Radiative correction to the equivalent-photon spectrum of a relativistic electron and the two-photon process

1987 ◽  
Vol 36 (1) ◽  
pp. 44-54 ◽  
Author(s):  
Martin Landr ◽  
Kjell J. Mork ◽  
Haakon A. Olsen
1998 ◽  
Vol 37 (S1) ◽  
pp. 12 ◽  
Author(s):  
L. Dong ◽  
V. N. Bagratashvili ◽  
S. I. Tsypina ◽  
Y. S. Zavorotny ◽  
A. O. Rybaltovskii ◽  
...  

2019 ◽  
Vol 212 ◽  
pp. 04006
Author(s):  
Evgeny Kozyrev ◽  
Evgeny Solodov ◽  
Vladimir Druzhinin

We report the results on the channels e+e−→ π+π−π0π0π0(η), e+e−→ π+π−η. Also we present the study of the two-photon process e+e−→ e+e−η' in the double-tag mode. The results for the form factor are compared with the predictions based on pQCD and VMD. The results are obtained by using the full data set of about 470 fb−1 collected by the BABAR experiment at the PEP-II e+e−collider at a center-of-mass energy of about 10.6 GeV.


1978 ◽  
Vol 76 ◽  
pp. 121-122
Author(s):  
R.C. Bohlin ◽  
J.P. Harrington ◽  
T.P. Stecher

The ultraviolet emission lines that were me asured in the spectrum obtained from our rocket observation of NGC 7662 have been compared with those predicted by a set of models. The models allow a determination of the carbon abundance which is found to be solar and the C/0 ratio which is equal to unity. In order to obtain a good fit, dielectronic recombination and charge exchange between neutral hydrogen and C IV were included, both of which increase the concentration of C III. The observed continuum consists of light from the central star and from the nebula, which contributed primarily via the two photon process in the H° and the Balmer continuum.


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