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Primordial black holes and their gravitational-wave signatures. [PDF]
Bagui E +20 more
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AI-powered prediction of hybrid nanofluid dynamics over a cylinder via LM optimized neural network approach. [PDF]
Imran M +5 more
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Field-particle energy transfer during chorus emissions in space. [PDF]
Liu CM +8 more
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Correction to Temperature and Bekenstein-Hawking Entropy of Kiselev Black Hole Surrounded by Quintessence. [PDF]
Wang C.
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Stellar Astrophysical Fluid Dynamics
2003In all phases of the life of a star, hydrodynamical processes play a major role. This volume gives a comprehensive overview of the state of knowledge in stellar astrophysical fluid dynamics, and its publication marked the 60th birthday of Douglas Gough, Professor of Theoretical Physics at the University of Cambridge and leading contributor to stellar ...
Thompson, M.J. +1 more
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Computational Astrophysical Fluid Dynamics
Astrophysics and Space Science, 2000zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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Numerical Fluid Dynamics in Astrophysics
2009The matter of astrophysical objects (e. g., a star or a galaxy) can often be approximated as a gas or fluid, i. e., the equations of fluid dynamics are adequate to describe the astrophysical phenomena. Hereafter, for simplification, the word fluid will be used as a synonym for both fluid and gas.
Hillebrandt, W. +2 more
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Principles of Astrophysical Fluid Dynamics
2007Fluid dynamical forces drive most of the fundamental processes in the Universe and so play a crucial role in our understanding of astrophysics. This comprehensive textbook, first published in 2007, introduces the necessary fluid dynamics to understand a wide range of astronomical phenomena, from stellar structures to supernovae blast waves, to ...
Cathie Clarke, Bob Carswell
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Topics in Astrophysical Fluid Dynamics
2006This brief description of some fluid dynamical problems of astrophysical interest focuses on two effects that are characteristic of the subject: self-gravity and radiative forces. Self-gravity is important in determining the basic structures of cosmic bodies as well as producing some intriguing instabilities. Radiation, by which we observe these bodies,
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