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[a]B.F.L. Ward

Role of IR-Improvement in LHC/FCC Physics

   B. Shakerin    S. A. Yost
Abstract

One may use amplitude-based resummation in QED \otimes QCD to achieve IR-improvement of unintegrable singularities in the infrared regime to arbitrary precision in principle. We illustrate such improvement in specific examples in precision LHC/FCC physics.

BU-HEPP-20-05, Dec., 2020

In the context of QCD, in addition to the original discussion 111F. Berends, private communication, at 1988 ICHEP Conference Dinner, Munich, Germany. of whether the naive Jackson-Scharre [1] or the exact YFS-style [2] resummation is more accurate for a given level of exactness, we have the issue of a hard cut-off for the IR versus resummed IR integrability. Somewhat unexpectedly, in the current era of QCD with precision tags 1.0%\lesssim 1.0\% with accompanying EW precision tags at the per mille level for processes such as single heavy gauge boson production at the LHC, the “new” issue of ISR radiation from quarks has arisen featuring the choice between QED PDF’s with massless light quarks vs exact Feynman diagrams with short-distance quark masses and non-QED PDF’s. The precision data should be able to settle these additional issues as it resolves the original discussion for the QCD case. Even higher precision may open further issues – such is the nature of progress in precision applications of quantum field theory.

We have pursued exact amplitude-based resummation realized on an event-by-event basis via shower/matrix element(ME) matched MC’s in order to achieve enhanced precision for a given level of exactness while addressing the present paradigm in precision physics at the LHC and the futuristic FCC. Currently, we have a realization of IR-improved parton showers in the Herwig6.5 [3] environment in the MC Herwiri1.031 [4] by two of us (BFLW and SAY). Via the MC@NLO [5] and the MG5_aMC@NLO [6] frameworks this MC is elevated to the exact NLO shower/ME matched level as MC@NLO/Herwiri1.031 [7] and MG5_aMC@NLO/Herwiri1.031 [8], respectively. We have the realization of IR-improved (IRI) Pythia8 [10] by one of us (BFLW) in the Pythia8 [9] environment, with its corresponding NLO shower/ME matched MG5_aMC@NLO/IRI-Pythia8. More recently, two of us (BFLW and SAY), using the Herwig6.5 environment, have realized in the MC 𝒦𝒦{\cal KK}MC-hh [11] exact 𝒪(α2L){\cal O}(\alpha^{2}L) CEEX EW corrections in a hadronic MC.

As two of us (BFLW, SAY) have shown  [4, 7], IR-improvement in Herwig6.5 via Herwiri1.031 leads to improved precision in both the central |η|2.5|\eta_{\ell}|\lesssim 2.5 region for the ATLAS, CMS, D0 and CDF data and in the more forward region of LHCb where 2.0<η<4.52.0<\eta_{\ell}<4.5. Here, |η||\eta_{\ell}| is the lepton pseudorapidity in respective single Z/γZ/\gamma^{*} production production with decay to lepton pairs. One of us (BFLW) [12] has shown the availability of the IR-improved semi-analytical paradigm for the latter processes. In what follows, we present an update the application of our methods in the analysis of LHC W+ n jets data, in the FCC discovery physics and in the interplay of IR-improved parton showers with exact 𝒪(α2L){\cal O}(\alpha^{2}L) CEEX EW corrections in 𝒦𝒦{\cal KK}MC-hh.

We note that 2017 was the 50th anniversary of the seminal paper by S. Weinberg [13] in which he formulated his foundational model of leptons in creating the spontaneously broken SU2L×U1SU_{2L}\times U_{1} EW theory [14, 15], one of the key components of the SM, which we may now call the Standard Theory (ST) 222See D.J. Gross, talk, SM@50 Symposium, Cleveland, OH, June, 2018.. Progress on precision theory has been essential to the establishment of the ST[13, 14, 15, 16, 17]. As we celebrate 50 years of the ST (SM) [18], we are also obliged to look to the future with the FCC [19], CLIC, ILC, or CEPC on the horizion [20], where, for example, we note that the FCC

Refer to caption
Figure 1: FCC device planned for the future at CERN as depicted in Ref. [19].

will feature a 100 TeV hadron collider and a tera-Z e+ee^{+}e^{-} colliding beam device, as illustrated in Fig. 1. The success of the latter devices will be strongly correlated with the progress of precision theory.

