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Steadiness of Stabilized Randall–Sundrum Model with Respect to Casimir Effectстатья
Информация о цитировании статьи получена из
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 1 октября 2025 г.
- Авторы: Rakhmetov E.R., Volobuev I.P., Keizerov S.I.
- Журнал: Physics of Particles and Nuclei
- Том: 56
- Номер: 2
- Год издания: 2025
- Издательство: Pleiades Publishing, Inc.
- Местоположение издательства: New York, USA
- Первая страница: 168
- Последняя страница: 172
- DOI: 10.1134/s1063779624701363
- Аннотация: The paper considers the Casimir effect in the stabilized Randall–Sundrum model, which arisesdue to the propagation of the gravitational field and the Goldberger–Wise scalar field in the five-dimensionalbulk between two branes. The Casimir energy density of the scalar modes is calculated analytically. Using thedimensional regularization method and writing the regularized energy density as the Hurwitz zeta function,divergences are identified and the Casimir energy density of the scalar modes is renormalized. Similar estimatesare made for the Casimir energy density of tensor modes. An estimate of the Casimir effect is madeconsidering all the modes on the equations and parameters of the model. It is found that such quantum correctionsdo not change the form of the solution of the equations of motion of the model and lead only to anegligible decrease in the background scalar field on the Planck brane and the distance between the branes;i.e., the model is stable with respect to the Casimir effect.
- Добавил в систему: Волобуев Игорь Павлович
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