scholarly journals Clustering of LAT light curves: a clue to the origin of high-energy emission in gamma-ray bursts

2014 ◽  
Vol 443 (4) ◽  
pp. 3578-3585 ◽  
Author(s):  
L. Nava ◽  
G. Vianello ◽  
N. Omodei ◽  
G. Ghisellini ◽  
G. Ghirlanda ◽  
...  

Author(s):  
Joshua S. Bloom

This chapter discusses the definition, emission, and central engine of gamma-ray bursts (GRBs). Before the afterglow era, GRBs were essentially defined by observations of their high-energy emission. The landscape of such observations—the light curves and spectra of the events—exhibits at once great diversity and elements of commonality that bind different events together. GRBs are like fingerprints: no two are alike, but they share common properties. Those common elements provide strong constraints both on the nature of the “engine” that supplies the energy to the event and the physical processes that drive the emission we see. Since the 1990s, GRB monitors in space have observed more than one hundred GRBs. Since 2004, the NASA GRB satellite called Swift has been discovering GRBs at a rate of about two per week.



2012 ◽  
Vol 754 (2) ◽  
pp. 121 ◽  
Author(s):  
◽  
M. Ackermann ◽  
M. Ajello ◽  
L. Baldini ◽  
G. Barbiellini ◽  
...  


2012 ◽  
Vol 547 ◽  
pp. A95 ◽  
Author(s):  
F. Longo ◽  
E. Moretti ◽  
L. Nava ◽  
R. Desiante ◽  
M. Olivo ◽  
...  


2018 ◽  
Vol 27 (13) ◽  
pp. 1842003 ◽  
Author(s):  
Lara Nava

The number of gamma-ray bursts (GRBs) detected at high energies ([Formula: see text][Formula: see text]GeV) has seen a rapid increase over the last decade, thanks to observations from the Fermi-Large Area Telescope. The improved statistics and quality of data resulted in a better characterization of the high-energy emission properties and in stronger constraints on theoretical models. In spite of the many achievements and progresses, several observational properties still represent a challenge for theoretical models, revealing how our understanding is far from being complete. This paper reviews the main spectral and temporal properties of [Formula: see text][Formula: see text]GeV emission from GRBs and summarizes the most promising theoretical models proposed to interpret the observations. Since a boost for the understanding of GeV radiation might come from observations at even higher energies, the present status and future prospects for observations at very-high energies (above [Formula: see text][Formula: see text]100[Formula: see text]GeV) are also discussed. The improved sensitivity of upcoming facilities, coupled to theoretical predictions, supports the concrete possibility for future ground GRB detections in the high/very-high energy domain.



1985 ◽  
Vol 288 ◽  
pp. L37 ◽  
Author(s):  
S. M. Matz ◽  
D. J. Forrest ◽  
W. T. Vestrand ◽  
E. L. Chupp ◽  
G. H. Share ◽  
...  


2015 ◽  
Vol 45 (11) ◽  
pp. 119505-119505
Author(s):  
Bo ZHANG ◽  
XueFeng WU




2007 ◽  
Vol 671 (2) ◽  
pp. 1886-1895 ◽  
Author(s):  
Kohta Murase ◽  
Katsuaki Asano ◽  
Shigehiro Nagataki


Author(s):  
N. Omodei ◽  
G. Vianello ◽  
F. Piron ◽  
V. Vasileiou ◽  
S. Razzaque


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