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  • Produktbild: Nuclei in the Cosmos
  • Produktbild: Nuclei in the Cosmos

Nuclei in the Cosmos

Aus der Reihe Graduate Texts in Contemporary Physics

Fr. 72.90

inkl. gesetzl. MwSt., Versandkostenfrei

Beschreibung

Produktdetails

Einband

Taschenbuch

Erscheinungsdatum

27.06.2012

Herausgeber

Heinz Oberhummer

Verlag

Springer Berlin

Seitenzahl

236

Maße (L/B/H)

23.5/15.5/1.4 cm

Gewicht

388 g

Auflage

Softcover reprint of the original 1st ed. 1991

Sprache

Englisch

ISBN

978-3-642-48842-9

Beschreibung

Produktdetails

Einband

Taschenbuch

Erscheinungsdatum

27.06.2012

Herausgeber

Heinz Oberhummer

Verlag

Springer Berlin

Seitenzahl

236

Maße (L/B/H)

23.5/15.5/1.4 cm

Gewicht

388 g

Auflage

Softcover reprint of the original 1st ed. 1991

Sprache

Englisch

ISBN

978-3-642-48842-9

Herstelleradresse

Springer-Verlag KG
Sachsenplatz 4-6
1201 Wien
AT

Email: GPSR Kontakt

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  • Produktbild: Nuclei in the Cosmos
  • Produktbild: Nuclei in the Cosmos
  • Experimental Determination of Stellar Reaction Rates.- 1. Introduction.- 2. Direct Measurements.- 3. Indirect Approaches.- 4. Reactions Involving Radioactive Nuclides.- References.- Radioactive Ion Beams in Nuclear Astrophysics.- 1. Introduction.- 2. Interest of Radioactive Ion Beams in Nuclear Astrophysics.- 2.1 Nuclear Reactions of Astrophysical Interest Involving Radioactive Nuclei.- 2.2 Indirect Methods.- 2.3 Radioactive Ion Beams Versus Radioactive Targets.- 2.4 Remarks.- 3. Production of Radioactive Ion Beams.- 3.1 The Two Methods.- 3.2 Radioactive Ion Beams Produced by the Two-Accelerator Method.- 3.3 Proposals for RIB Production by the Two-Accelerator Method.- 4. Special Experimental Techniques in Nuclear Astrophysics Using Radioactive Ion Beams.- 4.1 Introduction.- 4.2 Targets.- 4.3 On-line Detectors.- 4.4 Off-line Detectors.- 5. Conclusions.- References.- Direct Reaction Mechanism in Astrophysically Relevant Processes.- 1. Introduction.- 2. Qualitative Features of Nuclear Reaction Mechanisms.- 3. Nuclear Reactions in Astrophysical Scenarios.- 4. Optical Potentials.- 5. Theoretical Descriptions of Direct Reactions.- 6. Examples.- 6.1 Transfer Reactions with Non-resonant Behaviour.- 6.2 Transfer Reactions with Resonant Behaviour.- 6.3 Direct Capture.- 7. Summary.- Acknowledgements.- References.- Nuclear Reaction Rates — from Laboratory Experiments and in the Stellar Plasma.- 1. Introduction.- 2. Theoretical Models for Extrapolating Measured Data.- 2.1 Example: The 12C(?,?)16O E1 Capture Reaction.- 2.2 The 12C(?,?)16O E2 Capture at Astrophysical Energies.- 3. Electron Screening in Laboratory Experiments.- 4. Screening Effects in the Plasma.- References.- Abundances in Galaxies.- 1. Introduction.- 2. Big Bang Nucleosynthesis and Light Element Abundances.- 3. Abundance Trends Between and Across Galaxies.- 4. Stellar Populations in Our Galaxy.- 5. Differential Abundance Variations Among Elements.- References.- Nuclei in Cosmic Rays.- 1. Introduction.- 2. Techniques for Measuring Composition from Satellites and Balloons.- 2.1 Electronic Detectors: The “Chicago Egg”.- 2.2 An Emulsion Experiment: JACEE.- 3. Results of Satellite and Balloon Experiments.- 4. How to Measure Cosmic Ray Composition above 1015 eV.- 4.1 Outline of Extensive Air Showers.- 4.2 Extensive Air Shower Properties Sensitive to Primary Particle Mass.- 4.3 A Proposed Experiment: KASCADE.- 5. Summary.- References.- Primordial Nucleosynthesis: Beyond the Standard Model.- 1. Introduction.- 2. Standard Primordial Nucleosynthesis.- 3. Observational Tests of the Standard Model.- 3.1 Helium.- 3.2 Lithium.- 4. The QCD Phase Transition.- 5. Neutrinos in the Early Universe.- 5.1 Sterile Neutrinos.- 5.2 Neutrino Oscillations.- 6. Cosmic Strings.- 7. Conclusions.- References.- Production of Heavy Elements in Inhomogeneous Cosmologies.- 1. Introduction.- 2. The QCD Transition in the Early Universe.- 3. The Standard Big Bang.- 4. Inhomogeneous Big Bang Scenarios.- 4.1 Light Element Production.- 4.2 The Formation of Heavy Elements.- 5. Computational Method.- 5.1 Inhomogeneous Big Bang in a Two Zone Model.- 5.2 The Nuclear Network.- 5.3 Important Reaction Rates and Their Determination.- 6. Results.- Acknowledgements.- References.- The s-Process: Branchings and Chronometers.- 1. Introduction.- 2. Chronometers — Models and Reality.- 3. s-Process Concepts.- 3.1 The Classical Approach.- 3.2 Stellar s-Process Models.- 4. s-Process Time Scales.- 4.1 Helium Shell Burning.- 4.2 Remixing to the Interstellar Medium and the Age of the Galaxy.- 4.3 Summary of Potential Chronometers.- 5. Selected Examples.- 5.1 176Lu — a Defect Cosmic Clock.- 5.2 The Branchings at 185W and 186Re — Neutron Density and r-Process Age.- 6. Conclusions.- References.- Beta Decay Far from Stability and Double Beta Decay, and Consequences for Astrophysics.- 1. Introduction.- 2. Calculations of Beta Decay Properties of Nuclei Far from Stability.- 2.1 Half-lives.- 2.2 ?-Delayed Fission and ?-Delayed Neutron Emission.- 3. Beta Decay Far from Stability and the Astrophysical r-Process.- 3.1 Synthesis of Heavy Elements in the Universe.- 4. The r-Process and the Age of the Universe.- 5. Age of the Universe, Cosmology and Neutrino Mass.- 6. Double Beta Decay and Neutrino Mass.- 6.1 Neutrino Mass and Particle Theories (GUTs, SUSYs).- 6.2 Double Beta Decay and Neutrino Mass.- 7. Conclusion.- References.