The paper is organized as follows. We briefly review the parton shower implementation of exact amplitude-based resummation theory, after which we turn to the interplay of IR-improved DGLAP-CS QCD theory and shower/ME matched precision via comparisons with LHC data on W+nW+n jets and via predictions for FCC discovery physics. Finally, we discuss the interplay of IR-improved DGLAP-CS QCD theory and exact 𝒪(α2L){\cal O}(\alpha^{2}L) CEEX EW corrections in single Z/γZ/\gamma^{*} production at the LHC.

The parton shower implementation of exact amplitude-based resummation theory has as its starting point the master formula

dσ¯res=eSUMIR(QCED)n,m=01n!m!j1=1nd3kj1kj1\displaystyle d\bar{\sigma}_{\rm res}=e^{\rm SUM_{IR}(QCED)}\Large{\sum}_{{n,m}=0}^{\infty}\frac{1}{n!m!}\int\prod_{j_{1}=1}^{n}\frac{d^{3}k_{j_{1}}}{k_{j_{1}}} (1)
j2=1md3kj2kj2d4y(2π)4eiy(p1+q1p2q2kj1kj2)+DQCED\displaystyle\prod_{j_{2}=1}^{m}\frac{d^{3}{k^{\prime}}_{j_{2}}}{{k^{\prime}}_{j_{2}}}\int\frac{d^{4}y}{(2\pi)^{4}}e^{iy\cdot(p_{1}+q_{1}-p_{2}-q_{2}-\sum k_{j_{1}}-\sum{k^{\prime}}_{j_{2}})+D_{\rm QCED}} (2)
β¯~n,m(k1,,kn;k1,,km)d3p2p2 0d3q2q2 0,\displaystyle{\tilde{\bar{\beta}}_{n,m}(k_{1},\ldots,k_{n};k^{\prime}_{1},\ldots,k^{\prime}_{m})}\frac{d^{3}p_{2}}{p_{2}^{\,0}}\frac{d^{3}q_{2}}{q_{2}^{\,0}}, (3)

where new (YFS-style) non-Abelian residuals β¯~n,m(k1,,kn;k1,,km)\tilde{\bar{\beta}}_{n,m}(k_{1},\ldots,k_{n};k^{\prime}_{1},\ldots,k^{\prime}_{m}) have nn hard gluons and mm hard photons. Definitions of the infrared functions SUMIR(QCED){\rm SUM_{IR}(QCED)} and DQCED{D_{\rm QCED}} and of the residuals are given in Ref. [7]. In the framework of shower/ME matching, we have the replacements β¯~n,mβ¯~^n,m\tilde{\bar{\beta}}_{n,m}\rightarrow\hat{\tilde{\bar{\beta}}}_{n,m}. These replacements allow us, via the basic formula

dσ=i,j𝑑x1𝑑x2Fi(x1)Fj(x2)𝑑σ^res(x1x2s),{d\sigma}=\sum_{i,j}\int dx_{1}dx_{2}{F_{i}(x_{1})F_{j}(x_{2})}d\hat{\sigma}_{\rm res}(x_{1}x_{2}s), (4)

to proceed with connection to MC@NLO as explained in Ref. [7].

Our (BS, BFLW) recent applications [21, 22] make comparisons between the LHC data on W+nW+n jets, n=1,2,3, and the exact NLO ME matched QCD parton shower predictions in the MG5_aMC@NLO framework with the parton shower realized via Herwig6.5 and Herwiri1.031 respectively for the unimproved and IR-improved results. We illustrate such results in Figs. 2 and  3 for the

(a)(b)Refer to captionRefer to caption
Figure 2: Comparison of CMS 8TeV cms energy W+1W+\geq 1 jet (a) and W+2W+\geq 2 jets (b) data for the respective leading jet and second leading jet pTp_{T} distributions and the IR-improved(herwiri) and unimproved (herwig) exact NLO ME matched parton shower predictions.
(a)(b)Refer to captionRefer to caption
Figure 3: Comparison of CMS 8TeV cms energy W+3W+\geq 3 jets (a) and W+1W+\geq 1 jet (b) data for the respective 3rd-leading jet pTp_{T} and HTH_{T} distributions and the IR-improved(herwiri) and unimproved (herwig) exact NLO ME matched parton shower predictions.

