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http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/285Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | K. Singh, Shailesh | - |
| dc.contributor.author | Biswal, S. K. | - |
| dc.contributor.author | Bhuyan, M. | - |
| dc.contributor.author | Jha, T. K. | - |
| dc.contributor.author | Patra, S. K. | - |
| dc.date.accessioned | 2022-03-25T07:28:50Z | - |
| dc.date.available | 2022-03-25T07:28:50Z | - |
| dc.date.issued | 2015-08-03 | - |
| dc.identifier.issn | 2321-8649 | - |
| dc.identifier.issn | 2321-9289 | - |
| dc.identifier.uri | http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/285 | - |
| dc.description.abstract | using the nuclear equation of states for a large variety of relativistic and non-relativistic force parameters, we calculate the static and rotating masses and radii of neutron stars. From these equation of states, we evaluate the properties of rotating neutron stars, such as rotational frequencies, moment of inertia, quadrupole deformation parameter, rotational ellipticity and gravitational wave strain amplitude. The estimated gravitational wave strain amplitude of the star is found to be~sim 10-23 | en_US |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | ;CHAENG/2013/51628 | - |
| dc.subject | Relativistic and Non-relativistic mean field formalisms | en_US |
| dc.subject | static and rotating neutron star | en_US |
| dc.subject | gravitational waves | en_US |
| dc.subject | equation of state | en_US |
| dc.title | Properties of Rotating Neutron Star | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | Vol. 3 No. 1 (2015) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 149-Article Text-234-1-10-20190821.pdf | 756.07 kB | Adobe PDF | View/Open |
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