What can deuterium tell us?

DEC 01, 1974

The recently observed relative abundance of this isotope in our galaxy may be a remnant of the fireball phase of the universe.

DOI: 10.1063/1.3129034

David N. Schramm

Robert V. Wagoner

What is behind the unusual flurry of activity concerned with the isotope deuterium? Simply this: Because of its unique properties, the distribution of deuterium in the universe constitutes a powerful clue to the history of the development of matter.

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References

1. I. Friedman, A. C. Redfield, B. Schoen, J. Harris, Rev. Geophys. 2, 177 (1964).https://doi.org/RVGPA3
2. G. Boato, Geochim. Cosmochim. Acta 6, 209 (1954).https://doi.org/GCACAK
3. R. Beer, F. W. Taylor, Astrophys. J. 179, 309 (1973).https://doi.org/ASJOAB
4. J. T. Trauger, F. L. Roesler, N. P. Carleton, W. A. Traub, Astrophys. J. Lett. 184, L137 (1973).https://doi.org/AJLEAU
5. N. Grevesse, Colloque de Liège 19, 251 (1970).
6. D. C. Black, Nature Phys. Sci. 234, 148 (1971).https://doi.org/NPSCA6
7. D. C. Black, Geochim. Cosmochim. Acta 36, 347 (1972).https://doi.org/GCACAK
8. J. Geiss, H. Reeves, Astron. and Astrophys. 18, 126 (1972).https://doi.org/AAEJAF
9. S. Weinreb, Nature 195, 367 (1962).https://doi.org/NATUAS
10. D. A. Cesarsky, A. T. Moffet, J. M. Pasachoff, Astrophys. J. Lett. 180, L1 (1973).https://doi.org/AJLEAU
11. J. M. Pasachoff, D. A. Cesarsky, Astrophys. J., to be published (1974).
12. K. B. Jefferts, A. A. Penzias, R. W. Wilson, Astrophys. J. 179, L57 (1973).https://doi.org/ASJOAB
13. R. W. Wilson, A. A. Penzias, K. B. Jefferts, P. R. Solomon, Astrophys. J. Lett. 179, L107 (1973).https://doi.org/AJLEAU
14. L. Spitzer, J. F. Drake, E. B. Jenkins, D. C. Morton, J. B. Rogerson, D. G. York, Astrophys. J. Lett. 181, L116 (1973).https://doi.org/AJLEAU
15. J. B. Rogerson, Jr, D. G. York, Astrophys. J. Lett. 186, L95 (1973).https://doi.org/AJLEAU
16. A. G. W. Cameron, in Explosive Nucleosynthesis (D. N. Schramm, W. D. Arnett, eds.), University of Texas Press, Austin (1973).
17. P. N. Solomon, N. J. Woolf, Astrophys. J. Lett. 180, L89 (1973).https://doi.org/AJLEAU
18. W. D. Watson, Astrophys. J. Lett. 181, L129 (1973).https://doi.org/AJLEAU
19. W. D. Watson, Astrophys. J. Lett. 182, L73 (1973).https://doi.org/AJLEAU
20. J. H. Black, A. Dalgarno, Astrophys. J. Lett. 184, L101 (1973).https://doi.org/AJLEAU
21. H. Reeves, J. Audouze, W. A. Fowler, D. N. Schramm, Astrophys. J. 179, 909 (1973).https://doi.org/ASJOAB
22. J. Truran, A. G. W. Cameron, Astrophys. and Space Sci. 14, 179 (1971).https://doi.org/APSSBE
23. R. J. Talbot, Jr, W. D. Arnett, Astrophys. J. 186, 51 (1973).https://doi.org/ASJOAB
24. W. A. Fowler, J. L. Greenstein, F. Hoyle, Geophys. J. R. Astron. Soc. 6, 148 (1962).https://doi.org/GEOJAN
25. C. Ryter, H. Reeves, E. Gradsztajn, J. Audouze, Astron. and Astrophys. 8, 389 (1970).https://doi.org/AAEJAF
26. H. Reeves, W. A. Fowler, F. Hoyle, Nature 226, 727 (1970).https://doi.org/NATUAS
27. M. Meneguzzi, J. Audouze, H. Reeves, Astron. and Astrophys. 15, 337 (1971).https://doi.org/AAEJAF
28. H. Mitler, Astrophys. and Space Sci. 17, 186 (1972).https://doi.org/APSSBE
29. J. Audouze, J. Lequeux, H. Reeves, Astron. and Astrophys. 28, 85 (1973).https://doi.org/AAEJAF
30. D. C. Morton, A. M. Smith, T. Stecher, Astrophys. J., to be published.
31. S. A. Colgate, Astrophys. J. Lett. 181, L53 (1973).https://doi.org/AJLEAU
32. S. A. Colgate, in Explosive Nucleosynthesis (D. N. Schramm, W. D. Arnett, eds.), University of Texas Press, Austin (1973).
33. S. A. Colgate, Astrophys. J. 187, 321 (1974).https://doi.org/ASJOAB
34. F. Hoyle, W. A. Fowler, Nature 241, 384 (1973).https://doi.org/NATUAS
35. H. Reeves, paper presented at the 13th International Cosmic Ray Conference, Denver (1973).
36. R. I. Epstein, W. D. Arnett, D. N. Schramm, Astrophys, J., in press.
37. E. R. Harrison, PHYSICS TODAY, June 1968; page 31.
38. C. W. Misner, K. S. Thorne, J. A. Wheeler, Gravitation, W. A. Freeman, San Francisco (1973).
39. A. Sandage, G. Tamman, E. Hardy, Astrophys. J. 172, 253 (1972).https://doi.org/ASJOAB
40. R. G. Hughes, M. Longair, Mon. Not. Roy. Astron. Soc. 135, 131 (1967).https://doi.org/MNRAA4
41. P. J. E. Peebles, Physical Cosmology, Princeton U.P. (1971).
42. P. J. E. Peebles, Phys. Rev. Letts. 16, 410 (1966); https://doi.org/PRLTAO
P. J. E. Peebles, Astrophys. J. 146, 542 (1966); https://doi.org/ASJOAB
R. V. Wagoner, W. A. Fowler, F. Hoyle, Astrophys. J. 148, 3 (1967); https://doi.org/ASJOAB
R. V. Wagoner, Science 155, 1369 (1967).https://doi.org/SCIEAS
43. R. V. Wagoner, Astrophys. J. 179, 343 (1973).https://doi.org/ASJOAB
44. R. V. Wagoner, in Proceedings of I.A.U. Symposium no. 63, Cracow, Poland (1973).
45. J. R. Gott, J. Gunn, D. N. Schramm, B. Tinsley, Orange aid preprint, Caltech (1974).
46. A. R. Sandage, in Proceedings of the Symposium on the Galaxy and the Distance Scale (Essex, England), in press (1974).
47. A. R. Sandage, Astrophys. J. 178, 1 (1972).https://doi.org/ASJOAB
48. B. Tinsley, Astrophys. J. Lett. 173, L93 (1972).https://doi.org/AJLEAU
49. T. Weaver, G. Chapline, Astrophys. J. Lett. 192, L57 (1974).https://doi.org/AJLEAU

More about the Authors

David N. Schramm. Enrico Fermi Institute, University of Chicago.

Robert V. Wagoner. Stanford University.