CMS [23] 8 TeV cms energy W+nW+\geq n jet data, n=1, 2, 3. Consistent with Refs. [7], the IR-improved results are closer to the data for low pT(HT)p_{T}(H_{T}).

Two of us (BFLW and SAY) have investigated the effect of IR-improvement on the discovery reach of a standard candle process such as single Z/γZ/\gamma^{*} production at the FCC using the predicted inclusive cross section for Z/γZ/\gamma^{*} as a function of pT,minp_{T,min} 333This observable was suggested by M.L. Mangano, private communication, 2016. which is explained and shown in Fig. 6 in Ref. [24]. In the latter figiure we plot predictions for the following: MG5_aMC@NLO/A, A= Herwig6.5, Herwiri1.031, Herwig++ and Pythia8, all with the common renormalization and factorization scale of MZM_{Z}/2 and all with the common renormalization and factorization scale of HTH_{T}/2 (denoted by ’UNFIX’ in the legend in the figure) ; MG5_aMC@NLO/Herwig6.5 and fixed order NLO both with the common renormalization and factorization MZM_{Z}; and, fixed order NLO with the common renormalization and factorization scale HTH_{T}/2. Here, HTH_{T} is the sum of the transverse masses of the final state particles – see Ref. [24] for the remaining details. Our results show that the dynamical scale choice makes a big difference in the expectations, the fixed-order NLO results agree, as it is expected, with the MG5_aMC@NLO/Herwig6.5 results for both of the scale choices, and the IR-improved and unimproved predictions agree within the statistical uncertainties.

Finally, in Refs. [25, 26, 27] two of us (BFLW and SAY), in collaboration with S. Jadach and Z. Was, have analyzed the effects of the exact 𝒪(α2L){\cal O}(\alpha^{2}L) CEEX EW corrections in 𝒦𝒦{\cal KK}MC-hh on the analysis of the ZZ observables used in the ATLAS MWM_{W} measurement in Ref. [28]. We find new effects that should be considered at or above the per mille level. For example, the new modulation we see in the lepton pTp_{T} spectrum seems to match the trends in the data vs theory comparisons shown in Figs. 15 a and b in Ref. [28]. More specifically, we have found new effects sensitive to the transverse degrees of freedom in the ISR radiation as well as significant ISR effects in observables primarily sensitive to collinear ISR degrees of freedom, as we illustrate here in Table  1.

Table 1: Illustrations of ISR and IFI Effects

Numerical Results

No ISR LuxQED ISR 𝒦𝒦{\cal KK}MC-hh ISR ISR-no ISR With IFI %(IFI - no IFI)
Uncut σ\sigma 939.86(1) pb 944.04(1) pb 944.99(2) pb 0.546(2)% 944.91(2) pb 0.0089(4)-0.0089(4)%
Cut σ\sigma 439.10(1) pb 440.93(1) pb 442.36(1) pb 0.742(3)% 422.33(1) pb 0.0070(5)-0.0070(5)%
AFBA_{\rm FB} 0.01125(2) 0.01145(2) 0.1129(2) (3.9±2.8)×105(3.9\pm 2.8)\times 10^{-5} 0.01132(2) (2.9±1.1)×105(2.9\pm 1.1)\times 10^{-5}
A4A_{4} 0.06102(3) 0.06131(3) 0.06057(3) (4.4±0.5)×104(-4.4\pm 0.5)\times 10^{-4} 0.06102(3) (4.5±0.3)×104(4.5\pm 0.3)\times 10^{-4}

The ISR and IFI effects on AFBA_{FB} is of order 10510^{-5} while the effect on A4A_{4} is of order 10410^{-4}

in 𝒦𝒦{\cal KK}MC-hh. LuxQED gives an ISR effect on the order of 10410^{-4} for both AFBA_{FB} and A4A_{4}.

We are extending the analysis in Refs. [25, 26, 26] to IR-improved showers with the new MC 𝒦𝒦{\cal KK}MC-hh/Herwiri1.031 as explained and illustrated in Ref. [24].

Acknowledgments

This work was partially supported by The Citadel Foundation. We thank the INP, Krakow, PL for computational resources. One of us (BFLW) thanks Prof. Gian Giudice for the support and kind hospitality of the CERN TH Department.

