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10 papers · 1 filter
Evolution of Debris of a Tidally Disrupted Star by a Massive Black Hole: Development of a Hybrid Scheme of the SPH and TVD Methods
Hyung Mok Lee, Sungsoo S. Kim
The evolution of the stellar debris after tidal disruption due to the super massive black hole's tidal force is difficult to solve numerically because of the large dynamical range…
Contributions to the Cosmic Ray Flux above the Ankle: Clusters of Galaxies
Hyesung Kang, Jörg P. Rachen, Peter L. Biermann
Motivated by the suggestion of Kang, Ryu \& Jones (1996) that particles can be accelerated to high energies via diffusive shock acceleration process at the accretion shocks formed…
Accreting Matter around Clusters of Galaxies: One-Dimensional Considerations
Dongsu Ryu, Hyesung Kang
During the formation of the large scale structure of the Universe, matter accretes onto high density peaks. Accreting collisionless dark matter (DM) forms caustics around them, whi…
Charge and Spin Response of the Spin--Polarized Electron Gas
Kyung-Soo Yi, J. J. Quinn
The charge and spin response of a spin--polarized electron gas is investigated including terms beyond the random phase approximation. We evaluate the charge response, the longitudi…
Diffusive Shock Acceleration in Oblique MHD Shocks: Comparison with Monte Carlo Methods and Observations
Hyesung Kang, T. W. Jones
We report simulations of diffusive particle acceleration in oblique magnetohydrodynamical (MHD) shocks. These calculations are based on extension to oblique shocks of a numerical m…
Monopole-Bubble in Early Universe
Yoonbai Kim, Kei-ichi Maeda, Nobuyuki Sakai
The nucleation and evolution of bubbles are investigated in the model of an -symmetric scalar field coupled to gravity in the high temperature limit. It is shown that, in add…