Newman-Penrose formalism and exact vacuum solutions to conformal Weyl gravity
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21340%2F24%3A00380196" target="_blank" >RIV/68407700:21340/24:00380196 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1103/PhysRevD.110.124006" target="_blank" >https://doi.org/10.1103/PhysRevD.110.124006</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1103/PhysRevD.110.124006" target="_blank" >10.1103/PhysRevD.110.124006</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Newman-Penrose formalism and exact vacuum solutions to conformal Weyl gravity
Popis výsledku v původním jazyce
We study the exterior solution for a static, spherically symmetric source in Weyl conformal gravity in terms of the Newman-Penrose formalism. We first show that both the static, uncharged black hole solution of Mannheim and Kazanas and the static, charged Reissner-Nordstr & ouml;m-like solution can be found more easily in this formalism than in the traditional coordinate-basis approach, where the metric tensor components are taken as the basic variables. Second, we show that the Newman-Penrose formalism offers a particularly convenient framework that is well suited for the discussion of conformal gravity solutions corresponding to Petrov "type-D" spacetimes. This is illustrated with a two-parameter class of wormhole solutions that includes the Ellis-Bronnikov wormhole solution of Einstein's gravity as a limiting case. Other salient issues, such as the gauge equivalence of solutions and the inclusion of the electromagnetic field are also discussed.
Název v anglickém jazyce
Newman-Penrose formalism and exact vacuum solutions to conformal Weyl gravity
Popis výsledku anglicky
We study the exterior solution for a static, spherically symmetric source in Weyl conformal gravity in terms of the Newman-Penrose formalism. We first show that both the static, uncharged black hole solution of Mannheim and Kazanas and the static, charged Reissner-Nordstr & ouml;m-like solution can be found more easily in this formalism than in the traditional coordinate-basis approach, where the metric tensor components are taken as the basic variables. Second, we show that the Newman-Penrose formalism offers a particularly convenient framework that is well suited for the discussion of conformal gravity solutions corresponding to Petrov "type-D" spacetimes. This is illustrated with a two-parameter class of wormhole solutions that includes the Ellis-Bronnikov wormhole solution of Einstein's gravity as a limiting case. Other salient issues, such as the gauge equivalence of solutions and the inclusion of the electromagnetic field are also discussed.
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
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2024
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Physical Review D
ISSN
2470-0010
e-ISSN
2470-0029
Svazek periodika
110
Číslo periodika v rámci svazku
12
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
16
Strana od-do
—
Kód UT WoS článku
001375053200005
EID výsledku v databázi Scopus
2-s2.0-85211045180