A dissipative extension to ideal hydrodynamics
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arXiv
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| Format: | Preprint |
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2024
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| _version_ | 1866909204359413760 |
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| author | Hatton, Marcus J. Hawke, Ian |
| author_facet | Hatton, Marcus J. Hawke, Ian |
| contents | We present a formulation of special relativistic, dissipative hydrodynamics (SRDHD) derived from the well-established Müller- Israel-Stewart (MIS) formalism using an expansion in deviations from ideal behaviour. By re-summing the non-ideal terms, our approach extends the Euler equations of motion for an ideal fluid through a series of additional source terms that capture the effects of bulk viscosity, shear viscosity and heat flux. For efficiency these additional terms are built from purely spatial derivatives of the primitive fluid variables. The series expansion is parametrized by the dissipation strength and timescale coefficients, and is therefore rapidly convergent near the ideal limit. We show, using numerical simulations, that our model reproduces the dissipative fluid behaviour of other formulations. As our formulation is designed to avoid the numerical stiffness issues that arise in the traditional MIS formalism for fast relaxation timescales, it is roughly an order of magnitude faster than standard methods near the ideal limit. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2405_09495 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | A dissipative extension to ideal hydrodynamics Hatton, Marcus J. Hawke, Ian General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena Computational Physics Fluid Dynamics We present a formulation of special relativistic, dissipative hydrodynamics (SRDHD) derived from the well-established Müller- Israel-Stewart (MIS) formalism using an expansion in deviations from ideal behaviour. By re-summing the non-ideal terms, our approach extends the Euler equations of motion for an ideal fluid through a series of additional source terms that capture the effects of bulk viscosity, shear viscosity and heat flux. For efficiency these additional terms are built from purely spatial derivatives of the primitive fluid variables. The series expansion is parametrized by the dissipation strength and timescale coefficients, and is therefore rapidly convergent near the ideal limit. We show, using numerical simulations, that our model reproduces the dissipative fluid behaviour of other formulations. As our formulation is designed to avoid the numerical stiffness issues that arise in the traditional MIS formalism for fast relaxation timescales, it is roughly an order of magnitude faster than standard methods near the ideal limit. |
| title | A dissipative extension to ideal hydrodynamics |
| topic | General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena Computational Physics Fluid Dynamics |
| url | https://arxiv.org/abs/2405.09495 |