Gamma-ray bursts as an instrument for testing cosmological models

Author(s):  
S.I. Shirokov ◽  
A.A. Raikov ◽  
Y.V. Baryshev ◽  
V.V. Sokolov ◽  
V.V. Vlasyuk
2016 ◽  
Vol 10 ◽  
pp. 33-43
Author(s):  
Alexander Bonilla Rivera ◽  
Jairo Ernesto Castillo Hernandez

2010 ◽  
Vol 411 (2) ◽  
pp. 1213-1222 ◽  
Author(s):  
Marek Demianski ◽  
Ester Piedipalumbo ◽  
Claudio Rubano

1996 ◽  
Vol 472 (1) ◽  
pp. 25-33 ◽  
Author(s):  
John M. Horack ◽  
Thomas M. Koshut ◽  
Robert S. Mallozzi ◽  
A. Gordon Emslie ◽  
Charles A. Meegan

1995 ◽  
Vol 231 (1-2) ◽  
pp. 377-388 ◽  
Author(s):  
Charles D. Dermer ◽  
Thomas J. Weiler

2020 ◽  
Vol 499 (1) ◽  
pp. 391-403 ◽  
Author(s):  
Narayan Khadka ◽  
Bharat Ratra

ABSTRACT We use measurements of the peak photon energy and bolometric fluence of 119 gamma-ray bursts (GRBs) extending over the redshift range of 0.3399 ≤ z ≤ 8.2 to simultaneously determine cosmological and Amati relation parameters in six different cosmological models. The resulting Amati relation parameters are almost identical in all six cosmological models, thus validating the use of the Amati relation in standardizing these GRBs. The GRB data cosmological parameter constraints are consistent with, but significantly less restrictive than, those obtained from a joint analysis of baryon acoustic oscillation and Hubble parameter measurements.


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