1992
DOI: 10.1103/physrevd.45.839
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How large is the total cross section at supercollider energies?

Abstract: Although the value of the total cross section is critical for the operation and physics exploitation of supercolliders, we have until now been unable to anticipate its magnitude. Extrapolations of lowenergy data patterned after models with a varying degree of dynamical justification, and invariably a too large number of free parameters to be truly predictive, led to a wide range of predictions. We point out that a series of new measurements at the Fermilab Tevatron Collider on forward-scattering parameters dra… Show more

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Cited by 36 publications
(50 citation statements)
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“…That is the case in the formalisms by Margolis et al [25,26,27] and the more recent version sometimes referred to as Aspen model, by Block et al [28,29]. However, despite its efficiency in the description of the forward quantities in the elastic channel, as well as differential cross sections at small values of the momentum transfer a serious drawback with the Aspen model concerns the absence of the expected connections with nonperturbative QCD.…”
Section: Eikonalized Approachmentioning
confidence: 89%
See 1 more Smart Citation
“…That is the case in the formalisms by Margolis et al [25,26,27] and the more recent version sometimes referred to as Aspen model, by Block et al [28,29]. However, despite its efficiency in the description of the forward quantities in the elastic channel, as well as differential cross sections at small values of the momentum transfer a serious drawback with the Aspen model concerns the absence of the expected connections with nonperturbative QCD.…”
Section: Eikonalized Approachmentioning
confidence: 89%
“…The convenience of the general structure adopted in the parametrizations (10), (13), (14) and (15) can be traced back to the early work of Margolis et al [25,26,27] and references therein.…”
Section: Eikonalized Approachmentioning
confidence: 99%
“…The proton-proton cross section at 10 8 TeV energy is roughly 100 mb [13]. The interaction length of a proton in the atmosphere corresponding to this interaction cross section is 40 g cm −2 , i.e.…”
Section: The Highest Energy Cosmic Rays: a Paradoxmentioning
confidence: 98%
“…This relation seems to be a plausible possibility and in this paper we will show that the dynamical gluon mass, as well as the IR finite coupling constant associated to it [14], are in fact the natural regulators for the cross sections calculations. Since the behavior of the running coupling constant is constrained by the value of the dynamical gluon mass [12,14], we will be able to substitute the two ad hoc parameters in the "mini-jet" models [6,7,8], namely the infrared mass scale (m 0 ) and the effective value of the running coupling constant (α s ), by a physically well motivated one. In this way, beyond the natural interpretation of the arbitrary infrared mass scale in terms of a dynamical one, it is possible to decrease the number of parameters in this line of models.…”
Section: Introductionmentioning
confidence: 99%
“…The energy dependence of the cross sections is driven especially by gluon-gluon scattering processes, where the behavior of the gluon distribution function at small x exhibits the power law g(x, Q 2 ) ∼ x −J (see [6,7,8] and references therein). In this case it is the gluon-gluon subprocess cross section that is potentially divergent at small transferred momenta.…”
Section: Introductionmentioning
confidence: 99%