Time-like Showers and Matching with Antennae

Slides:



Advertisements
Similar presentations
Work done in collaboration with Stefano Frixione 1 Leonardo Bertora, 2004 April 14 Jet and Di-jet production in Photon–Photon collisions Leonardo Bertora.
Advertisements

Monte Carlo Event Generators
Maria Jose Costa, CERN DIS 2004 April 14 th -18 th 2004, Slovakia b -mass effects in 3 and 4 jets events with the DELPHI detector at LEP b u,d,s.
Jet cross sections at NNLO accuracy Thomas Gehrmann, Universität Zürich The first three years of the LHC - MITP 2013.
Les Houches 2007 VINCIA Peter Skands Fermilab / Particle Physics Division / Theoretical Physics In collaboration with W. Giele, D. Kosower.
Monte Carlo event generators for LHC physics Mike Seymour University of Manchester CERN Academic Training Lectures July 7 th – 11 th 2003
Wine & Cheese Seminar 17 th March1 Recent Developments in Monte Carlo Event Generators Peter Richardson IPPP, Durham University Durham University.
Freiburg, Apr Designer Showers and Subtracted Matrix Elements Peter Skands CERN & Fermilab.
Les Houches 12 th June1 Generator Issues Peter Richardson IPPP, Durham University.
Forward Jet Production at HERA, Patrick Ryan, Univ. of Wisconsin EPS2005, July 21, Patrick Ryan University of Wisconsin On Behalf of the H1 and.
Les Houches 14 th June1 Matching Matrix Elements and Parton Showers Peter Richardson IPPP, Durham University.
LoopFest VI, Fermilab, April 2007 Parton Showers and NLO Matrix Elements Peter Skands Fermilab / Particle Physics Division / Theoretical Physics In collaboration.
Recent Advances in QCD Event Generators
A Comparison of Three-jet Events in p Collisions to Predictions from a NLO QCD Calculation Sally Seidel QCD’04 July 2004.
Ursula Bassler, LPNHE-Paris, RUN II MC workshop 1 Monte Carlo Tuning: The HERA Experience Monte Carlo Models for DIS events Description of inclusive hadronic.
Parton Showers and Matrix Element Merging in Event Generator- a Mini-Overview Introduction to ME+PS Branching and Sudakov factor (no branching) Matching.
Hadron Collisions, Heavy Particles, & Hard Jets Seminaire, LAPTH Annecy, Novembre 2005 (Butch Cassidy and the Sundance Kid) Real life is more complicated.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #14.
Working group C summary Hadronic final states theory Mrinal Dasgupta.
Copenhagen, Apr QCD Phenomenology at Hadron Colliders Peter Skands CERN TH / Fermilab.
The Dipole-Antenna approach to Shower Monte Carlo's W. Giele, HP2 workshop, ETH Zurich, 09/08/06 Introduction Color ordering and Antenna factorization.
Aachen, November 2007 Event Generators 2 Advanced Topics Peter Skands CERN / Fermilab Evolution First dayHands-on-sessions.
Measurement of α s at NNLO in e+e- annihilation Hasko Stenzel, JLU Giessen, DIS2008.
Squarks & Gluinos + Jets: from ttbar to SUSY at the LHC Peter Skands (Fermilab) with T. Plehn (MPI Munich), D. Rainwater (U Rochester), & T. Sjöstrand.
Radiation in high-^s final states Peter Skands (FNAL) with T. Plehn (MPI Munich) & D. Rainwater (U Rochester) ILC Workshop, Snowmass CO, Aug 2005.
Unintegrated parton distributions and final states in DIS Anna Stasto Penn State University Work in collaboration with John Collins and Ted Rogers `
Peter Skands Theoretical Physics, Fermilab Eugene, February 2009 Higher Order Aspects of Parton Showers.
Computational Methods in Particle Physics: On-Shell Methods in Field Theory David A. Kosower University of Zurich, January 31–February 14, 2007 Lecture.
Peter Skands Theoretical Physics, Fermilab Towards Precision Models of Collider Physics High Energy Physics Seminar, December 2008, Pittsburgh.
