Chapter 3

Accelerated Many-Core GPU Computing for Physics and Astrophysics on Three Continents

Rainer Spurzem

National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing, China,

Astronomisches Rechen-Institut, Zentrum für Astronomie, University of Heidelberg, Heidelberg, Germany, and

Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, China

Peter Berczik

National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing, China, and

Astronomisches Rechen-Institut, Zentrum für Astronomie, University of Heidelberg, Heidelberg, Germany

Ingo Berentzen

Zentrum für Astronomie, University of Heidelberg, Heidelberg, Germany

Wei Ge and Xiaowei Wang

Institute of Process Engineering, Chinese Academy of Sciences, Beijing, China

Hsi-Yu Schive

Department of Physics, National Taiwan University, Taibei, Taiwan

Keigo Nitadori

RIKEN AICS Institute, Kobe, Japan

Tsuyoshi Hamada

Nagasaki Advanced Computing Center, Nagasaki University, Nagasaki, Japan

José Fiestas

Astronomisches Rechen-Institut, Zentrum für Astronomie, University of Heidelberg, Heidelberg, Germany

3.1 INTRODUCTION

Theoretical numerical modeling has become a third pillar of sciences in addition to theory and experiment (in the case of astrophysics, the experiment is mostly substituted by observations). Numerical modeling allows one to compare theory with experimental or observational data in unprecedented detail, and it also provides theoretical insight into physical processes ...

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