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• W4387368431 endingPage "38" @default.
• W4387368431 startingPage "38" @default.
• W4387368431 abstract "Abstract Gravitational waves (GWs) emanating from unstable quasi-normal modes in neutron stars (NSs) could be accessible with the improved sensitivity of the current GW detectors or with the next-generation GW detectors and, therefore, can be employed to study the NS interior. Assuming f -mode excitation in isolated pulsars with typical energy of pulsar glitches and considering potential f -mode GW candidates for A+ (upgraded LIGO detectors operating at fifth observing run design sensitivity) and Einstein Telescope (ET), we demonstrate the inverse problem of NS asteroseismology within a Bayesian formalism to constrain the nuclear parameters and NS equation of state (EOS). We describe the NS interior within relativistic mean-field formalism. Taking the example of glitching pulsars, we find that for a single event in A+ and ET, among the nuclear parameters, the nucleon effective mass ( m *) within 90% credible interval can be restricted within 10% and 5%, respectively. At the same time, the incompressibility ( K ) and the slope of the symmetry energy ( L ) are only loosely constrained. Considering multiple (10) events in A+ and ET, all the nuclear parameters are well constrained, especially m *, which can be constrained to 3% and 2% in A+ and ET, respectively. Uncertainty in the observables of a 1.4 M ⊙ NS such as radius ( <?CDATA ${R}_{1.4{M}_{odot }}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow> <mml:mi>R</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>1.4</mml:mn> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> </mml:mrow> </mml:msub> </mml:math> ), f -mode frequency ( <?CDATA ${f}_{1.4{M}_{odot }}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow> <mml:mi>f</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>1.4</mml:mn> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> </mml:mrow> </mml:msub> </mml:math> ), damping time ( <?CDATA ${tau }_{1.4{M}_{odot }}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow> <mml:mi>τ</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>1.4</mml:mn> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> </mml:mrow> </mml:msub> </mml:math> ), and a few EOS properties including squared speed of sound ( c s 2 ) are also estimated." @default.
• W4387368431 created "2023-10-06" @default.
• W4387368431 creator A5025842819 @default.
• W4387368431 creator A5026518696 @default.
• W4387368431 creator A5032483770 @default.
• W4387368431 date "2023-10-01" @default.
• W4387368431 modified "2023-10-16" @default.
• W4387368431 title "Constraining Nuclear Parameters Using Gravitational Waves from f-mode Oscillations in Neutron Stars" @default.
• W4387368431 cites W1522916454 @default.
• W4387368431 cites W1552854258 @default.
• W4387368431 cites W1851389139 @default.
• W4387368431 cites W1964418840 @default.
• W4387368431 cites W1965312202 @default.
• W4387368431 cites W1973820399 @default.
• W4387368431 cites W1975784697 @default.
• W4387368431 cites W1979429224 @default.
• W4387368431 cites W1992251131 @default.
• W4387368431 cites W1993688832 @default.
• W4387368431 cites W1997544533 @default.
• W4387368431 cites W2011301426 @default.
• W4387368431 cites W2011483031 @default.
• W4387368431 cites W2013166541 @default.
• W4387368431 cites W2013385927 @default.
• W4387368431 cites W2024754150 @default.
• W4387368431 cites W2026494651 @default.
• W4387368431 cites W2035388669 @default.
• W4387368431 cites W2047551422 @default.
• W4387368431 cites W2060819359 @default.
• W4387368431 cites W2066888900 @default.
• W4387368431 cites W2071108515 @default.
• W4387368431 cites W2072032173 @default.
• W4387368431 cites W2079013965 @default.
• W4387368431 cites W2087447386 @default.
• W4387368431 cites W2094400046 @default.
• W4387368431 cites W2103857591 @default.
• W4387368431 cites W2114371620 @default.
• W4387368431 cites W2115081904 @default.
• W4387368431 cites W2121998732 @default.
• W4387368431 cites W2124050845 @default.
• W4387368431 cites W2146292423 @default.
• W4387368431 cites W2160857147 @default.
• W4387368431 cites W2161759996 @default.
• W4387368431 cites W2163741880 @default.
• W4387368431 cites W2165591715 @default.
• W4387368431 cites W2169791324 @default.
• W4387368431 cites W2270205340 @default.
• W4387368431 cites W2413988422 @default.
• W4387368431 cites W2420525394 @default.
• W4387368431 cites W2461117145 @default.
• W4387368431 cites W2531534365 @default.
• W4387368431 cites W2617710911 @default.
• W4387368431 cites W2747055148 @default.
• W4387368431 cites W2765081049 @default.
• W4387368431 cites W2767183428 @default.
• W4387368431 cites W2782616980 @default.
• W4387368431 cites W2792912078 @default.
• W4387368431 cites W2807309204 @default.
• W4387368431 cites W2847346208 @default.
• W4387368431 cites W2888098253 @default.
• W4387368431 cites W2905166052 @default.
• W4387368431 cites W2918121884 @default.
• W4387368431 cites W2931388211 @default.
• W4387368431 cites W2971836485 @default.
• W4387368431 cites W2975828310 @default.
• W4387368431 cites W2980723814 @default.
• W4387368431 cites W3013021119 @default.
• W4387368431 cites W3042920238 @default.
• W4387368431 cites W3047823159 @default.
• W4387368431 cites W3096193999 @default.
• W4387368431 cites W3098164306 @default.
• W4387368431 cites W3100881821 @default.
• W4387368431 cites W3101410117 @default.
• W4387368431 cites W3102587511 @default.
• W4387368431 cites W3103145119 @default.
• W4387368431 cites W3104042330 @default.
• W4387368431 cites W3104191132 @default.
• W4387368431 cites W3105850678 @default.
• W4387368431 cites W3121166662 @default.
• W4387368431 cites W3122052225 @default.
• W4387368431 cites W3129656243 @default.
• W4387368431 cites W3138611124 @default.
• W4387368431 cites W3153199549 @default.
• W4387368431 cites W3164490304 @default.
• W4387368431 cites W3179364416 @default.
• W4387368431 cites W3182570346 @default.
• W4387368431 cites W3183648706 @default.
• W4387368431 cites W3196511915 @default.
• W4387368431 cites W3197057878 @default.
• W4387368431 cites W3197095402 @default.
• W4387368431 cites W3201232423 @default.
• W4387368431 cites W3202074548 @default.
• W4387368431 cites W3217566643 @default.
• W4387368431 cites W4200084910 @default.
• W4387368431 cites W4200123111 @default.
• W4387368431 cites W4220859069 @default.
• W4387368431 cites W4283695393 @default.
• W4387368431 cites W4288445691 @default.
• W4387368431 cites W4293830450 @default.

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