Numerically analyzing self-interacting dark matter
Utkarsh Patel, Sudhanwa Patra (IIT Bhilai)

TL;DR
This paper investigates self-interacting dark matter with a light mediator, analyzing the transfer cross-section dynamics, velocity dependence, and parameter space, while offering an efficient numerical approach and a minimal leptophilic model extension.
Contribution
It introduces an efficient numerical method for calculating SIDM cross-sections and provides an analytical analysis using Hulthén potential, along with a minimal leptophilic model extension.
Findings
Numerical results are more efficient with fewer $$ modes.
Transfer cross-section depends on mediator mass and velocity.
A minimal leptophilic extension of the standard model is proposed.
Abstract
We consider the scenario of self-interacting dark matter(SIDM) with a light mediator in a model-independent way, which can alleviate two long-standing issues of the small scale cosmology namely cusp vs. core and too-big-to-fail. A Yukawa potential is chosen to achieve mediator exchange between DM particles as part of their self-interactions. The dynamics of self-interacting transfer cross-section are studied for a range of mediator mass(). Also, a relationship is established between the cross-section and DM particles' relative velocity, which ensures the solution to the DM crisis at small scales. Our obtained numerical results are efficient compared to the earlier works in the context that a lesser number of modes have been used by us to achieve the same level of accuracy in the cross-section calculations. For a better understanding of the SIDM parameter space, we perform…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Advanced Thermodynamics and Statistical Mechanics
