A Model for Cosmic Magnetic Field Amplification: Effects of Pressure Anisotropy Perturbations
Magnetic field amplification in the early universe is a long-standing problem that has been extensively studied through theoretical and numerical approaches, focusing on turbulent dynamos and the growth of collisionless plasma instabilities. In the post-recombination era, pressure anisotropy drives...
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| Format: | Article |
| Language: | English |
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MDPI AG
2024-12-01
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| Series: | Universe |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2218-1997/11/1/9 |
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