Results 41 to 50 of about 4,215,064 (363)
QCD equation of state at finite chemical potentials for relativistic nuclear collisions [PDF]
International Journal of Modern Physics A, 2021 We review the equation of state of QCD matter at finite densities. We discuss the construction of the equation of state with net baryon number, electric charge, and strangeness using the results of lattice QCD simulations and hadron resonance gas models.
A. Monnai, B. Schenke, C. Shen
semanticscholar +1 more source
Equation of State in Relativistic Magnetohydrodynamics: variable versus constant adiabatic index [PDF]
, 2007 The role of the equation of state for a perfectly conducting, relativistic magnetized fluid is the main subject of this work. The ideal constant $\Gamma$-law equation of state, commonly adopted in a wide range of astrophysical applications, is compared ...
A. Mignone +50 more
core +3 more sources
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
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
Neutron Star Cooling Within the Equation of State With Induced Surface Tension
Particles, 2020 We study the thermal evolution of neutron stars described within the equation of state with induced surface tension (IST) that reproduces properties of normal nuclear matter, fulfills the proton flow constraint, provides a high-quality description of ...
Stefanos Tsiopelas, Violetta Sagun
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Nuclear equation of state [PDF]
AIP Conference Proceedings, 2001 Nuclear equation of state plays an important role in the evolution of the Universe, in supernova explosions and, thus, in the production of heavy elements, and in stability of neutron stars. The equation constrains the two- and three-nucleon interactions and the quantum chromodynamics in nonperturbative regime.
openaire +2 more sources
Chiral dynamics of the nuclear equation of state [PDF]
, 1998 We present a new chiral power expansion scheme for the nuclear equation of state. The scheme is effective in the sense that it is constructed to work around nuclear saturation density.
Lutz, Matthias
core +3 more sources
An improved equation of state for air plasma simulations [PDF]
The Physics of Fluids, 2021 This work is concerned with the development of a novel, accurate equation of state for describing partially ionized air plasma in local thermodynamic equilibrium. One key application for this new equation of state is the simulation of lightning strike on
F. Träuble, S. Millmore, N. Nikiforakis
semanticscholar +1 more source
Compact Stars in the vBag Model and Its f-Mode Oscillations
Universe, 2023 Electromagnetic (EM) observations and gravitational wave (GW) measurements enable us to determine the mass and radius of neutron stars (NSs) and their tidal deformability, respectively.
Heng-Yi Zhou, Wei Wei, Xia Zhou
doaj +1 more source
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
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