Exploring sub-GeV dark matter via $s$-wave, $p$-wave, and resonance annihilation with CMB data

Fuente: arXiv
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Autores principales: Wang, Yu-Ning, Duan, Xin-Chen, Tang, Tian-Peng, Wang, Ziwei, Tsai, Yue-Lin Sming
Formato: Preprint
Publicado: 2025
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author Wang, Yu-Ning
Duan, Xin-Chen
Tang, Tian-Peng
Wang, Ziwei
Tsai, Yue-Lin Sming
author_facet Wang, Yu-Ning
Duan, Xin-Chen
Tang, Tian-Peng
Wang, Ziwei
Tsai, Yue-Lin Sming
contents We revisit constraints on sub-GeV dark matter (DM) annihilation via $s$-wave, $p$-wave, and resonance processes using current and future CMB data from Planck, FIRAS, and upcoming experiments such as LiteBIRD, CMB-S4, PRISTINE, and PIXIE. For $s$-wave annihilation, we provide updated limits for both $e^{+}e^{-}$ and $ππ$ channels, with the profile likelihood method yielding stronger constraints than the marginal posterior method. In the $p$-wave case, we comprehensively present a model-independent inequality for the $95\%$ upper limits from FIRAS, PRISTINE, and PIXIE, with future experiments expected to surpass current BBN limits. For resonance annihilation, we report -- for the first time -- the $95\%$ upper limits on the decay branching ratio of the mediator particle, when the resonance peaks during the recombination epoch. Overall, our study highlights the complementary strengths of $μ$-distortion and CMB anisotropies in probing sub-GeV DM annihilation.
format Preprint
id arxiv_https___arxiv_org_abs_2502_18263
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Exploring sub-GeV dark matter via $s$-wave, $p$-wave, and resonance annihilation with CMB data
Wang, Yu-Ning
Duan, Xin-Chen
Tang, Tian-Peng
Wang, Ziwei
Tsai, Yue-Lin Sming
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We revisit constraints on sub-GeV dark matter (DM) annihilation via $s$-wave, $p$-wave, and resonance processes using current and future CMB data from Planck, FIRAS, and upcoming experiments such as LiteBIRD, CMB-S4, PRISTINE, and PIXIE. For $s$-wave annihilation, we provide updated limits for both $e^{+}e^{-}$ and $ππ$ channels, with the profile likelihood method yielding stronger constraints than the marginal posterior method. In the $p$-wave case, we comprehensively present a model-independent inequality for the $95\%$ upper limits from FIRAS, PRISTINE, and PIXIE, with future experiments expected to surpass current BBN limits. For resonance annihilation, we report -- for the first time -- the $95\%$ upper limits on the decay branching ratio of the mediator particle, when the resonance peaks during the recombination epoch. Overall, our study highlights the complementary strengths of $μ$-distortion and CMB anisotropies in probing sub-GeV DM annihilation.
title Exploring sub-GeV dark matter via $s$-wave, $p$-wave, and resonance annihilation with CMB data
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2502.18263