Epicyclic oscillations in the Hartle-Thorne external geometry
Epicyclic oscillations in the Hartle-Thorne external geometry
About this item
Full title
Author / Creator
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
The external Hartle-Thorne geometry, which describes the space-time outside a slowly-rotating compact star, is characterized by the gravitational mass \(M\), angular momentum \(J\) and quadrupole moment \(Q\) of the star and gives a convenient description which, for the rotation frequencies of more than 95 % of known pulsars, is sufficiently accura...
Alternative Titles
Full title
Epicyclic oscillations in the Hartle-Thorne external geometry
Authors, Artists and Contributors
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2219322397
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2219322397
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1905.00730
