1 The Microscopic Universe and the Energy Frontier Don Lincoln Fermilab f University of Manitoba November 18, 2005.

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Presentation transcript:

1 The Microscopic Universe and the Energy Frontier Don Lincoln Fermilab f University of Manitoba November 18, 2005

2 Innermost Space High Energy Particle Physics is a study of the smallest pieces of matter. It investigates the deepest and most fundamental aspects of nature. It investigates (among other things) the nature of the universe immediately after the Big Bang. It also explores physics at temperatures not common for the past 14 billion years (or so).

3 4x seconds Now (13.7 billion years) Stars form (1 billion years) Atoms form (380,000 years) Nuclei form (180 seconds) ??? (Before that) Nucleons form ( seconds) Quarks differentiate ( seconds?)

4 The Universe at s  The Standard Model Frontier

5 (Too?) Simple: “Bits of matter stick together by exchanging stuff.” The Standard Model includes: –6 quarks (those little fellows in the nucleus) and their antiparticles. –6 leptons (e.g. an electron) and their antiparticles –4 “force carrier” particles Precisely: “All known matter is composed of composites of quarks and leptons which interact by exchanging force carriers.” In a few words…

6 Periodic Table of Fundamental Particles -1 +2/3 - 1/3 0 Mass  All point-like (down to m) spin-1/2 Fermions Families “generations” reflect increasing mass and a theoretical organization u, d,, e are “normal matter” These all interact by exchanging spin 1 bosons

7

8 Compelling Questions That Can Be Addressed by Particle Physics (there are many others) How do particles get mass? Are there higher symmetries manifesting, themselves as new particles and forces? Are there hidden dimensions (perhaps explaining the weakness of gravity)?

9 Mass: The Higgs Particle Electroweak unification postulates the existence of the Higgs field. The field interacts with all other particles to impart mass - think of walking through molasses. The field is a microscopic property of space-time, at least one real particle will result. The collider programs at Fermilab, Large Hadron Collider, and the International Linear Collider are dedicated, in part, to the search for and study of this particle.

10 Beyond That? Even with the Higgs, the Standard Model requires fine tuning of parameters to avoid infinite Higgs masses from quantum corrections – the theory is “ugly.” This and other theoretical thoughts lead to strong belief that the SM is merely a low energy or effective theory valid up to some scale. At this higher energy scale additional physics may (will?) appear. Supersymmetry or SUSY is one of the most popular theoretical options.

11 SUSY In SUSY every particle and force carrier has a massive partner: squarks, selectrons, gluinos… Since they are massive they’ve not been produced in current machines. The discovery requires more energetic accelerators – something which is being enthusiastically pursued.

12 Or…Extra Dimensions!? Amazingly enough, a higher dimensional world (time, 3-D, plus “n” additional dimensions) can accommodate a theory with all four forces. Only gravity can communicate with/to other dimensions, it’s “strength” is diluted in ours. That is, the graviton, or gravity carrier can spread it’s influence among all the spatial dimensions. Experiments are underway searching for signals of these dimensions. The “other” dimensions “Our World” q graviton q

13 How do we test these theories?

14 The Two Basic Ideas: –Find a source of particles with high kinetic energy. –Study the debris resulting from collisions inside detectors. The Sources: –Cosmic Rays –Accelerators –The higher the energy the more numerous the number and types of particles. The Detectors: –A series of special purpose devices that track and identify collision products p pp

15 Fermilab Proton-Antiproton Collider Main Injector & Recycler Tevatron Booster pp p DØ  p source Batavia, Illinois Chicago 1 Hydrogen Bottle 2 Linear Accelerator 3 Booster 4 Main/Injector 5 Antiproton Source 6 2 TeV

16 A Schematic Detector Hadronic layers Tracking system Magnetized volume Calorimeter Induces shower in dense material Innermost tracking layers use silicon Muon detector Interaction point Absorber material Bend angle  momentum Electron Experimental signature of a quark or gluon Muon Jet: q or g “Missing transverse energy” Signature of a non-interacting (or weakly interacting) particle like a neutrino EM layers fine sampling p pp

