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Atomic Masses in Astrophysics

  • Marcel Arnould

Abstract

Very neutron-rich or neutron-deficient nuclei, even up to the drip lines (and sometimes beyond!) are expected to be produced or to exist in certain astrophysical circumstances. A correct description of these events requires in particular a reliable prediction of the masses of the involved highly unstable nuclei.

Keywords

Neutron Star Mass Formula Drip Line Neutron Drip Line Mass Prediction 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. 1.
    W. D. Arnett, Astrophys. J. Suppl. 35:145 (1977).ADSCrossRefGoogle Scholar
  2. 2.
    T. A. Weaver, G. B. Zimmerman and S. E. Woosley, Astrophys. J. 225:1021 (1978).ADSCrossRefGoogle Scholar
  3. 3.
    C. N. Davids, this Conference.Google Scholar
  4. 4.
    J. P. Cox and R. T. Giuli, “Principles of Stellar Structure”, Gordon and Breach, New York (1968).Google Scholar
  5. 5.
    H. A. Bethe, G. E. Brown, J. Applegate and J. M. Lattimer, preprint (1978).Google Scholar
  6. 6.
    M. J. Murphy, preprint (submitted to Astrophys. J.) (1978).Google Scholar
  7. 7.
    H. von Groote, E. R. Hilf and K. Takahashi, Atomic Data Nucl. Data Tables 17:418 (1976).ADSCrossRefGoogle Scholar
  8. 8.
    S. Liran and N. Zeldes, Atomic Data Nucl. Data Tables 17:431 (1976).ADSCrossRefGoogle Scholar
  9. 9.
    J. Jänecke, Atomic Data Nucl. Data Tables 17:455 (1976).ADSCrossRefGoogle Scholar
  10. 10.
    F. Tondeur, Nucl. Phys. A303:185 (1978).ADSGoogle Scholar
  11. 11.
    F. Tondeur, Z. Phys. A288:97 (1978).ADSGoogle Scholar
  12. 12.
    J. M. Lattimer and D. G. Ravenhall, Astrophys. J. 223:314 (1978).ADSCrossRefGoogle Scholar
  13. 13.
    D. Q. Lamb, J. M. Lattimer, C. J. Pethick and D. G. Ravenhall, Phys. Rev. Lett. 41:1623 (1978).ADSCrossRefGoogle Scholar
  14. 14.
    V. Trimble, Rev. Mod. Phys. 47:877 (1975).ADSCrossRefGoogle Scholar
  15. 15.
    M. F. El Eid, private communication (1979).Google Scholar
  16. 16.
    W. Hillebrandt, Space Sci. Rev. 21:639 (1978).ADSCrossRefGoogle Scholar
  17. 17.
    T. Kodama and K. Takahashi, Nucl. Phys. A239:489 (1975).ADSGoogle Scholar
  18. 18.
    A. G. W. Cameron, Space Sci. Rev. 15:121 (1973).ADSCrossRefGoogle Scholar
  19. 19.
    W. D. Myers, Atomic Data Nucl. Data Tables 17:411 (1976).ADSCrossRefGoogle Scholar
  20. 21.
    P. A. Seeger and W. M. Howard, Atomic Data Nucl. Data Tables 17:428 (1976).ADSCrossRefGoogle Scholar
  21. 22.
    E. Comay and I. Kelson, Atomic Data Nucl. Data Tables 17:463 (1976).ADSCrossRefGoogle Scholar
  22. 23.
    J. Jänecke and B. P. Eynon, Atomic Data Nucl. Data Tables 17: 467 (1976).ADSCrossRefGoogle Scholar
  23. 24.
    M. Beiner, R. J. Lombard and D. Mas, Atomic Data Nucl. Data Tables 17:450 (1976).,ADSCrossRefGoogle Scholar
  24. 25.
    E. Anders, H. Higuchi, J. Gros, H. Takahashi and J. Morgan, Science 190:1262 (1975).ADSGoogle Scholar
  25. 26.
    L. M. Libby, W. F. Libby and S. K. Runcorn, Nature 278:613 (1979).ADSCrossRefGoogle Scholar
  26. 27.
    F.-K. Thielemann, M. Arnould and W. Hillebrandt, Astron. Astrophys. 74:175 (1979).ADSGoogle Scholar
  27. 28.
    W. A. Fowler, in: “Proceedings of the Robert A. Welch Foundation Conference on Chemical Research XXI — Cosmochemistry”, W. O. Milligan, ed., Robert A. Welch Foundation, Houston (1978).Google Scholar
  28. 29.
    P. A. Seeger and D. N. Schramm, Astrophys. J. 160:L157 (1970).ADSCrossRefGoogle Scholar
  29. 30.
    G. Baym and C. J. Pethick, Ann. Rev. Nucl. Sci. 25:27 (1975).ADSCrossRefGoogle Scholar
  30. 31.
    F. Tondeur, Astron. Astrophys. 14:453 (1971).ADSGoogle Scholar
  31. 32.
    F. Tondeur, Astron. Astrophys. 72:88 (1979).ADSGoogle Scholar
  32. 33.
    G. Baym, C. J. Pethick and P. Sutherland, Astrophys. J. 170:299 (1971).ADSCrossRefGoogle Scholar
  33. 34.
    K. Koebke, M. El Eid and E. Hilf, Z. Phys. 271:21 (1974).ADSCrossRefGoogle Scholar
  34. 35.
    H. Heintzmann, W. Hillebrandt, M. El Eid and E. Hilf, Z. Naturforsch. 29A:933 (1974).ADSGoogle Scholar
  35. 36.
    Z. Barkat, J. Buchler and L. Ingber, Astrophys. J. 176:723 (1972).ADSCrossRefGoogle Scholar
  36. 37.
    J. Negele and D. Vautherin, Nucl. Phys. A207;321 (1973).Google Scholar
  37. 38.
    F. Tondeur, Thesis, Université Libre de Bruxelles (unpublished) (1977).Google Scholar
  38. 39.
    W. D. Myers and W. J. Swiatecki, Nucl. Phys. 81:1 (1966).Google Scholar
  39. 40.
    J. M. Lattimer, F. Mackie, D. G. Ravenhall and D. N. Schramm, Astrophys. J. 213:225 (1977).ADSCrossRefGoogle Scholar
  40. 41.
    F. J. Dyson, “Neutron Stars and Pulsars”, Fermi Lecture at the Scuola Normale Superiore di Pisa, Accademia Nacionale dei Lincei, Roma (1971).Google Scholar
  41. 42.
    W. Ober, in: “Ninth Texas Symposium on Relativistic Astrophysics” (to appear), Munich (1978).Google Scholar
  42. 43.
    J. Audouze and J. W. Truran, Astrophys. J. 202:204 (1975).ADSCrossRefGoogle Scholar
  43. 44.
    M. Arnould, unpublished (1976).Google Scholar

Copyright information

© Plenum Press, New York 1980

Authors and Affiliations

  • Marcel Arnould
    • 1
    • 2
  1. 1.Institut d’Astronomie et d’AstrophysiqueUniversité Libre de BruxellesBelgium
  2. 2.Chercheur Qualifié F.N.R.S.Belgium

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