The Gamma Ray Burst section of the White Paper on the Status and Future of Very High Energy Gamma Ray Astronomy: A Brief Preliminary Report

A. D. Falcone, D. A. Williams, M. G. Baring, R. Blandford, V. Connaughton, P. Coppi, C. Dermer, B. Dingus, C. Fryer, N. Gehrels, J. Granot, D. Horan, J. I. Katz, K. Kuehn, P. Mészáros, J. Norris, P. Saz Parkinson, A. Pe'Er, E. Ramirez-Ruiz, S. RazzaqueX. Wang, B. Zhang

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

This is a short report on the preliminary findings of the gamma ray burst (GRB) working group for the white paper on the status and future of very high energy (VHE;>50GeV) gamma-ray astronomy. The white paper discusses the status of past and current attempts to observe GRBs at GeV-TeV energies, including a handful of low-significance, possible detections. The white paper concentrates on the potential of future ground-based gamma-ray experiments to observe the highest energy emission ever recorded for GRBs, particularly for those that are nearby and have high Lorentz factors in the GRB jet. It is clear that the detection of VHE emission would have strong implications for GRB models, as well as cosmic ray origin. In particular, the extended emission phase (including both afterglow emission and possible flaring) of nearby long GRBs could provide the best possibility for detection. The difficult-to-obtain observations during the prompt phase of nearby long GRBs and short GRBs could also provide particularly strong constraints on the opacity and bulk Lorentz factors surrounding the acceleration site. The synergy with upcoming and existing observatories will, of course, be critical for both identification of GRBs and for multiwavelength/multimessenger studies.

Original languageEnglish (US)
Title of host publicationGamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference
Pages611-615
Number of pages5
DOIs
StatePublished - Dec 1 2008
EventSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 - Santa Fe, NM, United States
Duration: Nov 5 2007Nov 9 2007

Publication series

NameAIP Conference Proceedings
Volume1000
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007
CountryUnited States
CitySanta Fe, NM
Period11/5/0711/9/07

Fingerprint

gamma ray astronomy
gamma ray bursts
energy
opacity
afterglows
cosmic rays
observatories
gamma rays

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Falcone, A. D., Williams, D. A., Baring, M. G., Blandford, R., Connaughton, V., Coppi, P., ... Zhang, B. (2008). The Gamma Ray Burst section of the White Paper on the Status and Future of Very High Energy Gamma Ray Astronomy: A Brief Preliminary Report. In Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference (pp. 611-615). (AIP Conference Proceedings; Vol. 1000). https://doi.org/10.1063/1.2943545
Falcone, A. D. ; Williams, D. A. ; Baring, M. G. ; Blandford, R. ; Connaughton, V. ; Coppi, P. ; Dermer, C. ; Dingus, B. ; Fryer, C. ; Gehrels, N. ; Granot, J. ; Horan, D. ; Katz, J. I. ; Kuehn, K. ; Mészáros, P. ; Norris, J. ; Parkinson, P. Saz ; Pe'Er, A. ; Ramirez-Ruiz, E. ; Razzaque, S. ; Wang, X. ; Zhang, B. / The Gamma Ray Burst section of the White Paper on the Status and Future of Very High Energy Gamma Ray Astronomy : A Brief Preliminary Report. Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. 2008. pp. 611-615 (AIP Conference Proceedings).
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abstract = "This is a short report on the preliminary findings of the gamma ray burst (GRB) working group for the white paper on the status and future of very high energy (VHE;>50GeV) gamma-ray astronomy. The white paper discusses the status of past and current attempts to observe GRBs at GeV-TeV energies, including a handful of low-significance, possible detections. The white paper concentrates on the potential of future ground-based gamma-ray experiments to observe the highest energy emission ever recorded for GRBs, particularly for those that are nearby and have high Lorentz factors in the GRB jet. It is clear that the detection of VHE emission would have strong implications for GRB models, as well as cosmic ray origin. In particular, the extended emission phase (including both afterglow emission and possible flaring) of nearby long GRBs could provide the best possibility for detection. The difficult-to-obtain observations during the prompt phase of nearby long GRBs and short GRBs could also provide particularly strong constraints on the opacity and bulk Lorentz factors surrounding the acceleration site. The synergy with upcoming and existing observatories will, of course, be critical for both identification of GRBs and for multiwavelength/multimessenger studies.",
author = "Falcone, {A. D.} and Williams, {D. A.} and Baring, {M. G.} and R. Blandford and V. Connaughton and P. Coppi and C. Dermer and B. Dingus and C. Fryer and N. Gehrels and J. Granot and D. Horan and Katz, {J. I.} and K. Kuehn and P. M{\'e}sz{\'a}ros and J. Norris and Parkinson, {P. Saz} and A. Pe'Er and E. Ramirez-Ruiz and S. Razzaque and X. Wang and B. Zhang",
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Falcone, AD, Williams, DA, Baring, MG, Blandford, R, Connaughton, V, Coppi, P, Dermer, C, Dingus, B, Fryer, C, Gehrels, N, Granot, J, Horan, D, Katz, JI, Kuehn, K, Mészáros, P, Norris, J, Parkinson, PS, Pe'Er, A, Ramirez-Ruiz, E, Razzaque, S, Wang, X & Zhang, B 2008, The Gamma Ray Burst section of the White Paper on the Status and Future of Very High Energy Gamma Ray Astronomy: A Brief Preliminary Report. in Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. AIP Conference Proceedings, vol. 1000, pp. 611-615, Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007, Santa Fe, NM, United States, 11/5/07. https://doi.org/10.1063/1.2943545

