Abstract

No abstract available.

Full Article  |  PDF Article

References

  • View by:
  • |
  • |
  • |

  1. C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.
  2. First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).
    [CrossRef]
  3. M. G. Ingraham, D. C. Hess, and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.
    [CrossRef]
  4. H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).
    [CrossRef]
  5. P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I≧3/2 reported for both odd isotopes.
    [CrossRef]

1949 (1)

P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I≧3/2 reported for both odd isotopes.
[CrossRef]

1948 (1)

M. G. Ingraham, D. C. Hess, and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.
[CrossRef]

1934 (1)

H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).
[CrossRef]

1932 (1)

First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).
[CrossRef]

Brix, P.

P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I≧3/2 reported for both odd isotopes.
[CrossRef]

Hayden, R. J.

M. G. Ingraham, D. C. Hess, and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.
[CrossRef]

Hess, D. C.

M. G. Ingraham, D. C. Hess, and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.
[CrossRef]

Ingraham, M. G.

M. G. Ingraham, D. C. Hess, and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.
[CrossRef]

Keim, C. P.

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

Kopfermann, H.

P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I≧3/2 reported for both odd isotopes.
[CrossRef]

Pohl, M.

First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).
[CrossRef]

Savage, H. W.

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

Schmidt, T.

H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).
[CrossRef]

Schueler, H.

H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).
[CrossRef]

von Hevesy, G.

First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).
[CrossRef]

Weaver, Boyd S.

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

Nature (1)

First reported by G. von Hevesy and M. Pohl, Nature 130, 846 (1932). Activity variously reported as being due to Sm148 by T. R. Wilkins and A. J. Dempster, Phys. Rev. 54, 315 (1938); to Sm152 by A. J. Dempster, Phys. Rev. 75, 1125 (1948); and to RaD impurity by C. Haenny, M. Najar, and M. Gaillond, Helv. Phys. Acta 22, 611 (1949).
[CrossRef]

Phys. Rev. (1)

M. G. Ingraham, D. C. Hess, and R. J. Hayden, Phys. Rev. 73, 180 (1948), conclude Sm146 is probably <0.002 percent natural abundance.
[CrossRef]

Z. Physik (2)

H. Schueler and T. Schmidt, Z. Physik 92, 148 (1934); P. Brix, Z. Physik 126, 431 (1949).
[CrossRef]

P. Brix and H. Kopfermann, Z. Physik 126, 344 (1949). I≧3/2 reported for both odd isotopes.
[CrossRef]

Other (1)

C. P. Keim, H. W. Savage, and Boyd S. Weaver, submitted to Phys. Rev.

Cited By

OSA participates in CrossRef's Cited-By Linking service. Citing articles from OSA journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (1)

Fig. 1
Fig. 1

Spectrum shifts in enhanced samarium samples. Top spectrum Sm144, bottom Sm154.