Indirect Probes of Dark Matter and Globular Cluster Properties From Dark Matter Annihilation within the Coolest White Dwarfs

Abstract

White Dwarfs (WD) capture Dark Matter (DM) as they orbit within their host halos. These captured particles may subsequently annihilate, heating the stellar core and preventing the WD from cooling. The potential wells of WDs are considerably deeper and core temperatures significantly cooler than those of main sequence stars. Consequently, DM evaporation is less important in WDs and DM with masses $M_χ \gtrsim 100\, \kev$ and annihilation cross-sections orders of magnitude below the canonical thermal cross-section ($\sigmav \gtrsim 10^{-46}\, \cm^3$/s) can significantly alter WD cooling in particular astrophysical environments. We consider WDs in globular clusters (GCs) and dwarf galaxies. If the parameters of the DM particle are known, then the temperature of the coolest WD in a GC can be used to constrain the DM density of the cluster's halo (potentially even ruling out the presence of a halo if the inferred density is of order the ambient Galactic density). Recently several direct detection experiments have seen signals whose origins might be due to low mass DM. In this paper, we show that if these claims from CRESST, DAMA, CDMS-Si, and CoGeNT could be interpreted as DM, then observations of NGC 6397 limit the fraction of DM in that cluster to be $f_{\mathrm{DM}}\lesssim 10^{-3}$. This would be an improvement over existing constraints of 3 orders of magnitude and clearly rule out a significant DM halo for this cluster...

13 pages, 7 figures

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Cited by in corpus (11)

• Neon Cluster Formation and Phase Separation During White Dwarf Cooling
• Nuclear and dark matter heating in massive white dwarf stars
• Direct Detection of Atomic Dark Matter in White Dwarfs
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• The Effects of Asymmetric Dark Matter on Stellar Evolution I: Spin-Dependent Scattering
• Constraining primordial black holes as a fraction of dark matter through accretion disk luminosity
• Could compact stars in globular clusters constrain dark matter?
• Properties of globular clusters formed in dark matter mini-halos
• The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
• On the Ejection of Dark Matter from Globular Clusters
• Period change of binary pulsars due to the accretion of dark matter particles