The Gamma Ray Burst section of the White Paper on the Status and Future of Very High Energy Gamma Ray Astronomy : A Brief Preliminary Report. / Falcone, A. D.; Williams, D. A.; Baring, M. G.; Blandford, R.; Connaughton, V.; Coppi, P.; Dermer, C.; Dingus, B.; Fryer, C.; Gehrels, N.; Granot, J.; Horan, D.; Katz, J. I.; Kuehn, K.; Mészáros, P.; Norris, J.; Parkinson, P. Saz; Pe'Er, A.; Ramirez-Ruiz, E.; Razzaque, S.; Wang, X.; Zhang, B.

Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. 2008. p. 611-615 (AIP Conference Proceedings; Vol. 1000).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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T1 - The Gamma Ray Burst section of the White Paper on the Status and Future of Very High Energy Gamma Ray Astronomy

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AU - Falcone, A. D.

AU - Williams, D. A.

AU - Baring, M. G.

AU - Blandford, R.

AU - Connaughton, V.

AU - Coppi, P.

AU - Dermer, C.

AU - Dingus, B.

AU - Fryer, C.

AU - Gehrels, N.

AU - Granot, J.

AU - Horan, D.

AU - Katz, J. I.

AU - Kuehn, K.

AU - Mészáros, P.

AU - Norris, J.

AU - Parkinson, P. Saz

AU - Pe'Er, A.

AU - Ramirez-Ruiz, E.

AU - Razzaque, S.

AU - Wang, X.

AU - Zhang, B.

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AB - This is a short report on the preliminary findings of the gamma ray burst (GRB) working group for the white paper on the status and future of very high energy (VHE;>50GeV) gamma-ray astronomy. The white paper discusses the status of past and current attempts to observe GRBs at GeV-TeV energies, including a handful of low-significance, possible detections. The white paper concentrates on the potential of future ground-based gamma-ray experiments to observe the highest energy emission ever recorded for GRBs, particularly for those that are nearby and have high Lorentz factors in the GRB jet. It is clear that the detection of VHE emission would have strong implications for GRB models, as well as cosmic ray origin. In particular, the extended emission phase (including both afterglow emission and possible flaring) of nearby long GRBs could provide the best possibility for detection. The difficult-to-obtain observations during the prompt phase of nearby long GRBs and short GRBs could also provide particularly strong constraints on the opacity and bulk Lorentz factors surrounding the acceleration site. The synergy with upcoming and existing observatories will, of course, be critical for both identification of GRBs and for multiwavelength/multimessenger studies.

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Falcone AD, Williams DA, Baring MG, Blandford R, Connaughton V, Coppi P et al. The Gamma Ray Burst section of the White Paper on the Status and Future of Very High Energy Gamma Ray Astronomy: A Brief Preliminary Report. In Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. 2008. p. 611-615. (AIP Conference Proceedings). https://doi.org/10.1063/1.2943545