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Hadron Star Models

Published online by Cambridge University Press:  14 August 2015

Jeffrey M. Cohen  and
Gerhard Börner
Jeffrey M. Cohen*
Affiliation:
High Energy Astrophysics Laboratory, Goddard Space Flight Center, Greenbelt, Md., U.S.A.
Gerhard Börner*
Affiliation:
High Energy Astrophysics Laboratory, Goddard Space Flight Center, Greenbelt, Md., U.S.A.
*
∗Permanent address: Physics Department, University of Pennsylvania, Philadelphia, Pa. 19104. National Academy of Science – NRC Senior Research Associate.
∗∗Permanent address: Max-Planck Institut für Physik and Astrophysik, München, Germany. National Academy of Science – NRC Research Associate.

Abstract

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The properties of fully relativistic rotating hadron star models are discussed using models based on recently developed equations of state. All of these stable neutron star models are bound with binding energies as high as ∼ 25%. During hadron star formation, much of this energy will be released. The consequences, resulting from the release of this energy, are examined.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 53: Physics of Dense Matter , 1974 , pp. 237 - 250
Copyright
Copyright © Reidel 1974 

References

Arnett, W. D.: 1969, Astrophys. Space Sci. 5, 180.CrossRefGoogle Scholar
Barkat, Z.: 1971, Astrophys. J. 163, 433.Google Scholar
Barkat, Z.: 1973 (to be published).Google Scholar
Barkat, Z., Buchler, J. R., and Wheeler, J. C.: 1970, Astrophys. Letters 6, 117.Google Scholar
Barkat, Z., Buchler, J. R., and Wheeler, J. C.: 1971, Astrophys. J. 8, 21.Google Scholar
Barkat, Z., Wheeler, J. C., and Buchler, J. C.: 1972, Astrophys. J. 171, 651.Google Scholar
Baym, G., Pethick, C., and Sutherland, P.: 1971, Astrophys. J. 170, 299.Google Scholar
Bethe, H. A. and Ashkin, J.: 1953, in Serge, E. (ed.), Experimental Nuclear Physics 1, 233. John Wiley and Sons Inc., N.Y. Google Scholar
Bethe, H. A. and Johnson, M.: 1973 (to be published).Google Scholar
Bethe, H. A., Börner, G., and Sato, K.: 1970, Astron. Astrophys. 7, 279.Google Scholar
Börner, G. and Cohen, J. M.: 1972, Astron. Astrophys. 19, 109.Google Scholar
Börner, G., Cohen, J. M., and Ramaty, R.: 1973 (to be published).Google Scholar
Bozoki, G. and Lande, K.: 1973 (to be published).Google Scholar
Brill, D. R. and Cohen, J. M.: 1966, Phys. Rev. 143, 1011.Google Scholar
Chandrasekhar, S.: 1939, Introduction to the Study of Stellar Structure, Dover Press, N. Y. Google Scholar
Cohen, J. M.: 1970, Astrophys. Space Sci. 6, 263.CrossRefGoogle Scholar
Cohen, J. M.: 1972, General Relativity and Gravitation Res. 3, 221.Google Scholar
Cohen, J. M. and Brill, D. R.: 1968, Nuovo Cimento 50B, 209.Google Scholar
Cohen, J. M. and Cameron, A. G. W.: 1971, Astrophys. Space Sci. 10, 227.Google Scholar
Cohen, J. M. and Cohen, M. D.: 1969, Nuovo Cimento 60B, 241.Google Scholar
Cohen, J. M., Langer, W. D., Rosen, L. C., and Cameron, A. G. W.: 1970, Astrophys. Space Sci. 6, 228.Google Scholar
Cohen, J. M., Lapidus, A., and Cameron, A. G. W.: 1969, Astrophys. Space Sci. 5, 113.Google Scholar
Colgate, S. A.: 1971, Astrophys. J. 163, 221.CrossRefGoogle Scholar
Finzi, A. and Wolf, R. A.: 1969, Astrophys. J. Letters 155, L107.Google Scholar
Gold, T.: 1968, Nature 218, 731.Google Scholar
Gordon (Pecker-Wimel), C.: 1972a, Astron. Astrophys. 20, 79.Google Scholar
Gordon (Pecker-Wimel), C.: 1972b, Astron. Astrophys. 20, 87.Google Scholar
Harrison, B., Thorne, K. S., Wakano, M., and Wheeler, J. A.: 1965, Gravitation Theory and Gravitational Collapse, University of Chicago Press, Ill.Google Scholar
Larson, R. B. and Starrfield, S.: 1971, Astron. Astrophys. 13, 190.Google Scholar
Leung, V. C. and Wang, C. G.: 1971, Astrophys. J. 170, 499.Google Scholar
Lucy, L.: 1967, Astron. J. 72, 813.Google Scholar
Maran, S. P., Brandt, J. C., and Stecher, T. P.: 1971, The Gum Nebula and Related Problems, Goddard Space Flight Center Report X-683-71-375.Google Scholar
Mazarakis, M. and Stevens, W.: 1972, Astrophys. J. Letters 171, L97.Google Scholar
Oppenheimer, J. R. and Volkoff, G.: 1939, Phys. Rev. 55, 374.Google Scholar
Paczynski, B.: 1970, Acta Astron. 20, 47.Google Scholar
Paczynski, B.: 1972, Astrophys. Letters 11, 53.Google Scholar
Paczynski, B. and Ziolkowski, J.: 1967, Acta Astron. 17, 7.Google Scholar
Ramaty, R. and Boldt, E. A.: 1971, in Maran, S. P., Brandt, J. C., and Stecher, T. P. (eds.), The Gum Nebula and Related Problems, Goddard Space Flight Center Report X-683-71-375, p. 97.Google Scholar
Rose, W. K.: 1969, Astrophys. J. 155, 491.Google Scholar
Roxburgh, I. W.: 1967, Nature 215, 838.Google Scholar
Schwarzschild, M.: 1957, Structure and Evolution of the Stars, Dover Press, N.Y. Google Scholar
Tolman, R. C.: 1939, Phys. Rev. 56, 364.Google Scholar
Wheeler, J. C., Barkat, Z., and Buchler, J. R.: 1970, Astrophys. J. Letters 162, L129.Google Scholar