FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3201232423> ?p ?o ?g. }

• W3201232423 abstract "Due to improvements in the sensitivity of gravitational wave (GW) detectors, the detection of GWs originating from the fundamental quasi-normal mode (f-mode) of neutron stars has become possible. The future detection of GWs originating from the f-mode of neutron stars will provide a potential way to improve our understanding of the nature of nuclear matter inside neutron stars. In this work, we investigate the constraint imposed by the f-mode oscillation of neutron stars on the symmetry energy of nuclear matter using Bayesian analysis and parametric EOS. It is shown that if the frequency of the f-mode of a neutron star of known mass is observed precisely, the symmetry energy at twice the saturation density (E sym(2ρ 0)) of nuclear matter can be constrained within a relatively narrow range. For example, when all the following parameters are within the given intervals: 220 ≤ K 0 ≤ 260 MeV, 28 ≤ E sym(ρ 0) ≤ 36 MeV, 30 ≤ L ≤ 90 MeV, −800 ≤ J 0 ≤ 400 MeV, − 400 ≤ K sym ≤ 100 MeV, −200 ≤ J sym ≤ 800 MeV, E sym(2ρ 0) will be constrained to within MeV if the f-mode frequency of a canonical neutron star (1.4 M⊙) is observed to be 1.720 kHz with a 1% relative error. Furthermore, if only f-mode frequency detection is available, i.e. there is no stellar mass measurement, a precisely detected f-mode frequency can also impose an accurate constraint on the symmetry energy. For example, given the same parameter space and the same assumed observed f-mode frequency mentioned above, and assuming that the stellar mass is in the range of 1.2–2.0 M⊙, E sym(2ρ 0) will be constrained to within . In addition, it is shown that a higher slope of 69 ≤ L ≤ 143 MeV will give a higher posterior distribution of E sym(2ρ 0), ." @default.
• W3201232423 created "2021-09-27" @default.
• W3201232423 creator A5036392167 @default.
• W3201232423 creator A5062499328 @default.
• W3201232423 creator A5071957113 @default.
• W3201232423 date "2021-07-21" @default.
• W3201232423 modified "2023-10-11" @default.
• W3201232423 title "Constraint on nuclear symmetry energy from f-mode oscillation of neutron stars" @default.
• W3201232423 cites W1964418840 @default.
• W3201232423 cites W1968821782 @default.
• W3201232423 cites W1971043198 @default.
• W3201232423 cites W1976116689 @default.
• W3201232423 cites W1978574491 @default.
• W3201232423 cites W2005670731 @default.
• W3201232423 cites W2007709299 @default.
• W3201232423 cites W2012610774 @default.
• W3201232423 cites W2016515266 @default.
• W3201232423 cites W2018944415 @default.
• W3201232423 cites W2022836438 @default.
• W3201232423 cites W2025008996 @default.
• W3201232423 cites W2035391277 @default.
• W3201232423 cites W2047273920 @default.
• W3201232423 cites W2056583859 @default.
• W3201232423 cites W2076752847 @default.
• W3201232423 cites W2085233824 @default.
• W3201232423 cites W2087447386 @default.
• W3201232423 cites W2094626656 @default.
• W3201232423 cites W2114371620 @default.
• W3201232423 cites W2116035961 @default.
• W3201232423 cites W2121998732 @default.
• W3201232423 cites W2160857147 @default.
• W3201232423 cites W2260725527 @default.
• W3201232423 cites W2270205340 @default.
• W3201232423 cites W2337252298 @default.
• W3201232423 cites W2531534365 @default.
• W3201232423 cites W2612254546 @default.
• W3201232423 cites W2758413352 @default.
• W3201232423 cites W2768001799 @default.
• W3201232423 cites W2772938691 @default.
• W3201232423 cites W2807168552 @default.
• W3201232423 cites W2807309204 @default.
• W3201232423 cites W2883327832 @default.
• W3201232423 cites W2894417874 @default.
• W3201232423 cites W2906101518 @default.
• W3201232423 cites W2910356444 @default.
• W3201232423 cites W2912230473 @default.
• W3201232423 cites W2915919237 @default.
• W3201232423 cites W2920838744 @default.
• W3201232423 cites W2941032245 @default.
• W3201232423 cites W2966356230 @default.
• W3201232423 cites W3013021119 @default.
• W3201232423 cites W3098164306 @default.
• W3201232423 cites W3098175373 @default.
• W3201232423 cites W3099651099 @default.
• W3201232423 cites W3100913711 @default.
• W3201232423 cites W3101008895 @default.
• W3201232423 cites W3101249161 @default.
• W3201232423 cites W3101406695 @default.
• W3201232423 cites W3102587511 @default.
• W3201232423 cites W3103204141 @default.
• W3201232423 cites W3103463281 @default.
• W3201232423 cites W3103657055 @default.
• W3201232423 cites W3104270151 @default.
• W3201232423 cites W3104611130 @default.
• W3201232423 cites W3106358816 @default.
• W3201232423 cites W3120569425 @default.
• W3201232423 cites W3121841919 @default.
• W3201232423 cites W3122209580 @default.
• W3201232423 cites W3132010812 @default.
• W3201232423 doi "https://doi.org/10.1088/1572-9494/ac1669" @default.
• W3201232423 hasPublicationYear "2021" @default.
• W3201232423 type Work @default.
• W3201232423 sameAs 3201232423 @default.
• W3201232423 citedByCount "2" @default.
• W3201232423 countsByYear W32012324232022 @default.
• W3201232423 crossrefType "journal-article" @default.
• W3201232423 hasAuthorship W3201232423A5036392167 @default.
• W3201232423 hasAuthorship W3201232423A5062499328 @default.
• W3201232423 hasAuthorship W3201232423A5071957113 @default.
• W3201232423 hasConcept C111919701 @default.
• W3201232423 hasConcept C121332964 @default.
• W3201232423 hasConcept C150846664 @default.
• W3201232423 hasConcept C152568617 @default.
• W3201232423 hasConcept C185544564 @default.
• W3201232423 hasConcept C186370098 @default.
• W3201232423 hasConcept C192887742 @default.
• W3201232423 hasConcept C2524010 @default.
• W3201232423 hasConcept C2776036281 @default.
• W3201232423 hasConcept C2778439541 @default.
• W3201232423 hasConcept C2779886137 @default.
• W3201232423 hasConcept C3079626 @default.
• W3201232423 hasConcept C33923547 @default.
• W3201232423 hasConcept C41008148 @default.
• W3201232423 hasConcept C44870925 @default.
• W3201232423 hasConcept C48677424 @default.
• W3201232423 hasConcept C54355233 @default.
• W3201232423 hasConcept C62520636 @default.
• W3201232423 hasConcept C86803240 @default.
• W3201232423 hasConceptScore W3201232423C111919701 @default.
• W3201232423 hasConceptScore W3201232423C121332964 @default.

• next