GGI October 2007 Red, Blue, and Green Things With Antennae Peter Skands CERN & Fermilab In collaboration with W. Giele, D. Kosower Giele, Kosower, PS :
Theory Seminar, SLAC, May 2007 Parton Showers and NLO Matrix Elements Peter Skands Fermilab / Particle Physics Division / Theoretical Physics In collaboration.
Sheffield Seminar 23 rd November1 Monte Carlos for LHC Physics Peter Richardson IPPP, Durham University Durham University.
David Milstead – Experimental Tests of QCD ITEP06 Winter School, Moscow Experimental Tests of QCD at Colliders: Part 1 David Milstead Stockholm University.
Introduction to Event Generators Peter Z. Skands Fermilab Theoretical Physics Department (Significant parts adapted from T. Sjöstrand (Lund U & CERN) )
Vincia: A new parton shower and matching algorithm W. Giele, ALCPG07 – LoopVerein session, 10/23/07 The new Vincia shower The pure Vincia shower The matched.
QCD Multijet Study at CMS Outline  Motivation  Definition of various multi-jet variables  Tevatron results  Detector effects  Energy and Position.
CERN October 2007 Exclusive Fashion Trends for Spring 2008 Peter Skands CERN & Fermilab.
Aachen, November 2007 Event Generators 3 Practical Topics Peter Skands CERN / Fermilab.
High P T Inclusive Jets Study High P T Inclusive Jets Study Manuk Zubin Mehta, Prof. Manjit kaur Panjab University, Chandigarh India CMS Meeting March,
Jets and α S in DIS Maxime GOUZEVITCH Laboratoire Leprince-Ringuet Ecole Polytechnique – CNRS/IN2P3, France On behalf of the collaboration On behalf of.
Measurement of b-quark mass effects for multi-jet events at LEP Juan A. Fuster Verdú EPS-2003 Aachen, July 2003.
October 2011 David Toback, Texas A&M University Research Topics Seminar1 David Toback Texas A&M University For the CDF Collaboration CIPANP, June 2012.
1 Forward Jet/  0 Production in DIS at HERA On behalf of the H1 and ZEUS Collaborations ICHEP August 2004, Beijing Didar Dobur, University of Freiburg.
Modern Approach to Monte Carlo’s (L1) The role of resolution in Monte Carlo’s (L1) Leading order Monte Carlo’s (L1) Next-to-Leading order Monte Carlo’s.
Heavy Particles & Hard Jets: from ttbar at the Tevatron to SUSY at the LHC Peter Skands (Fermilab) with T. Plehn (Edinburgh & MPI Munich), D. Rainwater.
IFIC. 1/15 Why are we interested in the top quark? ● Heaviest known quark (plays an important role in EWSB in many models) ● Important for quantum effects.
Modern Approach to Monte Carlo’s (L1) The role of resolution in Monte Carlo’s (L1) Leading order Monte Carlo’s (L1) Next-to-Leading order Monte Carlo’s.
Next Generation of Parton Shower Models and Validation W. Giele, CTEQ workshop “Physics at the LHC: Early Challenges”, 05/14/07 Introduction A new parton.
Tools08 1 st July1 PDF issues for Monte Carlo generators Peter Richardson IPPP, Durham University.
seminar at Academia Sinica
Introduction to Monte Carlo Event Generators
Generation comparison for top physics in CMS
Overview of IPPP Monte Carlo Tools
Peter Richardson IPPP, Durham University
QCD CORRECTIONS TO bb →h h
F. Maltoni, T. McElmurry, S. Willenbrock
Dr. Terrance Figy Assistant Professor
More Precision, Less Work
Lecture 2 Evolution and resummation
QCD Radiative Corrections for the LHC
Implications of First LHC Data: Underlying Event Measurements
Dijet Azimuthal Distributions at DØ
Monte Carlo Simulations
Pythia and Vincia P. Skands (Fermilab) with W. Giele, D. Kosower, S. Mrenna, M. Sandhoff, T. Sjöstrand, D. Wicke.
Deeply Virtual Neutrino Scattering at Leading Twist
Towards Multijet Matching with Loops
Jet fragmentation results at CDF
Outline of the talk: ● Introduction ● QCD models
Y.Kitadono (Hiroshima ),
b-Quark Production at the Tevatron
Presentation transcript:

