Relative Pair Production Cross Sections in the Energy Region 50 to 300 Mev
- 15 June 1952
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 86 (6) , 1028-1035
- https://doi.org/10.1103/physrev.86.1028
Abstract
A cloud-chamber survey has been made of pairs produced in Al, Ag, Au, and Th foils by an x-ray beam from the 300-Mev betatron. By comparing the pairs produced in two of the foils mounted to intercept the same x-ray beam, values of the relative pair production cross sections for Ag to Al, Au to Al, and Th to Al were found to be, respectively, (3.4±1.4), (7.9±1.5), and (11.7±1.7) percent low compared with the Bethe-Heitler theory predictions. The results are consistent with a correction factor to the theoretical pair cross section given by []. The calculated number of Compton electrons between 50 and 200 Mev expected from the Al foil is 1201, from the Ag foil is 355, and from the Au foil is 113. The observed numbers with statistical errors indicated are, respectively, 1170±40, 354±30, and 70±18.
Keywords
This publication has 10 references indexed in Scilit:
- High Energy Bremsstrahlung and Pair ProductionPhysical Review B, 1951
- Absorption of 280-Mev PhotonsPhysical Review B, 1951
- Wire Recorded Magnetic Pulse Timing CircuitReview of Scientific Instruments, 1950
- Relative Cross Sections for Pair Production at 17.6 MevPhysical Review B, 1949
- Absorption of 17.6 Mev Gamma-Rays in C, Al, Cu, Sn, and PbPhysical Review B, 1949
- 88-Mev Gamma-Ray Cross SectionsPhysical Review B, 1949
- The Absorption of High Energy Quanta. I.Physical Review B, 1948
- Influence of Atomic Electrons on Radiation and Pair ProductionPhysical Review B, 1939
- On the stopping of fast particles and on the creation of positive electronsProceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character, 1934
- Über die Streuung von Strahlung durch freie Elektronen nach der neuen relativistischen Quantendynamik von DiracZeitschrift für Physik, 1929