Wolter, H. H.Gaitanos, T.Di Toro, M.Colonna, M.Ferini, G.Lalazissis, G. A.We present several possibilities offered by nuclear structure, the dynamics of intermediate energy heavy ion collisions and neutron stars to investigate the nuclear matter equation of state (EoS) beyond the ground state. In particular the high density nuclear EoS of asymmetric matter, i.e. the symmetry energy, is discussed.application/pdfhttps://eproceedings.epublishing.ekt.gr/index.php/hnps/article/view/263810.12681/hnps.2638engHellenic Nuclear Physics Society (HNPS)Πνευματική ιδιοκτησία (c) 2019 T. Gaitanos, G. Ferini, M. Colonna, M. Di Toro, G. A. Lalazissis, H. H. WolterAnnual Symposium of the Hellenic Nuclear Physics Society2654-00882654-007XAnnual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 15 (2006): HNPS2006; 196-201HNPS Advances in Nuclear Physics; Vol. 15 (2006): HNPS2006; 196-201heavy ion collisionsequation of stateneutron starssymmetry energystrangeness ratiomaximum mass constraintproton fractionNuclear matterfinite nucleiDirect Urca processConstraints on EOS from finite nuclei, heavy ion collisions and neutron starsinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion2020-01-01Πυρηνική φυσικήNuclear Physicsisi - Physics, Nuclear includes resources on the study of nuclear structure, decay, radioactivity, reactions, and scattering. Resources in this category focus on low-energy physics. High-energy physics is covered in the PHYSICS, PARTICLES & FIELDS category.Άρθρο συνεδρίουConference articleΕπιστημονικό άρθροScientific articleHellenic Nuclear Physics SocietyGreek Aggregator OpenArchives.gr | National Documentation Centre (EKT)other