Zobrazeno 1 - 10
of 20 534
pro vyhledávání: '"Justin L"'
Publikováno v:
Phys Rev D, vol 110, issue 10, pp. 103038. November 25th 2024
Radial mode stability is a necessary condition for the astrophysical viability of compact objects. In recent years, astrophysical models with two fluids have gain popularity, especially in their ability to model dark matter admixed neutron stars. Jus
Externí odkaz:
http://arxiv.org/abs/2408.04701
Autor:
Kianimoqadam, Alireza, Lapp, Justin L.
A novel method, the Gaussian Integral Method (GIM), is presented for calculating void fractions in Computational Fluid Dynamics-Discrete Element Method (CFD-DEM) simulations. GIM is versatile and applicable to various grid types, including structured
Externí odkaz:
http://arxiv.org/abs/2408.00909
Dissipative tidal interactions can be used to probe the out-of-equilibrium physics of neutron stars using gravitational wave observations. In this paper, we present the first post-Newtonian (PN) corrections to the orbital dynamics of a binary system
Externí odkaz:
http://arxiv.org/abs/2407.02584
Publikováno v:
Phys. Rev. D 110, 084034 (2024)
The ringdown gravitational wave signal arising e.g., in the final stage of a black hole binary merger, contains important information about the properties of the remnant, and can potentially be used to perform clean tests of general relativity. Howev
Externí odkaz:
http://arxiv.org/abs/2405.18303
Autor:
Brandon R. Grafiu
Publikováno v:
Horizons in Biblical Theology. 45:160-163
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::797f56125e9e4ca8806d89a517a28849
https://doi.org/10.1163/18712207-12341468
https://doi.org/10.1163/18712207-12341468
Accurately modeling the tidal response of neutron stars is crucial to connecting gravitational wave observations of binaries to ultra-dense nuclear physics. Most current models of the tidal response of relativistic stars either assume a static respon
Externí odkaz:
http://arxiv.org/abs/2403.03254
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