Editors: Pau Amaro-Seoane & Bernard Schutz
The last GW Note is by Jonathan Thornburg

Archive for the ‘GPU’ Category

How well do STARLAB and NBODY compare? II: Hardware and accuracy

Monday, January 30th, 2012

arXiv:1201.5692

by Anders, P. and Baumgardt, H. and Gaburov, E. and Zwart, S. Portegies
14 pages incl. 3 pages with figures and 4 pages of tables (analysis results), MNRAS in press

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Interaction of Recoiling Supermassive Black Holes with Stars in Galactic Nuclei

Thursday, January 19th, 2012

arXiv:1201.3407

by Li, Shuo and Liu, F. K. and Berczik, Peter and Chen, Xian and Spurzem, Rainer
38 pages, 10 figues; accepted for publication in ApJ

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PSDF: Particle Stream Data Format for N-Body Simulations

Tuesday, January 10th, 2012

arXiv:1201.1694

by Farr, Will M. and Ames, Jeff and Hut, Piet and Makino, Junichiro and McMillan, Steve and Muranushi, Takayuki and Nakamura, Koichi and Nitadori, Keigo and Zwart, Simon Portegies
5 pages; submitted to New Astronomy

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Implementation of a Parallel Tree Method on a GPU

Saturday, December 24th, 2011

arXiv:1112.4539

by Nakasato, Naohito
Journal of Computational Science, 2011; See our recent update at http://galaxy.u-aizu.ac.jp/trac/note/wiki/Octree_On_GPU

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A Dynamical N-body Model for the Central Region of $\omega$ Centauri

Wednesday, November 23rd, 2011

arXiv:1111.5011

by Jalali, B. and Baumgardt, H. and Kissler-Patig, M. and Gebhardt, K. and Noyola, E. and Lützgendorf, N. and de Zeeuw, P. T.
Accepted for publication in A&A

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Testing Photometric Diagnostics for the Dynamical State and Possible IMBH presence in Globular Clusters

Wednesday, August 24th, 2011

arXiv:1108.4425

by Noyola, Eva and Baumgardt, Holger
Accepted for publication in ApJ

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Evolution of growing black holes in axisymmetric galaxy cores

Monday, August 22nd, 2011

arXiv:1108.3993

by Fiestas, Jose and Porth, Oliver and Berczik, Peter and Spurzem, Rainer
15 pages, 7 figures,accepted by MNRAS

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Tidal disruption rate of stars by supermassive black holes obtained by direct N-body simulations

Thursday, August 18th, 2011

arXiv:1108.2270

by Brockamp, M. and Baumgardt, H. and Kroupa, P.
19 pages, 11 figures, accepted for publication in MNRAS

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A sparse octree gravitational N-body code that runs entirely on the GPU processor

Sunday, June 19th, 2011

arXiv:1106.1900

by Bédorf, Jeroen and Gaburov, Evghenii and Zwart, Simon Portegies
Submitted to Journal of Computational Physics. 34 pages, 13 figures, single column

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Collisional formation of very massive stars in dense clusters

Friday, September 3rd, 2010

arXiv:1009.0283

by Moeckel, Nickolas and Clarke, Cathie J.
8 pages, submitted to MNRAS. Includes revisions per referee’s comments

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MYRIAD: A new N-body code for simulations of Star Clusters

Friday, June 18th, 2010

arXiv:1006.3326

by Konstantinidis, Simos and Kokkotas, Kostas D.
24 pages, 28 figures

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Statistical constraints on binary black hole inspiral dynamics

Tuesday, June 15th, 2010

arXiv:1005.5560

by Galley, Chad R. and Herrmann, Frank and Silberholz, John and Tiglio, Manuel and Guerberoff, Gustavo

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Young massive star clusters

Thursday, February 11th, 2010

arXiv:1002.1961

by Zwart, Simon Portegies and McMillan, Steve and Gieles, Mark
Only 88 pages. To be published in ARAA. Final version to be submitted on Friday 12 February

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Numerical modeling of gravitational wave sources accelerated by OpenCL

Thursday, January 21st, 2010

arXiv:1001.3631

by Khanna, Gaurav and McKennon, Justin
14 pages, 4 figures

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An exploration of CUDA and CBEA for a gravitational wave source-modelling application

Friday, September 25th, 2009

arXiv:0909.4039

by Khanna, Gaurav and McKennon, Justin
8 pages, 4 figures, Accepted for publication in Parallel and Distributed Computing and Systems (PDCS 2009)

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Supercomputing and stellar dynamics

Wednesday, September 9th, 2009

arXiv:0909.0879

by Capuzzo-Dolcetta, R.
Invited talk to the 2009 general Conference of the Societa’ Astronomica Italiana. 6 pages including 1 figure

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Oct-tree Method on GPU

Friday, September 4th, 2009

arXiv:0909.0541

by Nakasato, N.
Poster paper to be appeared in SC09

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