Study of potential self-annihilation signal from dark matter particles in some prospective astrophysical dark matter sources

TL;DR

This paper investigates potential signals from dark matter self-annihilation in astrophysical sources using gamma-ray and radio observations, aiming to enhance indirect detection methods.

Contribution

It introduces a dual-method approach combining gamma-ray and radio observations to identify dark matter self-annihilation signals.

Findings

Identified promising astrophysical sources for dark matter detection

Developed a methodology for analyzing gamma-ray and radio data

Provided insights into the characteristics of potential dark matter signals

Abstract

With the growing interest in indirect detection for dark matter signature, the thesis aims to investigate the signal originating from the self-annihilation of dark matter candidates. The methods for targeting the dark matter signal are two-fold, on one hand, we explore the gamma rays resulting from dark matter particles. On the other hand, we focus on complementary radio properties.