Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-26T20:25:21.136Z Has data issue: false hasContentIssue false
  • English
  • Français

The Effects of Nuclear Forces on the Maximum Mass Limit of Neutron Stars

Published online by Cambridge University Press:  07 February 2017

Sachiko Tsuruta
Sachiko Tsuruta*
Affiliation:
Goddard Space Flight Center, Greenbelt, Md., U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The original models of neutron stars must be improved by including effects of nuclear interaction. This paper compares the models reached by various groups, and presents an improved model by the Kyoto group. The maximum mass varies between 0.2 M⊙ and 3 M⊙ in the various models. The Vγ model is recommended for use in the absence of further information on the equation of state at high densities.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 352 - 355
Copyright
Copyright © Reidel 1971 

References

Cohen, J. M., Langer, W. D., Rosen, L. C., and Cameron, A. G. W.: 1970, Astrophys. Space Sci. 6, 228.CrossRefGoogle Scholar
Harrison, B. K., Thorne, K. S., Wakano, M., and Wheeler, J. A.: 1965, Gravitation Theory and Gravitational Collapse , University of Chicago Press, Chicago, Ill. Google Scholar
Hartle, J. B. and Thorne, K. S.: 1968, Astrophys. J. 153, 807.CrossRefGoogle Scholar
Levinger, J. S. and Simmons, L. M.: 1961, Phys. Rev. 124, 916.CrossRefGoogle Scholar
Mizutani, T.: 1970, , .Google Scholar
Nemeth, J. and Sprung, D. W. L.: 1968, Phys. Rev. 176, 1496.CrossRefGoogle Scholar
Oppenheimer, J. R. and Volkoff, G. M.: 1939, Phys. Rev. 55, 374.CrossRefGoogle Scholar
Ostriker, J. P. and Gunn, J. E.: 1969, Astrophys. J. 157, 1395.CrossRefGoogle Scholar
Tsuruta, S. and Cameron, A. G. W.: 1966, Can. J. Phys. 44, 1895.CrossRefGoogle Scholar
Wang, C. G., Rose, W. K., and Schlenker, S. L.: 1970, Astrophys. J. Letters 160, L17.CrossRefGoogle Scholar