, Loukas
    Gramling, Johanna
    Haisch, Ulrich
    Harnik, Roni
    Hibbs, Anthony
    Hoh, Siewyan
    Hopkins, Walter
    Ippolito, Valerio
    Jacques, Thomas
    Kahlhoefer, Felix
    Khoze, Valentin V.
    Kirk, Russell
    Korn, Andreas
    Kotov, Khristian
    PHYSICS OF THE DARK UNIVERSE, 2015, 9-10 : 8 - 23
  • [35] Dark matter microhalos from simplified models
    Blinov, Nikita
    Dolan, Matthew J.
    Draper, Patrick
    Shelton, Jessie
    PHYSICAL REVIEW D, 2021, 103 (10)
  • [36] Simplified models for displaced dark matter signatures
    Oliver Buchmueller
    Albert De Roeck
    Kristian Hahn
    Matthew McCullough
    Pedro Schwaller
    Kevin Sung
    Tien-Tien Yu
    Journal of High Energy Physics, 2017
  • [37] Dark matter pair production in the MSSM and in simplified dark matter models at the LHC
    Borschensky, Christoph
    Coniglio, Gabriele
    Jaeger, Barbara
    EUROPEAN PHYSICAL JOURNAL C, 2019, 79 (05):
  • [38] Dark matter pair production in the MSSM and in simplified dark matter models at the LHC
    Christoph Borschensky
    Gabriele Coniglio
    Barbara Jäger
    The European Physical Journal C, 2019, 79
  • [39] Global fits of simplified models for dark matter with GAMBITII. Vector dark matter with an s-channel vector mediator
    Christopher Chang
    Pat Scott
    Tomás E. Gonzalo
    Felix Kahlhoefer
    Martin White
    The European Physical Journal C, 83
  • [40] Monojet versus the rest of the world I: t-channel models
    Michele Papucci
    Alessandro Vichi
    Kathryn M. Zurek
    Journal of High Energy Physics, 2014