17–24 Jul 2024
Prague
Europe/Prague timezone

Effect of thermal fluctuations on dark matter annihilation cross section

19 Jul 2024, 19:00
2h
Foyer Floor 2

Foyer Floor 2

Poster 08. Astro-particle Physics and Cosmology Poster Session 2

Speaker

Prabhat Butola (Homi Bhabha National Institute, Mumbai & The Institute of Mathematical Sciences, Chennai)

Description

We are interested in thermal corrections to dark matter (DM) annihilation cross sections in a MSSM-inspired BSM theory, having bino-like Majorana DM ($\chi$), annihilating to SM fermions through Yukawa interactions via a charged scalar channel in freeze-out scenario. We apply real-time formalism of thermal field theory (TFT) to investigate corrections due to thermal fluctuations of DM annihilation cross section at NLO. We utilize generalized Grammer and Yennie approach in TFT to assure IR divergence cancellation with $K$-polarization sum of real and virtual corrections at NLO to DM annihilation processes $(\chi \bar{\chi} \rightarrow f \bar{f})$. We calculate the thermal correction to the finite remainder in TFT. Our Calculations shows quadratic thermal dependence of annihilation cross section of DM $( \sigma_T \propto {\cal{O}}(T^2))$ considering scalar to be heavy compared to DM and SM fermions.

Alternate track 03. Beyond the Standard Model
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Primary author

Prabhat Butola (Homi Bhabha National Institute, Mumbai & The Institute of Mathematical Sciences, Chennai)

Co-authors

D Indumathi (The Institute of Mathematical Sciences, Chennai) Pritam Sen (Tata Institute of Fundamental Research)

Presentation materials