05705nam 2200709 a 450 991046156910332120200520144314.066135564241-280-37851-497866135564241-60750-974-1(CKB)2670000000174829(EBL)888737(OCoLC)785394746(SSID)ssj0000656061(PQKBManifestationID)12262271(PQKBTitleCode)TC0000656061(PQKBWorkID)10631452(PQKB)11781905(MiAaPQ)EBC888737(Au-PeEL)EBL888737(CaPaEBR)ebr10551718(CaONFJC)MIL355642(EXLCZ)99267000000017482920111020d2011 uy 0engur|n|---|||||txtccrFrom the big bang to the nucleosynthesis[electronic resource] /Italian Physical Society ; edited by A. Bracco and E. NappiAmsterdam ;Washington, D.C. IOS Press20111 online resource (467 p.)Proceedings of the International School of Physics "Enrico Fermi",0074-784X ;course 178Description based upon print version of record.1-60750-973-3 Includes bibliographical references.Title page; Indice; Preface; Gruppo fotografico dei partecipanti al Corso; SUPERNOVAE AND NEUTRON STARS; Stellar evolution: From hydrostatic burning to core collapse; Introduction; Astrophysical nuclear reaction rates; Hydrostatic burning stages; Hydrogen burning; Solar neutrinos; Helium burning; Carbon, neon, oxygen, silicon burning; Core collapse supernovae; Electron captures in core-collapse supernovae - the general picture; Weak-interaction rates and presupernova evolution; The role of electron capture during collapse; Making heavy elements in explosive nucleosynthesis; The nu p processThe r-processNeutrino nucleosynthesis; The Facility for Antiproton and Ion Research (FAIR); The theory of Neutron Stars and the role of Nuclear Physics; Introduction; Overall structure of a Neutron Star; The outer crust; The inner crust; The outer core; The inner core; The free Fermi gas of nucleons; The Equation of State; The compressibility; Momentum distribution; The symmetry energy; The single particle density of states; The Pauli paramagnetism; Other microscopic physical quantities; Introducing the interaction; Sketch of the nucleon-nucleon interaction; Theoretical many-body methodsThe Brueckner-Bethe-Goldstone expansionThe variational method; The relativistic approach; The V low approach; Trying a link to QCD: the chiral symmetry approach; Neutron matter at very low density. An exercise in many-body theory; A single G-matrix problem; The ""exact"" EoS; Going to nuclear structure; The Thomas-Fermi approximation and implementations; The density functional method; Nuclear Physics and Neutron Star structure; The Neutron Star inner crust; The Neutron Star core and mass-radius relationship; Conclusions and outlook; Spin-isospin modes: Implications for astrophysicsIntroductionThe compression modes and incompressibility of nuclear matter; Spin-isospin excitations; GT strength in fp-shell nuclei; Determination of GT- strength; Determination of GT+ strength and its astrophysical implications; Conclusions and outlook; NUCLEAR STRUCTURE AND NUCLEAR ASTROPHYSICS WITH RADIOACTIVE BEAMS; Nuclear-astrophysics experiments with relativistic radioactive beams; Introduction; Experiments with high-energy radioactive beams at GSI; Mass measurements; The dipole response of exotic nuclei; Future perspectives-NuSTAR at FAIR; The FAIR facilityThe radioactive beam facilityExperiments with slowed-down and stopped beams; The low-energy branch; High-resolution in-flight spectroscopy (HISPEC); Decay spectroscopy (DESPEC); The advanced trapping system MATS; The laser-spectroscopy experiment LASPEC; Reactions with Relativistic Radioactive Beams (R3B); Experiments with stored and cooled beams; Isomeric beams, lifetimes, and masses (ILIMA); Reactions at internal targets in the NESR (EXL); Electron scattering with short-lived nuclei (ELISe); The Antiproton-Ion-Collider AIC; ConclusionNuclear structure studies at RIKEN: New measurements with in-flight fast radioactive beamsPhysicists have devoted much effort to reproducing the conditions of the primordial universe in laboratory conditions in their quest to work out a comprehensive theory of the appearance and evolution of nuclear matter. Whether it be trying to recreate the predicted primordial state of high-energy density matter in which quarks and gluons are effectively deconfined - the so-called Quark Gluon Plasma (QGP) - or exploring the structure and reaction properties of very unstable nuclei in experiments using radioactive beams, they have striven to understand the events which characterized the Big BangInternational School of Physics ""Enrico Fermi""NucleosynthesisCongressesBig bang theoryCongressesElectronic books.NucleosynthesisBig bang theory539.7Bracco A890399Nappi E633973Società italiana di fisica.International School of Physics "Enrico Fermi"MiAaPQMiAaPQMiAaPQBOOK9910461569103321From the big bang to the nucleosynthesis1989001UNINA