ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 1 ISMD 2010 Rick Field University of Florida The Quest to Find New Physics Outline.

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Presentation transcript:

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 1 ISMD 2010 Rick Field University of Florida The Quest to Find New Physics Outline of Talk  “New physics” in  “New physics” in high multiplicity “min-bias” events at the LHC!  We hope much more “new physics” is soon to come from the LHC.  Why expect “new physics”?  What “new physics”?  When “new physics”?  How to find “new physics”?

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 2 International Symposium on Multiparticle Dynamics Rick Field (theorist?) “Jet Formation in QCD” 22 Years! Rick Field (experimenter?) “Min Bias and the Underlying Events in Run 2 at CDF”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 3 International Symposium on Multiparticle Dynamics Rick Field (theorist?) “Jet Formation in QCD” 28 Years! Rick Field (phenomenologist?) “The Quest to Find New Physics”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 4 “New Physics” 1977  What happens when two hadrons collide at high energy?  Most of the time the hadrons ooze through each other and fall apart (i.e. no hard scattering). The outgoing particles continue in roughly the same direction as initial proton and antiproton.  Occasionally there will be a large transverse momentum meson. Question: Where did it come from?  We assumed it came from quark-quark elastic scattering, but we did not know how to calculate it! FF “Black-Box Model”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 5 “New Physics” 1977  What happens when two hadrons collide at high energy?  Most of the time the hadrons ooze through each other and fall apart (i.e. no hard scattering). The outgoing particles continue in roughly the same direction as initial proton and antiproton.  Occasionally there will be a large transverse momentum meson. Question: Where did it come from?  We assumed it came from quark-quark elastic scattering, but we did not know how to calculate it! FF “Black-Box Model” Feynman quote from FF1 “The model we shall choose is not a popular one, so that we will not duplicate too much of the work of others who are similarly analyzing various models (e.g. constituent interchange model, multiperipheral models, etc.). We shall assume that the high P T particles arise from direct hard collisions between constituent quarks in the incoming particles, which fragment or cascade down into several hadrons.”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 6 Quark-Quark Black-Box Model FF Quark Distribution Functions determined from deep-inelastic lepton-hadron collisions Quark Fragmentation Functions determined from e + e - annihilations Quark-Quark Cross-Section Unknown! Deteremined from hadron-hadron collisions. No gluons!

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 7 Quark-Quark Black-Box Model FF Predict overall event topology (FFF1 paper 1977) “Beam-Beam Remnants” Predict increase with increasing CM energy W

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 8 QCD Approach: Quarks & Gluons FFF Parton Distribution Functions Q 2 dependence predicted from QCD Quark & Gluon Fragmentation Functions Q 2 dependence predicted from QCD Quark & Gluon Cross-Sections Calculated from QCD

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 9 QCD Approach: Quarks & Gluons FFF Parton Distribution Functions Q 2 dependence predicted from QCD Quark & Gluon Fragmentation Functions Q 2 dependence predicted from QCD Quark & Gluon Cross-Sections Calculated from QCD Feynman quote from FFF2 “We investigate whether the present experimental behavior of mesons with large transverse momentum in hadron-hadron collisions is consistent with the theory of quantum-chromodynamics (QCD) with asymptotic freedom, at least as the theory is now partially understood.”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 10 Feynman Talk at Coral Gables (December 1976) “Feynman-Field Jet Model” 1 st transparency Last transparency

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 11 New Physics in “Min-Bias”? … “Semi-hard” parton- parton collision (p T < ≈2 GeV/c) Multiple-parton interactions (MPI)! The Inelastic Cross Section  CMS Two-Particle Correlations at 7 TeV.

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 12 Two Particle Angular Correlations  Signal, S, is two particles in the same event. Background, B, is two particles in two different events.  Correlation, R, is ~(S-B)/B. See the very nice talk by Xavier Janssen at this meeting for more details!

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 13 Two Particle Angular Correlations Bose-Einstein CMS “min-bias” 7 TeV

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 14 Two Particle Angular Correlations CMS “min-bias” 7 TeV

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 15 Two Particle Angular Correlations CMS “min-bias” 7 TeV

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 16 High Multiplicity at 7 TeV

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 17 CMS High Multiplicity Trigger  A dedicated high multiplicity trigger was implemented in the two levels of the CMS trigger system. Level 1 (L1): Sum of the total ET (ECAL, HCAL, and HF) > 60 GeV.  High-level trigger (HLT): number of online tracks built from the three layers of pixel detectors >70 (85). Statistics for high multiplicity enhanced by ~1,000!

