Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki
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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2016, Volume 104, Issue 9, Pages 660–661
DOI: https://doi.org/10.7868/S0370274X16210104 (Mi jetpl5108) 		 
This article is cited in 57 scientific papers (total in 57 papers)

MISCELLANEOUS

Black hole and hawking radiation by type-II Weyl fermions

G. E. Volovikab

a Landau Institute for Theoretical Physics, 142432 Chernogolovka, Russia
b Low Temperature Laboratory, Aalto University, FI-00076 Aalto, Finland
Full-text PDF (136 kB) Citations (57)
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DOI: https://doi.org/10.7868/S0370274X16210104
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.
Funding agency Grant number
European Research Council 694248-TOPVAC
I acknowledge financial support from the European Research Council, Advanced Grant project 694248–TOPVAC.
Received: 03.10.2016
English version:
Journal of Experimental and Theoretical Physics Letters, 2016, Volume 104, Issue 9, Pages 645–648
DOI: https://doi.org//10.1134/S0021364016210050
Bibliographic databases:
Document Type: Article
Language: English
Citation: G. E. Volovik, “Black hole and hawking radiation by type-II Weyl fermions”, Pis'ma v Zh. Èksper. Teoret. Fiz., 104:9 (2016), 660–661; JETP Letters, 104:9 (2016), 645–648
Citation in format AMSBIB
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    • This publication is cited in the following 57 articles:
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    		Письма в Журнал экспериментальной и теоретической физики Pis'ma v Zhurnal Иksperimental'noi i Teoreticheskoi Fiziki
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