Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/117950
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Type: Conference paper
Title: Neutron to dark matter decay in neutron stars
Author: Motta, T.F.
Guichon, P.A.M.
Thomas, A.W.
Citation: International Journal of Modern Physics A: particles and fields; gravitation; cosmology; nuclear physics, 2018, vol.33, iss.31
Publisher: World Scientific
Issue Date: 2018
ISSN: 0217-751X
1793-656X
Conference Name: Conference on Particles and Cosmology (5 Mar 2018 - 9 Mar 2018 : Nanyang Technol Univ, Singapore, SINGAPORE)
Statement of
Responsibility: 
T. F. Motta, P. A. M. Guichon and A. W. Thomas
Abstract: Recent proposals have suggested that a previously unknown decay mode of the neutron into a dark matter particle could solve the long lasting measurement problem of the neutron decay width. We show that, if the dark particle in neutron decay is the major component of the dark matter in the universe, this proposal is in disagreement with modern astrophysical data concerning neutron star masses.
Rights: © World Scientific Publishing Company
DOI: 10.1142/S0217751X18440207
Grant ID: http://purl.org/au-research/grants/arc/CE1101004
http://purl.org/au-research/grants/arc/DP150103164
Published version: https://www.worldscientific.com/
Appears in Collections:Aurora harvest 8
Physics publications

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