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Title:High Energy Emission from Gamma Ray Bursts
Authors:ID Yang, Lili, University of Nova Gorica (Author)
Files: This document has no files that are freely available to the public. This document may have a physical copy in the library of the organization, check the status via COBISS. Link is opened in a new window
Language:English
Work type:Not categorized
Typology:3.14 - Invited Lecture at Foreign University
Organization:UNG - University of Nova Gorica
Abstract:Gamma Ray Bursts (GRBs) are the most energetic explosions in the universe, and they have been proposed as the most promising candidate sources of ultra-high energy cosmic rays (UHECRs). As a result of interactions of UHECR within the host environment and during their propagation towards Earth, high energy neutrinos and photons are also expected from both prompt and afterglow emission. In this talk, I will review the standard theory of particle acceleration and production in a GRB fireball, and multi-wavelength and multi-messeger observations of GRB emission. I will present the prediction of PeV — EeV neutrino production and evidence of GeV gamma ray radiation, and the expected detection in IceCube, Pierre Auger Observatory and CTA (the next generation of Imaging Atmospheric Cherenkov Telescopes). The investigation of high-energy particles will provide insight into the nature and complicated mechanisms of GRBs.
Keywords:Gamma-Ray Bursts, high-energy emission, blastwave afterglow
Place of performance:University of Science and Technology, Hefei China
Year of performance:2016
PID:20.500.12556/RUNG-2834-423cb8d2-5d73-21fa-315c-559ce4b097f3 New window
COBISS.SI-ID:4594427 New window
NUK URN:URN:SI:UNG:REP:5NBCFVKF
Publication date in RUNG:06.12.2016
Views:5661
Downloads:0
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