| dc.contributor.author | Banerjee, Shibaji | |
| dc.contributor.author | Ghosh, Sanjay Kumar | |
| dc.contributor.author | Raha, Sibaji | |
| dc.date.accessioned | 2012-10-18T11:01:32Z | |
| dc.date.available | 2012-10-18T11:01:32Z | |
| dc.date.issued | 2000-01 | |
| dc.identifier | FOR ACCESS PROBLEM CONTACT LIBRARIAN, BOSE INSTITUTE | en_US |
| dc.identifier.citation | Banerjee S, Ghosh SK and Raha S. (2000) The Chandrasekhar limit for quark stars, Journal of Physics G26, L1 - L4 | en_US |
| dc.identifier.uri | http://iopscience.iop.org/0954-3899/26/1/101/ | |
| dc.description | doi:10.1088/0954-3899/26/1/101 | en_US |
| dc.description.abstract | The Chandrasekhar limit for quark stars is evaluated from simple energy balance
relations, as proposed by Landau for white dwarfs or neutron stars. It has been found that the limit
for quark stars depends on, in addition to the fundamental constants, the bag constant. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | IOP Publishing | en_US |
| dc.subject | Chandrasekhar limit | en_US |
| dc.subject | quark stars | en_US |
| dc.title | The Chandrasekhar limit for quark stars | en_US |
| dc.title.alternative | Journal of Physics G | en_US |
| dc.type | Article | en_US |
