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Research team:
P.I. Prof. dr. Edward van den Heuvel
Co.I. Prof. dr. Peter Sloot,
dr. Simon Portegies Zwart,
Supported by NWO Computational Science (#635.000.001)
dr. Michael Sipior,
Alessia Gualandris
Ojective: We are in the process of realizing a N-body
lab with the aim to study the evolution of dense stellar
systems. The UvA N-body lab (MoDeStA for Modeling
Dense Star Clusters in Amsterdam)
contains special purpose GRAPE hardware, which is dedicated
to gravitational force calculations, attached to the Yellow
node of the UvA Beowulf computer, which is a cluster of
general-purpose computers. In this environment we are
developing highly efficient software libraries containing
N-body kernels, such as the direct method, hierarchical
methods, and others. The unique combination of GRAPE
hardware with a cluster results in speed up of both the
direct force calculations, by running them on GRAPE, and a
speed up the remaining calculations by parallelizing them over the
Beowulf. This allows to remove e.g. known bottle-necks in
hierarchical methods executing on GRAPE hardware attached
to a single host computer. Together with existing
intelligent batch processing tools and interactive
visualization technology the N-body lab is now a very
powerful generic infrastructure. We are now in the process
of studying the dynamical evolution of dense stellar
systems (globular clusters and galactic bulges) and the
formation and evolution of intermediate mass black holes in
dense star clusters. The latter research resulted in a
publication in Nature, last April. Currently we are in the
process of studying the effect of the presence of binary
stars on the evolution toward and through core collapse in
globular clusters. During core collapse, which is a
consequence of the long term evolution of a system in near
equilibrium and with a negative heat capacity, very unusual
close interactions between stars occur, the outcomes of
which are still unknown. Below we itemize our progress in
the structure predetermined by NWO-EW
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