Generation of spiral shock wave in the simulation of formation of accretion disk in primitive planetary system
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概要
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Smoothed Particle Hydrodynamics (SPH) simulation is carried out to find the possibility of spiral shock wave in accretion disk in primitive planetary system. In order to avoid uncertainness due to artificial viscous term, we employ SPH method combined with Riemann solver in this study. We have shown that the spiral shock wave can be formed in primitive planetary system under the limiting initial conditions of temperature and angular velocity.
著者
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Orito Erimi
Graduate School of Humanities and Sciences, Ochanomizu University
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Kawamura Tetuya
Graduate School of Humanities and Sciences, Ochanomizu University
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Orito Erimi
Graduate School Of Humanities And Sciences Ochanomizu University
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Kawamura Tetuya
Ochanomizu Univ.
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Kawamura Tetuya
Graduate School Of Humanities And Sciences Ochanomizu University
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Kawamura Tetuya
Graduate School Of Humanities And Sciences Ochanimizu University
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