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2011 QCD and High Energy Interactions - Rencontres de Moriond ...

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In Ref. 6 , the saturated Froissart bound above s = sF leads to a cross section of the form:<br />

σt(s > sF ) = σt(sF ) + (π/so) · ln 2 (s/sF ). (2)<br />

The parameter sF is <strong>de</strong>termined from the position of a knee observed in the energy <strong>de</strong>pen<strong>de</strong>nce<br />

of σsd at √ s = √ s knee (see Fig. 1 in Ref. 6 ). The knee is attributed to a saturation in multiple<br />

wee-parton exchanges, manifesting as the scaling parameter so of the sub-energy-squared of<br />

the diffractive system, s ′ ≡ M 2 (see Eq. 1), which i<strong>de</strong>ntifies so as a mass-squared, so ≡ M 2 o .<br />

Thus, Mo is reasonably interpreted as the mass of a saturated partonic glueball-like exchange,<br />

whimsically named superball in Ref. 5 . Inserting so into Eq. (2) in place of m 2 π yields an analytic<br />

expression for the total cross section for s > sF .<br />

Predicting the total cross section at the LHC using Eq. (2) requires knowledge of σt(sF ).<br />

The cross section at √ sF = 22 GeV, however, has substantial Reggeon-exchange contributions,<br />

<strong>and</strong> also contributions from the interference between the nuclear <strong>and</strong> Coulomb amplitu<strong>de</strong>s. A<br />

complete <strong>de</strong>scription must take into consi<strong>de</strong>ration all these contributions, using Regge or partonmo<strong>de</strong>l<br />

amplitu<strong>de</strong>s to <strong>de</strong>scribe Reggeon exchanges, <strong>and</strong> dispersion relations to obtain the real part<br />

of the amplitu<strong>de</strong> from measured total cross sections up to Tevatron energies. In the RENORM<br />

mo<strong>de</strong>l, we follow a strategy that bypasses all these hurdles. For completeness, we outline below<br />

all the steps in the cross section evaluation process:<br />

(i) Use the Froissart formula as a saturated bound;<br />

(ii) Eq. (2) should then <strong>de</strong>scribe the cross section above the knee in σsd vs √ s, which occurs<br />

at √ s F = 22 GeV, <strong>and</strong> therefore should be valid at the Tevatron at √ s = 1800 GeV;<br />

(iii) replace m 2 π by m 2 superball = so/(¯hc) 2 ≈ (3.7 ± 1.5)/0.389 GeV 2 in the coefficient C = π/m 2 π;<br />

(iv) note that Reggeon-exchange contributions at √ s = 1800 GeV are negligible (see Ref. 12 );<br />

(v) obtain the total cross section at the LHC as:<br />

σ lhc<br />

t = σ cdf<br />

t + π<br />

⎡<br />

2 ⎤<br />

2<br />

⎣<br />

−<br />

⎦ . (3)<br />

so<br />

Using the CDF σ CDF<br />

t<br />

ln sLHC<br />

sF<br />

ln sCDF<br />

sF<br />

= 80.03 ± 2.24 mb at √ s = 1.8 TeV, this formula predicts the cross<br />

sections shown in Table 1. The values for σel <strong>and</strong> σinel are also shown, obtained using the ratios<br />

of R el/t ≡ σel/σt of the global fit of Ref. 12 . The result for σt at √ s = 14 TeV falls within the<br />

Table 1: Predicted σt, σel <strong>and</strong> σinel pp cross sections [mb] at LHC; uncertainties are dominated by that in so.<br />

√ s σt σel σinel<br />

7 TeV 98 ± 8 27 ± 2 71 ± 6<br />

8 TeV 100 ± 8 28 ± 2 72 ± 6<br />

14 TeV 109 ± 12 32 ± 4 76 ± 8<br />

range of cross sections predicted by the various authors in Ref. 5 , <strong>and</strong> is in good agreement with<br />

the value of 114 ± 5 mb of the global fit of Ref. 12 , where the uncertainty was propagated from<br />

the ±δɛ value reported in the paper using the correlation between σt <strong>and</strong> ɛ through σt ∼ s ɛ .<br />

The February <strong>2011</strong> (pre-<strong>Moriond</strong>) ATLAS result for √ s = 7 TeV was 7 :<br />

σinel(ξ > 10 −5 ) = 57.2 ± 0.1(stat.) ± 0.4(syst.) ± 6.3(Lumi) mb (4)<br />

Based on a PYTHIA (PHOJET) extrapolation, a σinel = 63.3 ± 7.0 mb (60.1 ± 6.6 mb) was<br />

obtained. These results/predictions provi<strong>de</strong>d the motivation for updating the RENORM prediction<br />

<strong>and</strong> presenting the result in <strong>Moriond</strong>-<strong>2011</strong>.

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