2023ApJ...942L..30S


Query : 2023ApJ...942L..30S

2023ApJ...942L..30S - Astrophys. J., 942, L30 (2023/January-2)

Deciphering the ∼18 TeV Photons from GRB 221009A.

SAHU S., MEDINA-CARRILLO B., SANCHEZ-COLON G. and RAJPOOT S.

Abstract (from CDS):

On 2022 October 9, an extremely powerful gamma-ray burst, GRB 221009A, was detected by several instruments. Despite being obstructed by the Milky Way galaxy, its afterglow outburst outshone all other GRBs seen before. LHAASO detected several thousand very high energy photons extending up to 18 TeV. Detection of such energetic photons is unexpected due to the large opacity of the universe. It is possible that in the afterglow epoch, the intrinsic very high energy photon flux from the source might have increased manifolds, which could compensate for the attenuation by pair production with the extragalactic background light. We propose such a scenario and show that very high energy photons can be observed on the Earth from the interaction of very high energy protons with the seed synchrotron photons in the external forward shock region of the GRB jet.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Gamma-ray bursts - Particle astrophysics

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GRB 180720B gB 00 02 06.99 -02 55 07.8           ~ 215 0
2 SN 2019oyw SN* 02 58 10.510 -08 57 27.20           ~ 218 0
3 GRB 190114C gB 03 38 01.18 -26 56 47.8           ~ 343 0
4 GRB 221009A gB 19 13 03.85 +19 46 22.7           ~ 433 0
5 2HWC J1928+177 gam 19 28 25.0 +17 49 04           ~ 16 0
6 LHAASO J1929+1745 gam 19 29.0 +17 45           ~ 10 0

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