Results 71 to 80 of about 4,215,064 (363)
A New Fourth Order Compression Dependent Equation of State
East European Journal of PhysicsThis study introduces a new first- to fourth-order exponential equation of state (EOS) to enhance accuracy across varying compression levels. The proposed exponential EOS is compared to the widely used fourth-order Birch-Murnaghan EOS, and it not only ...
Abhay P. Srivastava +3 more
doaj +1 more source
Calculation of Thermodynamic properties of Fluid Using a New Equation of State [PDF]
Iranian Journal of Chemistry & Chemical Engineering, 1992 Using the Lennard-Jones (12-6) potential, a new equation of state is obtained that can predict properties of both gases and liquids relatively well. This equation of state is given as (Z-a)V2=(A/V2)-B, where Z is the compressibility factor, A and B are ...
Gh. Parsafar, F. Kermanpour
doaj
Ab Initio Phase Diagram of Chromium to 2.5 TPa
Applied Sciences, 2022 Chromium possesses remarkable physical properties such as hardness and corrosion resistance. Chromium is also a very important geophysical material as it is assumed that lighter Cr isotopes were dissolved in the Earth’s molten core during the planet’s ...
Samuel R. Baty +4 more
doaj +1 more source
Equation of State from Lattice QCD Calculations
, 2011 We provide a status report on the calculation of the Equation of State (EoS) of QCD at finite temperature using lattice QCD. Most of the discussion will focus on comparison of recent results obtained by the HotQCD and Wuppertal-Budapest (W-B ...
Gupta, Rajan
core +1 more source
GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations [PDF]
, 2017 Gravitational waves detected from the binary neutron star (NS) merger GW170817 constrained the NS equation of state by placing an upper bound on certain parameters, describing the binary’s tidal interactions.
D. Radice +3 more
semanticscholar +1 more source
Ability of LIGO and LISA to probe the equation of state of the early Universe [PDF]
Journal of Cosmology and Astroparticle Physics, 2019 The expansion history of the Universe between the end of inflation and the onset of radiation-domination (RD) is currently unknown. If the equation of state during this period is stiffer than that of radiation, w > 1/3, the gravitational wave (GW ...
Daniel G. Figueroa, Erwin H. Tanin
semanticscholar +1 more source
FEBS Letters, EarlyView.Atovaquone is an antimalarial requiring potentiation for sufficient efficacy. We pursued strategies to enhance its activity, showing that 4‐nitrobenzoate inhibits 4‐hydroxybenzoate polyprenyltransferase, decreasing ubiquinone biosynthesis. Since atovaquone competes with ubiquinol in mitochondria, 4‐nitrobenzoate facilitates its action, potentiating ...
Ignasi Bofill Verdaguer +7 more
wiley +1 more source
CURVES OF THERMODYNAMIC STATES IN SOME FLUIDS WITH DISPERSION
TASK Quarterly, 2017 Variations in the thermodynamic state of a dispersive medium, caused by sound, are studied. A bubbly liquid and a Maxwell fluid are considered as examples. Curves in the plane of thermodynamic states are plotted.
ANNA PERELOMOVA
doaj +1 more source
An equation of state for dark matter [PDF]
, 2011 Dark matter, believed to be present in many galaxies, is interpreted as a hydrodynamical system in interaction with the gravitational field and nothing else.
Fronsdal, Christian, Wilcox, Thomas J.
core
Towards a precision calculation of the effective number of neutrinos Neff in the Standard Model: the QED equation of state [PDF]
Journal of Cosmology and Astroparticle Physics, 2019 We revisit and quantify in this work several aspects of Standard Model physics at finite temperature that drive the theoretical value of the cosmological parameter, the effective number of neutrinos Neff, away from 3 in the early universe.
Jack J. Bennett +3 more
semanticscholar +1 more source