- Access by Xinjiang University
A Determination of by Means of Photoelectrons Excited by X-Rays
Phys. Rev. 43, 417 – Published 15 March, 1933
DOI: https://doi.org/10.1103/PhysRev.43.417
Abstract
A value of has been obtained by a magnetic deflection method by making use of x-ray photoelectrons and the magnetic spectrograph. Electrons were ejected from thin evaporated or sputtered films of gold, silver, copper and platinum by the x-radiation from a molybdenum target metal tube placed close to the film and working at an input of 1.5 kilowatts. The velocity of ejection of the photoelectrons was computed from the difference between the energies associated with Mo radiation and the various absorption limits of the metal films. Relativity corrections were made since these velocities correspond to from 8000 to 15,000 equivalent volts. The and components of the molybdenum line were clearly resolved since the magnetic field was kept very constant by the use of a potentiometer and continuous hand control. The weighted mean value of obtained from five plates is 1.7570±0.0026× e.m.u. per gram. This result is based upon a value of as taken from x-ray crystal measurements. By taking from x-ray data the resulting value of is independent of the uncertainty involved in the crystal grating constant.
References (28)
- A. Bestelmeyer, Handb. d. Radiologie 5, 1-79 (1919)
- W. Gerlach, Handb. d. Physik 22, 41-82 (1926)
- H. D. Babcock, Astrophys. J. 58, 149 (1923) ibid.69, 43 (1929)
- W. V. Houston, Phys. Rev. 30, 608 (1927)
- F. Wolf, Ann. d. Physik 83, 849 (1927)
- R. T. Birge, Phys. Rev. Sup. 1, 48 (1929)
- J. S. Campbell and W. V. Houston, Phys. Rev. 39, 601 (1932)
- Charlotte Perry and E. L. Chaffee, Phys. Rev. 36, 904 (1930)
- F. Kirchner, Ann. d. Physik, 8, 975 (1931) ibid.12, 503 (1932)
- W. N. Bond (Proc. Phys. Soc. 44, 374 (1932)
- R. T. Birge, Phys. Rev. 40, 228 (1932)
- A. Bestelmeyer (Ann. d. Physik 22, 429 (1907))
- H. Robinson and W. F. Rawlinson, Phil. Mag. 28, 277 (1914)
- M. de Broglie, C. R. 172, 274, 527, 746, 806 (1921)
- H. Robinson, Proc. Roy. Soc. A104, 455 (1923)
- E. C. Watson, Phys. Rev. 30, 479 (1927)
- R. T. Birge, Rev. Mod. Phys. 1, 72 (1929)
- W. Duane, H. H. Palmer and Chi-Sun Yeh, Proc. Nat. Acad. Sci. 7, 237 (1921)
- W. DuaneH. H. PalmerChi-Sun YehAnn. d. Physik 5 (1), 494 (1929)
- R. T. Birge, Phys. Rev. 40, 247 (1932)
- C. H. Cartwright and J. Strong, Rev. Sci. Inst. 2, 189 (1931)
- A. H. Compton, Rev. Sci. Inst. 2, 365 (1931)
- Y. Tu, Phys. Rev. 40, 662 (1932)
- Dunnington (Phys. Rev. 42, 734 (1932) 42, 736 (1932)
- Arthur J. M. Johnson, Phys. Rev. 34, 7 (1929)
- E. Lindberg, Zeits. f. Physik 54, 632 (1929)
- G. D. Van Dyke and G. A. Lindsay, Phys. Rev. 30, 562 (1927)
- M. Siegbahn, Spektroskopie der Rontgenstrahlen, 2nd edition, page 265 (1931)