Heating neutron stars with GeV dark matter
Heating neutron stars with GeV dark matter
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Publisher
Berlin/Heidelberg: Springer Berlin Heidelberg
Journal title
Language
English
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Publisher
Berlin/Heidelberg: Springer Berlin Heidelberg
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A
bstract
An old neutron star (NS) may capture halo dark matter (DM) and get heated up by the deposited kinetic energy, thus behaving like a thermal DM detector with sensitivity to a wide range of DM masses and a variety of DM-quark interactions. Near future infrared telescopes will measure NS temperatures down to a few thousand Kelvin and pr...
Alternative Titles
Full title
Heating neutron stars with GeV dark matter
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TN_cdi_doaj_primary_oai_doaj_org_article_c59f9c2a8af245d09f7ce7be5d9e974a
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_c59f9c2a8af245d09f7ce7be5d9e974a
Other Identifiers
ISSN
1029-8479
E-ISSN
1029-8479
DOI
10.1007/JHEP07(2020)181
