High Energy Physics Seminars

Radiation from Gamma Ray Bursts (GRBs) at high energies

by Dr. Reetanjali Maharana (Center for Theoretical Physics, Sichuan University, China)

Monday, December 24, 2018 from to (Asia/Kolkata)
at TIFR, Mumbai ( AG-69 )
Description
Gamma ray bursts are one of the most energetic astrophysical objects with an isotropic energy of 1053-55 ergs. They have long been speculated as possible acceleration sites for high energy gamma rays and neutrinos. We have calculated the neutrino flux from GRBs during their prompt as well afterglow phases. I will discuss the high energy neutrinos as a follow up of gravitational waves associated with short GRBs and hence could be an useful probe in understanding the baryon loading in GRBs. I will also discuss our results on observational evidence for presence of chocked short GRBs, from their duration distribution for gamma-ray emission and the future prospect associated with it.