Short Duration Gamma-Ray Bursts and Their Outflows in Light of GW170817
The detection of GW170817, it’s extensive multi-wavelength follow-up campaign, and the large amount of theoretical development and interpretation that followed, have resulted in a significant step forward in the understanding of the binary neutron star merger phenomenon as a whole. One of its aspect...
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| Published in | Frontiers in astronomy and space sciences Vol. 7 |
|---|---|
| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
Frontiers Media S.A
09.11.2020
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| Subjects | |
| Online Access | Get full text |
| ISSN | 2296-987X 2296-987X |
| DOI | 10.3389/fspas.2020.578849 |
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| Abstract | The detection of GW170817, it’s extensive multi-wavelength follow-up campaign, and the large amount of theoretical development and interpretation that followed, have resulted in a significant step forward in the understanding of the binary neutron star merger phenomenon as a whole. One of its aspects is seeing the merger as a progenitor of short gamma-ray bursts (SGRB), which will be the subject of this review. On the one hand, GW170817 observations have confirmed some theoretical expectations, exemplified by the confirmation that binary neutron star mergers are the progenitors of SGRBs. In addition, the multimessenger nature of GW170817 has allowed for gathering of unprecedented data, such as the trigger time of the merger, the delay with which the gamma-ray photons were detected, and the brightening afterglow of an off-axis event. All together, the incomparable richness of the data from GW170817 has allowed us to paint a fairly detailed picture of at least one SGRB. I will detail what we learned, what new questions have arisen, and the perspectives for answering them when a sample of GW170817-comparable events have been studied. |
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| AbstractList | The detection of GW170817, it’s extensive multi-wavelength follow-up campaign, and the large amount of theoretical development and interpretation that followed, have resulted in a significant step forward in the understanding of the binary neutron star merger phenomenon as a whole. One of its aspects is seeing the merger as a progenitor of short gamma-ray bursts (SGRB), which will be the subject of this review. On the one hand, GW170817 observations have confirmed some theoretical expectations, exemplified by the confirmation that binary neutron star mergers are the progenitors of SGRBs. In addition, the multimessenger nature of GW170817 has allowed for gathering of unprecedented data, such as the trigger time of the merger, the delay with which the gamma-ray photons were detected, and the brightening afterglow of an off-axis event. All together, the incomparable richness of the data from GW170817 has allowed us to paint a fairly detailed picture of at least one SGRB. I will detail what we learned, what new questions have arisen, and the perspectives for answering them when a sample of GW170817-comparable events have been studied. |
| Author | Lazzati, Davide |
| Author_xml | – sequence: 1 givenname: Davide surname: Lazzati fullname: Lazzati, Davide |
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| CitedBy_id | crossref_primary_10_3390_universe9060279 crossref_primary_10_3389_fspas_2024_1386748 crossref_primary_10_3389_fspas_2024_1384488 crossref_primary_10_4236_ijaa_2023_133012 crossref_primary_10_3847_1538_4357_acd114 crossref_primary_10_1103_PhysRevLett_128_211101 crossref_primary_10_1088_1361_6382_ad7b99 crossref_primary_10_3390_universe10010005 crossref_primary_10_1140_epjp_s13360_020_00911_w crossref_primary_10_4236_ijaa_2024_142008 |
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| Title | Short Duration Gamma-Ray Bursts and Their Outflows in Light of GW170817 |
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