Black hole and Hawking radiation by type-II Weyl fermions

G. E. Volovik

doi:10.1134/S0021364016210050

Black hole and Hawking radiation by type-II Weyl fermions

G. E. Volovik^*

^*Corresponding author for this work

Landau Institute for Theoretical Physics

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Abstract

The type-II Weyl and type-II Dirac fermions may emerge behind the event horizon of black holes. Correspondingly the black hole can be simulated by creation of the region with overtilted Weyl or Dirac cones. The filling of the electronic states inside the “black hole” is accompanied by Hawking radiation. The Hawking temperature in the Weyl semimetals can reach the room temperature, if the black hole region is sufficiently small, and thus the effective gravity at the horizon is large.

Original language	English
Pages (from-to)	645–648
Number of pages	4
Journal	JETP Letters
Volume	104
Issue number	9
Early online date	3 Nov 2016
DOIs	https://doi.org/10.1134/S0021364016210050
Publication status	Published - Nov 2016
MoE publication type	A1 Journal article-refereed

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10.1134/S0021364016210050

Black hole and Hawking radiation by type-II Weyl fermionsAccepted author manuscript, 488 KB

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Black hole and Hawking radiation by type-II Weyl fermions

Abstract

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TOPVAC: From Topological Matter to Relativistic Quantum Vacuum

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Black hole and Hawking radiation by type-II Weyl fermions

Abstract

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TOPVAC: From Topological Matter to Relativistic Quantum Vacuum

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