Fundamental physics and the absence of sub-millisecond pulsars
Fundamental physics and the absence of sub-millisecond pulsars
About this item
Full title
Author / Creator
Haskell, B , Zdunik, J L , tin, M , Bejger, M , Wijnands, R and Patruno, A
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
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Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
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Scope and Contents
Contents
Observations of the spin distribution of rapidly rotating neutron stars show evidence for a lack of stars spinning at frequencies larger than \(f\approx 700\) Hz, well below the predictions of theoretical equations of state. This has generally been taken as evidence of an additional spin-down torque operating in these systems and it has been sugges...
Alternative Titles
Full title
Fundamental physics and the absence of sub-millisecond pulsars
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Author / Creator
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Record Identifier
TN_cdi_proquest_journals_2073339816
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073339816
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1805.11277
