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- W2486134448 abstract "Pulsars are spinning extremely rapidly with periods as short as about $1.4$ milliseconds and delays of a few milliseconds per year at most, thus providing the most accurate clocks in the Universe. Nevertheless, sudden spin ups have been detected in some pulsars like the emblematic Vela pulsar. These abrupt changes in the pulsar's rotation period have long been thought to be the manifestation of a neutron superfluid permeating the inner crust of neutron stars. However, the neutron superfluid has been recently found to be so strongly coupled to the crust that it does not carry enough angular momentum to explain the Vela data. We explore the extent to which pulsar-timing observations can be reconciled with the standard glitch theory considering the lack of knowledge of the dense-matter equation of state." @default.
- W2486134448 created "2016-08-23" @default.
- W2486134448 creator A5003741507 @default.
- W2486134448 date "2016-07-20" @default.
- W2486134448 modified "2023-09-26" @default.
- W2486134448 title "Constraint on the internal structure of a neutron star from Vela pulsar glitches" @default.
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- W2486134448 doi "https://doi.org/10.48550/arxiv.1607.05943" @default.
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