# Simply split SIMPs

**Authors:** Nicol\'as Bernal, Xiaoyong Chu, Josef Pradler

arXiv: 1702.04906 · 2017-06-28

## TL;DR

This paper investigates self-interacting dark matter models with nearly degenerate states, analyzing relic density, self-scattering mechanisms, and potential signals for future dark matter detection, aiming to address small-scale structure issues.

## Contribution

It introduces a simple model with pseudo-Dirac fermions or scalars for self-interacting dark matter, exploring relic density calculations and detection prospects.

## Key findings

- Self-scattering regulated by mass-splitting and abundance ratios.
- Relic density can be set via 4-to-2 reactions or freeze-in.
- Potential signals in future dark matter searches.

## Abstract

Dark Matter which interacts strongly with itself, but only feebly with the Standard Model is a possibility that has been entertained to solve apparent small-scale structure problems that are pertinent to the non-interacting cold Dark Matter paradigm. In this paper, we study the simple case in which the self-scattering rate today is regulated by kinematics and/or the abundance ratio, through the mass-splitting of nearly degenerate pseudo-Dirac fermions $\chi_1$ and $\chi_2$ or real scalars $\phi_1$ and $\phi_2$. We calculate the relic density of these states in a scenario where self-scattering proceeds through off-diagonal couplings with a vector particle $V$ (Dark Photon) and where the abundance is set through number-depleting 4-to-2 reactions in the hidden sector, or, alternatively, via freeze-in. We study the implications of the considered models and their prospect of solving astrophysical small-scale structure problems. We also show how the introduction of the (meta-)stable heavier state may be probed in future dark matter searches.

## Full text

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## Figures

18 figures with captions in the complete paper: https://tomesphere.com/paper/1702.04906/full.md

## References

109 references — full list in the complete paper: https://tomesphere.com/paper/1702.04906/full.md

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Source: https://tomesphere.com/paper/1702.04906