D
Daiichiro Sugimoto
Researcher at Florida State University College of Arts and Sciences
Publications - 95
Citations - 2291
Daiichiro Sugimoto is an academic researcher from Florida State University College of Arts and Sciences. The author has contributed to research in topics: Stellar evolution & Stars. The author has an hindex of 22, co-authored 95 publications receiving 2248 citations. Previous affiliations of Daiichiro Sugimoto include Kyoto University & University of Tokyo.
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A special-purpose computer for gravitational many-body problems
Daiichiro Sugimoto,Yoshihiro Chikada,Junichiro Makino,Tomoyoshi Ito,Toshikazu Ebisuzaki,Masayuki Umemura +5 more
TL;DR: In this paper, a pipeline-based processor was constructed using a "pipeline" architecture to simulate many-body systems with long-range forces, and the architecture can be readily parallelized to make teraflop machines a feasible possibility.
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GRAPE-4: A Massively Parallel Special-Purpose Computer for Collisional N-Body Simulations
TL;DR: The architecture and performance of the GRAPE-4 system, a massively parallel special-purpose computer for N-body simulation of gravitational collisional systems, is described.
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Carbon Deflagration Supernova, an Alternative to Carbon Detonation
TL;DR: In this article, a carbondeflagration supernova model was proposed by using a full hydrodynamic computation, where a deflagration wave propagates through the core due to convective heat transport, does not grow into detonation.
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Evolution of the stars
TL;DR: In this paper, modern theories on the evolution of stars are extended to the phases of helium burning, carbon burning, and later burnings as far as possible, and theoretical results are compared wth the Hertzsprung-Russell diagrams of star clusters.
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The Crab Nebula's progenitor
Ken'ichi Nomoto,Warren M. Sparks,Robert A. Fesen,Theodore R. Gull,S. Miyaji,Daiichiro Sugimoto +5 more
TL;DR: In this article, the initial mass of the Crab Nebula's progenitor star was estimated by comparing the observed nebular chemical abundances with detailed evolutionary calculations for 2.4 and 2.6-solar-mass helium cores of stars with masses of 8 to 10 solar masses.