Difference between revisions of "Statistics for Experimenters"
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: the distribtuion approximates the Binomial Distribution for the special case when the probability of the event occuring is small. | : 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 | ||
+ | :P(k,\mu) = \frac{\mu^{k}e^{-\mu}}{k!} | ||
;Gaussian/Normal Distribution | ;Gaussian/Normal Distribution |
Revision as of 21:24, 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
- P(k,\mu) = \frac{\mu^{k}e^{-\mu}}{k!}
- 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 =