Effect of the brightest gamma-ray burst (GRB 221009A) on low energy gamma-ray counts at sea level
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arXiv
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| Autores principales: | , , , |
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| Formato: | Preprint |
| Publicado: |
2023
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| _version_ | 1866914715180990464 |
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| author | Thakur, Pranali Datar, Gauri Vichare, Geeta Chelliah, Selvaraj |
| author_facet | Thakur, Pranali Datar, Gauri Vichare, Geeta Chelliah, Selvaraj |
| contents | A gamma-ray burst, named GRB 221009A, occurred on 9 October 2022 and is the brightest ever observed GRB, whose frequency is now estimated as once in 10,000 years. This GRB was reported to be observed from many space missions, VLF receivers, and ground observations in optical and radio data. Additionally, a strikingly large number of very high energy (VHE) photons associated with this GRB were observed by the gamma-ray and cosmic ray observatory LHAASO. Though gamma rays of cosmic origin usually tend to be absorbed by the atmosphere, the high fluence of this GRB, along with the observation of more than 5000 VHE photons (0.5 to 18 TeV) by LHAASO from the ground, emphasises the need to explore other possible ground observations of this GRB.
The present paper examines the effect of this GRB using gamma-ray data in a low energy range (0.2-6) MeV obtained using NaI (Tl) detectors located at Tirunelveli (Geographic coordinates: 8.71°N, 77.76°E), India. With RA = 288.3° and Dec = 19.8°, the exceptionally bright fluence of this GRB was geographically centred on India. We report no significant change in the observations associated with GRB 221009A. We discuss the extent of attenuation of gamma-rays in the atmosphere that could explain the reported observations. Further, we investigate the likelihood of ground observation of gamma-rays ($<$10 MeV) for a much more intense hypothetical GRB, and estimate the parameters, such as distance, fluence, and isotropic energy of such a GRB. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2310_08244 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Effect of the brightest gamma-ray burst (GRB 221009A) on low energy gamma-ray counts at sea level Thakur, Pranali Datar, Gauri Vichare, Geeta Chelliah, Selvaraj High Energy Astrophysical Phenomena Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics A gamma-ray burst, named GRB 221009A, occurred on 9 October 2022 and is the brightest ever observed GRB, whose frequency is now estimated as once in 10,000 years. This GRB was reported to be observed from many space missions, VLF receivers, and ground observations in optical and radio data. Additionally, a strikingly large number of very high energy (VHE) photons associated with this GRB were observed by the gamma-ray and cosmic ray observatory LHAASO. Though gamma rays of cosmic origin usually tend to be absorbed by the atmosphere, the high fluence of this GRB, along with the observation of more than 5000 VHE photons (0.5 to 18 TeV) by LHAASO from the ground, emphasises the need to explore other possible ground observations of this GRB. The present paper examines the effect of this GRB using gamma-ray data in a low energy range (0.2-6) MeV obtained using NaI (Tl) detectors located at Tirunelveli (Geographic coordinates: 8.71°N, 77.76°E), India. With RA = 288.3° and Dec = 19.8°, the exceptionally bright fluence of this GRB was geographically centred on India. We report no significant change in the observations associated with GRB 221009A. We discuss the extent of attenuation of gamma-rays in the atmosphere that could explain the reported observations. Further, we investigate the likelihood of ground observation of gamma-rays ($<$10 MeV) for a much more intense hypothetical GRB, and estimate the parameters, such as distance, fluence, and isotropic energy of such a GRB. |
| title | Effect of the brightest gamma-ray burst (GRB 221009A) on low energy gamma-ray counts at sea level |
| topic | High Energy Astrophysical Phenomena Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2310.08244 |