scholarly journals Jet Asymmetry in High Energy Diffractive Production

2000 ◽  
Author(s):  
Stanley J Brodsky
Keyword(s):  
High Energy ◽  
Diffractive Production

scholarly journals Tensor pomeron, vector odderon and diffractive production of meson and baryon pairs in proton-proton collisions

2019 ◽  
Vol 206 ◽  
pp. 06005 ◽  
Author(s):  
Piotr Lebiedowicz ◽  
Otto Nachtmann ◽  
Antoni Szczurek
Keyword(s):  
Experimental Data ◽  
High Energy ◽  
Proton Proton ◽  
Proton Collisions ◽  
High Energies ◽  
Energy Proton ◽  
Diffractive Production ◽  
Proton Proton Collisions ◽  
Theoretical Results ◽  
The Continuum

We review some selected results of the tensor-pomeron and vectorodderon model of soft high-energy proton-proton scattering and central exclusive production of meson and baryon pairs in proton-proton collisions. We discuss the theoretical aspects of this approach and consider the phenomenological implications in a variety of processes at high energies, comparing to existing experimental data. We consider the diffractive dipion and dikaon production including the continuum and the dominant scalar and tensor resonance contributions as well as the photoproduction processes. The theoretical results are compared with existing CDF experimental data and predictions for planned or current LHC experiments, ALICE, ATLAS, CMS, LHCb are presented.

scholarly journals Impact factor for high-energy two and three jets diffractive production

2015 ◽  
Author(s):  
R. Boussarie ◽  
A.V. Grabovsky ◽  
L. Szymanowski ◽  
S. Wallon
Keyword(s):  
Impact Factor ◽  
High Energy ◽  
Diffractive Production

scholarly journals Diffractive production of Λ hyperons in the high-energy limit of strong interactions

2020 ◽  
Vol 102 (9) ◽  
Author(s):  
Francesco Giovanni Celiberto ◽  
Dmitry Yu. Ivanov ◽  
Alessandro Papa
Keyword(s):  
High Energy ◽  
Strong Interactions ◽  
Energy Limit ◽  
High Energy Limit ◽  
Diffractive Production

Diffractive production of vector mesons in high-energy photon-photon collisions

1982 ◽  
Vol 26 (5) ◽  
pp. 1175-1178
Author(s):  
L. Maharana ◽  
S. P. Misra ◽  
A. R. Panda
Keyword(s):  
High Energy ◽  
High Energy Photon ◽  
Vector Mesons ◽  
Energy Photon ◽  
Diffractive Production

scholarly journals Non-linear evolution and high energy diffractive production

2001 ◽  
Vol 521 (3-4) ◽  
pp. 233-238 ◽  
Author(s):  
E. Levin ◽  
M. Lublinsky
Keyword(s):  
High Energy ◽  
Linear Evolution ◽  
Diffractive Production ◽  
Non Linear

scholarly journals Jet asymmetry in high energy diffractive production

2001 ◽  
Vol 96 (1-3) ◽  
pp. 141-145
Author(s):  
C. Merino ◽  
Stanley J. Brodsky ◽  
J. Rathsman
Keyword(s):  
High Energy ◽  
Diffractive Production

scholarly journals Impact factor for high-energy two and three jets diffractive production

2014 ◽  
Vol 2014 (9) ◽  
Author(s):  
R. Boussarie ◽  
A. V. Grabovsky ◽  
L. Szymanowski ◽  
S. Wallon
Keyword(s):  
Impact Factor ◽  
High Energy ◽  
Diffractive Production

Diffractive Production of Vector Mesons in High-Energy Neutrino Interactions

1978 ◽  
Vol 40 (19) ◽  
pp. 1226-1229 ◽  
Author(s):  
J. Bell ◽  
J. P. Berge ◽  
D. V. Bogert ◽  
R. J. Cence ◽  
C. T. Coffin ◽  
...  
Keyword(s):  
High Energy ◽  
Vector Mesons ◽  
High Energy Neutrino ◽  
Neutrino Interactions ◽  
Energy Neutrino ◽  
Diffractive Production

The E-ring: interactions with plasma and implications for its evolution

1984 ◽  
Vol 75 ◽  
pp. 599-602
Author(s):  
T.V. Johnson ◽  
G.E. Morfill ◽  
E. Grun
Keyword(s):  
Time Scale ◽  
Particle Density ◽  
High Energy ◽  
Particle Removal ◽  
Density Region ◽  
Drag Forces ◽  
Orbit Evolution ◽  
History Of ◽  
Ring Particle ◽  
Ring Material

A number of lines of evidence suggest that the particles making up the E-ring are small, on the order of a few microns or less in size (Terrile and Tokunaga, 1980, BAAS; Pang et al., 1982 Saturn meeting; Tucson, AZ). This suggests that a variety of electromagnetic and plasma affects may be important in considering the history of such particles. We have shown (Morfill et al., 1982, J. Geophys. Res., in press) that plasma drags forces from the corotating plasma will rapidly evolve E-ring particle orbits to increasing distance from Saturn until a point is reached where radiation drag forces acting to decrease orbital radius balance this outward acceleration. This occurs at approximately Rhea's orbit, although the exact value is subject to many uncertainties. The time scale for plasma drag to move particles from Enceladus' orbit to the outer E-ring is ~104yr. A variety of effects also act to remove particles, primarily sputtering by both high energy charged particles (Cheng et al., 1982, J. Geophys. Res., in press) and corotating plasma (Morfill et al., 1982). The time scale for sputtering away one micron particles is also short, 102 - 10 yrs. Thus the detailed particle density profile in the E-ring is set by a competition between orbit evolution and particle removal. The high density region near Enceladus' orbit may result from the sputtering yeild of corotating ions being less than unity at this radius (e.g. Eviatar et al., 1982, Saturn meeting). In any case, an active source of E-ring material is required if the feature is not very ephemeral - Enceladus itself, with its geologically recent surface, appears still to be the best candidate for the ultimate source of E-ring material.

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