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``Cosmological'' scenario for A-B phase transition in superfluid 3He

Yu. M. Bunkov, O. D. Timofeevskaya

cond-mat.supr-conarXiv:cond-mat/9706004

Abstract

At a very rapid superfluid transition in 3He, follows after a reaction with single neutron, the creation of topological defects (vortices) has recently been demonstrated in accordance with the Kibble-Zurek scenario for the cosmological analogue. We discuss here the extension of the Kibble-Zurek scenario to the case when alternative symmetries may be broken and different states nucleated independently. We have calculated the nucleation probability of the various states of superfluid 3He during a superfluid transition. Our results can explain the transition from supercooled A phase to the B phase, triggered by nuclear reaction. The new scenario is an alternative to the well-known ``baked Alaska'' scenario.

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