scholarly journals Uncorrelated jet model for particle spectra and elastic proton-proton scattering at very high energy

1971 ◽  
Vol 27 (1) ◽  
pp. 45-63 ◽  
Author(s):  
E.H. De Groot ◽  
Th.W. Ruijgrok
1970 ◽  
Vol 2 (3) ◽  
pp. 572-577 ◽  
Author(s):  
A. O. Barut ◽  
W. Plywaski

1971 ◽  
Author(s):  
L. G. Ratner ◽  
R. J. Ellis ◽  
G. Vannini ◽  
B. A. Babcock ◽  
A. D. Krisch ◽  
...  

2015 ◽  
Vol 2015 ◽  
pp. 1-14 ◽  
Author(s):  
V. A. Okorokov

The diffraction slope parameter is investigated for elastic proton-proton and proton-antiproton scattering based on all the available experimental data at low and intermediate momentum transfer values. Energy dependence of the elastic diffraction slope is approximated by various analytic functions. The expanded “standard” logarithmic approximations with minimum number of free parameters allow description of the experimental slopes in all the available energy range reasonably. The estimations of asymptotic shrinkage parameterαP′are obtained for various|t|domains based on all the available experimental data. Various approximations differ from each other both in the low energy and very high energy domains. Predictions for diffraction slope parameter are obtained for elastic proton-proton scattering from NICA up to future collider (FCC/VLHC) energies, for proton-antiproton elastic reaction in FAIR energy domain for various approximation functions.


2018 ◽  
Vol 33 (40) ◽  
pp. 1850242 ◽  
Author(s):  
L. Stodolsky

The description of very high energy proton–proton cross-sections in terms of a “black disc” with an “edge” allows a simple generalization to highest energy proton–nucleus cross-sections. This results in a leading ln2W term and a ln W term whose coefficient depends linearly on the radius of the nucleus (W the c.m. energy). The necessary parameters are determined from the fits to p–p data. Since the coefficient of the ln W term is rather large, it is doubtful that the regime of ln2W dominance can be reached with available energies in accelerators or cosmic rays. However, the ln W term can be relevant for highest energy cosmic rays in the atmosphere, where a large increase for the cross-section on nitrogen is expected. Tests of the theory should be possible by studying the coefficient of ln W at p-nucleus colliders.


1966 ◽  
Vol 35 (5) ◽  
pp. 834-839
Author(s):  
Masako Bando ◽  
Yoshio Takada

1972 ◽  
Vol 47 (2) ◽  
pp. 589-602 ◽  
Author(s):  
Mamoru Kawasaki ◽  
Yoshinori Susuki ◽  
Minoru Yonezawa

1981 ◽  
Vol 65 (3) ◽  
pp. 1102-1104
Author(s):  
Y. Tzeng ◽  
C. W. Wong

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