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Cross Section Calculations in Theories of Self-Interacting Dark Matter

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arxiv 2206.14395 v1 pith:DLYP2HPJ submitted 2022-06-29 hep-ph astro-ph.COastro-ph.GAhep-exhep-th

Cross Section Calculations in Theories of Self-Interacting Dark Matter

classification hep-ph astro-ph.COastro-ph.GAhep-exhep-th
keywords crosssectionchanneldarkmattersigmaobtainedreaction
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study an asymmetric dark matter model with self-interacting dark matter consisting of a Dirac fermion $\chi$ coupled to a scalar or vector mediator, such that the reaction $\chi + \chi \to \chi + \chi$ is well described by perturbation theory. We compute the scattering cross section $\sigma$, the transfer cross section $\sigma_T$, and the viscosity cross section $\sigma_V$ for this reaction. As one part of our study, we give analytic and numerical comparisons of results obtained with the inclusion of both $t$-channel and $u$-channel exchanges and results obtained in an approximation that has often been used in the literature that includes only the $t$-channel contribution. The velocity dependences of these cross sections are studied in detail and shown to be in accord with observational data.

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Cited by 1 Pith paper

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    Neutron dark decays modify the equation of state and either mildly suppress or strongly enhance bulk viscosity in neutron star merger conditions, depending on the in-medium decay rate.