BOOK ABSTRACT: Isospin physics entails the exploration of novel phenomena associated with the mass-to-charge, or neutron-to-proton, asymmetry of finite nuclei and nuclear matter. These properties influence the response of nuclei in energetic nuclear collisions, the dynamics of supernovae, as well as the structure and evolution of neutron stars. The ultimate goal of this new field of study is to generate an understanding of the nuclear many-body system in terms of an isospin-dependent nuclear equation of state and in-medium nucleonic interactions.

Equation of State of Dense Isospin-Asymmetric Nuclear Matter for Astrophysical Applications

BOMBACI, IGNAZIO
2001-01-01

Abstract

BOOK ABSTRACT: Isospin physics entails the exploration of novel phenomena associated with the mass-to-charge, or neutron-to-proton, asymmetry of finite nuclei and nuclear matter. These properties influence the response of nuclei in energetic nuclear collisions, the dynamics of supernovae, as well as the structure and evolution of neutron stars. The ultimate goal of this new field of study is to generate an understanding of the nuclear many-body system in terms of an isospin-dependent nuclear equation of state and in-medium nucleonic interactions.
2001
Bombaci, Ignazio
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/175151
 Attenzione

Attenzione! I dati visualizzati non sono stati sottoposti a validazione da parte dell'ateneo

Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
social impact