Analysis Techniques in High Energy Physics

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Analysis Techniques in High Energy Physics

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Title: Analysis Techniques in High Energy Physics


1
Analysis Techniquesin High Energy Physics
  • Claude A Pruneau
  • Wayne State Univeristy

2
Overview
  • Some Observables of Interest
  • Elementary Observables
  • More Complex Observables
  • Typical Analysis of (Star) data

3
Some Observables of Interest
  • Total Interaction/Reaction Cross Section
  • Differential Cross Section I.e. cross section vs
    particle momentum, or production angle, etc.
  • Particle life time or width
  • Branching Ratio
  • Particle Production Fluctuation (HI)

4
Cross Section
  • Total Cross Section of an object determines how
    big it is and how likely it is to collide with
    projectile thrown towards it randomly.

Small cross section
Large cross section
5
Scattering Cross Section
  • Differential Cross Section

dW - solid angle
Flux
q scattering angle
Target
Unit Area
  • Average number of scattered into dW
  • Total Cross Section

6
Particle life time or width
  • Most particles studied in particle physics or
    high energy nuclear physics are unstable and
    decay within a finite lifetime.
  • Some useful exceptions include the electron, and
    the proton. However these are typically studied
    for their own sake but to address some other
    observable
  • Particles decay randomly (stochastically) in
    time. The time of their decay cannot be
    predicted. Only the the probability of the decay
    can be determined.
  • The probability of decay (in a certain time
    interval) depends on the life-time of the
    particle. In traditional nuclear physics, the
    concept of half-life is commonly used.
  • In particle physics and high energy nuclear
    physics, the concept of mean life time or simple
    life time is usually used. The two are connected
    by a simple multiplicative constant.

7
Half-Life
8
Half-Life and Mean-Life
  • The number of particle (nuclei) left after a
    certain time t can be expressed as follows
  • where t is the mean life time of the particle
  • t can be related to the half-life t1/2 via
    the simple relation

9
Examples - particles
Mass (MeV/c2) t or G c t Type
Proton (p) 938.2723 gt1.6x1025 y Very long Baryon
Neutron (n) 939.5656 887.0 s 2.659x108 km Baryon
N(1440) 1440 350 MeV Very short! Baryon resonance
D(1232) 1232 120 MeV Very short!! Baryon resonance
L 1115.68 2.632x10-10 s 7.89 cm Strange Baryon resonance
Pion (p-) 139.56995 2.603x10-8 s 7.804 m Meson
Rho - r(770) 769.9 151.2 MeV Very short Meson
Kaon (K-) 493.677 1.2371 x 10-8 s 3.709 m Strange meson
D- 1869.4 1.057x10-12 s 317 mm Charmed meson
10
Examples - Nuclei
11
Particle Widths
  • By virtue of the fact that a particle decays, its
    mass or energy (Emc2), cannot be determined with
    infinite precision, it has a certain width noted
    G.
  • The width of an unstable particle is related to
    its life time by the simple relation
  • h is the Planck constant.

12
Decay Widths and Branching Fractions
  • In general, particles can decay in many ways
    (modes).
  • Each of the decay modes have a certain relative
    probability, called branching fraction or
    branching ratio.
  • Example (K0s) Neutral Kaon (Short)
  • Mean life time (0.89260.0012)x10-10 s
  • ct 2.676 cm
  • Decay modes and fractions

mode Gi/ G
p p- (68.61 0.28)
p0 p0 (31.39 0.28)
p p- g (1.78 0.05) x10-3
13
Elementary Observables
  • Momentum
  • Energy
  • Time-of-Flight
  • Energy Loss
  • Particle Identification
  • Invariant Mass Reconstruction

14
Momentum Measurements
  • Definition
  • Newtonian Mechanics
  • Special Relativity
  • But how does one measure p?

15
Momentum Measurements Technique
  • Use a spectrometer with a constant magnetic field
    B.
  • Charged particles passing through this field with
    a velocity v are deflected by the Lorentz
    force.
  • Because the Lorentz force is perpendicular to
    both the B field and the velocity, it acts as
    centripetal force Fc.
  • One finds

16
Momentum Measurements Technique
  • Knowledge of B and R needed to get p
  • B is determined by the construction/operation of
    the spectrometer.
  • R must be measured for each particle.
  • To measure R, STAR and CLEO both use a similar
    technique.
  • Find the trajectory of the charged particle
    through detectors sensitive to particle energy
    loss and capable of measuring the location of the
    energy deposition.

