Non-adiabatic evolution of dark sector in the presence of U(1)<sub>L<sub>μ</sub> </sub> – <sub>L<sub>τ</sub> </sub> gauge symmetry

نویسندگان

چکیده

Abstract In secluded dark sector scenario, the connection between visible and can be established through a portal coupling its presence opens up possibility of non-adiabatic evolution sector. To study sector, we have considered U(1) L μ – τ ⊗ X extension standard model (SM). Here is charged only under gauge symmetry whereas SM fields are singlet this symmetry. Due to tree-level kinetic mixing bosons, evolves non-adiabatically thermal equilibrium governed by coupling. Depending on values (ϵ), ( g ), mass matter m χ ) vector boson Z' temperature as well various non-equilibrium stages in detail. Furthermore also investigated constraints parameters from laboratory astrophysical searches. We found that parameter space for significantly constrained ≲ 100 MeV observations beam dump experiments, stellar cooling etc. The relic density satisfied region our consistent with bounds direct detection, self interaction (SIDM) ratio r ≡ / = 10 -3 these will more relaxed larger . However measurement diffuse γ-ray background flux cosmic microwave (CMB) anisotropy strongest -1 smaller , they not significant.

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ژورنال

عنوان ژورنال: Journal of Cosmology and Astroparticle Physics

سال: 2022

ISSN: ['1475-7516', '1475-7508']

DOI: https://doi.org/10.1088/1475-7516/2022/05/019