Matches in SemOpenAlex for { <https://semopenalex.org/work/W3199760176> ?p ?o ?g. }
Showing items 1 to 100 of
100
with 100 items per page.
- W3199760176 abstract "It is commonly believed that neutron stars exceeding the maximum mass limit for stability could be formed in the aftermath of binary neutron star mergers, enjoying a short life of metastability before losing centrifugal support and collapsing to a black hole. It is suggested here that a similar scenario could take place when the remnant's excess mass is supported by an ultra-strong $(gtrsim 10^{17},mbox{G})$ magnetic field that could be generated during, and shortly after, coalescence. We show that such 'magnetically supramassive' neutron stars could stave off collapse and survive for a few years before their magnetic energy is sufficiently dissipated due to ambipolar diffusion. In addition, we speculate on multi-messenger signatures of such objects and discuss the robustness of our results against limitations placed by neutron superfluidity and magneto-thermal evolution." @default.
- W3199760176 created "2021-09-27" @default.
- W3199760176 creator A5078390614 @default.
- W3199760176 creator A5089259984 @default.
- W3199760176 date "2022-03-23" @default.
- W3199760176 modified "2023-10-05" @default.
- W3199760176 title "Magnetically supramassive neutron stars" @default.
- W3199760176 cites W1784683006 @default.
- W3199760176 cites W1967825921 @default.
- W3199760176 cites W1973052444 @default.
- W3199760176 cites W1987757367 @default.
- W3199760176 cites W1999246800 @default.
- W3199760176 cites W2039300833 @default.
- W3199760176 cites W2041399476 @default.
- W3199760176 cites W2052310773 @default.
- W3199760176 cites W2061952754 @default.
- W3199760176 cites W2071946612 @default.
- W3199760176 cites W2091009532 @default.
- W3199760176 cites W2094188491 @default.
- W3199760176 cites W2111626561 @default.
- W3199760176 cites W2167184407 @default.
- W3199760176 cites W2208525224 @default.
- W3199760176 cites W2491175809 @default.
- W3199760176 cites W2498126760 @default.
- W3199760176 cites W2756219395 @default.
- W3199760176 cites W2766754978 @default.
- W3199760176 cites W2807309204 @default.
- W3199760176 cites W2964291139 @default.
- W3199760176 cites W3037896639 @default.
- W3199760176 cites W3100744095 @default.
- W3199760176 cites W3102278469 @default.
- W3199760176 cites W3102641179 @default.
- W3199760176 cites W3104052639 @default.
- W3199760176 cites W3122474491 @default.
- W3199760176 cites W3124243090 @default.
- W3199760176 cites W3124929351 @default.
- W3199760176 cites W3127156547 @default.
- W3199760176 cites W4244093240 @default.
- W3199760176 doi "https://doi.org/10.1103/physrevd.105.l061302" @default.
- W3199760176 hasPublicationYear "2022" @default.
- W3199760176 type Work @default.
- W3199760176 sameAs 3199760176 @default.
- W3199760176 citedByCount "5" @default.
- W3199760176 countsByYear W31997601762022 @default.
- W3199760176 countsByYear W31997601762023 @default.
- W3199760176 crossrefType "journal-article" @default.
- W3199760176 hasAuthorship W3199760176A5078390614 @default.
- W3199760176 hasAuthorship W3199760176A5089259984 @default.
- W3199760176 hasBestOaLocation W31997601762 @default.
- W3199760176 hasConcept C115260700 @default.
- W3199760176 hasConcept C121332964 @default.
- W3199760176 hasConcept C1276947 @default.
- W3199760176 hasConcept C149792144 @default.
- W3199760176 hasConcept C150846664 @default.
- W3199760176 hasConcept C152568617 @default.
- W3199760176 hasConcept C185544564 @default.
- W3199760176 hasConcept C192887742 @default.
- W3199760176 hasConcept C25536358 @default.
- W3199760176 hasConcept C25621703 @default.
- W3199760176 hasConcept C26873012 @default.
- W3199760176 hasConcept C44870925 @default.
- W3199760176 hasConcept C62520636 @default.
- W3199760176 hasConcept C82706917 @default.
- W3199760176 hasConcept C89464430 @default.
- W3199760176 hasConceptScore W3199760176C115260700 @default.
- W3199760176 hasConceptScore W3199760176C121332964 @default.
- W3199760176 hasConceptScore W3199760176C1276947 @default.
- W3199760176 hasConceptScore W3199760176C149792144 @default.
- W3199760176 hasConceptScore W3199760176C150846664 @default.
- W3199760176 hasConceptScore W3199760176C152568617 @default.
- W3199760176 hasConceptScore W3199760176C185544564 @default.
- W3199760176 hasConceptScore W3199760176C192887742 @default.
- W3199760176 hasConceptScore W3199760176C25536358 @default.
- W3199760176 hasConceptScore W3199760176C25621703 @default.
- W3199760176 hasConceptScore W3199760176C26873012 @default.
- W3199760176 hasConceptScore W3199760176C44870925 @default.
- W3199760176 hasConceptScore W3199760176C62520636 @default.
- W3199760176 hasConceptScore W3199760176C82706917 @default.
- W3199760176 hasConceptScore W3199760176C89464430 @default.
- W3199760176 hasIssue "6" @default.
- W3199760176 hasLocation W31997601761 @default.
- W3199760176 hasLocation W31997601762 @default.
- W3199760176 hasLocation W31997601763 @default.
- W3199760176 hasOpenAccess W3199760176 @default.
- W3199760176 hasPrimaryLocation W31997601761 @default.
- W3199760176 hasRelatedWork W1529801410 @default.
- W3199760176 hasRelatedWork W1864702457 @default.
- W3199760176 hasRelatedWork W2014334174 @default.
- W3199760176 hasRelatedWork W2115126629 @default.
- W3199760176 hasRelatedWork W2139702176 @default.
- W3199760176 hasRelatedWork W2963621444 @default.
- W3199760176 hasRelatedWork W3084104036 @default.
- W3199760176 hasRelatedWork W3104025681 @default.
- W3199760176 hasRelatedWork W3104178734 @default.
- W3199760176 hasRelatedWork W3124441074 @default.
- W3199760176 hasVolume "105" @default.
- W3199760176 isParatext "false" @default.
- W3199760176 isRetracted "false" @default.
- W3199760176 magId "3199760176" @default.
- W3199760176 workType "article" @default.