2018
Can an off-axis gamma-ray burst jet in GW170817 explain all the electromagnetic counterparts?
Abstract: Gravitational waves from a merger of two neutron stars (NSs) were discovered for the first time in GW170817, together with diverse electromagnetic (EM) counterparts. To make constraints on a relativistic jet from the NS merger, we calculate the EM signals in (1) the short gamma-ray burst sGRB 170817A from an off-axis jet, (2) the optical-infrared macronova (or kilonova), especially the blue macronova, from a jetpowered cocoon, and (3) the X-ray and radio afterglows from the interaction between the jet and inte…
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Cited by 89 publications
(56 citation statements)
References 189 publications
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“…(iii) The jet head breakout velocity was constrained as 0.52 < v b /c < 1. This result is in agreement with Ioka & Nakamura (2018).…”
Section: Resultssupporting
confidence: 93%
“…(iii) The jet head breakout velocity was constrained as 0.52 < v b /c < 1. This result is in agreement with Ioka & Nakamura (2018).…”
Section: Resultssupporting
confidence: 93%
“…(iii) The jet head breakout velocity was constrained as 0.52 < v b /c < 1. This result is in agreement with Ioka & Nakamura (2018). This new constraint is more robust but in an overall agreement with previous studies (in agreement with Metzger et al 2018; partially in agreement with theoretical estimations based on numerical relativity simulations: Shibata et al 2017 andFujibayashi et al 2018).…”
Section: Gw170817supporting
confidence: 92%
“…For the top-hat jet, the luminosity declines rapidly beyond the jet core due to the de-beaming effect (we can see a similar behavior for E γ,iso in Kasliwal et al 2017;Granot et al 2017;Ioka & Nakamura 2018). Since a wing component may dominate the emission outside of the core (Matsumoto et al 2019a;Ioka & Nakamura 2019), the observed luminosity becomes brighter for top-hat with a Gaussian wing jets (black) and for Gaussian jets (blue).…”
Section: Off-axis and Jet-wing Event Ratessupporting
confidence: 54%
“…There have been numerous suggestions that dimmer and softer transients, for example low-luminosity GRBs (ll GRBs), are regular GRBs observed off-axis (e.g., Nakamura 1998;Eichler & Levinson 1999;Woosley et al 1999;Ioka & Nakamura 2001;Yamazaki et al 2003;Waxman 2004). Similar suggestions (Goldstein et al 2017;Murguia-Berthier et al 2017;Ioka & Nakamura 2018) were made shortly following the detection of the very weak short GRB (sGRB) 170817A (Abbott et al 2017b;Goldstein et al 2017;Savchenko et al 2017). However, these suggestions did not take into account the compactness problem (Kasliwal et al 2017).…”
Section: Introductionsupporting
confidence: 52%
