FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2011483031> ?p ?o ?g. }

• W2011483031 endingPage "891" @default.
• W2011483031 startingPage "865" @default.
• W2011483031 abstract "Glitches -- sudden increases in spin rate -- are observed in many pulsars. One mechanism advanced to explain glitches in the youngest pulsars is that they are caused by a starquake, a sudden rearrangement of the crust of the neutron star. Starquakes have the potential to excite some of the oscillation modes of the neutron star, which means that they are of interest as a source of gravitational waves. These oscillations could also have an impact on radio emission. In this paper we make upper estimates of the amplitude of the oscillations produced by a starquake, and the corresponding gravitational wave emission. We then develop a more detailed framework for calculating the oscillations excited by the starquake, using a toy model of a solid, incompressible star where all strain is lost instantaneously from the star at the glitch. For this toy model, we give plots of the amplitudes of the modes excited, as the shear modulus and rotation rate of the star are varied. We find that for our specific model, the largest excitation is generally of a mode similar to the $f$-mode of an incompressible fluid star, but that other modes of the star are excited to a significant degree over small parameter ranges of the rotation rate." @default.
• W2011483031 created "2016-06-24" @default.
• W2011483031 creator A5032550153 @default.
• W2011483031 creator A5071655875 @default.
• W2011483031 date "2014-11-13" @default.
• W2011483031 modified "2023-10-09" @default.
• W2011483031 title "Developing a model for neutron star oscillations following starquakes" @default.
• W2011483031 cites W1964733540 @default.
• W2011483031 cites W1965068220 @default.
• W2011483031 cites W1982340328 @default.
• W2011483031 cites W1984499552 @default.
• W2011483031 cites W2011591061 @default.
• W2011483031 cites W2017072609 @default.
• W2011483031 cites W2031924745 @default.
• W2011483031 cites W2032873331 @default.
• W2011483031 cites W2046622493 @default.
• W2011483031 cites W2050601393 @default.
• W2011483031 cites W2051459879 @default.
• W2011483031 cites W2064436382 @default.
• W2011483031 cites W2064814638 @default.
• W2011483031 cites W2066471981 @default.
• W2011483031 cites W2070559138 @default.
• W2011483031 cites W2074794433 @default.
• W2011483031 cites W2075558044 @default.
• W2011483031 cites W2075605610 @default.
• W2011483031 cites W2087051663 @default.
• W2011483031 cites W2087062135 @default.
• W2011483031 cites W2095345838 @default.
• W2011483031 cites W2121119114 @default.
• W2011483031 cites W2124050845 @default.
• W2011483031 cites W2126084610 @default.
• W2011483031 cites W2134227032 @default.
• W2011483031 cites W2498126760 @default.
• W2011483031 cites W3099344419 @default.
• W2011483031 cites W3103443493 @default.
• W2011483031 cites W3123045640 @default.
• W2011483031 cites W4254798263 @default.
• W2011483031 doi "https://doi.org/10.1093/mnras/stu2123" @default.
• W2011483031 hasPublicationYear "2014" @default.
• W2011483031 type Work @default.
• W2011483031 sameAs 2011483031 @default.
• W2011483031 citedByCount "20" @default.
• W2011483031 countsByYear W20114830312015 @default.
• W2011483031 countsByYear W20114830312017 @default.
• W2011483031 countsByYear W20114830312019 @default.
• W2011483031 countsByYear W20114830312020 @default.
• W2011483031 countsByYear W20114830312021 @default.
• W2011483031 countsByYear W20114830312022 @default.
• W2011483031 countsByYear W20114830312023 @default.
• W2011483031 crossrefType "journal-article" @default.
• W2011483031 hasAuthorship W2011483031A5032550153 @default.
• W2011483031 hasAuthorship W2011483031A5071655875 @default.
• W2011483031 hasBestOaLocation W20114830311 @default.
• W2011483031 hasConcept C110363677 @default.
• W2011483031 hasConcept C121332964 @default.
• W2011483031 hasConcept C150846664 @default.
• W2011483031 hasConcept C180205008 @default.
• W2011483031 hasConcept C181500209 @default.
• W2011483031 hasConcept C184779094 @default.
• W2011483031 hasConcept C190330329 @default.
• W2011483031 hasConcept C192887742 @default.
• W2011483031 hasConcept C2524010 @default.
• W2011483031 hasConcept C2778439541 @default.
• W2011483031 hasConcept C2780688901 @default.
• W2011483031 hasConcept C33923547 @default.
• W2011483031 hasConcept C44870925 @default.
• W2011483031 hasConcept C54355233 @default.
• W2011483031 hasConcept C62520636 @default.
• W2011483031 hasConcept C74050887 @default.
• W2011483031 hasConcept C86803240 @default.
• W2011483031 hasConcept C88991977 @default.
• W2011483031 hasConceptScore W2011483031C110363677 @default.
• W2011483031 hasConceptScore W2011483031C121332964 @default.
• W2011483031 hasConceptScore W2011483031C150846664 @default.
• W2011483031 hasConceptScore W2011483031C180205008 @default.
• W2011483031 hasConceptScore W2011483031C181500209 @default.
• W2011483031 hasConceptScore W2011483031C184779094 @default.
• W2011483031 hasConceptScore W2011483031C190330329 @default.
• W2011483031 hasConceptScore W2011483031C192887742 @default.
• W2011483031 hasConceptScore W2011483031C2524010 @default.
• W2011483031 hasConceptScore W2011483031C2778439541 @default.
• W2011483031 hasConceptScore W2011483031C2780688901 @default.
• W2011483031 hasConceptScore W2011483031C33923547 @default.
• W2011483031 hasConceptScore W2011483031C44870925 @default.
• W2011483031 hasConceptScore W2011483031C54355233 @default.
• W2011483031 hasConceptScore W2011483031C62520636 @default.
• W2011483031 hasConceptScore W2011483031C74050887 @default.
• W2011483031 hasConceptScore W2011483031C86803240 @default.
• W2011483031 hasConceptScore W2011483031C88991977 @default.
• W2011483031 hasIssue "1" @default.
• W2011483031 hasLocation W20114830311 @default.
• W2011483031 hasLocation W20114830312 @default.
• W2011483031 hasLocation W20114830313 @default.
• W2011483031 hasLocation W20114830314 @default.
• W2011483031 hasOpenAccess W2011483031 @default.
• W2011483031 hasPrimaryLocation W20114830311 @default.
• W2011483031 hasRelatedWork W1510622019 @default.
• W2011483031 hasRelatedWork W2014334174 @default.

• next