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A star cluster simulation (credit: Inti Pelupessy)

A star cluster simulation coupling N-body dynamics and stellar evolution using the Astrophysical Multi-purpose Software Environment (credit: Inti Pelupessy).

Dr Tjarda Boekholt

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Research theme

  • Astronomy and astrophysics

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Theoretical astrophysics and plasma physics at RPC
tjarda.boekholt@physics.ox.ac.uk
  • About
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On the reliability of N-body simulations

Computational Astrophysics and Cosmology Springer Nature 2:1 (2015) 2

Authors:

Tjarda Boekholt, Simon Portegies Zwart
More details from the publisher

A Keplerian-based Hamiltonian splitting for gravitational N-body simulations

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 440:1 (2014) 719-730

Authors:

G Gonçalves Ferrari, T Boekholt, SF Portegies Zwart
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ON THE MINIMAL ACCURACY REQUIRED FOR SIMULATING SELF-GRAVITATING SYSTEMS BY MEANS OF DIRECT N-BODY METHODS

The Astrophysical Journal Letters American Astronomical Society 785:1 (2014) l3

Authors:

Simon Portegies Zwart, Tjarda Boekholt
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