General classification of charged test particle circular orbits in Reissner-Nordström spacetime
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F17%3AA0000025" target="_blank" >RIV/47813059:19240/17:A0000025 - isvavai.cz</a>
Výsledek na webu
<a href="https://link.springer.com/article/10.1140%2Fepjc%2Fs10052-017-4769-x" target="_blank" >https://link.springer.com/article/10.1140%2Fepjc%2Fs10052-017-4769-x</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1140/epjc/s10052-017-4769-x" target="_blank" >10.1140/epjc/s10052-017-4769-x</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
General classification of charged test particle circular orbits in Reissner-Nordström spacetime
Popis výsledku v původním jazyce
We investigate charged particles' circular motion in the gravitational field of a charged mass distribution described by the Reissner–Nordström spacetime. We introduce a set of independent parameters completely characterizing the different spatial regions in which circular motion is allowed. We provide a most complete classification of circular orbits for different sets of particle and source charge-to-mass ratios. We study both black holes and naked singularities and show that the behavior of charged particles depend drastically on the type of source. Our analysis shows in an alternative manner that the behavior of circular orbits can in principle be used to distinguish between black holes and naked singularities. From this analysis, special limiting values for the dimensionless charge of black hole and naked singularity emerge, namely, Q/M = 1/2, Q/M = sqroot (13)/5 and Q/M = sqroot (2/3) for the black hole case and Q/M = 1, Q/M = 5/(2 sqroot 6), Q/M = 3 sqroot (6)/7, and finally Q/M = sqroot (9/8) for the naked singularity case. Similarly and surprisingly, analogous limits emerge for the orbiting particles charge-to-mass ratio epsilon, for positive charges epsilon = 1, epsilon = 2 and epsilon = M/Q. These limits play an important role in the study of the coupled electromagnetic and gravitational interactions, and the investigation of the role of the charge in the gravitational collapse of compact objects.
Název v anglickém jazyce
General classification of charged test particle circular orbits in Reissner-Nordström spacetime
Popis výsledku anglicky
We investigate charged particles' circular motion in the gravitational field of a charged mass distribution described by the Reissner–Nordström spacetime. We introduce a set of independent parameters completely characterizing the different spatial regions in which circular motion is allowed. We provide a most complete classification of circular orbits for different sets of particle and source charge-to-mass ratios. We study both black holes and naked singularities and show that the behavior of charged particles depend drastically on the type of source. Our analysis shows in an alternative manner that the behavior of circular orbits can in principle be used to distinguish between black holes and naked singularities. From this analysis, special limiting values for the dimensionless charge of black hole and naked singularity emerge, namely, Q/M = 1/2, Q/M = sqroot (13)/5 and Q/M = sqroot (2/3) for the black hole case and Q/M = 1, Q/M = 5/(2 sqroot 6), Q/M = 3 sqroot (6)/7, and finally Q/M = sqroot (9/8) for the naked singularity case. Similarly and surprisingly, analogous limits emerge for the orbiting particles charge-to-mass ratio epsilon, for positive charges epsilon = 1, epsilon = 2 and epsilon = M/Q. These limits play an important role in the study of the coupled electromagnetic and gravitational interactions, and the investigation of the role of the charge in the gravitational collapse of compact objects.
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/GJ16-03564Y" target="_blank" >GJ16-03564Y: Konfigurace hmoty akreující v silném gravitačním poli kombinovaném s polem elektromagnetickým</a><br>
Návaznosti
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Ostatní
Rok uplatnění
2017
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
European Physical Journal C
ISSN
1434-6044
e-ISSN
1434-6052
Svazek periodika
77
Číslo periodika v rámci svazku
4
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
18
Strana od-do
'206-1'-'206-18'
Kód UT WoS článku
000403593700001
EID výsledku v databázi Scopus
2-s2.0-85017032397