SABIR, I. und BHATTI, M.Z., 2026. Ghost star evolution with dissipative fluid in modified gravity. Nuclear Physics, Section B. 1 Januar 2026. Vol. 1022, , . DOI 10.1016/j.nuclphysb.2025.117284.
Elsevier - Harvard (with titles)Sabir, I., Bhatti, M., 2026. Ghost star evolution with dissipative fluid in modified gravity. Nuclear Physics, Section B 1022. https://doi.org/10.1016/j.nuclphysb.2025.117284
American Psychological Association 7th editionSabir, I., & Bhatti, M. (2026). Ghost star evolution with dissipative fluid in modified gravity. Nuclear Physics, Section B, 1022. https://doi.org/10.1016/j.nuclphysb.2025.117284
Springer - Basic (author-date)Sabir I, Bhatti M (2026) Ghost star evolution with dissipative fluid in modified gravity. Nuclear Physics, Section B 1022. https://doi.org/10.1016/j.nuclphysb.2025.117284
Juristische Zitierweise (Stüber) (Deutsch)Sabir, I./ Bhatti, M.Z., Ghost star evolution with dissipative fluid in modified gravity, Nuclear Physics, Section B 2026.