Lessons from LHC elastic and diffractive data

We study the behavior of elastic and diffractive proton dissociation cross sections at high energy. First, we describe what would be expected to be observed at the Large Hadron Collider (LHC) based on conventional Regge theory. We emphasize the tension between these expectations and the recent LHC measurements, and we discuss the possibilty to modify the classic Reggeon Field Theory (RFT) in a physically-motivated way so as to accommodate the tendencies observed at the LHC. As a result, we show that we are able to achieve a "global" description of the wide variety of high energy elastic and diffractive data that are presently available, particularly from the LHC experiments. The model is based on only one pomeron pole, but includes multi-pomeron interactions and, significantly, includes the transverse momentum dependence of intermediate partons as a function of their rapidity, which provides the rapidity dependence of the multi-pomeron vertices. We give predictions for diffractive observables at LHC, and higher, energies.

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Tension in the LHC diffractive data?

10.1063/1.4915977 ◽

2015 ◽

Author(s):

Errol Gotsman

Keyword(s):

Diffractive Data

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Unitarisation dependence of diffractive scattering in light of high-energy collider data

Journal of High Energy Physics ◽

10.1007/jhep09(2021)005 ◽

2021 ◽

Vol 2021 (9) ◽

Author(s):

Arno Vanthieghem ◽

Atri Bhattacharya ◽

Rami Oueslati ◽

Jean-René Cudell

Keyword(s):

Imaginary Part ◽

Cross Sections ◽

Cosmic Ray ◽

High Energy ◽

Additional Parameter ◽

Elastic Amplitude ◽

The Real ◽

Diffractive Scattering ◽

Diffractive Data ◽

High Energy Collider

Abstract We study the consequences of high-energy collider data on the best fits to total, elastic, inelastic, and single-diffractive cross sections for pp and $$ p\overline{p} $$ p p ¯ scattering using different unitarisation schemes. We find that the data are well fitted both by eikonal and U-matrix schemes, but that diffractive data prefer the U-matrix. Both schemes may be generalised by means of an additional parameter; however, this yields only marginal improvements to the fits. We provide estimates for ρ, the ratio of the real part to the imaginary part of the elastic amplitude, for the different fits. We comment on the effect of the different schemes on present and future cosmic ray data.

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