Results 31 to 40 of about 3,655,682 (382)
Neutron Stars and the Nuclear Matter Equation of State
, 2021 Neutron stars provide a window into the properties of dense nuclear matter. Several recent observational and theoretical developments provide powerful constraints on their structure and internal composition.
J. Lattimer
semanticscholar +1 more source
Relativistic bound-state equations in three dimensions [PDF]
Phys.Rev.C54:507-522,1996, 1996 Firstly, a systematic procedure is derived for obtaining three-dimensional bound-state equations from four-dimensional ones. Unlike ``quasi-potential approaches'' this procedure does not involve the use of delta-function constraints on the relative four-momentum.
arxiv +1 more source
The effective Equation of State in Palatini $f(R)$ cosmology [PDF]
The European Physical Journal Plus, 2023, 2022 We investigate how the cosmological Equation of State can be used for scrutinizing extended theories of gravity, in particular, the Palatini $f(R)$ gravity. Specifically, the approach consists, at first, in investigating the effective Equation of State produced by a given model.
arxiv +1 more source
The cosmic equation of state [PDF]
Astrophysics and Space Science, 2014 7 Pages, 3 Figures.
openaire +3 more sources
Reaktor, 2017 Three equation of state are used to predict solubilities of solid n-pafaffins in supercritical fluids. The equations are the Redlich-Kwong, the Soave-Redlich-Kwong, and equation proposed by Hartono et.al. (2003; 2004).
Ratnawati Ratnawati
doaj +1 more source
Cosmological Einstein-Lambda-perfect-fluid solutions with asymptotic dust or radiation equation of state [PDF]
arXiv, 2023 This article introduces the notions of asymptotic dust and asymptotic radiation equations of state. With these non-linear generalizations of the well known dust or (incoherent) radiation equations of state the perfect-fluid equations loose any conformal covariance or privilege.
arxiv
A NICER View of PSR J0030+0451: Implications for the Dense Matter Equation of State [PDF]
Astrophysical Journal, 2019 Both the mass and radius of the millisecond pulsar PSR J0030+0451 have been inferred via pulse-profile modeling of X-ray data obtained by NASA’s Neutron Star Interior Composition Explorer (NICER) mission.
G. Raaijmakers +20 more
semanticscholar +1 more source
Reconstruction of the neutron star equation of state from $w$-quasinormal modes spectra with a piecewise polytropic meshing and refinement method [PDF]
Phys. Rev. D 99, 104005 (2019), 2019 In this paper we present a new approach to the inverse problem for relativistic stars using quasinormal modes and the piecewise polytropic parametrization of the equation of state. The algorithm is a piecewise polytropic meshing and refinement method that reconstructs the neutron star equation of state from experimental data of the mass and the $wI ...
arxiv +1 more source
Neutron-Star-Merger Equation of State
Universe, 2019 In this work, we discuss the dense matter equation of state (EOS) for the extreme range of conditions encountered in neutron stars and their mergers. The calculation of the properties of such an EOS involves modeling different degrees of freedom (such as
Veronica Dexheimer +7 more
doaj +1 more source
The influence of the equation of state on the cellular structure of gaseous detonations
The Physics of Fluids, 2021 The propagation of multidimensional gaseous detonations at elevated pressures was investigated numerically. Initial conditions at which deviations from ideal gas are expected (i.e., p0 > 2 MPa) were used to assess whether real gas effects influence their
S. Taileb +2 more
semanticscholar +1 more source