Matches in SemOpenAlex for { <https://semopenalex.org/work/W2098785268> ?p ?o ?g. }
- W2098785268 endingPage "3826" @default.
- W2098785268 startingPage "3813" @default.
- W2098785268 abstract "The observation of several neutron stars in the center of supernova remnants and with significantly lower values of the dipolar magnetic field than the average radio-pulsar population has motivated a lively debate about their formation and origin, with controversial interpretations. A possible explanation requires the slow rotation of the proto-neutron star at birth, which is unable to amplify its magnetic field to typical pulsar levels. An alternative possibility, the hidden magnetic field scenario, considers the accretion of the fallback of the supernova debris onto the neutron star as responsible for the submergence (or screening) of the field and its apparently low value. In this paper we study under which conditions the magnetic field of a neutron star can be buried into the crust due to an accreting, conducting fluid. For this purpose, we consider a spherically symmetric calculation in general relativity to estimate the balance between the incoming accretion flow and the magnetosphere. Our study analyses several models with different specific entropy, composition, and neutron star masses. The main conclusion of our work is that typical magnetic fields of a few times 1e12 G can be buried by accreting only 1e-3 - 1e-2 solar mass, a relatively modest amount of mass. In view of this result, the Central Compact Object scenario should not be considered unusual, and we predict that anomalously weak magnetic fields should be common in very young (< few kyr) neutron stars." @default.
- W2098785268 created "2016-06-24" @default.
- W2098785268 creator A5044341859 @default.
- W2098785268 creator A5064921777 @default.
- W2098785268 creator A5081605513 @default.
- W2098785268 creator A5088679659 @default.
- W2098785268 date "2016-01-14" @default.
- W2098785268 modified "2023-10-16" @default.
- W2098785268 title "Are pulsars born with a hidden magnetic field?" @default.
- W2098785268 cites W1625816871 @default.
- W2098785268 cites W1667100988 @default.
- W2098785268 cites W1829911009 @default.
- W2098785268 cites W1963775863 @default.
- W2098785268 cites W1965342489 @default.
- W2098785268 cites W1974420904 @default.
- W2098785268 cites W1977931004 @default.
- W2098785268 cites W1981256261 @default.
- W2098785268 cites W1981500873 @default.
- W2098785268 cites W1987080308 @default.
- W2098785268 cites W1988659034 @default.
- W2098785268 cites W1999806090 @default.
- W2098785268 cites W2000300526 @default.
- W2098785268 cites W2001329313 @default.
- W2098785268 cites W2004991496 @default.
- W2098785268 cites W2006965421 @default.
- W2098785268 cites W2009623936 @default.
- W2098785268 cites W2011706353 @default.
- W2098785268 cites W2018144815 @default.
- W2098785268 cites W2018228837 @default.
- W2098785268 cites W2018335595 @default.
- W2098785268 cites W2019966268 @default.
- W2098785268 cites W2024184076 @default.
- W2098785268 cites W2026679688 @default.
- W2098785268 cites W2028508953 @default.
- W2098785268 cites W2030167880 @default.
- W2098785268 cites W2030679611 @default.
- W2098785268 cites W2038843023 @default.
- W2098785268 cites W2043035774 @default.
- W2098785268 cites W2044468098 @default.
- W2098785268 cites W2047798125 @default.
- W2098785268 cites W2056583859 @default.
- W2098785268 cites W2062439144 @default.
- W2098785268 cites W2063437365 @default.
- W2098785268 cites W2074056412 @default.
- W2098785268 cites W2078067446 @default.
- W2098785268 cites W2079355094 @default.
- W2098785268 cites W2079795649 @default.
- W2098785268 cites W2089676823 @default.
- W2098785268 cites W2092350553 @default.
- W2098785268 cites W2094188491 @default.
- W2098785268 cites W2094255511 @default.
- W2098785268 cites W2099692135 @default.
- W2098785268 cites W2102617153 @default.
- W2098785268 cites W2103740830 @default.
- W2098785268 cites W2118877522 @default.
- W2098785268 cites W2123867568 @default.
- W2098785268 cites W2141211263 @default.
- W2098785268 cites W2143081723 @default.
- W2098785268 cites W2146217020 @default.
- W2098785268 cites W2147725736 @default.
- W2098785268 cites W2159504674 @default.
- W2098785268 cites W2167572849 @default.
- W2098785268 cites W3099680123 @default.
- W2098785268 cites W3099949215 @default.
- W2098785268 cites W3100833260 @default.
- W2098785268 cites W3100839224 @default.
- W2098785268 cites W3101097082 @default.
- W2098785268 cites W3101116000 @default.
- W2098785268 cites W3101176631 @default.
- W2098785268 cites W3101192738 @default.
- W2098785268 cites W3101414103 @default.
- W2098785268 cites W3102385973 @default.
- W2098785268 cites W3103628182 @default.
- W2098785268 cites W3103869615 @default.
- W2098785268 cites W3105358496 @default.
- W2098785268 cites W3106158664 @default.
- W2098785268 cites W3106255486 @default.
- W2098785268 cites W3106530127 @default.
- W2098785268 cites W3125519009 @default.
- W2098785268 cites W4292930532 @default.
- W2098785268 cites W4299635444 @default.
- W2098785268 cites W4300490512 @default.
- W2098785268 cites W4301386907 @default.
- W2098785268 doi "https://doi.org/10.1093/mnras/stv2926" @default.
- W2098785268 hasPublicationYear "2016" @default.
- W2098785268 type Work @default.
- W2098785268 sameAs 2098785268 @default.
- W2098785268 citedByCount "27" @default.
- W2098785268 countsByYear W20987852682016 @default.
- W2098785268 countsByYear W20987852682017 @default.
- W2098785268 countsByYear W20987852682018 @default.
- W2098785268 countsByYear W20987852682019 @default.
- W2098785268 countsByYear W20987852682020 @default.
- W2098785268 countsByYear W20987852682021 @default.
- W2098785268 countsByYear W20987852682022 @default.
- W2098785268 countsByYear W20987852682023 @default.
- W2098785268 crossrefType "journal-article" @default.
- W2098785268 hasAuthorship W2098785268A5044341859 @default.