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What determines the structure of short gamma-ray burst jets?
- Source :
- Urrutia, G, De Colle, F, Murguia-Berthier, A & Ramirez-Ruiz, E 2021, ' What determines the structure of short gamma-ray burst jets? ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 4363-4371 . https://doi.org/10.1093/mnras/stab723
- Publication Year :
- 2020
-
Abstract
- The discovery of GRB 170817A, the first unambiguous off-axis short gamma-ray burst arising from a neutron star merger, has challenged our understanding of the angular structure of relativistic jets. Studies of the jet propagation usually assume that the jet is ejected from the central engine with a top-hat structure and its final structure, which determines the observed light curve and spectra, is primarily regulated by the interaction with the nearby environment. However, jets are expected to be produced with a structure that is more complex than a simple top-hat, as shown by global accretion simulations. We present numerical simulations of short GRBs launched with a wide range of initial structures, durations and luminosities. We follow the jet interaction with the merger remnant wind and compute its final structure at distances $\gtrsim 10^{11}$~cm from the central engine. We show that the final jet structure, as well as the resulting afterglow emission, depend strongly on the initial structure of the jet, its luminosity and duration. While the initial structure at the jet is preserved for long-lasting SGRBs, it is strongly modified for jets barely making their way through the wind. This illustrates the importance of combining the results of global simulations with propagation studies in order to better predict the expected afterglow signatures from neutron star mergers. Structured jets provide a reasonable description of the GRB 170817A afterglow emission with an off-axis angle $\theta_{\rm obs} \approx 22.5^\circ$.<br />Comment: 9 pages, 7 Figures; Added discussion; Accepted for publication in MNRAS
- Subjects :
- DYNAMICS
Astrophysics::High Energy Astrophysical Phenomena
DIVERSITY
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
general [gamma-ray burst]
Approx
Spectral line
Astrophysical jet
COMPACT OBJECT MERGERS
Astrophysics::Galaxy Astrophysics
relativistic processes
High Energy Astrophysical Phenomena (astro-ph.HE)
Physics
RADIO
ADAPTIVE MESH REFINEMENT
NUMERICAL SIMULATIONS
numerical [methods]
Astronomy and Astrophysics
non-thermal [radiation mechanisms]
Light curve
Accretion (astrophysics)
Afterglow
jets [stars]
Neutron star
AFTERGLOW
OUTFLOWS
Space and Planetary Science
MERGING NEUTRON-STARS
RADIATION
High Energy Physics::Experiment
Gamma-ray burst
Astrophysics - High Energy Astrophysical Phenomena
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Urrutia, G, De Colle, F, Murguia-Berthier, A & Ramirez-Ruiz, E 2021, ' What determines the structure of short gamma-ray burst jets? ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 4363-4371 . https://doi.org/10.1093/mnras/stab723
- Accession number :
- edsair.doi.dedup.....991d5ea327f24d016dc033b0ccf80faf