Constraining asymmetric dark matter through observations of compact stars

Journal Article · Fri Apr 15 00:00:00 EDT 2011 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.83.083512· OSTI ID:21541453

Kouvaris, Chris; Tinyakov, Peter ^[1]

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1. CP3-Origins, University of Southern Denmark, Campusvej 55, Odense 5230 (Denmark)

We put constraints on asymmetric dark matter candidates with spin-dependent interactions based on the simple existence of white dwarfs and neutron stars in globular clusters. For a wide range of the parameters (WIMP mass and WIMP-nucleon cross section), weakly interacting massive particles (WIMPs) can be trapped in progenitors in large numbers and once the original star collapses to a white dwarf or a neutron star, these WIMPs might self-gravitate and eventually collapse forming a mini-black hole that eventually destroys the star. We impose constraints competitive to direct dark matter search experiments, for WIMPs with masses down to the TeV scale.

• OSTI ID: 21541453
• Journal Information: Physical Review. D, Particles Fields, Vol. 83, Issue 8; Other Information: DOI: 10.1103/PhysRevD.83.083512; (c) 2011 American Institute of Physics; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ASYMMETRY
BLACK HOLES
CROSS SECTIONS
INTERACTIONS
LIMITING VALUES
MASS
NEUTRON STARS
NONLUMINOUS MATTER
NUCLEONS
PARTICLES
SPIN
TRAPPING
WEAK INTERACTIONS
WHITE DWARF STARS
ANGULAR MOMENTUM
BARYONS
BASIC INTERACTIONS
DWARF STARS
ELEMENTARY PARTICLES
FERMIONS
HADRONS
MATTER
PARTICLE PROPERTIES
STARS