17 Calorimeters Tracker Muon System Electronics antiprotons 20 m A Real Experiment: DZero Proposed 1982 First Run: TeV Upgrade: Run II: TeV Star Trek: First Contact

18 International 570+ physicists 93 institutions 19 countries Canada: University of Alberta, Simon Fraser University, York University, McGill University

19 Silicon Microstrip Treacker 1M channels, 4 barrel layers axial + stereo strips H, F Disks/wedges 8 axial layers 8 stereo layers Central Fiber Tracker 80k Channels Calorimeter, 50k Channels Liquid argon calorimeter with uranium absorber scintillator shielding

20 Inner Tracking Electron Quark or Gluon Jet Muon

21 Run II: 24/7 Event Collection Proton-antiprotons collide at 7 MHz or seven million times per second Tiered electronics pick successively more interesting events –Level 1 2 kHz –Level 2 1 kHz About 100 crates of electronics readout the detectors and send data to a Level 3 farm of 100+ CPUs that reconstruct the data Level 3: 50 events or 12.5 Mbytes of data to tape per second Per year: 500 million events

22 Physics: Event Analysis Events are “reconstructed” offline by farms of ~100 CPUs. Each detector samples position, energy, or momentum, 1M+ channels Then computers build or reconstruct full event characteristics based upon these samples Interesting events or signals are culled from the background usually 100’s out of millions.

23 Fermilab DØ Experiment Worldwide Data Grid Autumn 2003 Simulation files SAM data transfer Reconstructed data Prague Lancaster Remote Simulation sites Tata Institute Wuppertal Michigan Kansas Michigan St. Boston Munich Indiana Imperial Stations for remote data analysis + more coming Oklahoma Arizona UK Remote Data Reconstruction sites NIKHEF Karlsruhe GridKA Lyon CCIN2P3 Westgrid Canada Texas

24 A Sample Event: Z  e + e - p p Z q q’ l l

25 Sample Distribution: Z mass Collect events and calculate mass for each event, then plot distributions Extract or measure properties such as mass or production rate as a function of beam brightness or luminosity. For example 1 pb -1 of luminosity means 1 event will be produced for a process of 1 pb cross section.

26 Now back to our three scheduled questions!

27 Past Higgs Searches and Current Limits Over the last decade or so, experiments at LEP or the European e + e – collider have been searching for the Higgs. Direct searches for Higgs production, similar to our Z mass measurement exclude m H < 114 GeV. Precision measurements of electroweak parameters combined with DZero’s new* Run I top quark mass measurement, favor m H = 117 GeV with an upper limit of m H = 251 GeV. * Nature 10 June 2004

28 Higgs Boson Production Problems 1.Background is indistinguishable from signal 2.Background is more than 1000 times more prevalent than signal gluon b b Higgs Signal gluon b b Background

29 Associated Production q Higgs W q W*W* qq  W *  WH q Higgs Z q Z*Z* qq  Z *  ZH The so-called Associated Production is the production of a Higgs boson in association with an electroweak boson (W/Z). Consequences 1. There is essentially no background 2. This process is 10× less likely than “bare” Higgs production

30 Current Tevatron Searches For any given Higgs mass, the production cross section, decays are calculable within the Standard Model There are a number of ongoing searches in a number of production and decay channels In the 120 GeV region a good bet would be to look for Higgs and associated W or Z production –Cross section ~ pb –e or  decays of W/Z help distinguish the signal p p W* q q’q’ H W

31 Search for HW production One very striking and distinctive signature Look for –an electron = track + EM calorimeter energy –neutrino = missing transverse energy –two b quarks = two jets each with a secondary vertex from the long lived quarks. p p W* q q’q’ H W e b b

32 Results Two events found, consistent with Standard Model Wbb production 12.5 pb upper cross section limit for pp  WH where H  bb m H =115 GeV. By the end of Run II an combining all channels, we should have sensitivity to ~130 GeV. electron neutrino b jet electron neutrino (MET) b jet

