Matches in SemOpenAlex for { <https://semopenalex.org/work/W2004332357> ?p ?o ?g. }
- W2004332357 endingPage "434" @default.
- W2004332357 startingPage "431" @default.
- W2004332357 abstract "The lack of isolated X-ray pulsars with spin periods longer than 12 s raises the question of where the population of evolved high-magnetic-field neutron stars has gone. Unlike canonical radiopulsars, X-ray pulsars are not subject to physical limits to the emission mechanism nor observational biases against the detection of sources with longer periods. Here we show that a highly resistive layer in the innermost part of the crust of neutron stars naturally limits the spin period to a maximum value of about 10–20 s. This highly resistive layer is expected if the inner crust is amorphous and heterogeneous in nuclear charge, possibly owing to the existence of a nuclear ‘pasta’ phase. Our findings suggest that the maximum period of isolated X-ray pulsars may be the first observational evidence for an amorphous inner crust, whose properties can be further constrained by future X-ray timing missions combined with more detailed models. A pulsar is a rotating neutron star that beams out electromagnetic waves. The absence of isolated X-ray pulsars with periods longer than 12 s could be a clue to the structural composition of a neutron star’s crust, as simulations show that an amorphous layer would prevent a pulsar from spinning down." @default.
- W2004332357 created "2016-06-24" @default.
- W2004332357 creator A5001612320 @default.
- W2004332357 creator A5034789352 @default.
- W2004332357 creator A5064921777 @default.
- W2004332357 date "2013-06-09" @default.
- W2004332357 modified "2023-10-16" @default.
- W2004332357 title "A highly resistive layer within the crust of X-ray pulsars limits their spin periods" @default.
- W2004332357 cites W1967825921 @default.
- W2004332357 cites W1992106524 @default.
- W2004332357 cites W1995411580 @default.
- W2004332357 cites W2011868702 @default.
- W2004332357 cites W2012921086 @default.
- W2004332357 cites W2015778997 @default.
- W2004332357 cites W2015851465 @default.
- W2004332357 cites W2020888000 @default.
- W2004332357 cites W2021318582 @default.
- W2004332357 cites W2022624204 @default.
- W2004332357 cites W2031762355 @default.
- W2004332357 cites W2050601393 @default.
- W2004332357 cites W2062480241 @default.
- W2004332357 cites W2063681063 @default.
- W2004332357 cites W2065234301 @default.
- W2004332357 cites W2070650982 @default.
- W2004332357 cites W2070838903 @default.
- W2004332357 cites W2074008137 @default.
- W2004332357 cites W2074166982 @default.
- W2004332357 cites W2076017426 @default.
- W2004332357 cites W2081762205 @default.
- W2004332357 cites W2092350553 @default.
- W2004332357 cites W2094414339 @default.
- W2004332357 cites W2102674778 @default.
- W2004332357 cites W2106045458 @default.
- W2004332357 cites W2146613440 @default.
- W2004332357 cites W2155388753 @default.
- W2004332357 cites W2159783297 @default.
- W2004332357 cites W3098680954 @default.
- W2004332357 cites W3099206884 @default.
- W2004332357 cites W3099680123 @default.
- W2004332357 cites W3101176631 @default.
- W2004332357 cites W3101312723 @default.
- W2004332357 cites W3102114083 @default.
- W2004332357 cites W3102418024 @default.
- W2004332357 cites W3102785608 @default.
- W2004332357 cites W3102876636 @default.
- W2004332357 cites W3105880739 @default.
- W2004332357 cites W3106257553 @default.
- W2004332357 cites W3121549928 @default.
- W2004332357 cites W3124671709 @default.
- W2004332357 doi "https://doi.org/10.1038/nphys2640" @default.
- W2004332357 hasPublicationYear "2013" @default.
- W2004332357 type Work @default.
- W2004332357 sameAs 2004332357 @default.
- W2004332357 citedByCount "118" @default.
- W2004332357 countsByYear W20043323572013 @default.
- W2004332357 countsByYear W20043323572014 @default.
- W2004332357 countsByYear W20043323572015 @default.
- W2004332357 countsByYear W20043323572016 @default.
- W2004332357 countsByYear W20043323572017 @default.
- W2004332357 countsByYear W20043323572018 @default.
- W2004332357 countsByYear W20043323572019 @default.
- W2004332357 countsByYear W20043323572020 @default.
- W2004332357 countsByYear W20043323572021 @default.
- W2004332357 countsByYear W20043323572022 @default.
- W2004332357 countsByYear W20043323572023 @default.
- W2004332357 crossrefType "journal-article" @default.
- W2004332357 hasAuthorship W2004332357A5001612320 @default.
- W2004332357 hasAuthorship W2004332357A5034789352 @default.
- W2004332357 hasAuthorship W2004332357A5064921777 @default.
- W2004332357 hasBestOaLocation W20043323572 @default.
- W2004332357 hasConcept C110363677 @default.
- W2004332357 hasConcept C121332964 @default.
- W2004332357 hasConcept C1276947 @default.
- W2004332357 hasConcept C144024400 @default.
- W2004332357 hasConcept C149923435 @default.
- W2004332357 hasConcept C192887742 @default.
- W2004332357 hasConcept C2776698055 @default.
- W2004332357 hasConcept C2908647359 @default.
- W2004332357 hasConcept C44870925 @default.
- W2004332357 hasConcept C8058405 @default.
- W2004332357 hasConcept C86888617 @default.
- W2004332357 hasConceptScore W2004332357C110363677 @default.
- W2004332357 hasConceptScore W2004332357C121332964 @default.
- W2004332357 hasConceptScore W2004332357C1276947 @default.
- W2004332357 hasConceptScore W2004332357C144024400 @default.
- W2004332357 hasConceptScore W2004332357C149923435 @default.
- W2004332357 hasConceptScore W2004332357C192887742 @default.
- W2004332357 hasConceptScore W2004332357C2776698055 @default.
- W2004332357 hasConceptScore W2004332357C2908647359 @default.
- W2004332357 hasConceptScore W2004332357C44870925 @default.
- W2004332357 hasConceptScore W2004332357C8058405 @default.
- W2004332357 hasConceptScore W2004332357C86888617 @default.
- W2004332357 hasIssue "7" @default.
- W2004332357 hasLocation W20043323571 @default.
- W2004332357 hasLocation W20043323572 @default.
- W2004332357 hasLocation W20043323573 @default.
- W2004332357 hasLocation W20043323574 @default.
- W2004332357 hasOpenAccess W2004332357 @default.