scholarly journals Phase space dependence of the multiplicity distribution in π+ andpp collisions at 250 GeV/c

1988 ◽  
Vol 37 (2) ◽  
pp. 215-229 ◽  
Author(s):  
◽  
M. Adamus ◽  
N. M. Agababyan ◽  
I. V. Ajinenko ◽  
Yu. A. Belokopytov ◽  
...  
2014 ◽  
Vol 89 (5) ◽  
Author(s):  
T. Anticic ◽  
B. Baatar ◽  
J. Bartke ◽  
H. Beck ◽  
L. Betev ◽  
...  

2018 ◽  
Vol 58 (8) ◽  
pp. 082027 ◽  
Author(s):  
W.W. Heidbrink ◽  
L. Bardoczi ◽  
C.S. Collins ◽  
G.J. Kramer ◽  
R.J. La Haye ◽  
...  

1985 ◽  
Vol 63 (11) ◽  
pp. 1449-1452 ◽  
Author(s):  
M. T. Hussein ◽  
N. M. Hassan ◽  
M. K. Hegab

The multiplicity distribution and the inelasticity coefficient are studied for proton–proton collisions at incident energies of 6, 19, 25, and 69 GeV. A theoretical model is proposed, based on a sequential decay system formed by the two interacting protons. The Monte Carlo technique is used to calculate the phase-space integral and for simulation of events for the different reactions.


2009 ◽  
Vol 24 (supp01) ◽  
pp. 133-143
Author(s):  
Hai-Ming Hu

The following sections are included: Inclusive Distributions Exclusive Cross Sections and Form Factors Multiplicity Distribution Kinematical and Dynamical Correlations Topological Event Shapes Bose-Einstein Correlations (BEC) Possible Fractal Structure of Final State Phase-Space


1995 ◽  
Vol 68 (1) ◽  
pp. 65-71 ◽  
Author(s):  
A. Dąbrowska ◽  
P. S. Freier ◽  
R. Holyński ◽  
W. V. Jones ◽  
A. Jurak ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.


1991 ◽  
Vol 161 (2) ◽  
pp. 13-75 ◽  
Author(s):  
Lev V. Prokhorov ◽  
Sergei V. Shabanov

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