The 3.5 keV X-ray line signature from annihilating and decaying dark matter in Weinberg model
Seungwon Baek, P. Ko, Wan-Il Park

TL;DR
This paper explains the 3.55 keV X-ray line as a signature of annihilating or decaying dark matter within Weinberg's model, proposing scenarios for dark matter production consistent with observed relic abundance and astrophysical constraints.
Contribution
It introduces a viable dark matter model within Weinberg's framework that accounts for the X-ray line via annihilation or decay, highlighting the dominant production mechanism and consistency with cosmological bounds.
Findings
The X-ray line can be explained by p-wave annihilation of dark matter into photons.
Only the thermal decoupling scenario matches both the X-ray signal and relic abundance.
Dark matter production via Higgs decay (freeze-in) is the dominant non-thermal process.
Abstract
Recently two groups independently observed unidentified X-ray line signal at the energy 3.55 keV from the galaxy clusters and Andromeda galaxy. We show that this anomalous signal can be explained in annihilating dark matter model, for example, fermionic dark matter model in hidden sector with global symmetry proposed by Weinberg. There are two scenarios for the production of the annihilating dark matters. In the first scenario the dark matters with mass 3.55 keV decouple from the interaction with Goldstone bosons and go out of thermal equilibrium at high temperature ( 1 TeV) when they are still relativistic, their number density per comoving volume being essentially fixed to be the current value. The correct relic abundance of this warm dark matter is obtained by assuming that about relativistic degrees of freedom were present at the decoupling temperature…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Pulsars and Gravitational Waves Research
