Hubber, D.A., Allison, R.J., Smith, R. et al. (1 more author) (2013) A hybrid SPH/N-body method for star cluster simulations. Monthly Notices of the Royal Astronomical Society, 430 (3). pp. 1599-1616. ISSN 0035-8711
Abstract
We present a new hybrid smoothed particle hydrodynamics (SPH)/N-body method for modelling the collisional stellar dynamics of young clusters in a live gas background. By deriving the equations of motion from Lagrangian mechanics we obtain a formally conservative combined SPH–N-body scheme. The SPH gas particles are integrated with a second-order Leapfrog, and the stars with a fourth-order Hermite scheme. Our new approach is intended to bridge the divide between the detailed, but expensive, full hydrodynamical simulations of star formation and pure N-body simulations of gas-free star clusters. We have implemented this hybrid approach in the SPH code SEREN and perform a series of simple tests to demonstrate the fidelity of the algorithm and its conservation properties. We investigate and present resolution criteria to adequately resolve the density field and to prevent strong numerical scattering effects. Future developments will include a more sophisticated treatment of binaries.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | This article has been accepted for publication in MNRAS ©: 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Keywords: | hydrodynamics; methods: numerical; stars: kinematics and dynamics |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield) |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 03 Nov 2017 14:50 |
Last Modified: | 03 Nov 2017 14:50 |
Published Version: | https://doi.org/10.1093/mnras/sts694 |
Status: | Published |
Publisher: | Oxford University Press |
Refereed: | Yes |
Identification Number: | 10.1093/mnras/sts694 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:123332 |