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  • SPACE SCIENCES  (4)
  • 2020-2022
  • 1970-1974  (4)
  • 1
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    Properties of hadron matter. II - Dense baryon matter and neutron stars. (1971)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: In this article we have provided certain details of a nuclear-matter computation, based on the Brueckner-Bethe-Goldstone theory of nuclear reaction, which leads to an equation of state for matter in the density region of 10 to 500 trillion g/cu cm. We also explore the possibilities that at very high baryon densities or for very short baryon separations, the net baryon-baryon interaction may be negligible so that the results of dynamical models, like the statistical bootstrap model and the dual-resonance model, may be applicable to the study of dense baryon matter. Several plausible equations of state are constructed, and their effect on the limiting mass of the neutron star is examined.
    Keywords: SPACE SCIENCES
    Type: Astrophysical Journal; 170; Dec. 15
    Format: text
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    NASA TECHNICAL REPORTS
  • 2
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    Models for neutron-core stars based on realistic nuclear-matter calculations (1970)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: Neutron core star models based on realistic nuclear matter calculations and hyperons equation of state
    Keywords: SPACE SCIENCES
    Type: ; YAL SOCIETY (
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    NASA TECHNICAL REPORTS
  • 3
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    Properties of hadron matter. I - The equation of state (1971)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: Hadron matter thermodynamical properties at high temperatures, developing dual resonance dynamic model of high energy particle interactions
    Keywords: SPACE SCIENCES
    Type: ; ECTRON (
    Format: text
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    NASA TECHNICAL REPORTS
  • 4
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    Minimum mass of a neutron star. (1972)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: The equation of state at subnuclear densities is considered together with the average binding energy per nucleon and the possibilities for a conversion of a neutron star into a white dwarf. It is found that the stable minimum mass with a core of pure neutron gas is equal to 0.067 units in terms of the solar mass, and with a core clustered with heavy nuclei equals 0.093 units. The real minimum mass is probably somewhere between these two numbers.
    Keywords: SPACE SCIENCES
    Type: Nature Physical Science; 240; Dec. 11
    Format: text
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    NASA TECHNICAL REPORTS
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