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E-raamat: Solar Neutrino Physics: The Interplay between Particle Physics and Astronomy

  • Formaat: EPUB+DRM
  • Ilmumisaeg: 26-Feb-2020
  • Kirjastus: Blackwell Verlag GmbH
  • Keel: eng
  • ISBN-13: 9783527412730
  • Formaat - EPUB+DRM
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  • Formaat: EPUB+DRM
  • Ilmumisaeg: 26-Feb-2020
  • Kirjastus: Blackwell Verlag GmbH
  • Keel: eng
  • ISBN-13: 9783527412730

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A guide to the fascinating interplay between particle physics and astrophysics that highlights the discovery of neutrino oscillations

Written by three international experts on the topic, Solar Neutrino Physics offers a review of the status of solar physics with its strong link to neutrino physics. The book explores constitutive physics and the governing equations of standard solar models. The authors also review the theory of neutrinos in the Standard Model and the related detector experiments. The book contains a summary of the results from various experiments and develops a coherent view of the current state-of-the-art of solar neutrino physics.

Solar Neutrino Physics shows how solar models can be calibrated with the observational constraints of the age, mass, radius, and luminosity of the sun. The authors present general evolutionary properties of the sun as a star, past and future. They also discuss the solar neutrino production via the pp-chains and CNO-cycle, including the important role of the chemical composition of the sun. A very important source of information about the solar interior is offered by helioseismology, the study of solar oscillations. This important book:





Presents a high-level overview of the field of solar neutrino physics Brings together data and their interpretation of results obtained at various solar neutrino observatories Combines the theory of nuclear reactions with solar neutrino experiments Contains a review of SNO+, JUNO, LENA, Hyper-Kamiokande, and DUNE.

Written for astronomers, physicists, and high energy physicists, Solar Neutrino Physics contains a review of the field of neutrino physics, the relevant equations, and the impact of matter on the behavior of neutrino oscillations.
1 Introduction
1(2)
2 Solar Structure and Evolution
3(66)
2.1 Equations of Stellar Structure and Evolution
3(15)
2.1.1 Mechanical Structure
3(2)
2.1.2 Energy Conservation and Transport
5(1)
2.1.2.1 Energy Transport by Radiation and Conduction
5(2)
2.1.2.2 Criterion for Dynamical Instability
7(2)
2.1.2.3 Energy Transport: Convection
9(2)
2.1.3 Changes in Chemical Composition
11(1)
2.1.3.1 Convective Mixing
11(1)
2.1.3.2 Changes in Chemical Composition: Atomic Diffusion
12(3)
2.1.3.3 Changes in Chemical Composition: Nuclear Reactions
15(1)
2.1.3.4 Changes in Chemical Composition: Putting Everything Together
16(1)
2.1.4 Full Set of Equations and Boundary Conditions
17(1)
2.2 Constitutive Physics
18(13)
2.2.1 Equation of State
18(3)
2.2.2 Radiative Opacities
21(4)
2.2.3 Nuclear Reaction Rates
25(6)
2.3 Calibrating Standard Solar Models
31(5)
2.3.1 Observational Constraints
31(1)
2.3.1.1 Age, Mass, Radius, and Luminosity
31(1)
2.3.1.2 Surface Composition
32(3)
2.3.2 Adjusting the Free Parameters
35(1)
2.4 Standard Solar Models
36(6)
2.4.1 Previous and Future Evolution
36(3)
2.4.2 The Sun Today: An Overview
39(3)
2.5 Solar Neutrinos
42(6)
2.6 Helioseismology
48(6)
2.6.1 Overview
48(3)
2.6.2 Global Structure Inversions
51(2)
2.6.3 Other Constraints
53(1)
2.7 Solar Abundance Problem
54(4)
2.8 Uncertainties in SSMs
58(4)
2.8.1 Uncertainties in SSM Inputs
58(1)
2.8.1.1 Nuclear Reaction Rates
58(1)
2.8.1.2 Microscopic Diffusion
59(1)
2.8.1.3 Radiative Opacities
59(1)
2.8.1.4 Solar Radius, Luminosity, and Age
59(1)
2.8.1.5 Solar Composition
59(1)
2.8.1.6 Equation of State
60(1)
2.8.2 Global Uncertainties in SSMs
60(1)
2.8.2.1 Nuclear Reaction Rates
61(1)
2.8.2.2 Constitutive Physics
61(1)
2.8.2.3 Element Abundances
62(1)
2.9 Solar Models Beyond the SSM
62(7)
2.9.1 Nonstandard Solar Physics
63(2)
2.9.2 Nonstandard Particle Physics
65(4)
3 Neutrino Physics
69(70)
3.1 Neutrinos in the Standard Model
69(6)
3.2 Neutrino Oscillations
75(5)
3.3 Matter Effects
80(4)
3.4 Neutrino Oscillation Experiments
84(25)
3.4.1 Atmospheric Neutrinos
84(8)
3.4.2 Long Baseline Accelerator Neutrinos
92(5)
3.4.2.1 Long Baseline Experiments and θ13
97(3)
3.4.3 Reactor Neutrinos
100(9)
3.5 Conclusions and Open Questions
109(30)
3.5.1 What Is the Absolute Neutrino Mass Scale?
111(9)
3.5.2 Are Neutrinos Majorana or Dirac Particles?
120(7)
3.5.3 What Is the Neutrino Mass Ordering and How Large Is CP-δ?
127(8)
3.5.4 Are There Sterile Neutrinos?
135(4)
4 Solar Neutrino Experiments
139(56)
4.1 Introduction
139(2)
4.2 The 37Cl Experiment
141(4)
4.3 Kamiokande-II/III
145(8)
4.4 The 71Ga Experiments
153(9)
4.5 Super-Kamiokande
162(7)
4.6 SNO
169(9)
4.7 Borexino
178(13)
4.8 Summary and Open Questions
191(4)
5 Future Solar Neutrino Experiments
195(14)
5.1 SNO+
196(3)
5.2 Juno And Lena
199(5)
5.3 Hyper-Kamiokande
204(2)
5.4 Dune
206(3)
References 209(12)
Index 221
Lothar Oberauer is professor for Astroparticle physics at the Technical University of Munich, Germany.

Aldo Ianni is a senior researcher and head of Research Division at the Gran Sasso Laboratory, Italy.

Aldo Serenelli is Tenured Researcher at the Institute of Space Sciences, in Bellaterra, near Barcelona, Spain.