Difference between revisions of "Statistics for Experimenters"
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+ | = Definitions= | ||
+ | |||
+ | ;Accuracy | ||
+ | : A measure of how close the experimental result is to the "true" value | ||
+ | |||
+ | ; Precisison | ||
+ | : A meauser of close the result is determined without knowing the true vaule | ||
+ | : Precision is often used to predict the accuracy of a quantity to be measured (you don't know the answer before doing the experiment) | ||
+ | |||
+ | |||
+ | ;Random Error | ||
+ | : The error in a result due to the finite precision of an experiment | ||
+ | : A measure of the statistical fluctuations which result after repeated experimentation | ||
+ | |||
+ | ;Systematic Error | ||
+ | : Reproducable inaccuracies introduced by faulty equipment, calibration, or technique. | ||
+ | |||
+ | =Probability Distributions= | ||
;Binomial distribtuion | ;Binomial distribtuion | ||
+ | :random, independent process with two possible outcomes | ||
: best example is a coin toss, its either heads or tails | : best example is a coin toss, its either heads or tails | ||
: mean (<math>\mu</math>) = number of tries <math>n</math>(coin flips) * probability of success<math>p</math> (head, 1/2) | : mean (<math>\mu</math>) = number of tries <math>n</math>(coin flips) * probability of success<math>p</math> (head, 1/2) | ||
Line 8: | Line 27: | ||
: standard deviation (<math>\sigma</math>) = root of the mean (<math>\sqrt{\mu}</math>) | : standard deviation (<math>\sigma</math>) = root of the mean (<math>\sqrt{\mu}</math>) | ||
: use in counting experiments | : use in counting experiments | ||
− | : the distribtuion approximates the Binomial Distribution for the special case when | + | : the distribtuion approximates the Binomial Distribution for the special case when the probability of the event occuring is small. |
: In the cosmic ray telescope experiment the mean number of detected cosmic rays is much smaller than the number of cosmic rays passing by. | : In the cosmic ray telescope experiment the mean number of detected cosmic rays is much smaller than the number of cosmic rays passing by. | ||
+ | |||
+ | The probability distribution is given as | ||
+ | :<math>P(k,\mu) = \frac{\mu^{k}e^{-\mu}}{k!}</math> | ||
+ | |||
+ | where | ||
+ | |||
+ | : <math>k</math> = number of occurances | ||
+ | : <math>\mu</math> = mean | ||
;Gaussian/Normal Distribution | ;Gaussian/Normal Distribution | ||
: Full WIdth at Half Max (FWHM) = width of the distribution at half the value of the maximum probabilty (distibution peak) = <math>\Gamma</math> | : Full WIdth at Half Max (FWHM) = width of the distribution at half the value of the maximum probabilty (distibution peak) = <math>\Gamma</math> | ||
− | :standard deviation (<math>\sigma</math>) = <math>\frac{\Gamma} {2.354}</math> | + | :standard deviation (<math>\sigma</math>) = <math>\frac{\Gamma} {2 \sqrt{2 \ln 2}} = \frac{\Gamma} {2.354}</math> |
:error = <math>0.675 \sigma</math> | :error = <math>0.675 \sigma</math> |
Latest revision as of 21:26, 20 September 2007
Definitions
- Accuracy
- A measure of how close the experimental result is to the "true" value
- Precisison
- A meauser of close the result is determined without knowing the true vaule
- Precision is often used to predict the accuracy of a quantity to be measured (you don't know the answer before doing the experiment)
- Random Error
- The error in a result due to the finite precision of an experiment
- A measure of the statistical fluctuations which result after repeated experimentation
- Systematic Error
- Reproducable inaccuracies introduced by faulty equipment, calibration, or technique.
Probability Distributions
- Binomial distribtuion
- random, independent process with two possible outcomes
- best example is a coin toss, its either heads or tails
- mean ( ) = number of tries (coin flips) * probability of success (head, 1/2)
- standard deviation( ) =
- Poisson Distribution
- standard deviation ( ) = root of the mean ( )
- use in counting experiments
- the distribtuion approximates the Binomial Distribution for the special case when the probability of the event occuring is small.
- In the cosmic ray telescope experiment the mean number of detected cosmic rays is much smaller than the number of cosmic rays passing by.
The probability distribution is given as
where
- = number of occurances
- = mean
- Gaussian/Normal Distribution
- Full WIdth at Half Max (FWHM) = width of the distribution at half the value of the maximum probabilty (distibution peak) =
- standard deviation ( ) =
- error =