Matches in SemOpenAlex for { <https://semopenalex.org/work/W2082394338> ?p ?o ?g. }
- W2082394338 endingPage "012031" @default.
- W2082394338 startingPage "012031" @default.
- W2082394338 abstract "As several large scale interferometers are beginning to take data at sensitivities where astrophysical sources are predicted, the direct detection of gravitational waves may well be imminent. This would open the gravitational-wave window to our Universe and should lead to a much improved understanding of the most violent processes imaginable; the formation of black holes and neutron stars following core collapse supernovae and the merger of compact objects at the end of binary inspiral. Among the best candidate sources for gravitational waves are the oscillations, but mainly the rotational instabilities of neutron stars which can emit quite strong gravitational wave signals via which one may reveal the details of their structure. Magnetars also are neutron stars with ultra strong magnetic field whose periodic flaring activity is associated with starquakes. They are also a potential source of gravitational waves while even the quasi-periodic oscillations (QPOs) observed in the electromagnetic spectrum can reveal the details of their structure." @default.
- W2082394338 created "2016-06-24" @default.
- W2082394338 creator A5041628571 @default.
- W2082394338 creator A5070455294 @default.
- W2082394338 creator A5085046045 @default.
- W2082394338 date "2010-04-01" @default.
- W2082394338 modified "2023-09-24" @default.
- W2082394338 title "Neutron star dynamics and gravitational waves" @default.
- W2082394338 cites W1487511162 @default.
- W2082394338 cites W1573788291 @default.
- W2082394338 cites W1964401096 @default.
- W2082394338 cites W1964418840 @default.
- W2082394338 cites W1965530791 @default.
- W2082394338 cites W1966348857 @default.
- W2082394338 cites W1969102272 @default.
- W2082394338 cites W1971937909 @default.
- W2082394338 cites W1972429852 @default.
- W2082394338 cites W1974092659 @default.
- W2082394338 cites W1977167299 @default.
- W2082394338 cites W1978976062 @default.
- W2082394338 cites W1983220245 @default.
- W2082394338 cites W1991011406 @default.
- W2082394338 cites W1996865449 @default.
- W2082394338 cites W2011992138 @default.
- W2082394338 cites W2013098163 @default.
- W2082394338 cites W2013277967 @default.
- W2082394338 cites W2023418770 @default.
- W2082394338 cites W2029327327 @default.
- W2082394338 cites W2031532699 @default.
- W2082394338 cites W2031662487 @default.
- W2082394338 cites W2033954606 @default.
- W2082394338 cites W2034175782 @default.
- W2082394338 cites W2036056653 @default.
- W2082394338 cites W2037677064 @default.
- W2082394338 cites W2039591145 @default.
- W2082394338 cites W2043487112 @default.
- W2082394338 cites W2045694681 @default.
- W2082394338 cites W2048361494 @default.
- W2082394338 cites W2052152392 @default.
- W2082394338 cites W2056543278 @default.
- W2082394338 cites W2060022640 @default.
- W2082394338 cites W2065799762 @default.
- W2082394338 cites W2066021209 @default.
- W2082394338 cites W2080081613 @default.
- W2082394338 cites W2088556439 @default.
- W2082394338 cites W2094188491 @default.
- W2082394338 cites W2099145118 @default.
- W2082394338 cites W2103412490 @default.
- W2082394338 cites W2105635519 @default.
- W2082394338 cites W2111626561 @default.
- W2082394338 cites W2114371620 @default.
- W2082394338 cites W2117109647 @default.
- W2082394338 cites W2121998732 @default.
- W2082394338 cites W2127102623 @default.
- W2082394338 cites W2138229400 @default.
- W2082394338 cites W2140634668 @default.
- W2082394338 cites W2164195010 @default.
- W2082394338 cites W2168835871 @default.
- W2082394338 cites W2985369886 @default.
- W2082394338 cites W3098562513 @default.
- W2082394338 cites W3099667402 @default.
- W2082394338 cites W3101162189 @default.
- W2082394338 cites W3101176631 @default.
- W2082394338 cites W3101857842 @default.
- W2082394338 cites W3103002496 @default.
- W2082394338 cites W3103204141 @default.
- W2082394338 cites W3104901150 @default.
- W2082394338 cites W3105268825 @default.
- W2082394338 cites W3106080439 @default.
- W2082394338 cites W3106200698 @default.
- W2082394338 cites W3121514859 @default.
- W2082394338 cites W3122068828 @default.
- W2082394338 cites W3125160660 @default.
- W2082394338 cites W4236201237 @default.
- W2082394338 cites W4240257189 @default.
- W2082394338 doi "https://doi.org/10.1088/1742-6596/222/1/012031" @default.
- W2082394338 hasPublicationYear "2010" @default.
- W2082394338 type Work @default.
- W2082394338 sameAs 2082394338 @default.
- W2082394338 citedByCount "2" @default.
- W2082394338 countsByYear W20823943382012 @default.
- W2082394338 crossrefType "journal-article" @default.
- W2082394338 hasAuthorship W2082394338A5041628571 @default.
- W2082394338 hasAuthorship W2082394338A5070455294 @default.
- W2082394338 hasAuthorship W2082394338A5085046045 @default.
- W2082394338 hasBestOaLocation W20823943381 @default.
- W2082394338 hasConcept C101053622 @default.
- W2082394338 hasConcept C110363677 @default.
- W2082394338 hasConcept C121332964 @default.
- W2082394338 hasConcept C127592171 @default.
- W2082394338 hasConcept C1276947 @default.
- W2082394338 hasConcept C18444321 @default.
- W2082394338 hasConcept C190330329 @default.
- W2082394338 hasConcept C192887742 @default.
- W2082394338 hasConcept C2780688901 @default.
- W2082394338 hasConcept C44870925 @default.
- W2082394338 hasConcept C86888617 @default.
- W2082394338 hasConceptScore W2082394338C101053622 @default.