Astrophysics on the GRAPE family of special-purpose computers

The GRAPE-4, the world's fastest computer in 1995-1997, has produced some major scientific results through a wide diversity of large-scale simulations in astrophysics. Applications have included planetary formation, the evolution of star clusters and galactic nuclei, and the formation of galaxies and clusters of galaxies.

[1]  J. Makino Postcollapse Evolution of Globular Clusters , 1996, astro-ph/9608160.

[2]  Matthias Steinmetz Grapesph: cosmological smoothed particle hydrodynamics simulations with the special-purpose hardware GRAPE , 1996 .

[3]  Toshikazu Ebisuzaki,et al.  Evolution of Clusters of Galaxies (GRAPE) , 1993 .

[4]  Andreas Burkert,et al.  Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster , 1998 .

[5]  Piet Hut,et al.  A hierarchical O(N log N) force-calculation algorithm , 1986, Nature.

[6]  Toshikazu Ebisuzaki,et al.  A special-purpose computer for gravitational many-body problems , 1990, Nature.

[7]  Joseph L. Breeden,et al.  Chaos in Core Oscillations of Globular Clusters , 1995 .

[8]  Jeremy Goodman On Gravothermal Oscillations , 1987 .

[9]  Rainer Spurzem,et al.  Direct collisional simulation of 10000 particles past core collapse , 1996 .

[10]  Junichiro Makino,et al.  Treecode with a Special-Purpose Processor , 1991 .

[11]  Makoto Taiji,et al.  Fast and accurate molecular dynamics simulation of a protein using a special‐purpose computer , 1997 .

[12]  T. Suginohara,et al.  The Effect of Cooling on the Density Profile of Hot Gas in Clusters of Galaxies: Is Additional Physics Needed? , 1998, astro-ph/9803318.

[13]  Makoto Taiji,et al.  Scientific simulations with special purpose computers - the GRAPE systems , 1998 .

[14]  Matthias SteinmetzEwald Mueller The formation of disc galaxies in a cosmological context: structure and kinematics , 1995 .

[15]  P ? ? ? ? ? ? ? % ? ? ? ? , 1991 .

[16]  Holger Baumgardt,et al.  Dynamical Evolution of Star Clusters , 2001 .

[17]  John Kormendy,et al.  Inward Bound—The Search for Supermassive Black Holes in Galactic Nuclei , 1995 .

[18]  William K. Hartmann,et al.  Planetesimals to planets: Numerical simulation of collisional evolution , 1978 .

[19]  Michael Rauch,et al.  Damped Lyα Absorber at High Redshift: Large Disks or Galactic Building Blocks? , 1998 .

[20]  Carl J. Grillmair,et al.  The Centers of Early-Type Galaxies with HST.I.An Observational Survey , 1995 .

[21]  M. Rees,et al.  Massive black hole binaries in active galactic nuclei , 1980, Nature.

[22]  Matthias Steinmetz,et al.  The Effects of a Photoionizing Ultraviolet Background on the Formation of Disk Galaxies , 1996, astro-ph/9605043.

[23]  T. Ebisuzaki,et al.  Merging of Galaxies with Central Black Holes. I. Hierarchical Mergings of Equal-Mass Galaxies , 1996 .

[24]  Junichiro Makino,et al.  Effect of Suprathermal Particles on Gravothermal Oscillation , 1987 .

[25]  Matthias Steinmetz,et al.  A Comparison of X-ray and Strong Lensing Properties of Simulated X-ray Clusters , 1996 .

[26]  P. P. Eggleton,et al.  On the consequences of the gravothermal catastrophe , 1980 .

[27]  Puragra Guhathakurta,et al.  Globular Cluster Photometry With the Hubble Space Telescope. V. WFPC Study of M15's Central density Cusp , 1995, astro-ph/9512015.

[28]  Georges Meylan,et al.  Structure and dynamics of globular clusters , 1993 .

[29]  Toshiyuki Fukushige,et al.  Pre-collapse evolution of galactic globular clusters , 1995 .

[30]  Eiichiro Kokubo,et al.  Oligarchic growth of protoplanets , 1996 .

[31]  Jun Makino,et al.  Performance and accuracy of a GRAPE‐3 system for collisionless N‐body simulations , 1998 .

[32]  Toshikazu Ebisuzaki,et al.  Smoothed particle hydrodynamics with GRAPE-1A , 1993 .