Matches in SemOpenAlex for { <https://semopenalex.org/work/W2904173743> ?p ?o ?g. }
- W2904173743 endingPage "L20" @default.
- W2904173743 startingPage "L20" @default.
- W2904173743 abstract "Binary neutron-star mergers have long been associated with short-duration gamma-ray bursts (GRBs). This connection was confirmed with the first coincident detection of gravitational waves together with electromagnetic radiation from GW170817. The basic paradigm for short-duration GRBs includes an ultra-relativistic jet, but the low-luminosity prompt emission together with follow-up radio and X-ray observations have hinted that this picture may be different in the case of GW170817. In particular, it has been proposed that large amounts of the magnetic energy that is amplified after the merger, can be released when the remnant collapses to a black hole, giving rise to a quasi-spherical explosion impacting on the merger ejecta. Through numerical simulations we investigate this scenario for a range of viewing angles, injected energies and matter densities at the time of the collapse. Depending on the magnitude of the energy injection and the remnant density, we find two types of outflows: one with a narrow relativistic core and one with a wide-angle, but mildly relativistic outflow. Furthermore, very wide outflows are possible, but require energy releases in excess of 1052 erg." @default.
- W2904173743 created "2018-12-22" @default.
- W2904173743 creator A5034731703 @default.
- W2904173743 creator A5065179394 @default.
- W2904173743 creator A5086810336 @default.
- W2904173743 date "2019-01-10" @default.
- W2904173743 modified "2023-10-16" @default.
- W2904173743 title "Magnetically Inspired Explosive Outflows from Neutron-star Mergers" @default.
- W2904173743 cites W1784683006 @default.
- W2904173743 cites W1964366747 @default.
- W2904173743 cites W1978222213 @default.
- W2904173743 cites W2021214134 @default.
- W2904173743 cites W2027299393 @default.
- W2904173743 cites W2029413546 @default.
- W2904173743 cites W2087010948 @default.
- W2904173743 cites W2092164081 @default.
- W2904173743 cites W2234367346 @default.
- W2904173743 cites W2294018305 @default.
- W2904173743 cites W2528621457 @default.
- W2904173743 cites W2617648374 @default.
- W2904173743 cites W2748834466 @default.
- W2904173743 cites W2760756222 @default.
- W2904173743 cites W2763306320 @default.
- W2904173743 cites W2763877873 @default.
- W2904173743 cites W2765081049 @default.
- W2904173743 cites W2765149688 @default.
- W2904173743 cites W2765540850 @default.
- W2904173743 cites W2766263568 @default.
- W2904173743 cites W2766627241 @default.
- W2904173743 cites W2767122548 @default.
- W2904173743 cites W2774047286 @default.
- W2904173743 cites W2775700050 @default.
- W2904173743 cites W2783155909 @default.
- W2904173743 cites W2783251299 @default.
- W2904173743 cites W2785044988 @default.
- W2904173743 cites W2791376686 @default.
- W2904173743 cites W2792441154 @default.
- W2904173743 cites W2802066336 @default.
- W2904173743 cites W2810137848 @default.
- W2904173743 cites W2888298899 @default.
- W2904173743 cites W2899454908 @default.
- W2904173743 cites W3098100524 @default.
- W2904173743 cites W3098712443 @default.
- W2904173743 cites W3099140217 @default.
- W2904173743 cites W3099446416 @default.
- W2904173743 cites W3100506102 @default.
- W2904173743 cites W3101369724 @default.
- W2904173743 cites W3101823224 @default.
- W2904173743 cites W3101955839 @default.
- W2904173743 cites W3102025782 @default.
- W2904173743 cites W3102643218 @default.
- W2904173743 cites W3102644718 @default.
- W2904173743 cites W3102814886 @default.
- W2904173743 cites W3102820987 @default.
- W2904173743 cites W3104042330 @default.
- W2904173743 cites W3104461298 @default.
- W2904173743 cites W3104653986 @default.
- W2904173743 cites W3104946210 @default.
- W2904173743 cites W3105562500 @default.
- W2904173743 cites W3105575002 @default.
- W2904173743 cites W3105735429 @default.
- W2904173743 cites W3106258256 @default.
- W2904173743 doi "https://doi.org/10.3847/2041-8213/aaf73a" @default.
- W2904173743 hasPublicationYear "2019" @default.
- W2904173743 type Work @default.
- W2904173743 sameAs 2904173743 @default.
- W2904173743 citedByCount "14" @default.
- W2904173743 countsByYear W29041737432019 @default.
- W2904173743 countsByYear W29041737432020 @default.
- W2904173743 countsByYear W29041737432021 @default.
- W2904173743 countsByYear W29041737432022 @default.
- W2904173743 crossrefType "journal-article" @default.
- W2904173743 hasAuthorship W2904173743A5034731703 @default.
- W2904173743 hasAuthorship W2904173743A5065179394 @default.
- W2904173743 hasAuthorship W2904173743A5086810336 @default.
- W2904173743 hasBestOaLocation W29041737431 @default.
- W2904173743 hasConcept C104954878 @default.
- W2904173743 hasConcept C118396296 @default.
- W2904173743 hasConcept C119947313 @default.
- W2904173743 hasConcept C121332964 @default.
- W2904173743 hasConcept C12287442 @default.
- W2904173743 hasConcept C127592171 @default.
- W2904173743 hasConcept C1276947 @default.
- W2904173743 hasConcept C145472833 @default.
- W2904173743 hasConcept C153294291 @default.
- W2904173743 hasConcept C153385146 @default.
- W2904173743 hasConcept C154238967 @default.
- W2904173743 hasConcept C17599544 @default.
- W2904173743 hasConcept C178790620 @default.
- W2904173743 hasConcept C185544564 @default.
- W2904173743 hasConcept C185592680 @default.
- W2904173743 hasConcept C190330329 @default.
- W2904173743 hasConcept C192887742 @default.
- W2904173743 hasConcept C31258907 @default.
- W2904173743 hasConcept C41008148 @default.
- W2904173743 hasConcept C43481613 @default.
- W2904173743 hasConcept C44870925 @default.
- W2904173743 hasConcept C50341732 @default.