A Phenomenological Study of WIMP Models: A Summary of Everything We Discussed

We have considered a generic U(1)x model which provides an economical extension of SM to accommodate DM and active neutrino masses.


This content originally appeared on HackerNoon and was authored by Phenomenology Technology

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

3.6 Summary

\

\

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

:::

:::info Author:

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

:::

\


This content originally appeared on HackerNoon and was authored by Phenomenology Technology


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