Relativistic Dissipative Magnetohydrodynamics from the Boltzmann equation for a two-component gas
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| Format: | Preprint |
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2024
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| _version_ | 1866916256783794176 |
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| author | Kushwah, Khwahish Denicol, Gabriel S. |
| author_facet | Kushwah, Khwahish Denicol, Gabriel S. |
| contents | We derive the equations of motion of relativistic magnetohydrodynamics, as well as microscopic expressions for all of its transport coefficients, from the Boltzmann equation using the method of moments. In contrast to reference Phys. Rev. D 98(7) 2018, where a single component gas was considered, we perform our derivation for a locally neutral fluid composed of two massless particle species with opposite charges. We demonstrate that the magnetohydrodynamical equations of motion become dramatically different for this more realistic system. The shear-stress tensor no longer obeys a single differential equation; it breaks into three non-degenerate components with respect to the magnetic field, each evolving according to different dynamical equations. For large magnetic fields, we further show that the solution of this theory displays oscillatory behaviour that can no longer be described by an Israel-Stewart-like theory. Finally, we investigate the derived equations in a Bjorken flow scenario. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2402_01597 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Relativistic Dissipative Magnetohydrodynamics from the Boltzmann equation for a two-component gas Kushwah, Khwahish Denicol, Gabriel S. Nuclear Theory High Energy Astrophysical Phenomena High Energy Physics - Phenomenology We derive the equations of motion of relativistic magnetohydrodynamics, as well as microscopic expressions for all of its transport coefficients, from the Boltzmann equation using the method of moments. In contrast to reference Phys. Rev. D 98(7) 2018, where a single component gas was considered, we perform our derivation for a locally neutral fluid composed of two massless particle species with opposite charges. We demonstrate that the magnetohydrodynamical equations of motion become dramatically different for this more realistic system. The shear-stress tensor no longer obeys a single differential equation; it breaks into three non-degenerate components with respect to the magnetic field, each evolving according to different dynamical equations. For large magnetic fields, we further show that the solution of this theory displays oscillatory behaviour that can no longer be described by an Israel-Stewart-like theory. Finally, we investigate the derived equations in a Bjorken flow scenario. |
| title | Relativistic Dissipative Magnetohydrodynamics from the Boltzmann equation for a two-component gas |
| topic | Nuclear Theory High Energy Astrophysical Phenomena High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2402.01597 |