Radiation from rapidly rotating oblate neutron stars
Radiation from rapidly rotating oblate neutron stars
About this item
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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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Contents
A theoretical framework for emission originating from rapidly rotating oblate compact objects is described in detail. By using a Hamilton-Jacobi formalism, we show how the special relativistic rotational effects such as aberration of angles, Doppler boosting, and time dilatation naturally emerge from the general relativistic treatment of rotating c...
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Full title
Radiation from rapidly rotating oblate neutron stars
Authors, Artists and Contributors
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Record Identifier
TN_cdi_proquest_journals_2071837489
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2071837489
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1709.07292
