Post-Newtonian treatment of bar mode instability in rigidly rotating equilibrium configurations for...
Post-Newtonian treatment of bar mode instability in rigidly rotating equilibrium configurations for polytropic stars
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
We determine the onset point of secular instability for the nonaxisymmetric bar mode in rigidly rotating equilibrium configurations in the Post-Newtonian approximation, in order to apply it to neutron stars. The treatment is based on a precedent Newtonian analytic energy variational method which we have extended to the Post-Newtonian case. This met...
Alternative Titles
Full title
Post-Newtonian treatment of bar mode instability in rigidly rotating equilibrium configurations for polytropic stars
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2088839333
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2088839333
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.0205398
