Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries
Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries
Neutron stars accreting matter from low-mass binary companions are observed to undergo bursts of X-rays due to the thermonuclear explosion of material on the neutron star surface. We use recent results on superfluid and superconducting properties to show that the core temperature in these neutron stars may not be uniquely determined for a range of observed accretion rates. The degeneracy in inferred core temperatures could contribute to explaining the difference between neutron stars which have very short recurrence times between multiple bursts from those which have long recurrence times between bursts: short bursting sources have higher temperatures and normal neutrons in the stellar core, while long bursting sources have lower temperatures and superfluid neutrons. If correct, measurements of the lowest luminosity from among the short bursting sources and highest luminosity from among the long bursting sources can be used to constrain the critical temperature for the onset of neutron superfluidity.
L99-L103
Ho, Wynn C.G.
d78d4c52-8f92-4846-876f-e04a8f803a45
10 November 2011
Ho, Wynn C.G.
d78d4c52-8f92-4846-876f-e04a8f803a45
Ho, Wynn C.G.
(2011)
Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries.
Monthly Notices of the Royal Astronomical Society: Letters, 418 (1), .
(doi:10.1111/j.1745-3933.2011.01152.x).
Abstract
Neutron stars accreting matter from low-mass binary companions are observed to undergo bursts of X-rays due to the thermonuclear explosion of material on the neutron star surface. We use recent results on superfluid and superconducting properties to show that the core temperature in these neutron stars may not be uniquely determined for a range of observed accretion rates. The degeneracy in inferred core temperatures could contribute to explaining the difference between neutron stars which have very short recurrence times between multiple bursts from those which have long recurrence times between bursts: short bursting sources have higher temperatures and normal neutrons in the stellar core, while long bursting sources have lower temperatures and superfluid neutrons. If correct, measurements of the lowest luminosity from among the short bursting sources and highest luminosity from among the long bursting sources can be used to constrain the critical temperature for the onset of neutron superfluidity.
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Published date: 10 November 2011
Organisations:
Applied Mathematics
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Local EPrints ID: 195975
URI: http://eprints.soton.ac.uk/id/eprint/195975
ISSN: 1745-3933
PURE UUID: 23aeea07-bf9f-4c49-81ab-83c83455acf0
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Date deposited: 31 Aug 2011 13:04
Last modified: 14 Mar 2024 04:06
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