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Statistics for Particle Physics Lecture 1: Distributions

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Title: Statistics for Particle Physics Lecture 1: Distributions


1
Statistics for Particle PhysicsLecture 1
Distributions
  • Roger Barlow
  • Manchester University
  • TAE, Santander,10 July 2006

2
Statistics Why?
  • Statistics is not Physics. It is not
    fundamental.
  • But it is essential in our understanding of the
    experimental results which do led us towards the
    fundamental truths.
  • We learn this the hard way, as individuals and as
    a community

3
Two sorts of Statistics
  • Descriptive Statistics
  • How to convey information from complex data to
    audience (public, colleagues, superiors)
  • Simple numbers and plots
  • Driven by convention and common sense
  • Used by businessmen, journalists, and almost
    everybody
  • An Art
  • Inferential Statistics
  • What the data is trying to tell us about the
    process that produced it
  • Algorithms may be simple or complicated
  • Rigorous and verifiable
  • Used by Physicists, doctors, and farmers
  • A Science

4
Topic Distributions
  • Any non-deterministic model involves random
    distributions. (Discrete or continuous)
  • Lots of these Uniform, exponential, Chi-squared,
  • 3 most important
  • Binomial
  • Poisson
  • Gaussian

r
x
5
Binomial P(rn,p)
  • Tossing n coins. Probability of r heads and n-r
    tails is
  • P(rp,n)__n!__ pr(1-p) n-r
  • r! (n-r)!
  • Mean is ?np. Width described by ??np(1-p)
  • 1-p is often written q. Makes the formulae more
    elegant

5 trials
50 probability
90 probability
10 probability
6
When do we meet it?
  • Numbers of hits in Tracking chambers
  • Track-finding and Particle ID event efficiencies
    and multiplicities
  • Monte Carlo event generation (but see later)
  • Honestly, not very often

7
Poisson
  • Probability of r events when the mean is ? is
    P(r?)e- ? ? r
  • r!
  • Mean is ?. Standard deviation is ??.
  • Works for large and small ?

Mean 5.4
Mean 0.2
8
When do we get a Poisson distribution?
  • Discrete events in a continuum
  • Radioactive decays Geiger counter clicks are
    classic example
  • Numbers of events in data in particular numbers
    of rare events found. And numbers of events in
    histogram bins

9
The Gaussian
1 . ??2?
  • P(x?,?) exp (-(x- ?)2/ 2?2)

There is only one universal Gaussian picture.
Everything else is scaling and translation.
Peaks at x ? Width described by ? Bell-shaped
curve
10
When do we get Gaussians
  • Lots! Everything becomes Gaussian in some large
    n limit thanks to the Central Limit Theorem (CLT)
  • If y is a random variable made by the
    convolution of n random variables xi, then
  • my?mxi
  • ?2y??2xi
  • The distribution function for y becomes Gaussian
    for large n

11
The Standard Deviation
  • Any distribution has a mean ??x P(x) dx and a
    standard deviation given by
  • ?2?(x-?)2 P(x) dx
  • Standard deviations add in quadrature (apart from
    complications due to correlations.)
  • For the Gaussian only, 68 of P(x) lies with ? ?,
    95 within ? 2 ?, 99.7 within ? 3 ?

Apart from some pathological exceptions you
should pray you never meet
12
Convolutions that help us
  • Poisson Poisson Poisson
  • Separate sources add and can be treated as a
    single source
  • Poisson Binomial Poisson
  • A poisson source modified by a binomial detection
    efficiency gives a poisson number of detected
    events

13
Limit Binomial ? Poisson
  • Fixing n?p as n increases binomial becomes
    Poisson
  • So we can use Poisson for MC data, which is truly
    binomial (unlike real data, which is Poisson)

Poisson(r,0.2)
14
Limit Binomial ? Gaussian
All with p0.2
N10
N20
N80
N40
15
Limit Poisson ? Gaussian
16
Now try and example
  • Gaussian uniform
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