Literature DB >> 22923573

Gamma-ray bursts.

Neil Gehrels1, Péter Mészáros.   

Abstract

Gamma-ray bursts (GRBs) are bright flashes of gamma rays coming from the cosmos. They occur roughly once per day, typically last for tens of seconds, and are the most luminous events in the universe. More than three decades after their discovery, and after pioneering advances from space and ground experiments, they still remain mysterious. The launch of the Swift and Fermi satellites in 2004 and 2008 brought in a trove of qualitatively new data. In this Review, we survey the interplay between these recent observations and the theoretical models of the prompt GRB emission and the subsequent afterglow.

Entities:  

Year:  2012        PMID: 22923573     DOI: 10.1126/science.1216793

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  4 in total

1.  Teraelectronvolt emission from the γ-ray burst GRB 190114C.

Authors: 
Journal:  Nature       Date:  2019-11-20       Impact factor: 49.962

2.  Observation of inverse Compton emission from a long γ-ray burst.

Authors:  P Veres; P N Bhat; M S Briggs; W H Cleveland; R Hamburg; C M Hui; B Mailyan; R D Preece; O J Roberts; A von Kienlin; C A Wilson-Hodge; D Kocevski; M Arimoto; D Tak; K Asano; M Axelsson; G Barbiellini; E Bissaldi; F Fana Dirirsa; R Gill; J Granot; J McEnery; N Omodei; S Razzaque; F Piron; J L Racusin; D J Thompson; S Campana; M G Bernardini; N P M Kuin; M H Siegel; S B Cenko; P O'Brien; M Capalbi; A Daì; M De Pasquale; J Gropp; N Klingler; J P Osborne; M Perri; R L C Starling; G Tagliaferri; A Tohuvavohu; A Ursi; M Tavani; M Cardillo; C Casentini; G Piano; Y Evangelista; F Verrecchia; C Pittori; F Lucarelli; A Bulgarelli; N Parmiggiani; G E Anderson; J P Anderson; G Bernardi; J Bolmer; M D Caballero-García; I M Carrasco; A Castellón; N Castro Segura; A J Castro-Tirado; S V Cherukuri; A M Cockeram; P D'Avanzo; A Di Dato; R Diretse; R P Fender; E Fernández-García; J P U Fynbo; A S Fruchter; J Greiner; M Gromadzki; K E Heintz; I Heywood; A J van der Horst; Y-D Hu; C Inserra; L Izzo; V Jaiswal; P Jakobsson; J Japelj; E Kankare; D A Kann; C Kouveliotou; S Klose; A J Levan; X Y Li; S Lotti; K Maguire; D B Malesani; I Manulis; M Marongiu; S Martin; A Melandri; M J Michałowski; J C A Miller-Jones; K Misra; A Moin; K P Mooley; S Nasri; M Nicholl; A Noschese; G Novara; S B Pandey; E Peretti; C J Pérez Del Pulgar; M A Pérez-Torres; D A Perley; L Piro; F Ragosta; L Resmi; R Ricci; A Rossi; R Sánchez-Ramírez; J Selsing; S Schulze; S J Smartt; I A Smith; V V Sokolov; J Stevens; N R Tanvir; C C Thöne; A Tiengo; E Tremou; E Troja; A de Ugarte Postigo; A F Valeev; S D Vergani; M Wieringa; P A Woudt; D Xu; O Yaron; D R Young
Journal:  Nature       Date:  2019-11-20       Impact factor: 49.962

3.  Burst intensification by singularity emitting radiation in multi-stream flows.

Authors:  A S Pirozhkov; T Zh Esirkepov; T A Pikuz; A Ya Faenov; K Ogura; Y Hayashi; H Kotaki; E N Ragozin; D Neely; H Kiriyama; J K Koga; Y Fukuda; A Sagisaka; M Nishikino; T Imazono; N Hasegawa; T Kawachi; P R Bolton; H Daido; Y Kato; K Kondo; S V Bulanov; M Kando
Journal:  Sci Rep       Date:  2017-12-21       Impact factor: 4.379

4.  Electron energization dynamics in interaction of self-generated magnetic vortices in upstream of collisionless electron/ion shocks.

Authors:  N Naseri; S G Bochkarev; V Y Bychenkov; V Khudik; G Shvets
Journal:  Sci Rep       Date:  2022-05-05       Impact factor: 4.996

  4 in total

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