Results 11 to 20 of about 3,655,682 (382)
Information Equation of State [PDF]
Entropy, 2008 Landauer’s principle is applied to information in the universe. Once stars began forming there was a constant information energy density as the increasing proportion of matter at high stellar temperatures exactly compensated for the expanding ...
M. Paul Gough
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The Equation of State of Biogas [PDF]
Acta Universitatis Agriculturae et Silviculturae Mendelianae Brunensis, 2017 The presented work deals with a state behavior of real gas, biogas. Theoretical approach was utilized for processing of this work. Compressibility factor was calculated with help of two equation of state – Van der Waals equation and Redlich‑Kwong ...
Petr Trávníček +2 more
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Inverse Heat Conduction and Heat Exchangers, 2020 An equation of state (EOS) is a thermodynamic expression that relates pressure (P), temperature (T), and volume (V). This equation is used to describe the state of reservoir fluids at given conditions. The cubic equations of state (CEOS) such as Van der Waals, Redlich-Kwong, Soave, and Peng-Robinson are simple models that have been widely used in the ...
E. M. Mansour
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The phase equilibrium in a Lennard-Jones fluid: Possible applications in astrophysics [PDF]
Serbian Astronomical Journal, 2012 Using standard thermodynamics and previous results of the author, this paper aims to discuss the conditions for phase equilibrium in a Lennard-Jones fluid.
Čelebonović V.
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Tight multimessenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light-curve synthesis [PDF]
Monthly notices of the Royal Astronomical Society, 2021 We present a rapid analytic framework for predicting kilonova light curves following neutron star (NS) mergers, where the main input parameters are binary-based properties measurable by gravitational wave detectors (chirp mass and mass ratio, orbital ...
M. Nicholl +5 more
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Finite-temperature equation of state with hyperons [PDF]
EPJ Web of Conferences, 2022 We present the novel finite-temperature FSU2H* equation-of-state model that covers a wide range of temperatures and lepton fractions for the conditions in proto-neutron stars, neutron star mergers and supernovae.
Kochankovski Hristijan +2 more
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Impact loading of a space nuclear powerplant
Fracture and Structural Integrity, 2013 Preferred formulation of the problem in two space dimensions are described for solving the three fundamental equations of mechanics (conservation of mass, conservation of momentum, and conservation of energy).
Evgeny I. Kraus, Ivan I. Shabalin
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Virial equation of state as a new frontier for computational chemistry.
Journal of Chemical Physics, 2022 The virial equation of state (VEOS) provides a rigorous bridge between molecular interactions and thermodynamic properties. The past decade has seen renewed interest in the VEOS due to advances in theory, algorithms, computing power, and quality of ...
A. Schultz, D. Kofke
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Microfluidics: A Novel Approach for Dehydration Protein Droplets
Biosensors, 2021 The equation of state of colloids plays an important role in the modelling and comprehension of industrial processes, defining the working conditions of processes such as drying, filtration, and mixing.
Van Nhat Pham +3 more
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Universe, 2021 I review the issues related to the appearance of hyperons in neutron star matter, focusing in particular on the problem of the maximum mass supported by hyperonic equations of state. I discuss the general mechanism that leads to the formation of hyperons
Domenico Logoteta
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