References

  • [1] J.D. Jackson and D.L. Scharre, Nucl. Instum. Meth.128 (1975) 13.
  • [2] D. R. Yennie, S. C. Frautschi, and H. Suura, Ann. Phys. 13 (1961) 379; see also K. T. Mahanthappa, Phys. Rev. 126 (1962) 329, for a related analysis.
  • [3] G. Corcella et al., hep-ph/0210213; J. High Energy Phys. 0101 (2001) 010; G. Marchesini et al., Comput. Phys. Commun. 67 (1992) 465.
  • [4] S. Joseph et al., Phys. Rev. D81 (2010) 076008, arXiv:1001.1434.
  • [5] S. Frixione and B.Webber, J. High Energy Phys. 0206 (2002) 029; S. Frixione et al., arXiv:1010.0568; B. Webber, talk at CERN, 03/30/2011; S. Frixione, talk at CERN, 05/04/2011.
  • [6] A. Alwall et al., arXiv:1405.0301, and references therein.
  • [7] S.K. Majhi et al., Phys. Lett. B719 (2013) 367, arXiv:1208.4750; A. Mukhopadhyay and B.F.L. Ward, Mod. Phys. Lett. A 31 (2016) 1650063, arXiv:1412.8717.
  • [8] B. Shakerin and B.F.L. Ward, PoS(ICHEP2016) (2016) 1144; arXiv:1809.01492; BU-HEPP-17-05; BU-HEPP-18-02.
  • [9] T. Sjostrand, S. Mrenna and P. Skands, Comput. Phys. Commun. 178 (2008) 852; T. Sjostrand, arXiv:0809.0303, DOI:10.3204/DESY-PROC-2009-02/41; T. Sjostrand et al., Comput. Phys. Commun. 191 (2015) 159.
  • [10] B.F.L. Ward, Compt. Phys. Commun. 201 (2016) 29, arXiv:1504.00892.
  • [11] S. Jadach, B.F.L. Ward, Z. A. Was and S. A. Yost, Phys. Rev. D 94 (2016) 074006.
  • [12] B.F.L. Ward, Mod. Phys. Lett. A 31 (2016) 1650126, arXiv:1407.7290.
  • [13] Phys. Rev. Lett. 19 (1967) 1264.
  • [14] S. L. Glashow, Nucl. Phys. 22 (1961) 579.
  • [15] A. Salam, in Elementary Particle Theory, ed. N. Svartholm (Amquist and Wiksell, Stockholm, 1968).
  • [16] D.J. Gross and F. wilczek, Phys. Rev. Lett. 30 (1973) 1343.
  • [17] H.D. Ploitzer, Phys. Rev. Lett. 30 (1973) 1346.
  • [18] B.W. Lynn et al., to appear.
  • [19] M. Benedikt and F. Zimmermann, talk in 2017 FCC Week, Berlin, 2017.
  • [20] A. Blondel and P. Janot, arXiv:1912.11871; A. Blondel, in these Proceedings.
  • [21] B. Shakerin and B.F.L. Ward, BU-HEPP-17-04, arXiv:1809.01492, Phys. Rev. D 100 (2019) 034026; BU- HEPP-17-05.
  • [22] B. Shakerin and B.F.L. Ward, BU-HEPP-18-02; BU-HEPP-19-05, Int. J. Mod. Phys. A 35 (2020) 2050197, arXiv: 2011.08313.
  • [23] V. Khachatryan et al. [CMS Collaboration], Phys. Rev. D 95 (2017) 052002; arXiv:1610.04222 [hep-ex] – https://www.hepdata.net/record/76995.
  • [24] B.F.L. Ward et al., PoS(RADCOR2017) (2018)
  • [25] S. Jadach, B.F.L. Ward, Z. A. Was and S. A. Yost, Phys. Rev. D 94 (2016) 074006.
  • [26] S. Jadach, B.F.L. Ward, Z. A. Was and S. A. Yost, BU-HEPP-17-01, IFJPAN-IV-2017-15, arXiv:1707.06502, Phys. Rev. D 99 (2019) 076016.
  • [27] S. Jadach, B.F.L. Ward, Z. A. Was and S. A. Yost, BU-HEPP-19-10, arXiv: 2002.11692.
  • [28] M. Aaboud et al., arXiv:1701.07240.