Einstein-Grisaru-Zanon gravity

Detalles Bibliográficos
Parent link:Physics Letters B.— .— Amsterdam: Elsevier Science Publishing Company Inc.
Vol. 855.— 2024.— Article number 138811, 5 p.
Autor principal: Campos D. R.
Autor Corporativo: National Research Tomsk Polytechnic University (570)
Otros Autores: Ketov S. V. Sergey Vladimirovich
Sumario:Title screen
The leading (α′)3-correction to the gravitational low-energy effective action of closed (type II) superstring theory in four-spacetime dimensions defines the Einstein-Grisaru-Zanon gravity action that is applied for a calculation of the leading corrections to the Schwarzschild solution and the Hubble function in the Friedmann-Lemaitre-Robertson-Walker universe, in the first order with respect to the effective string-generated coupling. The solutions found are compared to the corresponding solutions in the Einstein-Bel-Robinson gravity that also modifies the Einstein gravity by the terms quartic in the spacetime curvature. We consider the black hole shadows in the Einstein-Grisaru-Zanon gravity theory and derive the upper bound on the string coupling parameter from the Hawking temperature of a black hole
Текстовый файл
AM_Agreement
Lenguaje:inglés
Publicado: 2024
Materias:
Acceso en línea:https://doi.org/10.1016/j.physletb.2024.138811
Formato: Electrónico Capítulo de libro
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=675432

MARC

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330 |a The leading (α′)3-correction to the gravitational low-energy effective action of closed (type II) superstring theory in four-spacetime dimensions defines the Einstein-Grisaru-Zanon gravity action that is applied for a calculation of the leading corrections to the Schwarzschild solution and the Hubble function in the Friedmann-Lemaitre-Robertson-Walker universe, in the first order with respect to the effective string-generated coupling. The solutions found are compared to the corresponding solutions in the Einstein-Bel-Robinson gravity that also modifies the Einstein gravity by the terms quartic in the spacetime curvature. We consider the black hole shadows in the Einstein-Grisaru-Zanon gravity theory and derive the upper bound on the string coupling parameter from the Hawking temperature of a black hole 
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701 1 |a Ketov  |b S. V.  |c physicist  |c Professor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences  |f 1960-  |g Sergey Vladimirovich  |9 19672 
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