| Co-Investigator(Kenkyū-buntansha) |
ポルス オンノ ケンブリッジ大学, 天体物理研究所, 研究員
クラーク キャシー ケンブリッジ大学, 天体物理研究所, 研究員
ホワイト サイモン D. ケンブリッジ大学, 天体物理研究所, 講師
BONNEL Iwan Institute of Astronomy, Cambridge Univ., 天体物理研究所, 研究員
アーセス スベール J. ケンブリッジ大学, 天体物理研究所, 研究員
エゲルトン ピーター P ケンブリッジ大学, 天体物理研究所, 副所長
HEGGIE Douglas C. Dept. of Math. & Statistics, Univ. of Edinburgh, 数理統計科学, 教授
INAGAKI Shogo Dept. of Astronomy, Kyoto University, 理学部, 助教授 (80115790)
OHNO Yosuke Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 学振特別研究員DC1
FUKUSHIGE Toshiyuki Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 学振特別研究員DC1
FUNATO Yoko Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 学振特別研究員DC1
UENO Munetaka Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 助手 (30242019)
TAIJI Makoto Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 助手 (10242025)
MAKINO Junichiro Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 助手 (50229340)
EBISUZAKI Toshikazu Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 助教授 (10183021)
SUGIMOTO Daiichiro Coll. of Arts & Sciences, Univ. of Tokyo, 教養学部, 教授 (10022592)
CLARKE Cathey Institute of Astronomy, Cambridge Univ.
EGGLETON Peter P. Inst. of Astronomy, Cambridge Univ.
WHITE Simon D.M. Inst. of Astronomy, Cambridge Univ.
POLS Onno Institute of Astronomy, Cambridge Univ.
AARSETH Sverre J. Inst. of Astronomy, Cambridge Univ.
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| Research Abstract |
We, in Japan side, are making a Tera flops machine for gravitational many body problems. The purpose of this project is to make softwares for our special-purpose Tera flops machines under a cooperation with the UK group. The summary of our 1993 fiscal year project is as follows:
1.Taiji and Hachisu have finished designing a new board for Hermite integrator, which is called HARP-3. A copy of the board will be transferred into Institute of Astronomy, Cambridge University until the end of June, 1994. Aarseth will use the board to develop his Hermite code for our Tera flops machine.
2.Aarseth has stayed at the University of Tokyo from 5th of March to 17th of March, 1994. He succeeded in implementing his Hermite code into our test machine, HARP-2, and proved that the Hermite code is useful to integrate the evolution of collisional N-body systems.
3.Hachisu, Funato, and Inagaki visited the Institute of Astronomy, Cambridge University and discussed with the UK group. We are now developing tools to treat binary evolutions, star captures, and star-star collisions in our N-body code.
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