| Possible Origin of Magnetic Fields in Very Dense Stars |
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| 摘 要： | We discuss the bosonization of a relativistic very dense Fermi gas in a magnetic field and the consequent BoseEinstein condensation of the resulting relativistic vector gas of charged particles. The model may be applied to paired spin-up electrons. We show that such systems may maintain self-consistently magnetic fields of order 10^10 - 10^13 G. That pairing could be the origin of large magnetic fields in some white dwarfs and neutron stars.For fields large enough (- 10^13 for white dwarfs), the system becomes unstable and collapses.
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| 关 键 词： | 磁场 费米气体 量子数 玻色子方程 |
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