LEADER 05692nam 2200745Ia 450 001 9910465776903321 005 20200520144314.0 010 $a1-281-16005-9 010 $a1-4294-8843-3 010 $a9786611160050 010 $a0-19-152322-4 035 $a(CKB)2560000000298253 035 $a(EBL)415331 035 $a(OCoLC)476241776 035 $a(SSID)ssj0000159939 035 $a(PQKBManifestationID)11154629 035 $a(PQKBTitleCode)TC0000159939 035 $a(PQKBWorkID)10158692 035 $a(PQKB)10827325 035 $a(SSID)ssj0000385425 035 $a(PQKBManifestationID)11321546 035 $a(PQKBTitleCode)TC0000385425 035 $a(PQKBWorkID)10374044 035 $a(PQKB)22527426 035 $a(StDuBDS)EDZ0000072464 035 $a(MiAaPQ)EBC415331 035 $a(Au-PeEL)EBL415331 035 $a(CaPaEBR)ebr10271455 035 $a(CaONFJC)MIL116005 035 $a(EXLCZ)992560000000298253 100 $a20070723d2007 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aFundamentals of neutrino physics and astrophysics$b[electronic resource] /$fCarlo Giunti, Chung W. Kim 210 $aOxford ;$aNew York $cOxford University Press$d2007 215 $a1 online resource (727 p.) 300 $aDescription based upon print version of record 311 $a0-19-850871-9 311 $a0-19-170886-0 320 $aIncludes bibliographical references (p. [671]-704) and index. 327 $aContents; 1 Historical introduction; 2 Quantized Dirac fields; 2.1 Dirac equation; 2.2 Representations of ? matrices; 2.3 Products of ? matrices; 2.4 Relativistic covariance; 2.5 Helicity; 2.6 Gauge transformations; 2.7 Chirality; 2.8 Solution of the Dirac equation; 2.9 Quantization; 2.10 Symmetry transformation of states; 2.11 C, P, and T transformations; 2.12 Wave packets; 2.13 Finite normalization volume; 2.14 Fierz transformations; 3 The Standard Model; 3.1 Electroweak Lagrangian; 3.2 Electroweak interactions; 3.3 Three generations; 3.4 The Higgs mechanism; 3.5 Fermion masses and mixing 327 $a3.6 Gauge bosons3.7 Effective low-energy CC and NC Lagrangians; 4 Three-generation mixing; 4.1 Diagonalization of the mass matrix; 4.2 Physical parameters in the mixing matrix; 4.3 Parameterization of the mixing matrix; 4.4 Degenerate masses; 4.5 Mixing matrix with one vanishing element; 4.6 CP violation; 4.7 Rephasing invariants; 4.8 Unitarity triangles; 4.9 Conditions for CP violation; 5 Neutrino interactions; 5.1 Neutrino-electron interactions; 5.2 Hadron decays; 5.3 Neutrino-nucleon scattering; 6 Massive neutrinos; 6.1 Dirac masses; 6.2 Majorana neutrinos 327 $a6.3 Mixing of three Majorana neutrinos6.4 One-generation Dirac-Majorana mass term; 6.5 Three-generation Dirac-Majorana mixing; 6.6 Special cases; 6.7 Majorana mass matrix; 7 Neutrino oscillations in vacuum; 7.1 Standard Derivation of the Neutrino Oscillation Probability; 7.2 Antineutrino case; 7.3 CPT, CP, and T transformations; 7.4 Two-neutrino mixing; 7.5 Types of neutrino oscillation experiments; 7.6 Averaged transition probability; 7.7 Large ?m[sup(2)] dominance; 7.8 Active small ?m[sup(2)]; 8 Theory of neutrino oscillations in vacuum; 8.1 Plane-wave approximation 327 $a8.2 Wave-packet treatment8.3 Size of neutrino wave packets; 8.4 Questions; 9 Neutrino oscillations in matter; 9.1 Effective potentials in matter; 9.2 Evolution of neutrino flavors; 9.3 The MSW effect; 9.4 Slab approximation; 9.5 Parametric resonance; 9.6 Geometrical representation; 10 Solar neutrinos; 10.1 Thermonuclear energy production; 10.2 Standard solar models; 10.3 Model-independent constraints on solar neutrino fluxes; 10.4 Homestake experiment; 10.5 Gallium experiments; 10.6 Water Cherenkov detectors; 10.7 Vacuum oscillations; 10.8 Resonant flavor transitions in the Sun 327 $a10.9 Regeneration of solar ?[sub(e)]'s in the Earth10.10 Global fit of solar neutrino data; 11 Atmospheric neutrinos; 11.1 Flux of atmospheric neutrinos; 11.2 Atmospheric neutrino experiments; 12 Terrestrial neutrino oscillation experiments; 12.1 Sensitivity; 12.2 Reactor experiments; 12.3 Accelerator experiments; 13 Phenomenology of three-neutrino mixing; 13.1 Neutrino oscillations in vacuum; 13.2 Matter effects; 13.3 Analysis of oscillation data; 14 Direct measurements of neutrino mass; 14.1 Beta decay; 14.2 Pion and tau decays; 14.3 Neutrinoless double-beta decay; 15 Supernova neutrinos 327 $a15.1 Supernova types 330 $aOur Universe is made of a dozen fundamental building blocks. Among these, neutrinos are the most mysterious - but they are the second most abundant particles in the Universe. This book provides detailed discussions of how to describe neutrinos, their basic properties, and the roles they play in nature. - ;This book deals with neutrino physics and astrophysics - a field in which some of the most exciting recent developments in particle physics, astrophysics and cosmology took place. The book is the most up-to-date, comprehensive and self-contained treatment of key issues in neutrino physics. It 606 $aNeutrino astrophysics 606 $aNeutrinos 608 $aElectronic books. 615 0$aNeutrino astrophysics. 615 0$aNeutrinos. 676 $a539.7215 700 $aGiunti$b Carlo$0509201 701 $aKim$b Chung Wook$f1934-$053010 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910465776903321 996 $aFundamentals of neutrino physics and astrophysics$9769390 997 $aUNINA