FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2037141034> ?p ?o ?g. }

• W2037141034 endingPage "30" @default.
• W2037141034 startingPage "25" @default.
• W2037141034 abstract "We study the quantum hadrodynamic (QHD) equation of state for neutron stars (with and without including hyperons) in the presence of strong magnetic fields. The calculated adiabatic index for magnetized neutron stars based on the QHD model exhibit rapid changes with density. This may provide some insight into the mechanism of star-quakes and flares in magnetars. We also investigate the strong magnetic field effects on the moments of inertia of neutron stars. The change of the moments of inertia associated with emitted magnetic flares is shown to match well with observed glitches in some magnetars. In our QHD model, the deduced masses and radii of neutron stars without hyperons are consistent with recent observations of high mass neutron stars, while those with hyperons turn out to be less than the recent high mass neutron star." @default.
• W2037141034 created "2016-06-24" @default.
• W2037141034 creator A5001693763 @default.
• W2037141034 creator A5014648014 @default.
• W2037141034 creator A5022476446 @default.
• W2037141034 creator A5025870780 @default.
• W2037141034 creator A5040680249 @default.
• W2037141034 date "2012-10-01" @default.
• W2037141034 modified "2023-10-04" @default.
• W2037141034 title "QHD description of the instability in strongly magnetized neutron stars" @default.
• W2037141034 cites W1977799138 @default.
• W2037141034 cites W1980706409 @default.
• W2037141034 cites W1985166842 @default.
• W2037141034 cites W1986515303 @default.
• W2037141034 cites W1997366329 @default.
• W2037141034 cites W2002148893 @default.
• W2037141034 cites W2007951420 @default.
• W2037141034 cites W2011932751 @default.
• W2037141034 cites W2012921086 @default.
• W2037141034 cites W2018144815 @default.
• W2037141034 cites W2036194941 @default.
• W2037141034 cites W2039300833 @default.
• W2037141034 cites W2040366672 @default.
• W2037141034 cites W2040451033 @default.
• W2037141034 cites W2050515876 @default.
• W2037141034 cites W2061952754 @default.
• W2037141034 cites W2065363033 @default.
• W2037141034 cites W2070650982 @default.
• W2037141034 cites W2074514304 @default.
• W2037141034 cites W2075949556 @default.
• W2037141034 cites W2079476663 @default.
• W2037141034 cites W2092350553 @default.
• W2037141034 cites W2093685504 @default.
• W2037141034 cites W2127968784 @default.
• W2037141034 cites W2129328202 @default.
• W2037141034 cites W2153430156 @default.
• W2037141034 cites W3105228776 @default.
• W2037141034 cites W3105880739 @default.
• W2037141034 doi "https://doi.org/10.1016/j.astropartphys.2012.09.005" @default.
• W2037141034 hasPublicationYear "2012" @default.
• W2037141034 type Work @default.
• W2037141034 sameAs 2037141034 @default.
• W2037141034 citedByCount "21" @default.
• W2037141034 countsByYear W20371410342013 @default.
• W2037141034 countsByYear W20371410342014 @default.
• W2037141034 countsByYear W20371410342015 @default.
• W2037141034 countsByYear W20371410342016 @default.
• W2037141034 countsByYear W20371410342017 @default.
• W2037141034 countsByYear W20371410342018 @default.
• W2037141034 countsByYear W20371410342019 @default.
• W2037141034 countsByYear W20371410342020 @default.
• W2037141034 countsByYear W20371410342021 @default.
• W2037141034 countsByYear W20371410342022 @default.
• W2037141034 crossrefType "journal-article" @default.
• W2037141034 hasAuthorship W2037141034A5001693763 @default.
• W2037141034 hasAuthorship W2037141034A5014648014 @default.
• W2037141034 hasAuthorship W2037141034A5022476446 @default.
• W2037141034 hasAuthorship W2037141034A5025870780 @default.
• W2037141034 hasAuthorship W2037141034A5040680249 @default.
• W2037141034 hasConcept C10238366 @default.
• W2037141034 hasConcept C110363677 @default.
• W2037141034 hasConcept C115260700 @default.
• W2037141034 hasConcept C121332964 @default.
• W2037141034 hasConcept C150846664 @default.
• W2037141034 hasConcept C154153549 @default.
• W2037141034 hasConcept C185544564 @default.
• W2037141034 hasConcept C192887742 @default.
• W2037141034 hasConcept C207821765 @default.
• W2037141034 hasConcept C44383333 @default.
• W2037141034 hasConcept C44870925 @default.
• W2037141034 hasConcept C53810900 @default.
• W2037141034 hasConcept C62520636 @default.
• W2037141034 hasConcept C74650414 @default.
• W2037141034 hasConcept C86888617 @default.
• W2037141034 hasConceptScore W2037141034C10238366 @default.
• W2037141034 hasConceptScore W2037141034C110363677 @default.
• W2037141034 hasConceptScore W2037141034C115260700 @default.
• W2037141034 hasConceptScore W2037141034C121332964 @default.
• W2037141034 hasConceptScore W2037141034C150846664 @default.
• W2037141034 hasConceptScore W2037141034C154153549 @default.
• W2037141034 hasConceptScore W2037141034C185544564 @default.
• W2037141034 hasConceptScore W2037141034C192887742 @default.
• W2037141034 hasConceptScore W2037141034C207821765 @default.
• W2037141034 hasConceptScore W2037141034C44383333 @default.
• W2037141034 hasConceptScore W2037141034C44870925 @default.
• W2037141034 hasConceptScore W2037141034C53810900 @default.
• W2037141034 hasConceptScore W2037141034C62520636 @default.
• W2037141034 hasConceptScore W2037141034C74650414 @default.
• W2037141034 hasConceptScore W2037141034C86888617 @default.
• W2037141034 hasLocation W20371410341 @default.
• W2037141034 hasOpenAccess W2037141034 @default.
• W2037141034 hasPrimaryLocation W20371410341 @default.
• W2037141034 hasRelatedWork W2014334174 @default.
• W2037141034 hasRelatedWork W2048733473 @default.
• W2037141034 hasRelatedWork W2054848191 @default.
• W2037141034 hasRelatedWork W2077874591 @default.
• W2037141034 hasRelatedWork W2115126629 @default.
• W2037141034 hasRelatedWork W2754366346 @default.

• next