Fifty Years of Energy Extraction from Rotating Black Hole: Revisiting Magnetic Penrose Process
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F19%3AA0000552" target="_blank" >RIV/47813059:19240/19:A0000552 - isvavai.cz</a>
Výsledek na webu
<a href="https://www.mdpi.com/2218-1997/5/5/125" target="_blank" >https://www.mdpi.com/2218-1997/5/5/125</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3390/universe5050125" target="_blank" >10.3390/universe5050125</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Fifty Years of Energy Extraction from Rotating Black Hole: Revisiting Magnetic Penrose Process
Popis výsledku v původním jazyce
Magnetic Penrose process (MPP) is not only the most exciting and fascinating process mining the rotational energy of black hole but it is also the favored astrophysically viable mechanism for high energy sources and phenomena. It operates in three regimes of efficiency, namely low, moderate and ultra, depending on the magnetization and charging of spinning black holes in astrophysical setting. In this paper, we revisit MPP with a comprehensive discussion of its physics in different regimes, and compare its operation with other competing mechanisms. We show that MPP could in principle foot the bill for powering engine of such phenomena as ultra-high-energy cosmic rays, relativistic jets, fast radio bursts, quasars, AGNs, etc. Further, it also leads to a number of important observable predictions. All this beautifully bears out the promise of a new vista of energy powerhouse heralded by Roger Penrose half a century ago through this process, and it has today risen in its magnetically empowered version of mid 1980s from a purely thought experiment of academic interest to a realistic powering mechanism for various high-energy astrophysical phenomena.
Název v anglickém jazyce
Fifty Years of Energy Extraction from Rotating Black Hole: Revisiting Magnetic Penrose Process
Popis výsledku anglicky
Magnetic Penrose process (MPP) is not only the most exciting and fascinating process mining the rotational energy of black hole but it is also the favored astrophysically viable mechanism for high energy sources and phenomena. It operates in three regimes of efficiency, namely low, moderate and ultra, depending on the magnetization and charging of spinning black holes in astrophysical setting. In this paper, we revisit MPP with a comprehensive discussion of its physics in different regimes, and compare its operation with other competing mechanisms. We show that MPP could in principle foot the bill for powering engine of such phenomena as ultra-high-energy cosmic rays, relativistic jets, fast radio bursts, quasars, AGNs, etc. Further, it also leads to a number of important observable predictions. All this beautifully bears out the promise of a new vista of energy powerhouse heralded by Roger Penrose half a century ago through this process, and it has today risen in its magnetically empowered version of mid 1980s from a purely thought experiment of academic interest to a realistic powering mechanism for various high-energy astrophysical phenomena.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
<a href="/cs/project/EF16_027%2F0008521" target="_blank" >EF16_027/0008521: Podpora mezinárodní mobility výzkumných pracovníků na SU</a><br>
Návaznosti
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Universe
ISSN
2218-1997
e-ISSN
—
Svazek periodika
5
Číslo periodika v rámci svazku
5
Stát vydavatele periodika
CH - Švýcarská konfederace
Počet stran výsledku
25
Strana od-do
„125-1“-„125-25“
Kód UT WoS článku
000470958800030
EID výsledku v databázi Scopus
2-s2.0-85067685205