1953
DOI: 10.1103/physrev.89.123
|View full text |Cite
|
Sign up to set email alerts
|

Bremsstrahlung Cross Section of 60-Mev Electrons in Lead

Abstract: Sixty-Mev electrons from a pulsed betatron passed through lead foils of thicknesses 0.001, 0.005, and 0.015 inch placed in a magnetic cloud chamber. Measurements of approximately 1100 large energy losses gave the differential bremsstrahlung cross section as a function of x-ray energy for the high energy portion of the x-ray spectrum. Corrections were applied for instrumental discrimination and for multiple radiation and ionization energy losses in the foils. While the shape of the top 30 percent of the x-ray s… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2

Citation Types

0
2
0

Year Published

1955
1955
2002
2002

Publication Types

Select...
5
1

Relationship

0
6

Authors

Journals

citations
Cited by 16 publications
(2 citation statements)
references
References 23 publications
0
2
0
Order By: Relevance
“…For instance, Krohn and Shrader 6 report a slight excess of photons in the high-energy end of the spectrum (for E/E m =0. 8, where E is the photon energy and E m the initial energy of the radiating electron), while Koch and Carter 2 find an excess in the region E/E m -0.5. In most cases, the spectral intensity has been normalized at an arbitrary energy.…”
Section: Cs 136mentioning
confidence: 97%
See 1 more Smart Citation
“…For instance, Krohn and Shrader 6 report a slight excess of photons in the high-energy end of the spectrum (for E/E m =0. 8, where E is the photon energy and E m the initial energy of the radiating electron), while Koch and Carter 2 find an excess in the region E/E m -0.5. In most cases, the spectral intensity has been normalized at an arbitrary energy.…”
Section: Cs 136mentioning
confidence: 97%
“…The observed total intensity is that indicated by monitoring using an "R" thimble imbedded in 3.9 cm of Lucite. The methods used have depended upon the detection of: the primary electrons after radiation 8,10 ; the secondary electrons from processes such as pair production 2-5 -12 and Compton scattering 9 ; and the secondary protons from the photodisintegration of the deuteron. 1 ' 6,7,11 The detectors used in the first three methods have been either magnetic spectrometers or magnetic cloud chambers, while the photoprotons from deuterium have in all such cases been detected in photographic emulsions.…”
Section: Cs 136mentioning
confidence: 99%