Variable Density Flows in Rotating Astrophysical Plasma. Linear Waves and Resonant Phenomena
Universe, 2021 New observational data and modeling of physical processes constantly appear in the young and rapidly developing branch of science of plasma astrophysics.
Maria Fedotova +2 more
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Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma [PDF]
, 2012 The effect of radiative heat-loss function and finite ion Larmor radius (FLR) corrections on the self-gravitational instability of infinite homogeneous viscous plasma has been investigated incorporating the effects of thermal conductivity and finite ...
Sachin Kaothekar, R. K. Chhajlani
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Magnetic turbulence in a table-top laser-plasma relevant to astrophysical scenarios [PDF]
Nature Communications, 2017 Turbulent magnetic fields abound in nature, pervading astrophysical, solar, terrestrial and laboratory plasmas. Understanding the ubiquity of magnetic turbulence and its role in the universe is an outstanding scientific challenge.
Gourab Chatterjee +9 more
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Thin current sheets caused by plasma flow gradients in space and astrophysical plasma [PDF]
Annales Geophysicae, 2010 Strong gradients in plasma flows play a major role in space and astrophysical plasmas. A typical situation is that a static plasma equilibrium is surrounded by a plasma flow, which can lead to strong plasma flow gradients at the separatrices between ...
D. H. Nickeler +2 more
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Plasma physics of extreme astrophysical environments [PDF]
Reports on Progress in Physics, 2014 Certain classes of astrophysical objects, namely magnetars and central engines of supernovae and gamma-ray bursts (GRBs), are characterized by extreme physical conditions not encountered elsewhere in the Universe. In particular, they possess magnetic fields that exceed the critical quantum field of 44 teragauss.
Uzdensky, Dmitri A., Rightley, Shane
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Introduction to plasma astrophysics characteristics of astrophysical plasma high density plasma.
Kakuyūgō kenkyū, 1989 Property of High Density Matter with density from 1g/cm3 to 1016g/cm3 is argued. Using the equation of state for high density matter, the equilibrium structure of high density star is discussed. There are two phases of high density stars. They are white dwarf and neutron star. Each has a maximum possible mass.
Takashi Nakamura
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Astrophysical Plasmas and Fluids [PDF]
, 1999 This book is a valuable introduction to astrophyscial plasmas and fluids for graduate students of astronomy preparing either for a research career in the field or just aspiring to achieve a decent degree of familiarity with 99% of the cosmos. The contents provide a true representation of the phenomenal diversity of dominant roles that plasmas and ...
V. Krishan
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Collisionless cooling of perpendicular electron temperature in the thermal quench of a magnetized plasma [PDF]
Scientific ReportsThermal quench of a nearly collisionless plasma against an isolated cooling boundary or region is an undesirable off-normal event in magnetic fusion experiments, but an ubiquitous process of cosmological importance in astrophysical plasmas.
Yanzeng Zhang, Jun Li, Xian-Zhu Tang
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Flux equipartition in astrophysical plasma turbulence. [PDF]
Sci AdvMarino R, Xie JH.
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Relativistic Magnetized Astrophysical Plasma Outflows in Black-Hole Microquasars [PDF]
Symmetry, 2021 In this work, we deal with collimated outflows of magnetized astrophysical plasma known as astrophysical jets, which have been observed to emerge from a wide variety of astrophysical compact objects.
T. Papavasileiou +2 more
semanticscholar +1 more source