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 18 Two Particle Angular Correlations  Lots of jets at high multiplicity! Average “Min-Bias” High Multiplicity “Min-Bias”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 19 Two Particle Angular Correlations Average “Min-Bias” High Multiplicity “Min-Bias”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 20 Two Particle Angular Correlations  Long range (in  ) same side correlations! What is this? Average “Min-Bias” High Multiplicity “Min-Bias”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 21 Long-Range Same-Side Correlations Not there in PYTHIA8! High Multiplicity “Min-Bias” Also not there in PYTHIA 6 and HERWIG++!

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 22 Correlation in Heavy Ion Collisions  Long range correlations expected in “collective flow” in heavy ion collisions.

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 23 Correlation in Heavy Ion Collisions  Long-range “Ridge”-like structure in  at  ≈ 0!

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 24 Proton-Proton vs Au-Au  I am not ready to jump on the quark-gluon plasma bandwagon quite yet! Proton-Proton Collisions 7 TeV Gold-Gold Collisions 200 GeV QGP

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 25 Jet-Jet Correlations  Are the “leading-log” or “modified leading-log” QCD Monte-Carlo Models missing an important QCD correlation?  The leading jet and the incident protons form a plane (yz-plane in the figure). This is the plane of the hard scattering.  Initial & final-state radiation prefers to lie in this plane. This is a higher order effect that you can see in the 2→3 or 2→4 matrix elements, but it is not there if you do 2→2 matrix elements and then add radiation using a naïve leading log approximation (i.e. independent emission).  I do not know to what extent this higher order jet-jet correlation is incorporated in the QCD Monte-Carlo models.  I would think that this jet-jet correlation would produce a long range (in  ) correlation with  ≈ 0 from two particles with one in the leading jet and one in the radiated jet. Why don’t we see this in the Monte-Carlo models?

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 26 Jet-Jet Correlations  Initial & Final-State Radiation: There should be more particles “in-the-plane” of the hard scattering (yz-plane in the figure) than “out-of –the-plane”.  I do not understand why this does not result in a long-range same-side correlation? ??

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 27 Why Expect “New Physics”?  Dark Matter: If gravity is described by Einstein’s equations, the Universe we observe cannot be explained without sizeable “dark components”. No Dark Matter candidate in Standard Model ! “New Physics” Neutralinos, Gravitinos, Axinos, Scalar Neutrinos, KK Photons, KK Neutrinos, 4th Gen. Neutrinos, Mirror Photons, Mirror Nuclei, Stable States from Technicolor, Sterile Neutrinos, Light scalars, Q-balls, D-matter, Braneworld Matter, Primordial Black Holes, Axions, …  Unitarity: Fermi contact interaction is tamed at high energies through an intermediate Massive Vector Boson (W). However, massive vectors develop a longitudinal component and unitarity is lost at high energies! H Violates Unitarity ! Restored via Goldstone Bosons! “New Physics”

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 28 What “New Physics”?  Supersymmetry:  Extra Dimensions: *Hidden Sectors (Y. Xie ICHEP talk) *Exotic particles of Various Spin and Gauge permutations (Berger ICHEP talk) *Quirks (Y. Xie ICHEP talk) *Supermodels At Early LHC (Ligeti ICHEP talk) *Exotic Higgs Decays (Several ICHEP talks) *Many Others LHC Street Lamp From James Wells (ICHEP 2010)

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 29 When “New Physics”?  Expect more new LHC physics in 2011 (if Steve Myers’ integrated luminosity projections are correct)! Steve Myers ICHEP 2010 Preliminary Projected LHC Total Int (fb -1 )  Also might see new physics at the Tevatron (e.g. A FB (top))!  I think the Tevatron and LHC programs complement each other nicely and I would like to see the Tevatron continue to run over the next several years! CDF has a high multiplicity min-bias trigger. They should look for long-range same-side correlations! If it is a QCD effect, it should be there at 1.96 TeV.

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 30 How to Find “New Physics”? Calculate the Standard Model and QCD as accurately as possible and look for deviations from these predictions in the data! CMS Difficult to produce enough events with large “transverse” multiplicity at a low hard scale!

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 31 Letter from Feynman July 1976

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 32 Letter from Feynman Page 1 Spelling?

ISMD 2010 Antwerp September 25, 2010 Rick Field – Florida/CDF/CMSPage 33 Letter from Feynman Page 3 It is fun! Onward!