Monopole magnetohydrodynamics on a plane: Magnetosonic waves and dynamo instability
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| Autores principales: | , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866913764780015616 |
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| author | Banerjee, Debarghya Moessner, Roderich Surówka, Piotr |
| author_facet | Banerjee, Debarghya Moessner, Roderich Surówka, Piotr |
| contents | Condensed matter systems can host emergent `vacua' with particles, fields and dimension different from that of the universe we inhabit. Motivated by the appearance of emergent gauge fields with both electric and magnetic charges, we consider the fate of electromagnetism in two dimensions in the presence of magnetic monopoles. We find that generically electromagnetic fields are damped due to resistive effects. However, we can still identify a magnetohydrodynamic regime. It exhibits magnetosonic waves which, unlike in $d=3$, are isotropic, to which there is a contribution from the odd viscosity coefficient present in the system. Further, we find a dynamo action, which unlike in $d=3$ requires compressibility of the flow. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_09562 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Monopole magnetohydrodynamics on a plane: Magnetosonic waves and dynamo instability Banerjee, Debarghya Moessner, Roderich Surówka, Piotr Strongly Correlated Electrons High Energy Physics - Theory Condensed matter systems can host emergent `vacua' with particles, fields and dimension different from that of the universe we inhabit. Motivated by the appearance of emergent gauge fields with both electric and magnetic charges, we consider the fate of electromagnetism in two dimensions in the presence of magnetic monopoles. We find that generically electromagnetic fields are damped due to resistive effects. However, we can still identify a magnetohydrodynamic regime. It exhibits magnetosonic waves which, unlike in $d=3$, are isotropic, to which there is a contribution from the odd viscosity coefficient present in the system. Further, we find a dynamo action, which unlike in $d=3$ requires compressibility of the flow. |
| title | Monopole magnetohydrodynamics on a plane: Magnetosonic waves and dynamo instability |
| topic | Strongly Correlated Electrons High Energy Physics - Theory |
| url | https://arxiv.org/abs/2406.09562 |