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Exploring the stability of ultra-compact anisotropic dark energy stars with maximum allowable mass in $$R+\chi (R^{2}+\eta R^{3})$$ gravity

Crossref DOI link: https://doi.org/10.1140/epjc/s10052-025-14120-1

Published Online: 2025-04-23

Update policy: https://doi.org/10.1007/springer_crossmark_policy

Authors

Nazar, Hammad https://orcid.org/0000-0001-6570-7953
Abbas, Ghulam https://orcid.org/0000-0002-4525-566X
Shahzad, M. R. https://orcid.org/0000-0001-9128-4018
Ashraf, Asifa https://orcid.org/0000-0001-5522-5491
Hakami, Ali H. https://orcid.org/0000-0001-6499-097X
Mubaraki, Ali M. https://orcid.org/0000-0003-1951-4565
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Text and Data Mining valid from 2025-04-23

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Article History

Received: 14 February 2025

Accepted: 22 March 2025

First Online: 23 April 2025

Copyright Information

Copyright Statement: 2025 The Author(s)

Copyright Holder: The Author(s)

Copyright Year: 2025