FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2885403764> ?p ?o ?g. }

• W2885403764 endingPage "851" @default.
• W2885403764 startingPage "840" @default.
• W2885403764 abstract "The joint detection of gravitational waves (GWs) and γ-rays from a binary neutron star (NS) merger provided a unique view of off-axis gamma-ray bursts (GRBs) and an independent measurement of the NS merger rate. Comparing the observations of GRB170817 with those of the regular population of short GRBs (sGRBs), we show that an order unity fraction of NS mergers result in sGRB jets that breakout of the surrounding ejecta. We argue that the luminosity function of sGRBs, peaking at |${approx } 2times 10^{52}, mbox{erg s}^{-1}$|⁠, is likely an intrinsic property of the sGRB central engine and that sGRB jets are typically narrow with opening angles θ0 ≈ 0.1. We perform Monte Carlo simulations to examine models for the structure and efficiency of the prompt emission in off-axis sGRBs. We find that only a small fraction (∼0.01–0.1) of NS mergers detectable by LIGO/VIRGO in GWs is expected to be also detected in prompt γ-rays and that GW170817-like events are very rare. For an NS merger rate of ∼1500 Gpc−3 yr−1, as inferred from GW170817, we expect within the next decade up to ∼12 joint detections with off-axis GRBs for structured-jet models and just ∼1 for quasi-spherical cocoon models where γ-rays are the result of shock breakout. Given several joint detections and the rates of their discoveries, the different structure models can be distinguished. In addition the existence of a cocoon with a reservoir of thermal energy may be observed directly in the ultraviolet, given a sufficiently rapid localization of the GW source." @default.
• W2885403764 created "2018-08-22" @default.
• W2885403764 creator A5042045018 @default.
• W2885403764 creator A5065941159 @default.
• W2885403764 creator A5078054206 @default.
• W2885403764 creator A5083349832 @default.
• W2885403764 date "2018-11-15" @default.
• W2885403764 modified "2023-10-16" @default.
• W2885403764 title "A lesson from GW170817: most neutron star mergers result in tightly collimated successful GRB jets" @default.
• W2885403764 cites W1499693082 @default.
• W2885403764 cites W1501419355 @default.
• W2885403764 cites W1785695798 @default.
• W2885403764 cites W1968854473 @default.
• W2885403764 cites W1975498920 @default.
• W2885403764 cites W1977998389 @default.
• W2885403764 cites W1993926965 @default.
• W2885403764 cites W2000494005 @default.
• W2885403764 cites W2014304222 @default.
• W2885403764 cites W2019258526 @default.
• W2885403764 cites W2020377857 @default.
• W2885403764 cites W2023347320 @default.
• W2885403764 cites W2037505457 @default.
• W2885403764 cites W2042725851 @default.
• W2885403764 cites W2049211861 @default.
• W2885403764 cites W2051539854 @default.
• W2885403764 cites W2054131667 @default.
• W2885403764 cites W2060963248 @default.
• W2885403764 cites W2061699768 @default.
• W2885403764 cites W2070722652 @default.
• W2885403764 cites W2081587002 @default.
• W2885403764 cites W2087010948 @default.
• W2885403764 cites W2143470469 @default.
• W2885403764 cites W2165154060 @default.
• W2885403764 cites W2168770294 @default.
• W2885403764 cites W2195134359 @default.
• W2885403764 cites W2226366548 @default.
• W2885403764 cites W2242359428 @default.
• W2885403764 cites W2410454631 @default.
• W2885403764 cites W2440100992 @default.
• W2885403764 cites W2517731919 @default.
• W2885403764 cites W2528621457 @default.
• W2885403764 cites W2610582255 @default.
• W2885403764 cites W2613466388 @default.
• W2885403764 cites W2624096832 @default.
• W2885403764 cites W2733741278 @default.
• W2885403764 cites W2748834466 @default.
• W2885403764 cites W2753129948 @default.
• W2885403764 cites W2765081049 @default.
• W2885403764 cites W2765149688 @default.
• W2885403764 cites W2765595587 @default.
• W2885403764 cites W2766140821 @default.
• W2885403764 cites W2766263568 @default.
• W2885403764 cites W2766627241 @default.
• W2885403764 cites W2766754978 @default.
• W2885403764 cites W2767047170 @default.
• W2885403764 cites W2767750257 @default.
• W2885403764 cites W2771824038 @default.
• W2885403764 cites W2774047286 @default.
• W2885403764 cites W2785044988 @default.
• W2885403764 cites W2786431263 @default.
• W2885403764 cites W2810137848 @default.
• W2885403764 cites W2963762503 @default.
• W2885403764 cites W3098985865 @default.
• W2885403764 cites W3099131260 @default.
• W2885403764 cites W3099186672 @default.
• W2885403764 cites W3099319082 @default.
• W2885403764 cites W3099724580 @default.
• W2885403764 cites W3100180434 @default.
• W2885403764 cites W3100506102 @default.
• W2885403764 cites W3100622788 @default.
• W2885403764 cites W3101043338 @default.
• W2885403764 cites W3101477063 @default.
• W2885403764 cites W3101522121 @default.
• W2885403764 cites W3101955293 @default.
• W2885403764 cites W3102192395 @default.
• W2885403764 cites W3102888176 @default.
• W2885403764 cites W3103322915 @default.
• W2885403764 cites W3104907073 @default.
• W2885403764 cites W3105001172 @default.
• W2885403764 cites W3105194328 @default.
• W2885403764 cites W3105939555 @default.
• W2885403764 cites W3106046884 @default.
• W2885403764 cites W3124479694 @default.
• W2885403764 doi "https://doi.org/10.1093/mnras/sty3093" @default.
• W2885403764 hasPublicationYear "2018" @default.
• W2885403764 type Work @default.
• W2885403764 sameAs 2885403764 @default.
• W2885403764 citedByCount "64" @default.
• W2885403764 countsByYear W28854037642018 @default.
• W2885403764 countsByYear W28854037642019 @default.
• W2885403764 countsByYear W28854037642020 @default.
• W2885403764 countsByYear W28854037642021 @default.
• W2885403764 countsByYear W28854037642022 @default.
• W2885403764 countsByYear W28854037642023 @default.
• W2885403764 crossrefType "journal-article" @default.
• W2885403764 hasAuthorship W2885403764A5042045018 @default.
• W2885403764 hasAuthorship W2885403764A5065941159 @default.
• W2885403764 hasAuthorship W2885403764A5078054206 @default.

• next