2026-06-27T12:35:51Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/1021832025-03-18T12:28:11Zcom_20.500.14352_14col_20.500.14352_15

Azad, Bahareh Blázquez Salcedo, José Luis Khoo, Fech Scen Kunz, Jutta 2024-03-12T19:09:30Z 2024-03-12T19:09:30Z 2024-01 0370-2693 10.1016/j.physletb.2023.138349 https://hdl.handle.net/20.500.14352/102183 1873-2445 https://www.sciencedirect.com/science/article/pii/S0370269323006834 We investigate the radial perturbations of Ellis-Bronnikov wormholes (l = 0) in a slowly rotating background expanded up to second order in rotation. We find indications that simple wormhole solutions such as Ellis-Bronnikov in General Relativity can be stabilized by rotation, thus favoring a viable traversable wormhole. This opens up the intriguing question whether the many other wormhole solutions with or without the support of exotic matter can become linearly mode stable when the wormhole rotates. eng http://creativecommons.org/licenses/by/4.0/ open access Attribution 4.0 International Are slowly rotating Ellis-Bronnikov wormholes stable? journal article