FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2073758422> ?p ?o ?g. }

• W2073758422 endingPage "155002" @default.
• W2073758422 startingPage "155002" @default.
• W2073758422 abstract "One of the key aspects in the comprehension of neutron star (NS) interiors is the identification of observables that may impose constraints on the equation of state (EoS). At present, limits are obtained mainly through the study of the mass–radius relationship, the maximum rotational frequency and the cooling behaviour. However, since gravitational wave (GW) observatories such as Advanced LIGO and Advanced VIRGO will open a new window of the observation of NSs in the very near future, identifying observables that may emerge from the analysis of the GW emission of NSs is crucial. To this end, we investigate non-radial oscillations of hadronic, hybrid and pure self-bound strange quark stars with maximum masses above the mass of the recently observed massive pulsars PSR J1614–2230 and PSR J0348–0432 with M ≈ 2 . For the hadronic EoS we employ different parametrizations of a relativistic mean-field model and the EoS of Akmal, Pandharipande and Ravenhall. For quark matter we use the Massachusetts Institute of Technology bag model, including the effect of strong interactions and colour superconductivity. We find that the first pressure mode for strange quark stars has a very different shape than for hadronic and hybrid stars. For strange quarks stars, the frequency of the mode is larger than ∼ 7 kHz and diverges at small stellar masses, but for hadronic and hybrid stars it is in the range ∼ 4–7 kHz. This allows an observational identification of strange stars even if extra information such as the mass, the radius or the gravitational redshift of the object is unavailable or uncertain. Also, we find as in previous works that the frequency of the g-mode associated with the quark–hadron discontinuity in a hybrid star is in the range 0.4–1 kHz for all masses. Thus, compact objects emitting GWs above 7 kHz should be interpreted as strange quark stars, and those emitting a signal within 0.4–1 kHz should be interpreted as hybrid stars." @default.
• W2073758422 created "2016-06-24" @default.
• W2073758422 creator A5018204427 @default.
• W2073758422 creator A5087758708 @default.
• W2073758422 date "2014-07-14" @default.
• W2073758422 modified "2023-10-18" @default.
• W2073758422 title "Discriminating hadronic and quark stars through gravitational waves of fluid pulsation modes" @default.
• W2073758422 cites W1765484090 @default.
• W2073758422 cites W1963681271 @default.
• W2073758422 cites W1968719016 @default.
• W2073758422 cites W1968879573 @default.
• W2073758422 cites W1969102272 @default.
• W2073758422 cites W1979654065 @default.
• W2073758422 cites W1983220245 @default.
• W2073758422 cites W1985178481 @default.
• W2073758422 cites W1988237471 @default.
• W2073758422 cites W2002443137 @default.
• W2073758422 cites W2006211107 @default.
• W2073758422 cites W2006350945 @default.
• W2073758422 cites W2006410710 @default.
• W2073758422 cites W2007779595 @default.
• W2073758422 cites W2011308300 @default.
• W2073758422 cites W2013166541 @default.
• W2073758422 cites W2022836438 @default.
• W2073758422 cites W2023379071 @default.
• W2073758422 cites W2023418770 @default.
• W2073758422 cites W2026081101 @default.
• W2073758422 cites W2033954606 @default.
• W2073758422 cites W2034175782 @default.
• W2073758422 cites W2049077024 @default.
• W2073758422 cites W2055309244 @default.
• W2073758422 cites W2064456825 @default.
• W2073758422 cites W2066484026 @default.
• W2073758422 cites W2076752847 @default.
• W2073758422 cites W2079707452 @default.
• W2073758422 cites W2082574025 @default.
• W2073758422 cites W2087182590 @default.
• W2073758422 cites W2088556439 @default.
• W2073758422 cites W2092350553 @default.
• W2073758422 cites W2094188491 @default.
• W2073758422 cites W2094626656 @default.
• W2073758422 cites W2110484638 @default.
• W2073758422 cites W2119818733 @default.
• W2073758422 cites W2121998732 @default.
• W2073758422 cites W2127956369 @default.
• W2073758422 cites W2135299713 @default.
• W2073758422 cites W2143095965 @default.
• W2073758422 cites W2167572849 @default.
• W2073758422 cites W2270205340 @default.
• W2073758422 cites W2292119714 @default.
• W2073758422 cites W3098547020 @default.
• W2073758422 cites W3102004927 @default.
• W2073758422 cites W3102142804 @default.
• W2073758422 cites W3103204141 @default.
• W2073758422 cites W3103648503 @default.
• W2073758422 cites W3105173305 @default.
• W2073758422 cites W3106065561 @default.
• W2073758422 cites W3122991543 @default.
• W2073758422 cites W3125255715 @default.
• W2073758422 cites W4242783256 @default.
• W2073758422 doi "https://doi.org/10.1088/0264-9381/31/15/155002" @default.
• W2073758422 hasPublicationYear "2014" @default.
• W2073758422 type Work @default.
• W2073758422 sameAs 2073758422 @default.
• W2073758422 citedByCount "35" @default.
• W2073758422 countsByYear W20737584222016 @default.
• W2073758422 countsByYear W20737584222017 @default.
• W2073758422 countsByYear W20737584222018 @default.
• W2073758422 countsByYear W20737584222019 @default.
• W2073758422 countsByYear W20737584222020 @default.
• W2073758422 countsByYear W20737584222021 @default.
• W2073758422 countsByYear W20737584222022 @default.
• W2073758422 countsByYear W20737584222023 @default.
• W2073758422 crossrefType "journal-article" @default.
• W2073758422 hasAuthorship W2073758422A5018204427 @default.
• W2073758422 hasAuthorship W2073758422A5087758708 @default.
• W2073758422 hasBestOaLocation W20737584222 @default.
• W2073758422 hasConcept C109214941 @default.
• W2073758422 hasConcept C110363677 @default.
• W2073758422 hasConcept C121332964 @default.
• W2073758422 hasConcept C1276947 @default.
• W2073758422 hasConcept C150846664 @default.
• W2073758422 hasConcept C153195114 @default.
• W2073758422 hasConcept C187783895 @default.
• W2073758422 hasConcept C190330329 @default.
• W2073758422 hasConcept C192887742 @default.
• W2073758422 hasConcept C196543993 @default.
• W2073758422 hasConcept C19694890 @default.
• W2073758422 hasConcept C2780688901 @default.
• W2073758422 hasConcept C28594881 @default.
• W2073758422 hasConcept C32848918 @default.
• W2073758422 hasConcept C44870925 @default.
• W2073758422 hasConcept C53810900 @default.
• W2073758422 hasConcept C62520636 @default.
• W2073758422 hasConcept C7602139 @default.
• W2073758422 hasConceptScore W2073758422C109214941 @default.
• W2073758422 hasConceptScore W2073758422C110363677 @default.
• W2073758422 hasConceptScore W2073758422C121332964 @default.

• next