scholarly journals Behavior of very high energy hadronic cross-sections

2017 ◽  
Vol 32 (31) ◽  
pp. 1730028 ◽  
Author(s):  
L. Stodolsky

Analysis of the data for proton and antiproton scattering leads to a simple picture for very high energy hadronic cross-sections. There is, asymptotically, a simple “black disc” with a smooth “edge”. The radius of the “disc” is expanding logarithmically with energy, while the “edge” is constant. These conclusions follow from extensive fits to accelerator and cosmic ray data, combined with the observation that a certain combination of elastic and total cross-sections allows extraction of the “edge”. An interesting feature of the results is that the “edge” is rather large compared to the “disc”. This explains the slow approach to “asymptopia” where the “disc” finally dominates.

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.


1970 ◽  
Vol 25 (13) ◽  
pp. 902-902 ◽  
Author(s):  
W. P. Hesse ◽  
D. O. Caldwell ◽  
V. B. Elings ◽  
R. J. Morrison ◽  
F. V. Murphy ◽  
...  

1970 ◽  
Vol 25 (14) ◽  
pp. 979-979 ◽  
Author(s):  
W. P. Hesse ◽  
D. O. Caldwell ◽  
V. B. Elings ◽  
R. J. Morrison ◽  
F. V. Murphy ◽  
...  

1970 ◽  
Vol 25 (9) ◽  
pp. 613-616 ◽  
Author(s):  
W. P. Hesse ◽  
D. O. Caldwell ◽  
V. B. Elings ◽  
R. J. Morrison ◽  
F. V. Murphy ◽  
...  

1996 ◽  
Vol 160 ◽  
pp. 363-364
Author(s):  
S.A. Dazeley ◽  
P.G. Edwards ◽  
J.R. Patterson ◽  
G.P. Rowell ◽  
M. Sinnott ◽  
...  

TheCollaboration ofAustralia andNippon for aGAmmaRayObservatory in theOutback operates two large telescopes at Woomera (South Australia), which detect the Čerenkov light images produced in the atmosphere by electronpositron cascades initiated by very high energy (~1 TeV or 1012eV) gamma rays. These gamma rays arise from a different mechanism than at EGRET energies: inverse Compton (IC) emission from relativistic electrons.The spoke-like images are recorded by a multi-pixel camera which facilitates the rejection of the large numbers of oblique and ragged cosmic ray images. A field of view ~3.5° is required. The Australian team operates a triple 4 m diameter mirror telescope, BIGRAT, with a 37 photomultiplier tube camera and energy threshold 600 GeV. The Japanese operate a single, highly accurate 3.8 m diameter f/1 telescope and high resolution 256 photomultipler tube camera. In 1998 a new 7 m telescope is planned for Woomera with a design threshold ~;200GeV.


1996 ◽  
Vol 4 (4) ◽  
pp. 351-363 ◽  
Author(s):  
G BATTISTONI ◽  
C BLOISE ◽  
C FORTI ◽  
M GRECO ◽  
J RANFT ◽  
...  

1949 ◽  
Vol 76 (8) ◽  
pp. 1273-1274 ◽  
Author(s):  
L. Leprince-Ringuet ◽  
F. Bousser ◽  
Hoang-Tchang-Fong ◽  
L. Jauneau ◽  
D. Morellet

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