Difference between revisions of "Statistics for Experimenters"
		
		
		
		
		
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= Definitions=  | = Definitions=  | ||
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;Systematic Error  | ;Systematic Error  | ||
| − | + | : Reproducable inaccuracies introduced by faulty equipment, calibration, or technique.  | |
| − | |||
=Probability Distributions=  | =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 28: | 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 =