Covariant conserved currents for scalar-tensor Horndeski theory
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F18%3A10390189" target="_blank" >RIV/00216208:11320/18:10390189 - isvavai.cz</a>
Nalezeny alternativní kódy
RIV/68407700:21340/18:00328085
Výsledek na webu
<a href="https://doi.org/10.1063/1.5003190" target="_blank" >https://doi.org/10.1063/1.5003190</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.5003190" target="_blank" >10.1063/1.5003190</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Covariant conserved currents for scalar-tensor Horndeski theory
Popis výsledku v původním jazyce
The scalar-tensor theories have become popular recently in particular in connection with attempts to explain present accelerated expansion of the universe, but they have been considered as a natural extension of general relativity long time ago. The Horndeski scalar-tensor theory involving four invariantly defined Lagrangians is a natural choice since it implies field equations involving at most second derivatives. Following the formalisms of defining covariant global quantities and conservation laws for perturbations of spacetimes in standard general relativity, we extend these methods to the general Horndeski theory and find the covariant conserved currents for all four Lagrangians. The current is also constructed in the case of linear perturbations involving both metric and scalar fields. As a specific illustration, we derive a superpotential that leads to the covariantly conserved current in the Branse-Dicke theory.
Název v anglickém jazyce
Covariant conserved currents for scalar-tensor Horndeski theory
Popis výsledku anglicky
The scalar-tensor theories have become popular recently in particular in connection with attempts to explain present accelerated expansion of the universe, but they have been considered as a natural extension of general relativity long time ago. The Horndeski scalar-tensor theory involving four invariantly defined Lagrangians is a natural choice since it implies field equations involving at most second derivatives. Following the formalisms of defining covariant global quantities and conservation laws for perturbations of spacetimes in standard general relativity, we extend these methods to the general Horndeski theory and find the covariant conserved currents for all four Lagrangians. The current is also constructed in the case of linear perturbations involving both metric and scalar fields. As a specific illustration, we derive a superpotential that leads to the covariantly conserved current in the Branse-Dicke theory.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10300 - Physical sciences
Návaznosti výsledku
Projekt
<a href="/cs/project/GB14-37086G" target="_blank" >GB14-37086G: Centrum Alberta Einsteina pro gravitaci a astrofyziku</a><br>
Návaznosti
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Ostatní
Rok uplatnění
2018
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Journal of Mathematical Physics
ISSN
0022-2488
e-ISSN
—
Svazek periodika
59
Číslo periodika v rámci svazku
4
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
22
Strana od-do
—
Kód UT WoS článku
000431271800022
EID výsledku v databázi Scopus
2-s2.0-85045103955