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Exploding Bose-Einstein condensates and collapsing neutron stars driven by critical magnetic fields

机译:爆炸的玻色 - 爱因斯坦凝聚物和坍缩的中子星驱动   通过临界磁场

摘要

The problem of a condensate of a relativistic neutral vector boson gasconstituted of particles bearing a magnetic moment is discussed. Such a vectorboson system is expected to be formed either by parallel spin-pairing ofneutrons in a sufficiently strong magnetic field, or by neutral atoms underspecific conditions of magnetic field strength and density. A strongself-magnetization arises due to a Bose-Einstein-like condensation. Then thesystem, which may resemble the superfluid said to exist in the core of neutronstars, becomes more unstable under transverse collapse than the ordinaryfermion gas. In the nonrelativistic limit of laboratory conditions, an analogywith the behavior of exploding Bose-Einstein condensates for critical values ofmagnetic field strength and particle density; reported by several authors, isbriefly discussed.
机译:讨论了相对论的中性矢量玻色子气体的凝结问题,该玻色子由带有磁矩的粒子构成。期望通过在足够强的磁场中将中子平行自旋配对或在磁场强度和密度的特定条件下由中性原子形成这样的矢量玻色子系统。由于类似玻色-爱因斯坦的凝聚,产生了强自磁化。然后,该系统可能类似于据说存在于中子星核中的超流体,在横向塌陷下比普通费米子气更加不稳定。在实验室条件的非相对论极限中,类似于磁场强度和粒子密度的临界值的玻色-爱因斯坦凝聚物爆炸的行为。简短地讨论了几位作者的报道。

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