|
Properties of Photons determined by Interferometric Spectroscopy H. A. GEBBIE*‡, R. A. BOHLANDER‡ & R. P. FUTRELLE†¶
‡Department of Physics and Astrophysics
¶Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, Colorado 80302
*Present address: Radio and Space Research Station, Slough, Buckinghamshire, England.
†Present address: Department of Theoretical Biology, University of Chicago, Chicago, Illinois 60627.
Black body spectroscopy has been neglected by experimentalists for fifty years. We propose to apply interferometric methods to black bodies with the prospect of getting temperature values based on frequency standards in the range from 90 K and upwards. When applied to higher temperature sources, the same methods could tell us new things about photons.
References
| 1. |
Hust, J. G., Cryogenics, 9, 443 (1969). |
| 2. |
Coblentz, W. W., Bull. Bureau Standards, 10, 1 (1913). |
| 3. |
Coblentz, W. W., Bull. Bureau Standards, 13, 459 (1916). |
| 4. |
Bourret, R. C., Nuovo Cim., 18, 347 (1960). |
| 5. |
Kano, Y., and Wolf, E., Proc. Phys. Soc., 80, 1273 (1962). |
| 6. |
Bedford, R. E., Proc. Fifth Symposium on Temperature (Washington, 1971). |
| 7. |
de Vos, G. C., Physica, 20, 669 (1954). |
| 8. |
Gebbie, H. A., Appl. Optics, 8, 347 (1969). |
| 9. |
Franklin, J. N., J. Math. Ana. Appl., 31, 682 (1970). |
| 10. |
Lummer, O., and Pringsheim, E., Verh. Deut. Physik Ges., 2, 163 (1900). |
| 11. |
Friedmann, F. L., and Sartori, L., The Classical Atom (Addison-Wesley, Reading, Mass., 1965). |
| 12. |
Perkins, W. A., Phys. Rev. D, 5, 1375 (1972). |
| 13. |
Pecker, J. C., Roberts, A. P., and Vigier, J. P., Nature, 237, 227 (1972). |
© 1972 Nature Publishing Group Privacy Policy |