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Penrose Process: Its Variants and Astrophysical Applications

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F21%3AA0000109" target="_blank" >RIV/47813059:19630/21:A0000109 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.mdpi.com/2218-1997/7/11/416" target="_blank" >https://www.mdpi.com/2218-1997/7/11/416</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3390/universe7110416" target="_blank" >10.3390/universe7110416</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Penrose Process: Its Variants and Astrophysical Applications

  • Original language description

    We present a review of the Penrose process and its modifications in relation to the Kerr black holes and naked singularities (superspinars). We introduce the standard variant of this process, its magnetic version connected with magnetized Kerr black holes or naked singularities, the electric variant related to electrically charged Schwarzschild black holes, and the radiative Penrose process connected with charged particles radiating in the ergosphere of magnetized Kerr black holes or naked singularities. We discuss the astrophysical implications of the variants of the Penrose process, concentrating attention to the extreme regime of the magnetic Penrose process leading to extremely large acceleration of charged particles up to ultra-high energy E &amp; SIM;1022 eV around magnetized supermassive black holes with mass M &amp; SIM;1010M &amp; ODOT; and magnetic intensity B &amp; SIM;104 G. Similarly high energies can be obtained by the electric Penrose process. The extraordinary case is represented by the radiative Penrose process that can occur only around magnetized Kerr spacetimes but just inside their ergosphere, in contrast to the magnetic Penrose process that can occur in a more extended effective ergosphere determined by the intensity of the electromagnetic interaction. The explanation is simple, as the radiative Penrose process is closely related to radiated photons with negative energy whose existence is limited just to the ergosphere.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA19-03950S" target="_blank" >GA19-03950S: Testing strong gravity via black holes</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2021

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Universe

  • ISSN

    2218-1997

  • e-ISSN

  • Volume of the periodical

    7

  • Issue of the periodical within the volume

    11

  • Country of publishing house

    CH - SWITZERLAND

  • Number of pages

    35

  • Pages from-to

    „416-1“-„416-35“

  • UT code for WoS article

    000724852200001

  • EID of the result in the Scopus database

    2-s2.0-85119121935