Dark Matter Research: A Look at the Standard Model

Written by phenomenology | Published 2025/02/14
Tech Story Tags: dark-matter | dark-matter-research | analyzing-dark-matter | outer-space | dark-matter-wimp-model | dark-matter-model | alp-langrangian | sm-gauge-symmetry

TLDRThe model that we consider is the minimal combination of type-I seesaw and effective ALP interaction with additional Z2 symmetry apart from the SM gauge symmetry via the TL;DR App

Table of Links

Acknowledgements

1 Introduction to thesis

1.1 History and Evidence

1.2 Facts on dark matter

1.3 Candidates to dark matter

1.4 Dark matter detection

1.5 Outline of the thesis

2 Dark matter through ALP portal and 2.1 Introduction

2.2 Model

2.3 Existing constraints on ALP parameter space

2.4 Dark matter analysis

2.5 Summary

3 A two component dark matter model in a generic 𝑈(1)𝑋 extension of SM and 3.1 Introduction

3.2 Model

3.3 Theoretical and experimental constraints

3.4 Phenomenology of dark matter

3.5 Relic density dependence on 𝑈(1)𝑋 charge 𝑥𝐻

3.6 Summary

4 A pseudo-scalar dark matter case in 𝑈(1)𝑋 extension of SM and 4.1 Introduction

4.2 Model

4.3 Theoretical and experimental constraints

4.4 Dark Matter analysis

4.5 Summary

5 Summary

Appendices

A Standard model

B Friedmann equations

C Type I seasaw mechanism

D Feynman diagrams in two-component DM model

Bibliography

2.2 Model

The model that we consider is the minimal combination of type-I seesaw and effective ALP interaction with additional Z2 symmetry apart from the SM gauge symmetry [108, 109]. The matter content of the model is shown in Table. 2.1.

This paper is available on arxiv under CC BY 4.0 DEED license.

Author:

(1) Shivam Gola, The Institute of Mathematical Sciences, Chennai.


Written by phenomenology | Phenomenology explores the depths of consciousness, fostering a deeper understanding of the world.
Published by HackerNoon on 2025/02/14