Time-like Showers and Matching with Antennae 3rd MCNet Meeting / Göstafest, Lund, January 2008 Time-like Showers and Matching with Antennae Peter Skands CERN & Fermilab In collaboration with R. Frederix, W. Giele, D. Kosower, T. Sjöstrand

Time-Like Showers and Matching with Antennae - 2 Parton Showers The final answer depends on: The choice of evolution variable The splitting functions (finite/subleading terms not fixed) The phase space map ( dΦn+1/dΦn ) The renormalization scheme (argument of αs) The infrared cutoff contour (hadronization cutoff) Step 1, Quantify uncertainty: vary all of these (within reasonable limits) Step 2, Systematically improve: Understand the importance of each and how it is canceled by Matching to fixed order matrix elements Higher logarithms, subleading color, etc, are included Step 3, Write a generator: Make the above explicit (while still tractable) in a Markov Chain context  matched parton shower MC algorithm Time-Like Showers and Matching with Antennae - 2

VINCIA Based on Dipole-Antennae So far: VIRTUAL NUMERICAL COLLIDER WITH INTERLEAVED ANTENNAE Gustafson, PLB175(1986)453; Lönnblad (ARIADNE), CPC71(1992)15. Azimov, Dokshitzer, Khoze, Troyan, PLB165B(1985)147 Kosower PRD57(1998)5410; Campbell,Cullen,Glover EPJC9(1999)245 Based on Dipole-Antennae Shower off color-connected pairs of partons Plug-in to PYTHIA 8.1 (C++) So far: Time-like QCD cascades (with massless quarks) 2 different shower evolution variables: pT-ordering (= ARIADNE ~ PYTHIA 8) Dipole-mass-ordering (~ Thrust ≠ PYTHIA 6, SHERPA) For each: an infinite family of antenna functions Laurent series in branching invariants with arbitrary finite terms Shower cutoff contour: independent of evolution variable IR factorization “universal” Several different choices for αs (evolution scale, pT, mother antenna mass, 2-loop, …) Phase space mappings: 2 different choices implemented Antenna-like (ARIADNE angle) or Parton-shower-like: Emitter + longitudinal Recoiler Dipoles (=Antennae, not CS) – a dual description of QCD a Giele, Kosower, PS : hep-ph/0707.3652 + Les Houches 2007 r b Time-Like Showers and Matching with Antennae - 3

Dipole-Antenna Showers Dipole branching and phase space ( Most of this talk, including matching by antenna subtraction, should be applicable to ARIADNE as well) Giele, Kosower, PS : hep-ph/0707.3652 Time-Like Showers and Matching with Antennae - 4

Example: Z decays VINCIA and PYTHIA8 (using identical settings to the max extent possible) αs(pT), pThad = 0.5 GeV αs(mZ) = 0.137 Nf = 2 Note: the default Vincia antenna functions reproduce the Z3 parton matrix element; Pythia8 includes matching to Z3 Frederix, Giele, Kosower, PS : Les Houches Proc., in preparation Time-Like Showers and Matching with Antennae - 5

Time-Like Showers and Matching with Antennae - 6 Example: Z decays Why is the dependence on the evolution variable so small? Conventional wisdom: evolution variable has huge effect Cf. coherent vs non-coherent parton showers, mass-ordered vs pT-ordered, etc. Dipole-Antenna showers resum radiation off pairs of partons  interference between 2 partons included in radiation function If radiation function = dipole formula  intrinsically coherent  angular ordering there by construction Remaining dependence on evolution variable much milder than for conventional showers The main uncertainty in this case lies in the choice of radiation function away from the collinear and soft regions  dipole-antenna showers under the hood … Gustafson, PLB175(1986)453 Time-Like Showers and Matching with Antennae - 6

Dipole-Antenna Functions Giele, Kosower, PS : hep-ph/0707.3652 Starting point: “GGG” antenna functions, e.g., ggggg: Generalize to arbitrary Laurent series:  Can make shower systematically “softer” or “harder” Will see later how this variation is explicitly canceled by matching  quantification of uncertainty  quantification of improvement by matching Gehrmann-De Ridder, Gehrmann, Glover, JHEP 09 (2005) 056 yar = sar / si si = invariant mass of i’th dipole-antenna Singular parts fixed, finite terms arbitrary Time-Like Showers and Matching with Antennae - 7

Quantifying Matching The unknown finite terms are a major source of uncertainty DGLAP has some, GGG have others, ARIADNE has yet others, etc… They are arbitrary (and in general process-dependent) Varying finite terms only with αs(MZ)=0.137, μR=1/4mdipole, pThad = 0.5 GeV Giele, Kosower, PS : hep-ph/0707.3652 Time-Like Showers and Matching with Antennae - 8

