Latest theoretical developments in top physics at hadron colliders Alexander Mitov Theory Division, CERN Based on works with: Michal Czakon ‘11 and (in.

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Presentation transcript:

Latest theoretical developments in top physics at hadron colliders Alexander Mitov Theory Division, CERN Based on works with: Michal Czakon ‘11 and (in progress) Cacciari, Czakon, Mangano and Nason ‘11 George Sterman (in progress)

Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012 Plan for the talk ① What is well established ① Open questions ① Recent results ① Brand new results (game changer; ~25-years in the waiting) The focus is on the total inclusive cross-section. Will comment on differential too.

What is well established Top-pair production is completely known within NLO/NNLL QCD Main features: Very large NLO corrections ~50% Theory uncertainty at ~10% Important for Higgs and bSM physics Experimental improvements down to 5% Current LHC data agrees well with SM theory Tevatron data generally agrees too. The notable exception: Forward-backward asymmetry from CDF. Important shift in gears: currently we have fully differential NLO calculations including top decays. This is the direction of the future. Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

Open questions Reliably increase the precision of the theoretical predictions? [more next] What to make of the forward – backward asymmetry? Can missing theory corrections be large? Yes! (almost universally assumed small) Is this enough to explain A FB ? Perhaps not! This will only be settled once the SM predictions have been exhausted (currently A FB (tT+X) is at LO!) Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

Recent results How to improve theory? All improvements in the last years are based on soft gluon resummation. This has recently been extended to full NNLL level … and analyzed by a number of groups: Conclusion: resummation is  very important at LL,  relatively important at NLL,  modest improvement at NNLL(+NLO) (compared to other missing contributions) at NNLL level total uncertainty is reduced: 10%  9% Lots of activity recently. Note of caution: resummation (or its truncation NNLO_approx) are not substitutes for NNLO. Ahrens, Ferroglia, Neubert, Pecjak, Yang Kidonakis Aliev, Lacker, Langenfeld, Moch, Uwer, Wiedermann Beneke, Falgari, Klein, Schwinn Cacciari, Czakon, Mangano, Mitov, Nason Cacciari, Czakon, Mangano, Mitov, Nason `11 Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012 Czakon, Mitov, Sterman `09 Beneke, Falgari, Schwinn ‘09

Recent results  Resummed results are better when close to threshold (as expected)  One can quantify the question: when are we close to threshold? (below 1 TeV or so)  Approx_NNLO is a subset of the resumed result. Overused recently. Has accidentally small scale dependence. Textbook example: by changing the collider energy go into (out of) the threshold region Cacciari, Czakon, Mangano, Mitov, Nason `11 Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

Recent results We have also prepared the tools for top physics: Top++ : a C++ program for the calculation of the total cross-section: Includes:  fixed order (NLO and NNLO_approx at present)  and resummation (full NNLL already there) It is meant to incorporate the full NNLO once available (to appear) Very user friendly. Czakon, Mitov `11 Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

Brand new results Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

Motivating question: can A FB be generated (or enhanced) by tT final state interactions? Work with George Sterman, to appear Brand new results Prompted, in turn, by older work in QED We have devised an all-order proof of the cancellations of such interactions The subtle point is: What is the remainder? All depends on observables’ definition. For inclusive observables (with conventional factorization) the remainder is small. For observables with rapidity gaps: large corrections are possible. See, for example, Brodsky, Gillespie`68 Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

NNLO result for qq  tT at Tevatron and LHC Work with M. Czakon, P. Barnreuther Recall: NLO corrections derived almost 25 years ago Nason, Dawson, Ellis `88 ‚89 Beenakker, Kuijf, van Neerven, Smith `89 First ever hadron collider calculation at NNLO with more than 2 colored partons. First ever NNLO hadron collider calculation with massive fermions. Brand new results Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

What is computed? The partonic cross-section computed numerically in 80 points. Then fitted. Many contributing partonic channels: All of the same complexity. No more conceptual challenges expected (just lots of CPU) Computed. Dominant at Tevatron (~85%) Relative velocity of tT

Results: partonic cross-section through NNLO LO – green NLO - blue NNLO - red (with errors) approximate NNLO - black β Notable features: Small numerical errors Agrees with limits Preliminary Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

What happens once we add the flux?  The difference increases! Approx_NNLO - blue Exact NNLO – red β Preliminary Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

Preliminary Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012 Here are the numbers for the Tevatron: NNLO: sigma_tot = % % [pb]. NNLO+NNLL: sigma_tot = % % [pb]. Preliminary Very week dependence on unknown parameters (sub 1%): gg NNLO, A, etc. 50% scales reduction compared to the NLO+NNLL analysis of Cacciari, Czakon, Mangano, Mitov, Nason ‘ % - 6.1%

Summary and Conclusions  Long (~15 years) and turbulent chapter in top physics is closing  It saw uses of soft gluon resummation to a number of approximations at NNLO  It was theoretically very fruitful: engine for theoretical developments  We have derived the full NNLO result qq  tt (numeric – very good precision)  at Tevatron it cuts scale uncertainty in half compared to NLO+NNLL  Words like approx_NNLO, etc., belong in the past.  Methods are very general and applicable to differential distributions  Applications for dijets and W+jet, H+jet, NNLO  Only restriction – availability of two-loop amplitudes and computing speed  We are on the verge of the NNLO revolution (NLO wish-list already exhausted ) Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

Backup slides

What’s needed for NNLO? There are 3 principle contributions: 2-loop virtual corrections (V-V) 1-loop virtual with one extra parton (R-V) 2 extra emitted partons at tree level (R-R) And 2 secondary contributions: Collinear subtraction for the initial state One-loop squared amplitudes (analytic) Korner, Merebashvili, Rogal `07 Known, in principle. Done numerically. Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

What’s needed for NNLO? V-V Required are the two loop amplitudes: qq  QQ and gg  QQ. Their high energy limits and their poles are known analytically Directly used here: The qq  QQ amplitude is known numerically Numerical work underway for the gg  QQ Czakon, Mitov, Moch ’07 Czakon, Mitov, Sterman ‘09 Ferroglia, Neubert, Pecjak, Yang ’09 Czakon `07 Czakon, Bärnreuther, to appear What’s the future here? Right now this is the biggest (and perhaps only) obstacle for NNLO phenomenology on a mass scale Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

A wonderful result By M. Czakon The method is general (also to other processes, differential kinematics, etc). Explicit contribution to the total cross-section given. Just been verified in an extremely non-trivial problem. What’s needed for NNLO? R-R Czakon `10-11 Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012

What’s needed for NNLO? R-V Counterterms all known (i.e. all singular limits) The finite piece of the one loop amplitude computed with a private code of Stefan Dittmaier. Extremely fast code! A great help! Many thanks! Bern, Del Duca, Kilgore, Schmidt ‘98-99 Catani, Grazzini ’00 Bierenbaum, Czakon, Mitov ‘11 Latest theoretical developments in top physics Alexander Mitov DIS2012, Bonn, 27/03/2012