Results 61 to 70 of about 3,816,107 (170)
The Evolution of Parallel Electron Temperature in Magnetospheric Reconnection Inflows
Geophysical Research LettersUsing data from NASA's Magnetospheric Multiscale mission captured in a reconnection inflow on the magnetospheric side of Earth's dayside magnetopause, we find a region where the heat flux density gradient term balances the parallel compression term in ...
Daniel J. Gershman +9 more
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Rip Cosmology via Inhomogeneous Fluid
Galaxies, 2013 The conditions for the appearance of the Little Rip, Pseudo Rip and Quasi Rip universes in the terms of the parameters in the equation of state of some dark fluid are investigated. Several examples of the Rip cosmologies are investigated.
Alexander V. Timoshkin +2 more
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A Multidimensional Relativistic Hydrodynamics Code with a General Equation of State
, 2010 The ideal gas equation of state with a constant adiabatic index, although commonly used in relativistic hydrodynamics, is a poor approximation for most relativistic astrophysical flows.
Aloy +14 more
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Non-Radial Oscillation Modes of Superfluid Neutron Stars Modeled with CompOSE
Universe, 2018 We compute the principal non-radial oscillation mode frequencies of Neutron Stars described with a Skyrme-like Equation of State (EoS), taking into account the possibility of neutron and proton superfluidity.
Prashanth Jaikumar +2 more
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The Atmosphere of a Black Hole
, 2016 We present a static, isotropic fluid solution around a black hole and its effects on the field equations and the horizon. We offer the solutions, their descriptions and we comment on their shortcomings. We derive from the proposed metric the density, the
Arik, Metin, Senikoglu, Yorgo
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Bound-State Solutions of Dirac Equation for Kratzer Potential with Pseudoscalar-Coulomb Term [PDF]
, 2022 Altuğ Arda, R. Sever
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Determination of the Equation of State of Dense Matter
, 2002 Nuclear collisions can compress nuclear matter to densities achieved within neutron stars and within core-collapse supernovae. These dense states of matter exist momentarily before expanding.
Danielewicz, P., Lacey, R., Lynch, W. G.
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What can we learn about the unstable equation-of-state branch from neutron-star mergers? [PDF]
, 2023 Maximiliano Ujevic +4 more
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Equation of state of HE detonation products
EPJ Web of Conferences, 2011 Computational analysis of steady-state HE detonation parameters is possible if one knows the equation of state of detonation products and thermal energy released at the Jouget point during detonation.
Nadykto B.A.
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