Non-minimally coupled vector boson dark matter

被引:9
|
作者
Barman, Basabendu [1 ]
Bernal, Nicolas [1 ]
Das, Ashmita [2 ]
Roshan, Rishav [3 ,4 ]
机构
[1] Univ Antonio Narino, Ctr Invest, Carrera 3 Este 47A-15, Bogota, Colombia
[2] Indian Inst Technol Madras, Ctr Strings Gravitat & Cosmol, Dept Phys, Chennai 600036, Tamil Nadu, India
[3] IIT Guwahati, Dept Phys, Gauhati 781039, India
[4] Phys Res Lab, Ahmadabad 380009, Gujarat, India
基金
欧盟地平线“2020”;
关键词
dark matter theory; gravity; particle physics-cosmology connection; physics of the early universe; PARTICLE; CANDIDATES; PHYSICS;
D O I
10.1088/1475-7516/2022/01/047
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a simple abelian vector dark matter (DM) model, where only the DM ((X) over tildee mu) couples non-minimally to the scalar curvature ( Re) of the background spacetime via an operator of the form " (X) over tilde(X) over tilde mu (X) over tilde mu (R) over tilde. By considering the standard freeze-out scenario, we show, it is possible to probe such a non-minimally coupled DM in direct detection experiments for a coupling strength xi similar to O (1030) and DM mass m(X) <= 55 TeV, satisfying Planck observed relic abundance and perturbative unitarity. We also discuss DM production via freeze-in, governed by the non-minimal coupling, that requires xi <= 10(-5) to produce the observed DM abundance over a large range of DM mass depending on the choice of the reheating temperature. We further show, even in the absence of the non-minimal coupling, it is possible to produce the whole observed DM abundance via 2-to-2 scattering of the bath particles mediated by massless gravitons.
引用
下载
收藏
页数:29
相关论文
共 50 条
  • [21] Non-minimally coupled tachyon and inflation
    Piao, YS
    Huang, QG
    Zhang, XM
    Zhang, YZ
    PHYSICS LETTERS B, 2003, 570 (1-2) : 1 - 4
  • [22] Stability analysis for non-minimally coupled dark energy models in the Palatini formalism
    Zuobin Wang
    Puxun Wu
    Hongwei Yu
    Astrophysics and Space Science, 2018, 363
  • [23] Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
    Setare, M. R.
    Saridakis, E. N.
    PHYSICS LETTERS B, 2009, 671 (03) : 331 - 338
  • [24] A non-minimally coupled quintom dark energy model on the warped DGP brane
    Nozari, K.
    Setare, M. R.
    Azizi, T.
    Behrouz, N.
    PHYSICA SCRIPTA, 2009, 80 (02)
  • [25] Stability analysis for non-minimally coupled dark energy models in the Palatini formalism
    Wang, Zuobin
    Wu, Puxun
    Yu, Hongwei
    ASTROPHYSICS AND SPACE SCIENCE, 2018, 363 (06)
  • [26] Late-time anisotropy sourced by a 2-form field non-minimally coupled to cold dark matter
    Orjuela-Quintana, J. Bayron
    Palacios-Cordoba, Jose L.
    Valenzuela-Toledo, Cesar A.
    PHYSICS OF THE DARK UNIVERSE, 2024, 46
  • [27] Schwarzschild quasi-normal modes of non-minimally coupled vector fields
    Garcia-Saenz, Sebastian
    Held, Aaron
    Zhang, Jun
    JOURNAL OF HIGH ENERGY PHYSICS, 2022, 2022 (05)
  • [28] Schwarzschild quasi-normal modes of non-minimally coupled vector fields
    Sebastian Garcia-Saenz
    Aaron Held
    Jun Zhang
    Journal of High Energy Physics, 2022
  • [29] Non-Abelian vector boson as FIMP dark matter
    Barman, Basabendu
    Bhattacharya, Subhaditya
    Zakeri, Mohammadreza
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2020, (02):
  • [30] Non-minimally coupled teleparallel scalar field reconstruction of matter bounce scenario
    Tripathy, S.K.
    Pal, Sasmita
    Mishra, B.
    European Physical Journal C, 2024, 84 (11):