Rapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matter
| dc.contributor.author | Bombaci, Ignazio | |
| dc.contributor.author | Thampan, Arun V. | |
| dc.contributor.author | Datta, Bhaskar | |
| dc.date.accessioned | 2006-10-19T04:41:45Z | |
| dc.date.available | 2006-10-19T04:41:45Z | |
| dc.date.issued | 2000-10-01 | |
| dc.description.abstract | For a new equation of state of strange quark matter, we construct equilibrium sequences of rapidly rotating strange stars in general relativity. The sequences are the normal and supramassive evolutionary sequences of constant rest mass. We also calculate equilibrium sequences for a constant value of Ω corresponding to the most rapidly rotating pulsar PSR 1937+21. In addition, we calculate the radius of the marginally stable orbit and its dependence on Ω, relevant for modeling of kilohertz quasi-periodic oscillations in X-ray binaries. | en |
| dc.format.extent | 68948 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | The Astrophysical Journal, 2000, Volume 541, Issue 2, pp. L71-L74 | en |
| dc.identifier.issn | 0004-637X | |
| dc.identifier.issn | 1538-4357(Online) | |
| dc.identifier.uri | http://hdl.handle.net/2289/1485 | |
| dc.language.iso | en | en |
| dc.publisher | The University of Chicago Press for the American Astronomical Society | en |
| dc.relation.uri | http://dx.doi.org/10.1086/312897 | en |
| dc.rights | (2000) by the American Astronomical Society. | en |
| dc.subject | Equation of State, | en |
| dc.subject | Relativity, | en |
| dc.subject | Stars: Neutron | en |
| dc.title | Rapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matter | en |
| dc.type | Article | en |