Constraints on Symmetric Dark Matter from Neutron Star Capture and Collapse
Fuente:
arXiv
Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866911095343546368 |
|---|---|
| author | Liu, Yuxin Liu, Zhen Pospelov, Maxim Reddy, Sanjay |
| author_facet | Liu, Yuxin Liu, Zhen Pospelov, Maxim Reddy, Sanjay |
| contents | Dark matter (DM) models with a conserved particle$-$antiparticle number, $n_χ-n_{\tilde χ}$, and the asymmetry in the cosmological abundance $n_χ\neq n_{\tilde χ}$, are known to be challenged by the existence of old neutron stars (NSs), as the sufficient accumulation of DM will lead to the collapse of NSs into black holes. We demonstrate that the applicability of these constraints is much wider and covers models with symmetric populations of DM, $n_χ= n_{\tilde χ}$, as the process of DM capture regulated by a nucleon-DM scattering can be inherently asymmetric, $σ_{χn}\neq σ_{\tildeχn}$. The asymmetry is induced by the interference of different types of $χ$-$n$ interactions, provided that their combination is odd under charge conjugation in the DM sector, $C_χ$, and even under combined parity $P_{χ+ n}$. We provide a complete analysis of DM-nucleon bilinear $χ$-$n$ interactions and find that this asymmetry is very generic. Using canonical NS parameters and local DM halo inputs, we exclude spin-averaged scattering cross sections down to $σ_{nχ}\!\gtrsim\!10^{-46}\,{\rm cm}^{2}$ at DM mass $m_χ\!\lesssim\!10^{10}\,{\rm GeV}$ for the maximally asymmetric capture rate, and show that the constraints persist down to very small values of the cross-section asymmetry, ${\cal A}=(σ_{χn}- σ_{\tildeχn})/(σ_{χn}+ σ_{\tildeχn})\gtrsim 10^{-5}$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_04961 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Constraints on Symmetric Dark Matter from Neutron Star Capture and Collapse Liu, Yuxin Liu, Zhen Pospelov, Maxim Reddy, Sanjay High Energy Physics - Phenomenology High Energy Astrophysical Phenomena Dark matter (DM) models with a conserved particle$-$antiparticle number, $n_χ-n_{\tilde χ}$, and the asymmetry in the cosmological abundance $n_χ\neq n_{\tilde χ}$, are known to be challenged by the existence of old neutron stars (NSs), as the sufficient accumulation of DM will lead to the collapse of NSs into black holes. We demonstrate that the applicability of these constraints is much wider and covers models with symmetric populations of DM, $n_χ= n_{\tilde χ}$, as the process of DM capture regulated by a nucleon-DM scattering can be inherently asymmetric, $σ_{χn}\neq σ_{\tildeχn}$. The asymmetry is induced by the interference of different types of $χ$-$n$ interactions, provided that their combination is odd under charge conjugation in the DM sector, $C_χ$, and even under combined parity $P_{χ+ n}$. We provide a complete analysis of DM-nucleon bilinear $χ$-$n$ interactions and find that this asymmetry is very generic. Using canonical NS parameters and local DM halo inputs, we exclude spin-averaged scattering cross sections down to $σ_{nχ}\!\gtrsim\!10^{-46}\,{\rm cm}^{2}$ at DM mass $m_χ\!\lesssim\!10^{10}\,{\rm GeV}$ for the maximally asymmetric capture rate, and show that the constraints persist down to very small values of the cross-section asymmetry, ${\cal A}=(σ_{χn}- σ_{\tildeχn})/(σ_{χn}+ σ_{\tildeχn})\gtrsim 10^{-5}$. |
| title | Constraints on Symmetric Dark Matter from Neutron Star Capture and Collapse |
| topic | High Energy Physics - Phenomenology High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2508.04961 |