| dc.contributor.author | Bhattacharyya, A. | |
| dc.contributor.author | Ghosh, Sanjay Kumar | |
| dc.contributor.author | Raha, Sibaji | |
| dc.date.accessioned | 2013-03-19T10:44:07Z | |
| dc.date.available | 2013-03-19T10:44:07Z | |
| dc.date.issued | 2006-04-13 | |
| dc.identifier | FOR ACCESS / DOWNLOAD PROBLEM -- PLEASE CONTACT LIBRARIAN, BOSE INSTITUTE, akc@bic.boseinst.ernet.in | en_US |
| dc.identifier.citation | Bhattacharyya A, Ghosh S K and Raha S (2006), QCD phase transition in rotating· neutron star, neutrino beaming and gamma-ray bursters, Phys. Lett. B635, 195. | en_US |
| dc.identifier.issn | 0370-2693 | |
| dc.identifier.uri | 1.Full Text Link -> | |
| dc.identifier.uri | http://ac.els-cdn.com/S0370269306002516/1-s2.0-S0370269306002516-main.pdf?_tid=79472e8a-9080-11e2-95c6-00000aab0f26&acdnat=1363689404_528acc88f007e8013e3865419263fb39 | en_US |
| dc.identifier.uri | ================================================= | en_US |
| dc.identifier.uri | 2. Scopus : Citation Link -> | en_US |
| dc.identifier.uri | http://www.scopus.com/record/display.url?eid=2-s2.0-33645088185&origin=resultslist&sort=plf-f&src=s&st1=phase+transition+in+rotating+neutron+star+neutrino+beaming+and+gamma-ray+bursters&st2=Bhattacharyya%2cA&sid=76C79A53CEA66A2F18D066CDF6DB744E.CnvicAmOODVwpVrjSeqQ%3a80&sot=b&sdt=b&sl=131&s=%28TITLE-ABS-KEY%28phase+transition+in+rotating+neutron+star+neutrino+beaming+and+gamma-ray+bursters%29+AND+AUTHOR-NAME%28Bhattacharyya%2cA%29%29&relpos=0&relpos=0&searchTerm=%28TITLE-ABS-KEY%28phase+transition+in+rotating+neutron+star+neutrino+beaming+and+gamma-ray+bursters%29+AND+AUTHOR-NAME%28Bhattacharyya%2CA%29%29 | en_US |
| dc.description | DOI: 10.1016/j.physletb.2006.02.065 | en_US |
| dc.description.abstract | We have studied the emission of neutrinos from a rotating hybrid star. We find that the emission is predominantly confined to a very small angle, provided the core of the star is in a mixed phase of quarks and hadrons and the size of such a mixed phase is small. Annihilation of neutrinos to produce gamma rays has been discussed. The estimated duration of the burst is found to be within the observational range. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | ELSEVIER SCIENCE BV | en_US |
| dc.subject | COLOR-DIELECTRIC MODEL | en_US |
| dc.subject | NUCLEAR-MATTER | en_US |
| dc.subject | QUARK MATTER | en_US |
| dc.subject | FIELD-THEORY | en_US |
| dc.title | QCD phase transition in rotating neutron star, neutrino beaming and gamma-ray bursters | en_US |
| dc.title.alternative | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics | en_US |
| dc.type | Article | en_US |
