Cuesta, H. J. M., Giraldo, F. H. Z., Pardo, W. D. A., Santrich, E. M., Franco, G. U. A., & Larrazabal, R. F. (2026). Asymptotic Freedom and Vacuum Polarization Determine the Astrophysical End State of Relativistic Gravitational Collapse: Quark--Gluon Plasma Star Instead of Black Hole.
Cita Chicago Style (17a ed.)Cuesta, Herman J. Mosquera, Fabián H. Zuluaga Giraldo, Wilmer D. Alfonso Pardo, Edgardo Marbello Santrich, Guillermo U. Avendaño Franco, y Rafael Fragozo Larrazabal. Asymptotic Freedom and Vacuum Polarization Determine the Astrophysical End State of Relativistic Gravitational Collapse: Quark--Gluon Plasma Star Instead of Black Hole. 2026.
Cita MLA (9a ed.)Cuesta, Herman J. Mosquera, et al. Asymptotic Freedom and Vacuum Polarization Determine the Astrophysical End State of Relativistic Gravitational Collapse: Quark--Gluon Plasma Star Instead of Black Hole. 2026.