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  • 1
    Online Resource
    Online Resource
    Landau Fermi-Liquid Theory : Concepts and Applications. (1992)
    Newark :John Wiley & Sons, Incorporated,
    Details
    Keywords: Machine-tool industry. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (214 pages)
    Edition: 1st ed.
    ISBN: 9783527617166
    URL: https://ebookcentral.proquest.com/lib/geomar/detail.action?docID=481751
    DDC: 530.1/3
    Language: English
    Note: LANDAU FERMI-LIQUID THEORY -- CONTENTS -- Preface -- 1 Landau Fermi-Liquid Theory and Low Temperature Properties of Normal Liquid ³He -- Introduction -- 1.1 Static Properties -- 1.1.1 Quasiparticles -- 1.1.2 Quasiparticle Energy and Interactions -- 1.1.3 Equilibrium Properties -- 1.2 Nonequilibrium Properties -- 1.2.1 Quasiparticle Energies and Interaction -- 1.2.2 The Kinetic Equation -- 1.2.3 The Conservation Laws -- 1.2.4 Transport Coefficients -- 1.3 Collective Effects -- 1.3.1 Sound in Fermi Liquids -- 1.3.2 Spin Waves and Related Phenomena -- 1.3.3 Response Functions, Inequalities, and Form Factors -- 1.4 Scattering of Quasiparticles and Finite Temperature Effects -- 1.4.1 Landau Parameters and Scattering Amplitudes -- 1.4.2 The Low Temperature Transport Coefficients of Liquid ³He -- Theory and Experiment -- 1.4.3 Finite Temperature Transport Coefficients -- 1.4.4 Finite Temperature Contributions to the Specific Heat and Magnetic Susceptibility -- 1.5 Concluding Remarks -- Appendix A: Some Useful Fermi Integrals -- Appendix B: Properties of Qµ -- Appendix C Fermi Liquid Parameters for Liquid ³He -- 2 Low Temperature Properties of Dilute Solutions of ³He in Superfluid 4He -- Introduction -- 2.1 Elementary Excitations of Dilute Solutions -- 2.2 Properties of one ³He Atom in 4He at T = 0 -- 2.2.1 Volume Occupied by ³He -- 2.2.2 ³He Effective Mass -- 2.3 Interactions of the ³He at Very Low Temperature -- 2.3.1 ³He Landau Parameters -- 2.3.2 Low Temperature Properties of Dilute Solutions -- 2.3.3 Phenomenological Effective Interaction -- 2.3.4 Microscopic Approaches to the Effective Interaction -- 2.4 Interaction Between the ³He and 4He -- 2.4.1 Effectives of Superfluid Flow on ³He Quasiparticles -- 2.4.2 Interaction of ³He Quasiparticles with Long-Wavelength Phonons -- 2.4.3 Scattering of Phonons by ³He Quasiparticles. , 2.4.4 First Sound in Dilute Solutions -- 2.4.5 Second Sound -- 2.4.6 Transport Properties -- 3 Further Developments -- Introduction -- 3.1 Liquid ³He -- 3.1.1 Quasiparticle Spectrum and Thermodynamic Properties -- 3.1.2 Measurements of Transport Properties -- 3.1.3 Density and Spin Fluctuations -- 3.1.4 Calculations of Scattering Amplitudes -- 3.1.5 Superfluid ³He and the Landau Theory of Fermi Liquids -- 3.2 Dilute Solutions of ³He in Superfluid 4He -- 3.2.1 Equilibrium and Transport Properties -- 3.2.2 Higher-Momentum Excitations -- 3.3 Spin-Polarized Systems -- 3.3.1 Spin-Polarized ³He -- 3.3.2 Dilute Solutions of ³He in 4He -- 3.3.3 Other Systems -- 3.4 Nuclear Applications -- 3.4.1 Particles and Quasiparticles -- 3.4.2 Quasiparticle Interactions in Nuclei and Nuclear Matter -- 3.5 Electrons in Metals -- INDEX.
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  • 2
    Electronic Resource
    Electronic Resource
    MODELS FOR COMPACT X-RAY SOURCES (1973)
    Oxford, UK : Blackwell Publishing Ltd
    Annals of the New York Academy of Sciences 224 (1973), S. 0 
    Details
    ISSN: 1749-6632
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1749-6632.1973.tb41458.x
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    Paper (German National Licenses)
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  • 3
    Electronic Resource
    Electronic Resource
    Can Pulsar Masses be Determined ? (1970)
    [s.l.] : Nature Publishing Group
    Nature 225 (1970), S. 353-354 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] To determine the mass it is necessary to observe the immediate shifts DW, DW and DW in the angular frequency (and its first two time derivatives) caused by the starquake. From these observations one can form the dimensionless parameter Q = (An)2/AQAii (1) In the two component model Q is given by ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/225353a0
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  • 4
    Electronic Resource
    Electronic Resource
    Superfluidity in Neutron Stars (1969)
    [s.l.] : Nature Publishing Group
    Nature 224 (1969), S. 673-674 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] As Ginzburg7 has observed, the electrons are very unlikely to be superconducting, because they form a highly degenerate relativistic plasma in which effects of Coulomb interactions, relative to the kinetic energy, are of the order e2/nc. In particular, their superconducting transition temperature ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/224673a0
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  • 5
    Electronic Resource
    Electronic Resource
    Electrical Conductivity of Neutron Star Matter (1969)
    [s.l.] : Nature Publishing Group
    Nature 224 (1969), S. 674-675 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The primary constituents of neutron star interiors are neutrons, protons and electrons, the number density of electrons and protons being typically a few per cent of the density of neutrons. The more mobile carriers are the relativistic electrons, and therefore the conductivity is given in terms of ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/224674a0
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  • 6
    Electronic Resource
    Electronic Resource
    Spin Up in Neutron Stars : The Future of the Vela Pulsar (1969)
    [s.l.] : Nature Publishing Group
    Nature 224 (1969), S. 872-874 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Assuming that the speed up of the Vela pulsar was caused by a “starquake”, a number of predictions can be made, and the event can be taken as evidence that the interior of the pulsar is a ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/224872a0
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