PPPM and TreePM Methods on GRAPE Systems for Cosmological N-Body Simulations
スポンサーリンク
概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2005-12-25
著者
-
Yoshikawa Kohji
Department Of Astronomy Faculty Of Science Kyoto University
-
FUKUSHIGE Toshiyuki
Department of General System Studies, College of Arts and Sciences, The University of Tokyo
-
Yoshikawa Kohji
Univ. Tsukuba Ibaraki
-
Fukushige Toshiyuki
Department Of General System Studies College Of Arts And Sciences The University Of Tokyo
-
Fukushige Toshiyuki
Department of Earth Science and Astronomy, College of Arts and Sciences, The University of Tokyo
関連論文
- Exploring Galaxy Evolution from Infrared Number Counts and Cosmic Infrared Background
- Simulation of the IRIS Far-infared Survey : A Guide for Infrared Galaxy Number Counts
- Theoretical Models of Multi-Waveband QSO Luminosity Functions
- Substructures Revealed by the Sunyaev-Zel'dovich Effect at 150 GHz in a High-Resolution Map of RX J1347-1145
- Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory : Nonlinearity and Redshift-Space Distortion Effects
- Soft X-Ray Transmission Spectroscopy of a Warm/Hot Intergalactic Medium with XEUS
- Locating the Warm-Hot Intergalactic Medium in the Simulated Local Universe
- Exploring Cluster Physics with High-Resolution Sunyaev-Zel'dovich Effect Images and X-Ray Data : The Case of the Most X-Ray-Luminous Galaxy Cluster RX J1347-1145
- Environmental Effect on the Subhalo Abundance : a Solution to the Missing Dwarf Problem
- GRAPE-6A : A Single-Card GRAPE-6 for Parallel PC-GRAPE Cluster Systems
- PGPG : An Automatic Generator of Pipeline Design for Programmable GRAPE Systems
- PROGRAPE-1: A Programmable, Multi-Purpose Computer for Many-Body Simulations
- GRAPE Project : A Decade of Special-Purpose Computers for Many-Body Simulations
- Smoothing of the Anisotropy of the Cosmic Background Radiation by Multiple Gravitational Scattering
- Rapid Orbital Decay of a Black Hole Binary in Merging Galaxies
- The PCI Interface for GRAPE Systems : PCI-HIB
- GRAPE-5: A Special-Purpose Computer for N-Body Simulations
- GRAPE-6 : Massively-Parallel Special-Purpose Computer for Astrophysical Particle Simulations
- PPPM and TreePM Methods on GRAPE Systems for Cosmological N-Body Simulations
- Mass-Loss Timescale of Star Clusters in an External Tidal Field : II. Effect of Mass Profile of Parent Galaxy
- Mass-Loss Timescale of Star Clusters in an External Tidal Field : I. Clusters on Circular Orbits
- Gravothermal Expansion in N-Body Systems
- Hydrodynamical Simulation of Clusters of Galaxies in X-Ray, mm, and submm Bands : Determination of Peculiar Velocity and the Hubble Constant
- Non-Equilibrium Ionization State of a Warm-Hot Intergalactic Medium