LEADER 01268nam0 2200277 i 450 001 SUN0046174 005 20090902120000.0 010 $a05-217-9310-6 100 $a20060608d2006 |0engc50 ba 101 $aeng 102 $aGB 105 $a|||| ||||| 200 1 $aˆThe ‰economics of education$ehuman capital, family background and inequality$fDaniele Checchi 210 $aCambridge$cCambridge university$d2006 215 $aXI, 278 p.$d24 cm. 620 $dCambridge$3SUNL000024 700 1$aChecchi$b, Daniele$3SUNV009663$09264 712 $aCambridge university$3SUNV000097$4650 801 $aIT$bSOL$c20181109$gRICA 912 $aSUN0046174 950 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI ECONOMIA$d03 PREST IIIFa1 verificare $e03 8135 950 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI GIURISPRUDENZA$d00 CONS XX.Ea.2 $e00 31976 995 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI ECONOMIA$bIT-CE0106$h8135$kPREST IIIFa1 verificare$oc$qa 995 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI GIURISPRUDENZA$h31976$kCONS XX.Ea.2$op$qa 996 $aEconomics of education$9716148 997 $aUNICAMPANIA LEADER 05705nam 2200709 a 450 001 9910461569103321 005 20200520144314.0 010 $a6613556424 010 $a1-280-37851-4 010 $a9786613556424 010 $a1-60750-974-1 035 $a(CKB)2670000000174829 035 $a(EBL)888737 035 $a(OCoLC)785394746 035 $a(SSID)ssj0000656061 035 $a(PQKBManifestationID)12262271 035 $a(PQKBTitleCode)TC0000656061 035 $a(PQKBWorkID)10631452 035 $a(PQKB)11781905 035 $a(MiAaPQ)EBC888737 035 $a(Au-PeEL)EBL888737 035 $a(CaPaEBR)ebr10551718 035 $a(CaONFJC)MIL355642 035 $a(EXLCZ)992670000000174829 100 $a20111020d2011 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aFrom the big bang to the nucleosynthesis$b[electronic resource] /$fItalian Physical Society ; edited by A. Bracco and E. Nappi 210 $aAmsterdam ;$aWashington, D.C. $cIOS Press$d2011 215 $a1 online resource (467 p.) 225 1 $aProceedings of the International School of Physics "Enrico Fermi",$x0074-784X ;$vcourse 178 300 $aDescription based upon print version of record. 311 $a1-60750-973-3 320 $aIncludes bibliographical references. 327 $aTitle 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 process 327 $aThe 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 methods 327 $aThe 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 astrophysics 327 $aIntroductionThe 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 facility 327 $aThe 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; Conclusion 327 $aNuclear structure studies at RIKEN: New measurements with in-flight fast radioactive beams 330 $aPhysicists have devoted much effort to reproducing the conditions of the primordial universe in laboratory conditions in their quest to work out a comprehensive theory of the appearance and evolution of nuclear matter. Whether it be trying to recreate the predicted primordial state of high-energy density matter in which quarks and gluons are effectively deconfined - the so-called Quark Gluon Plasma (QGP) - or exploring the structure and reaction properties of very unstable nuclei in experiments using radioactive beams, they have striven to understand the events which characterized the Big Bang 410 0$aInternational School of Physics ""Enrico Fermi"" 606 $aNucleosynthesis$vCongresses 606 $aBig bang theory$vCongresses 608 $aElectronic books. 615 0$aNucleosynthesis 615 0$aBig bang theory 676 $a539.7 701 $aBracco$b A$0890399 701 $aNappi$b E$0633973 712 02$aSocieta? italiana di fisica. 712 12$aInternational School of Physics "Enrico Fermi" 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910461569103321 996 $aFrom the big bang to the nucleosynthesis$91989001 997 $aUNINA