Gamma ray Production From Parametric Resonance in Cold Neutron Stars

Details Gamma ray Production From Parametric Resonance in Cold Neutron Stars Gamma ray Production From Parametric Resonance in Cold Neutron Stars

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.238g&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

Coherent oscillations of the proton condensate within a neutron star (e.g. in an inspiralling binary) could generate, via parametric resonance, a large amount of energy in gamma ray photons. The energy spectrum of such resonant photons is very far from equilibrium. These photons may be released suddenly upon collision with the binary companion and give rise to a gamma ray burst with a power of order 1052 erg/s.

Affiliated with

Also associated with

No associations

Rating

Gamma ray Production From Parametric Resonance in Cold Neutron Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gamma ray Production From Parametric Resonance in Cold Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma ray Production From Parametric Resonance in Cold Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-768160