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Fermilab

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Despite the successes of general relativity, we still do not understand gravity ... dynamical mass much greater than visible luminous material ... – PowerPoint PPT presentation

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Title: Fermilab


1
Introduction
  • John Womersley
  • Fermilab
  • DØ Run 2B Silicon Workshop
  • January 2001

2
Mass shapes the Universe
  • through gravitation, the only force that is
    important over astronomical distances
  • Despite the successes of general relativity, we
    still do not understand gravity in a quantum
    framework
  • but we believe we are getting closer to
    understanding the origin of mass

3
Mass in the cosmos
  • Masses of Atoms
  • rest masses of the fermions
  • binding energies
  • Dark Matter
  • dynamical mass much greater than visible luminous
    material
  • primordial nucleosynthesis, D/He abundance ? all
    this mass cannot be baryonic
  • new particles?

4
Mass of Hadrons
  • Mass of a proton 938 MeVMass of two u quarks
    plus a d quark 10 ? 5 MeV
  • 99 of the mass of a proton (and therefore of the
    mass of a hydrogen atom) is due to the binding
    energy
  • Quantum Chromodynamics (QCD)
  • the strong force that acts on quarks
  • a gauge theory (like electromagnetism)
  • unlike electromagnetism, the vector bosons of the
    theory (gluons) themselves carry the charge
    (color)
  • gluons are self-interacting
  • coupling constant runs rapidly force becomes
    strong for small momentum transfers
  • confinement

Compilation of experiments
5
Understanding QCD
  • Precisely testable QCD calculations are available
    for high momentum transfer processes at particle
    accelerators
  • e.g. DØ measurements of production of jets in?pp
    collisions
  • Soft QCD is calculable only numerically lattice
    gauge theory
  • initially somewhat disappointing
  • recent advances in computing, and in the
    techniques used, lead to reasonably credible
    results
  • predicted and measured hadron masses

6
Does this mean we understand mass?
  • There is not much doubt that QCD is the theory of
    the strong interaction, and we are making
    progress in understanding how to calculate
    reliably in this framework
  • and recall that 99 of the mass of the (visible)
    universe is QCD
  • But
  • we still need to understand fermion masses
  • second and third generations of quarks and
    leptons are much more massive
  • the masses exhibit patterns
  • we still need to understand vector boson masses
  • mass of the W and Z bosons is what makes the weak
    force weak

7
Fundamental particles and forces
masses
  • leptons q 1 e ? ? q 0 ?e ??
    ??
  • quarks q 2/3 u c t q 1/3 d s b
  • Forces
  • QCD
  • Electroweak force
  • interaction between quarks and leptons, mediated
    by photons (electromagnetism) and W and Z bosons
    (weak force)
  • same couplings to matter(except angles)
  • very different masses

mass 80.4 GeV
W
photon mass 0
8
What does mass mean?
  • For an elementary pointlike particle
  • propagates through the vacuum at v lt c
  • Lorentz transform mixes LH and RH helicity
    statessymmetry is broken
  • mass is equivalent to an interaction with the
    (Quantum Mechanical) vacuum
  • coupling strength mass
  • For a spin-1 state like a photon, there is an
    extra effect
  • massless ? two polarization states
  • massive ? three polarization states
  • where does this additional degree of freedom come
    from?

9
The Higgs Mechanism
  • Hence, in the Standard Model (Glashow, Weinberg,
    Salam, t Hooft, Veltmann)
  • electroweak symmetry breaking through
    introduction of a scalar field ? ? masses of W
    and Z
  • Higgs field permeates space with a finite vacuum
    expectation value
  • cosmological implications! (inflation)
  • If ? also couples to fermions ? generates fermion
    masses
  • An appealing picture is it correct?
  • One clear and testable prediction there exists a
    neutral scalar particle which is an excitation of
    the Higgs field
  • All its properties (production and decay rates,
    couplings) are fixed except its own mass
  • Highest priority of worldwide high energy physics
    program find it!

10
mH probability density, J. Ellis
(hep-ph/0011086)
15 fb-1
110-190 GeV
  • Physics ? Integrated Luminosity
  • Radiation dose
  • Instantaneous Luminosity Tracking
    confusion
  • Detector Upgrade

Schedule ?
11
Run 2B silicon strategy
  • At the start of this process, a minimal solution
    seemed attractive (to me at least)
  • labs guidance was clear (2.5M cost, etc.)
  • one might think that smaller quicker, easier
  • But we now have a better understanding
  • review committee report
  • there are too few SVX2e chips
  • there are likely to be problems with pattern
    recognition
  • difficult to insert a L00 inside the existing
    SMT
  • Hence we will define a more ambitious solution as
    our baseline plan

12
This meeting
  • Move towards this baseline design
  • my summary of the objective
  • a design whose cost can be estimated
  • a design whose performance can be simulated
  • permit us to order prototype sensors
  • Components
  • SVX4 chip (December 2000 decision)
  • a limited number of species of detectors
  • all detectors single sided
  • a layer 0 closer to the beam and a new beam pipe
  • improves impact parameter resolution despite
    increased material
  • more layers
  • resolve pattern recognition issues
  • but reduced coverage in rapidity and no F-disks

13
How to pay for this?
  • We are submitting a MRI proposal to NSF for 2M
  • the physics is sexy and easy to motivate
  • if funded, would enable us to build roughly the
    scale of detector we want with Fermilabs
    contribution remaining of order 2.5M
  • Our previous MRI record is successful, but no
    guarantees. . .
  • review technical and funding progress summer
    2001, may have to fall back at that time
  • Lets assume success and plan for it!

14
One note of caution
  • Installation and commissioning of the Run 2a
    detector is at a critical point
  • we must balance our enthusiasm for Run 2b with
    the need to ensure the success of the current run
  • It is appropriate for a few people in D0 to work
    at the ? 50 level on Run2b but for most of the
    rest of us it should remain a side activity.
    Please do not let your Run 2a responsibilities
    suffer.
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