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Thermal conduction by dark matter with velocity and momentum-dependent cross-sections

2014

We use the formalism of Gould and Raffelt to compute the dimensionless thermal conduction coefficients for scattering of dark matter particles with standard model nucleons via cross-sections that depend on the relative velocity or momentum exchanged between particles. Motivated by models invoked to reconcile various recent results in direct detection, we explicitly compute the conduction coefficients $\alpha$ and $\kappa$ for cross-sections that go as $v_{\rm rel}^2$, $v_{\rm rel}^4$, $v_{\rm rel}^{-2}$, $q^2$, $q^4$ and $q^{-2}$, where $v_{\rm rel}$ is the relative DM-nucleus velocity and $q$ is the momentum transferred in the collision. We find that a $v_{\rm rel}^{-2}$ dependence can sig…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterRelative velocityFOS: Physical sciencesAstronomy and AstrophysicsThermal conduction01 natural sciencesOuter coreComputational physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Solar coreAstrophysics - Solar and Stellar Astrophysics0103 physical sciencesThermalNucleon010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Dimensionless quantityAstrophysics - Cosmology and Nongalactic Astrophysics
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