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Cosmology, particle physics, and superfluid 3He

1996/06/01 by G. E. Volovik · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #Quantum, superfluid, helium dynamics #Superconductivity in MgB2 and Alloys #cond-mat #gr-qc #hep-th

paper · pdf · doi:10.1007/bf02548109

published as Czech.J.Phys.46:3048,1996 · Invited talk at LT-21 Conference, 20 pages, 3 figures available at request, compressed ps file of the camera-ready format with 3 figures is at ftp://boojum.hut.fi/pub/publications/lowtemp/LTL-96006.ps.gz

openalex publication_date 1996/06/01 · arxiv created 1996/07/30 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Many direct parallels connect superfluid 3He with the field theories describing the physical vacuum, gauge fields and elementary fermions. Superfluid 3He exhibits a variety of topological defects which can be detected with single-defect sensitivity. Modern scenarios of defect-mediated baryogenesis can be simulated by the interaction of the 3He vortices and domain walls with fermionic quasiparticles. Formation of defects in a symmetry-breaking phase transition in the early Universe, which could be responsible for large-scale structure formation and for microwave-background anisotropy, also may be modelled in the laboratory. This is supported by the recent observation of vortex formation in neutron-irradiated 3He-B where the "primordial fireball" is formed in an exothermic nuclear reaction.

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