Matches in SemOpenAlex for { <https://semopenalex.org/work/W2094528413> ?p ?o ?g. }
Showing items 1 to 87 of
87
with 100 items per page.
- W2094528413 abstract "Abstract Accretion of matter onto the surface of a white dwarf in a binary system can push it over the Chandrasekhar mass limit and may cause it to collapse into a naked or nearly naked neutron star without detectable optical emission 1–3 . Such optically quiet neutron star births should be accompanied by neutrino bursts which could be detected with underground neutrino detectors if the collapse took place in our own Galaxy or in very close nearby galaxies 4 . However, the frequency of such collapses is not known. It has been shown that the neutrino burst from gravitational core collapse produces, through neutrino-antineutrino annihilation outside the neutron star, an enormous burst of electron-positron pairs and gamma rays 5,6 . Here we show that if the mass surrounding the newly formed neutron star is less than about 3 × 10 −4 M ⊙ , the resultant gamma ray burst can be observed out to distances of at least 300 Mpc, and, consequently, that the observed rate of gamma ray bursts 7 limits the birthrate of such nearly naked neutron stars to about 1 per 10 3 years in galaxies similar to ours. Additional limits are set by the observed flux of 0.511 MeV Galactic annihilation radiation 8 and by the cosmic ray data. These rates are too small to contribute significantly to the birthrate of pulsars. They also imply that it is very unlikely that a neutrino burst unaccompanied by optical emission will be detected in the near future by underground detectors." @default.
- W2094528413 created "2016-06-24" @default.
- W2094528413 creator A5035893527 @default.
- W2094528413 creator A5046989946 @default.
- W2094528413 date "1992-07-01" @default.
- W2094528413 modified "2023-09-26" @default.
- W2094528413 title "Neutrinos from optically quiet births of neutron stars?" @default.
- W2094528413 cites W1964652668 @default.
- W2094528413 cites W1968854473 @default.
- W2094528413 cites W1973363208 @default.
- W2094528413 cites W1977197487 @default.
- W2094528413 cites W1981168904 @default.
- W2094528413 cites W1985996701 @default.
- W2094528413 cites W2018783042 @default.
- W2094528413 cites W2024297548 @default.
- W2094528413 cites W2033412613 @default.
- W2094528413 cites W2038099557 @default.
- W2094528413 cites W2042352559 @default.
- W2094528413 cites W2047171363 @default.
- W2094528413 cites W2081587002 @default.
- W2094528413 cites W2082017662 @default.
- W2094528413 cites W2087039667 @default.
- W2094528413 cites W2093903359 @default.
- W2094528413 cites W2097853078 @default.
- W2094528413 cites W2123530147 @default.
- W2094528413 cites W2171523116 @default.
- W2094528413 cites W3000312639 @default.
- W2094528413 cites W3011160802 @default.
- W2094528413 cites W3013252446 @default.
- W2094528413 cites W3040147003 @default.
- W2094528413 doi "https://doi.org/10.1016/0920-5632(92)90203-5" @default.
- W2094528413 hasPublicationYear "1992" @default.
- W2094528413 type Work @default.
- W2094528413 sameAs 2094528413 @default.
- W2094528413 citedByCount "0" @default.
- W2094528413 crossrefType "journal-article" @default.
- W2094528413 hasAuthorship W2094528413A5035893527 @default.
- W2094528413 hasAuthorship W2094528413A5046989946 @default.
- W2094528413 hasConcept C105500671 @default.
- W2094528413 hasConcept C121332964 @default.
- W2094528413 hasConcept C1276947 @default.
- W2094528413 hasConcept C150846664 @default.
- W2094528413 hasConcept C17599544 @default.
- W2094528413 hasConcept C185544564 @default.
- W2094528413 hasConcept C186453547 @default.
- W2094528413 hasConcept C192887742 @default.
- W2094528413 hasConcept C197445014 @default.
- W2094528413 hasConcept C44870925 @default.
- W2094528413 hasConcept C98444146 @default.
- W2094528413 hasConceptScore W2094528413C105500671 @default.
- W2094528413 hasConceptScore W2094528413C121332964 @default.
- W2094528413 hasConceptScore W2094528413C1276947 @default.
- W2094528413 hasConceptScore W2094528413C150846664 @default.
- W2094528413 hasConceptScore W2094528413C17599544 @default.
- W2094528413 hasConceptScore W2094528413C185544564 @default.
- W2094528413 hasConceptScore W2094528413C186453547 @default.
- W2094528413 hasConceptScore W2094528413C192887742 @default.
- W2094528413 hasConceptScore W2094528413C197445014 @default.
- W2094528413 hasConceptScore W2094528413C44870925 @default.
- W2094528413 hasConceptScore W2094528413C98444146 @default.
- W2094528413 hasLocation W20945284131 @default.
- W2094528413 hasOpenAccess W2094528413 @default.
- W2094528413 hasPrimaryLocation W20945284131 @default.
- W2094528413 hasRelatedWork W1549746228 @default.
- W2094528413 hasRelatedWork W1643007988 @default.
- W2094528413 hasRelatedWork W1662266746 @default.
- W2094528413 hasRelatedWork W1668927981 @default.
- W2094528413 hasRelatedWork W1673311387 @default.
- W2094528413 hasRelatedWork W2015948877 @default.
- W2094528413 hasRelatedWork W2061511586 @default.
- W2094528413 hasRelatedWork W2077007583 @default.
- W2094528413 hasRelatedWork W2084392953 @default.
- W2094528413 hasRelatedWork W2131521758 @default.
- W2094528413 hasRelatedWork W2577302008 @default.
- W2094528413 hasRelatedWork W2580597374 @default.
- W2094528413 hasRelatedWork W2763877873 @default.
- W2094528413 hasRelatedWork W3098531093 @default.
- W2094528413 hasRelatedWork W3098553117 @default.
- W2094528413 hasRelatedWork W3098859293 @default.
- W2094528413 hasRelatedWork W3100243237 @default.
- W2094528413 hasRelatedWork W3102121686 @default.
- W2094528413 hasRelatedWork W3102641179 @default.
- W2094528413 hasRelatedWork W3102820987 @default.
- W2094528413 isParatext "false" @default.
- W2094528413 isRetracted "false" @default.
- W2094528413 magId "2094528413" @default.
- W2094528413 workType "article" @default.