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The strength of smoothed particle hydrodynamics in modelling binary interactions

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thesis
posted on 28.03.2022, 15:25 by Thomas Reichardt
The common envelope interaction gives rise to the formation of close binaries comprising at least one evolved star, such as a white dwarf. The idea behind the common envelope interaction is attractively simple. However, hidden complexities hav prevented a full understanding of the interaction. Hydrodynamic simulations of this interaction have been pivotal in gaining an understanding of compact binary systems and phenomena that may result from them, such as novae and x-ray binaries. Unfortunately, notable disagreements still exist amongst simulations and between simulated parameters of post-common envelope binaries and observations, such as differing final separations. In this work, we perform common envelope simulations with a new smoothed particle hydrodynamics code, Phantom, which has never been trained on this problem before. The lack of a simulation domain boundary, along with excellent conservation of energy and angular momentum, allows us to track the interaction in its entirety. We start by reproducing the simulations of Passy et al. (2012) to calibrate the code. Phantom is then used to carry out preliminary simulations of the phases preceding the fast inspiral and its effects on later stages of the interaction. We also investigated how bound gas that falls back onto the binary after the inspiral phase, leading to a new interaction. Although some computational issues remain to be resolved, Phantom has thus far proved to be an excellent tool in the study of binary interactions.

History

Table of Contents

1. Introduction -- 2. SPH simulations of the common envelope interaction --3. Benchmark simulations -- 4. The pre-common envelope phase -- 5. Fallback of gas during the common envelope interaction -- 6. Summary, conclusions and future work.

Notes

Bibliography: pages 57-59 Theoretical thesis.

Awarding Institution

Macquarie University

Degree Type

Thesis MRes

Degree

MRes, Macquarie University, Faculty of Science and Engineering, Department of Physics and Astronomy

Department, Centre or School

Department of Physics and Astronomy

Year of Award

2016

Principal Supervisor

Orsola De Marco

Additional Supervisor 1

Jan Staff

Rights

Copyright Thomas Reichardt 2016. Copyright disclaimer: http://www.copyright.mq.edu.au

Language

English

Extent

1 online resource (x, 59 pages) colour illustrations

Former Identifiers

mq:45444 http://hdl.handle.net/1959.14/1077926