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Constraints on scalar asymmetric dark matter from black hole formation in neutron stars

McDermott, Samuel D. and Yu, Hai-Bo and Zurek, Kathryn M. (2012) Constraints on scalar asymmetric dark matter from black hole formation in neutron stars. Physical Review D, 85 (2). Art. No. 023519. ISSN 1550-7998. doi:10.1103/physrevd.85.023519. https://resolver.caltech.edu/CaltechAUTHORS:20190613-110922233

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Abstract

We consider possibly observable effects of asymmetric dark matter (ADM) in neutron stars. Since dark matter does not self-annihilate in the ADM scenario, dark matter accumulates in neutron stars, eventually reaching the Chandrasekhar limit and forming a black hole. We focus on the case of scalar ADM, where the constraints from Bose-Einstein condensation and subsequent black hole formation are most severe due to the absence of Fermi degeneracy pressure. We also note that in some portions of this constrained parameter space, nontrivial effects from Hawking radiation can modify our limits. We find that for scalar ADM with mass between 5 MeV and 13 GeV, the constraint from nearby neutron stars on the scattering cross section with neutrons ranges from σ_n ≲ 10^(−45) cm^2 to 10^(−47) cm^2.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/physrevd.85.023519DOIArticle
https://arxiv.org/abs/1103.5472arXivDiscussion Paper
Additional Information:© 2012 American Physical Society. (Received 21 April 2011; published 13 January 2012)
Issue or Number:2
Classification Code:PACS numbers: 95.35.+d, 98.80.Cq
DOI:10.1103/physrevd.85.023519
Record Number:CaltechAUTHORS:20190613-110922233
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190613-110922233
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96383
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:17 Jun 2019 14:57
Last Modified:16 Nov 2021 17:20

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