Measure Tracks decay from heavy flavor mesons - PowerPoint PPT Presentation

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Measure Tracks decay from heavy flavor mesons

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Title: Measure Tracks decay from heavy flavor mesons


1
Measure Tracks decay from heavy flavor mesons
2
Primary tracks
From D0 decays
3
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4
  • Why semiconductor?
  • Semiconductor with moderate bandgap (1.12 eV)
  • Thermal energy 1/40 ev
  • Little cooling required
  • Energy to create e/h pair (signal quanta) 3.6
    eV c.f Argon gas 15 eV
  • Scintillator 100-200ev
  • High carrier yield
  • Good energy resolution
  • Fano factor for Si, F 0.1

conduction band
forbidden gap
Valence band
5
  • Disadvantages?
  • Cost of Area covered
  • Detector material could be cheap Standard Si
  • Most cost in readout channels
  • Material budget
  • Radiation length can be significant
  • Tracking due to multiple scattering
  • Radiation damage
  • Replace often or design very well

6
  • P-N Junction
  • One of the crucial keys to solid state
    electronics is the nature of the P-N junction.
    When p-type and n-type materials are placed in
    contact with each other, the junction behaves
    very differently than either type of material
    alone. Specifically, current will flow readily in
    one direction (forward bias), creating the basic
    diode.
  • Near the junction, electrons diffuse across to
    combine with holes, creating a "depletion
    region".

7
Energy Loss in the Medium
8
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11
Different kind of Silicon detectors
  • Charge coupled devices (CCD)
  • Silicon pixel, strip detector ( a few hundreds of
    micros thick)
  • Silicon drift detector
  • CMOS APS detector Complementary
    metaloxidesemiconductor (CMOS) , active pixel
    sensor

12
CMOS APS
Epitaxy is a kind of interface between a thin
film and a substrate. The term epitaxy (Greek
epi "above" and taxis "in ordered manner")
describes an ordered crystalline growth on a
monocrystalline substrate.
Can use the standard Integrate Circuit production
process for the production. Rely on charge
diffusion instead of drifting.
13
  • From Equation 1.4 and 1.6, the depletion width is
    about 2 µm under normal reset condition.
  • the bulk of the p-epi region is free of electric
    field and the minority carriers diffuse rather
    than drift in this region

14
RHIC STAR Experiment
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17
Input for the simulator
  • For the charged particles The number of ionized
    electrons/hole pairs.
  • Energy deposition in the detector volume.
  • StMcTrack-gtdE().
  • H. Matis for thin layer of material better use
    the Bichsel distribution,
  • H. Bichsel, "Straggling in Thin Silicon
    Detectors," Review in Modern Physics, vol. 60,
    pp. 663, 1988
  • GEANT has implement other models for the thin
    layers energy fluctuations under different
    limitation of applications
  • Urban model
  • 1 PAI model
  • 2 ASHO model for 1
  • Will use the Bichsel distribution as input since
    its tested with the experiment.
  • For neutral particles including photons, the
    energy deposition in StMcTrack will be used to
    generate the number of ionizing electron/hole
    pairs unless we have other models for these
    particles.

18
  • For charged track,
  • the ionized electron/hole pairs originate
    randomly alone the track.
  • Number of ionized electrons is E/3.6eV where E is
    the energy deposition from the Bichsel
    distribution.
  • For photons and neutral particles
  • No good reference to my knowledge.
  • Si detector should have very low efficiency for
    high energy gamma-ray due to pair production.
  • Two possible ways to deal with it
  • Will use the GEANT to get energy deposition from
    the gamma-ray or neutral particles and assume all
    ionized electrons are from the point where gamma
    and silicon interact. (not quite reasonable)
  • Use Bischsel distribution if we the pair
    production vertex for high energy photons and the
    electron pair tracks (I think we should know).
  • For low energy gamma-rays, use the energy
    deposition from GEANT.

19
Boundary conditions questions fo hardware
experts.
  • whats the gap between pWell and nWell?
  • Are they fully depleted?
  • If the gap is zero, what are the depletion
    thickness?
  • Whats the thickness of p-epi layer? (14
    microns?)
  • Whats the substrate thichness, i.e. 50um-p_epi?
  • Whats the size of the p-well and n-well?
  • Whats the shape? Is the cubic shape reasonable
    approximation?

N Well
p Well
p Well
p-epi layer
p substrate
20
  • when the p substrate electron hit p-epi/p
    substrate interface, the interface is totally
    transparent.
  • When the electron fall into the depletion region
    between N-Well and P-Well or the N_well region,
    it will be fully collected into the readout
    electronics.
  • Electrons in the p-well region will be neglected.

p Well
  • When electrons hit the n-well/p-epi depletion
    region, has very little chance to be reflected
    but pass through. Consequently, the n-well/p-epi
    interface can be recognized as a boundary with
    total absorption
  • When electron hits the p-epi and p-well
    interface, the p-well/p-epi interface can be
    recognized as a boundary with total reflection
    for electrons in the epitaxial silicon because
    pWell are more heavily doped and field in the
    depletion region will reflect the electron away.
  • when the p-epi electron hit p-epi/p substrate,
    because p is more heavy doped, interface is
    recognized as a
  • boundary with total reflection for electrons in
    the epitaxial silicon

21
Question on interface between pixels.
Will the boundary be total transparent to the
electrons going across the pixel boundaries?
22
  • electron will recombine with the lattice during
    the diffusion and can not reach the electronics.
  • We used 10 µs as the electron lifetime in the
    epitaxial silicon after going over a number of
    references 37, 43, 45, 46 . Plugging it into
    Equation 2.48, we obtain a recombination rate on
    the order of 10-7. As the precise lifetime
    depends on material properties that is only
    available through experimental measurement, these
    estimated values serves only as the starting
    point for simulation and they need to be refined
    by comparing the simulation with the measurements
    (see page 40 of the Shengdongs thesis).
  • in the p-substrate region and p-well region,
    much higher doping density than p-epi and the
    quality is also lower, the electron lifetime in
    p-substrate is much shorter. Similar to the
    method in dealing with the epitaxial silicon, a
    lifetime of 10 ns is estimated for electrons in
    the bulk substrate and the corresponding
    recombination rate is on the order of 10-4.
    (see page 41 of shengdongs thesis).

p Well
23
Other simulation details
  • Diffusion simulation see page 17-page21 of
    Shendongs thesis.
  • The time increment ?t used is on the order of
    10-12 s, similar to those reported in references
    22, 28, 42, 47, quite close to the average
    collision time in Drude model48. Using an
    electron diffusion coefficient (Dn) 35 cm2/s,
    the step size s from Equation 2.47 is about 80
    nm, once again close to the mean-free-path of
    electrons in silicon estimated by Drude model
    (page42)
  • The charge recombination simulation in page 46
  • Total integration time is 200us.
  • This is the end of diffusion?
  • If therere still electron diffusion after this
    time
  • We will keep it and add it to the simulation for
    the next track hit the same pixel. This might
    have an impact for pileup
  • But according to Shengdongs thesis, this effect
    is very small.
  • A computationally convenient depth is usually
    selected as a total absorption boundary where
    electrons crossing it will not be counted anymore
    due to recombination. This topic will be treated
    systematically in Chapter 4 and Chapter 5.
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