33 The other candidate…. b jet electron neutrino (MET) electron b jet

34 Well actually… One Higgs has been unambiguously observed. and recently Hollywood gave some practical pointers …but we will keep looking! His name is Peter and he lives in Scotland

35 Supersymmetry Reminder: Postulates a symmetry between bosons and fermions such that all the presently observed particles have new, more massive super-partners. Theoretically attractive: –Additional particles cancel divergences in m H –SUSY closely approximates the standard model at low energies –Allows unification of forces at much higher energies –Provides a path to the incorporation of gravity and string theory: Local Supersymmetry = Supergravity –Lightest stable particle cosmic dark matter candidate Masses depend on unknown parameters, but expected to be 100 GeV - 1 TeV Put to good use in Season 4

36 SUSY Consequence SUSY quark “squark” SUSY lepton “slepton” SUSY boson “bosino”

37 The Golden Tri-lepton Supersymmetry Signature In one popular model the charged and neutral partners of the gauge and Higgs bosons, the charginos and neutralinos, are produced in pairs Decay into fermions and the Lightest Supersymmetric Particle (LSP), a candidate for dark matter. The signature is particularly striking: –Three leptons = track + EM calorimeter energy or tracks + muon tracks (could be eee, ee , e , , ee , etc… ). –neutrino = missing transverse energy

38 Trilepton Search Results In four tri-lepton channels three events total found. Consistent with Standard Model expectation of 2.9 events. Here is a like-sign muon candidate muons electron neutrino

39 Interesting events do turn up…but we are now severely constraining the allowed SUSY parameter space.

40 The Search for Extra Dimensions The strengths of the electromagnetic, strong, and weak forces change with energy, suggesting grand unification of these forces. It is believed that gravity becomes as strong as the other forces and unifies with them at the energy known as the Planck scale. Difficult to find a natural way to make gravity much weaker than other forces at lower energy scales It has been suggested that there are extra, compact, spatial dimensions, in which only gravity can propagate, and which are therefore hidden from our everyday experience. Gravity would therefore be as strong as other forces, but appears diluted and weak from our four space- time dimensional viewpoint in which we are “confined”…but once again… The Adventures Of Buckeroo Banzai Across The Eighth Dimension

41 A Model with “n” Dimensions. Gravity communicating with these extra dimensions could produce an unexpectedly large number of electron or photon pairs. Thus, analysis of the production rate of electrons and photon provides sensitivity to these extra dimensions. Large energies are required to produce such pairs. p p G q q’q’ e e

42 Di-electrogmagnetic objects are collected and the mass calculated (just as in our Z plot a few minutes ago). The observed mass spectrum is compared to a linear combination of –SM signals –Instrumental backgrounds –Extra Dimension Signals No evidence is found for hidden 95%CL –n = 2, 170  m –n = 3, 1.5 nm –n = 4, 5.7 pm –n = 5, 0.2 pm –n = 6, 21 fm –n = 7, 4.2 fm Note the long mass tail

43 Or a Single TeV -1 size Extra Dimension Another idea introduces a single dimension of the size of ~ m (or ~1 TeV -1 in “natural” units), where the carriers of the electroweak and strong force (photons, W and Z particles, and gluons) can propagate. We also see no evidence for a single extra dimension of ~1 TeV  1 size At 95% CL size limit 1.75x m Note the long mass tail

44 Once again there are interesting events! (way out on the mass tail.) ee pair  pair photons electrons

45 The Future: A Huge Data Set to Explore These analyses ~200 pb -1, have already logged 1050 pb -1 Expect to see 8000 pb -1 this run. These hints should become even more interesting …

46 Prospects The Tevatron is stretching the boundaries of the observed universe: –Constrain the SM and place limits on the Higgs mass or –Better yet: observe/discover the Higgs –Discover new physics … SUSY –Communicate with extra dimensions…. A thoroughly exciting challenge to answer the most basic questions… –What is the history of the universe? –What is the composition of the universe? –What is the structure of the universe? Toy Story “To the Microscopic Universe…. and Beyond!”