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^*

^*Tämän työn vastaava kirjoittaja

Russian Academy of Sciences, Landau Institute

Tutkimustuotos: Lehtiartikkeli › Article › Scientific › vertaisarvioitu

92 Sitaatiot (Scopus)

208 Lataukset (Pure)

Abstrakti

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.

Alkuperäiskieli	Englanti
Sivut	645–648
Sivumäärä	4
Julkaisu	JETP Letters
Vuosikerta	104
Numero	9
Varhainen verkossa julkaisun päivämäärä	3 marrask. 2016
DOI - pysyväislinkit	https://doi.org/10.1134/S0021364016210050
Tila	Julkaistu - marrask. 2016
OKM-julkaisutyyppi	A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä

Pääsy asiakirjaan

10.1134/S0021364016210050

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

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Link to publication in Scopus

TOPVAC: From Topological Matter to Relativistic Quantum Vacuum
Volovik, G., Nissinen, J., Eltsov, V., Rysti, J., Rantanen, R., Mäkinen, J., Zhang, K., Volard, M., Kamppinen, T. & Ikäheimo, A.
01/10/2016 → 30/09/2022
Projekti: EU: ERC grants

Siteeraa tätä

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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.",

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N2 - 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.

AB - 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.

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Black hole and Hawking radiation by type-II Weyl fermions

Abstrakti

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Muut tiedostot ja linkit

Sormenjälki

Projektit

TOPVAC: From Topological Matter to Relativistic Quantum Vacuum

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