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dc.contributor.authorBhattacharya, S.-
dc.contributor.authorChakrabortty, S.-
dc.contributor.authorGoyal, S.-
dc.date.accessioned2021-06-13T11:00:37Z-
dc.date.available2021-06-13T11:00:37Z-
dc.date.issued2021-06-13-
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1815-
dc.description.abstractWe discuss the field quantisation of a free massive Dirac fermion in the two causally disconnected static patches of the de Sitter spacetime, by using mode functions that are normalisable on the cosmological event horizon. Using this, we compute the entanglement entropy of the vacuum state corresponding to these two regions, for a given fermionic mode. Further extensions of this result to more general static spherically symmetric and stationary axisymmetric spacetimes are discussed. For the stationary axisymmetric Kerr-de Sitter spacetime in particular, the variations of the entanglement entropy with respect to various eigenvalues and spacetime parameters are depicted numerically. We also comment on such variations when instead we consider the non-extremal black hole event horizon of the same spacetime.en_US
dc.language.isoen_USen_US
dc.subjectde Sitteren_US
dc.subjectcosmological horizonen_US
dc.subjectfermionic entanglementen_US
dc.subjectstationary axisymmetric spacetimesen_US
dc.titleDirac fermion, cosmological event horizons and quantum entanglementen_US
dc.typeArticleen_US
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