Basic connection between superconductivity and superfluidity
Identifieur interne : 001F14 ( Main/Exploration ); précédent : 001F13; suivant : 001F15Basic connection between superconductivity and superfluidity
Auteurs : Mario Rabinowitz [États-Unis]Source :
- International Journal of Theoretical Physics [ 0020-7748 ] ; 1993-04-01.
English descriptors
- Teeft :
- Boson, Coherence length, Condensation temperature, Cooper pairing, Different equation, Effective mass, Experimental value, Fermi, Fermi atoms, Fermi electrons, Fermi energy, Fermion, First approximation, Heavy fermion superconductors, International journal, Interparticle spacing, L3he, Magnetic field, Metallic hydrogen, Metallic superconductors, Neutron stars, Number density, Overall number density, Oxide superconductors, Pairing, Particle pair, Physical review, Physical review letters, Rabinowitz, Rocket ship, Same paradigm, Singlet state, Superconductivity, Superconductors, Superfluid, Superfluid transition, Superfluid transition temperature, Superfluidity, Theoretical physics, Triplet state, Upper limit.
Abstract
Abstract: A basic and inherently simple connection is shown to exist between superconductivity and superfluidity. It is shown that the author's previously derived general equation, which agrees well with the superconducting transition temperatures for the heavy-electron superconductors, metallic superconductors, oxide superconductors, metallic hydrogen, and neutron stars, also works well for the superfluid transition temperature of 2.6 mK for liquid3He. Reasonable estimates are made from 10−3 to 109 K — a range of 12 orders of magnitude. The same paradigm applies to the superfluid transition temperature of liquid4He, but results in a slightly different equation. The superfluid transition temperature for dilute solutions of3He in superfluid4He is estimated to be ∼l–10μK. This paradigm works well in detail for metallic, cuprate, and organic superconductors.
Url:
DOI: 10.1007/BF00673760
Affiliations:
Links toward previous steps (curation, corpus...)
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- to stream Istex, to step Curation: 000061
- to stream Istex, to step Checkpoint: 000C78
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- to stream Main, to step Curation: 001F14
Le document en format XML
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It is shown that the author's previously derived general equation, which agrees well with the superconducting transition temperatures for the heavy-electron superconductors, metallic superconductors, oxide superconductors, metallic hydrogen, and neutron stars, also works well for the superfluid transition temperature of 2.6 mK for liquid3He. Reasonable estimates are made from 10−3 to 109 K — a range of 12 orders of magnitude. The same paradigm applies to the superfluid transition temperature of liquid4He, but results in a slightly different equation. The superfluid transition temperature for dilute solutions of3He in superfluid4He is estimated to be ∼l–10μK. This paradigm works well in detail for metallic, cuprate, and organic superconductors.</div></front></TEI><affiliations><list><country><li>États-Unis</li></country><region><li>Californie</li></region></list><tree><country name="États-Unis"><region name="Californie"><name sortKey="Rabinowitz, Mario" sort="Rabinowitz, Mario" uniqKey="Rabinowitz M" first="Mario" last="Rabinowitz">Mario Rabinowitz</name></region></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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