Matching A: splitting function Tree-level “real” matching term for X+k wX : |MX|2 S : Evolution operator {p} : momenta Pure Shower (all orders) “X + nothing” “X+something” A: splitting function Matched shower (including simultaneous tree- and 1-loop matching for any number of legs) Tree-level “real” matching term for X+k Loop-level “virtual+unresolved” matching term for X+k Giele, Kosower, PS : hep-ph/0707.3652 Time-Like Showers and Matching with Antennae - 9

Tree-level matching to X+1 Expand parton shower to 1st order (real radiation term) Matrix Element (Tree-level X+1 ; above thad)  Matching Term:  variations in finite terms (or dead regions) in Ai canceled (at this order) (If A too hard, correction can become negative  negative weights) Inverse phase space map ~ clustering Giele, Kosower, PS : hep-ph/0707.3652 Time-Like Showers and Matching with Antennae - 10

Quantifying Matching The unknown finite terms are a major source of uncertainty DGLAP has some, GGG have others, ARIADNE has yet others, etc… They are arbitrary (and in general process-dependent) Varying finite terms only with αs(MZ)=0.137, μR=1/4mdipole, pThad = 0.5 GeV Giele, Kosower, PS : hep-ph/0707.3652 Time-Like Showers and Matching with Antennae - 11

1-loop matching to X NLO “virtual term” from parton shower (= expanded Sudakov: exp=1 - … ) Matrix Elements (unresolved real plus genuine virtual) Matching condition same as before (almost): You can choose anything for Ai (different subtraction schemes) as long as you use the same one for the shower Tree-level matching just corresponds to using zero (This time, too small A  correction negative) Giele, Kosower, PS : hep-ph/0707.3652 Time-Like Showers and Matching with Antennae - 12

Note about “NLO” matching Shower off virtual matching term  unmatched O(α2) contribution to 3-jet observables (only canceled by 1-loop 3-parton matching) While normalization is improved, most shapes are not Tree-Level Matching “NLO” Matching Using αs(MZ)=0.137, μR=1/4mdipole, pThad = 0.5 GeV Time-Like Showers and Matching with Antennae - 13

Time-Like Showers and Matching with Antennae - 14 What happened? Brand new code, so bear in mind possibility of bugs Naïve conclusion: tree-level matching “better” than NLO? No, first remember that the shapes we look at are not “NLO” E.g., 1-T appears at O(α) below 1-T=2/3, and at O(α2) above An “NLO” thrust calculation would have to include at least 1-loop corrections to Z3 So: both calculations are LO/LL from the point of view of 1-T What is the difference then? Tree-level Z3 is the same (LO) The O(α) corrections to Z3, however, are different The first non-trivial corrections to the shape! So there should be a large residual uncertainty  the 1-loop matching is “honest” The real question: why did the tree-level matching not tell us? I haven’t completely understood it yet … but speculate it’s to do with detailed balance In tree-level matching, unitarity  Virtual = - Real  cancellations. Broken at 1 loop + the tree-level curves had different normalizations (covering the shape uncertainty?) Time-Like Showers and Matching with Antennae - 14

Time-Like Showers and Matching with Antennae - 15 What to do next? Further shower studies Interplay between shower ambiguities and hadronization “tuning” Shower+hadronization tuning in the presence of matching Go further with tree-level matching Demonstrate it beyond first order (include H,Z  4 partons) Automated tree-level matching (automated subtractions) Go further with one-loop matching Demonstrate it beyond first order (include 1-loop H,Z  3 partons) Should start to see genuine stabilization of shapes as well as normalizations Extend to the initial state Extend to massive particles Massive antenna functions, phase space, and evolution We’re only a few people working part-time, so plenty of room for collaboration Time-Like Showers and Matching with Antennae - 15

Extra Material Number of partons and number of quarks Frederix, Giele, Kosower, PS : Les Houches Proc., in preparation Number of partons and number of quarks Nq shows interesting dependence on ordering variable Time-Like Showers and Matching with Antennae - 16

Time-Like Showers and Matching with Antennae - 17 Comparison Time-Like Showers and Matching with Antennae - 17

MC4BSM http://theory.fnal.gov/mc4bsm/ Main Focus: Alternative (non-MSSM) TeV scale physics models http://theory.fnal.gov/mc4bsm/ Time-Like Showers and Matching with Antennae - 18