17
Star Time-Projection-Chamber (TPC)
  • Large Cylindrical Vessel filled with P10 gas
    (10 methane, 90 Ar)
  • Imbedded in a large solenoidal magnet
  • Longitudinal Electrical Field used to supply
    drive force needed to collect charge produced
    ionization of p10 gas by the passage of charged
    particles.

18
STAR TPC
19
Pad readout
  • 212 super-sectors

190 cm
Outer sector 6.2 19.5 mm2 pad 3940 pads
Inner sector 2.85 11.5 mm2 pad 1750 pads
127 cm
60 cm
20
Pixel Pad Readout
Readout arranged like the face of a clock - 5,690
pixels per sector
JT 20 The Berkeley Lab
21
Momentum Measurement
B0.5 T
p
Radius R
Trajectory is a helix in 3D a circle in the
transverse plane
Collision Vertex
22
Au on Au Event at CM Energy 130 A GeV
Data taken June 25, 2000. The first 12 events
were captured on tape!
Real-time track reconstruction Pictures from
Level 3 online display. ( lt 70 ms )
JT 22 The Berkeley Lab
23
Time-of-Flight (TOF) Measurements
  • Typically use scintillation detectors to provide
    a start and stop time over a fixed distance.
  • Electric Signal Produced by scintillation
    detector
  • Use electronic Discriminator
  • Use time-to-digital-converters (TDC) to measure
    the time difference stop start.
  • Given the known distance, and the measured time,
    one gets the velocity of the particle

Time
S (volts)
24
Energy Measurement
  • Definition
  • Newtonian
  • Special Relativity

25
Energy Measurement
  • Determination of energy by calorimetry
  • Particle energy measured via a sample of its
    energy loss as it passes through layers of
    radiator (e.g. lead) and sampling materials
    (scintillators)

26
More Complex Observables
  • Particle Identification
  • Invariant Mass Reconstruction
  • Identification of decay vertices

27
Particle Identification
  • Particle Identification or PID amounts to the
    determination of the mass of particles.
  • The purpose is not to measure unknown mass of
    particles but to measure the mass of unidentified
    particles to determine their species e.g.
    electron, pion, kaon, proton, etc.
  • In general, this is accomplished by using to
    complementary measurements e.g. time-of-flight
    and momentum, energy-loss and momentum, etc

28
PID by TOF
  • Since
  • The mass can be determined
  • In practice, this often amounts to a study of the
    TOF vs momentum.

29
PID with a TPC
  • The energy loss of charged particles passing
    through a gas is a known function of their
    momentum. (Bethe-Bloch Formula)

30
Particle Identification by dE/dx
Anti - 3He
dE/dx PID range 0.7 GeV/c for K/?
1.0 GeV/c for K/p
31
Invariant Mass Reconstruction
  • In special relativity, the energy and momenta of
    particles are related as follow
  • This relation holds for one or many particles. In
    particular for 2 particles, it can be used to
    determine the mass of parent particle that
    decayed into two daughter particles.

32
Invariant Mass Reconstruction (contd)
  • Invariant Mass
  • Invariant Mass of two particles
  • After simple algebra

33
But remember the jungle of tracks
Large likelihood of coupling together tracks that
do not actually belong together
34
Example Lambda Reconstruction
Good pairs have the right invariant mass and
accumulate in a peak at the Lambda mass.
Bad pairs produce a more or less continuous
background below and around the peak.
35
STAR STRANGENESS!
(Preliminary)
_
K
_
W-
L
W
f
K0s
L
X-
_
X
K
36
Finding V0s
proton
Primary vertex
pion
37
In case you thought it was easy
38
Strange Baryon Ratios
STAR Preliminary
39
Resonances
f K K-
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