Generalized uncertainty principle corrections in Rastall–Rainbow Casimir wormholes

被引：0

作者：

Battista, Emmanuele ^{[1
,2
,3
]}

Capozziello, Salvatore ^{[1
,2
,4
]}

Errehymy, Abdelghani ^{[5
,6
]}

机构：

[1] Dipartimento di Fisica Ettore Pancini, Complesso Universitario di Monte S. Angelo, Università degli Studi di Napoli Federico II, Via Cintia Edificio 6, Naples,80126, Italy

[2] Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, Via Cintia Edificio 6, Naples,80126, Italy

[3] Quantum Theory Center (ħQTC) & D-IAS, Southern Denmark University, Campusvej 55, Odense M,5230, Denmark

[4] Scuola Superiore Meridionale, Largo San Marcellino 10, Naples,80138, Italy

[5] Astrophysics Research Centre, School of Mathematics, Statistics and Computer Science, University of KwaZulu-Natal, Private Bag X54001, Durban,4000, South Africa

[6] Department of General and Theoretical Physics, L.N. Gumilyov Eurasian National University, Astana,010008, Kazakhstan

来源：

European Physical Journal C | 2024年 / 84卷 / 12期

关键词：

120;

D O I：

10.1140/epjc/s10052-024-13656-y

中图分类号：

学科分类号：

摘要：

We explore wormhole solutions sourced by Casimir energy density involving generalized uncertainty principle corrections within the framework of Rastall–Rainbow gravity. The questions of traversability and stability, as well as the presence of exotic matter, are carefully investigated. In particular, the stability issue is addressed via an approach that has not been previously employed in the context of wormholes. This method, which represents an improved version of the so-called Herrera cracking technique, has the potential to yield novel insights in the field of wormhole geometries.

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