| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10725160 | Physics Letters B | 2006 | 5 Pages |
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.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Abhijit Bhattacharyya, Sanjay K. Ghosh, Sibaji Raha,