Difference between revisions of "HomeWork Simulations of Particle Interactions with Matter"

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===a.) Show <v>===
 
===a.) Show <v>===
 +
Show  that
 +
 +
:<math><v> = 4/pi \left ( \frac{m}{2 \pi kT}\right )^{3/2} \left( \frac{2kT}{m}\right)^2 \frac{\Gamma(2)}{2}</math>
 
===b.) Energy Fluctuation===
 
===b.) Energy Fluctuation===
 +
Show that the energy fluctuation is
 +
 +
:<math>\frac{1}{4} m < \left ( v - <v>\right)^2> = \frac{3}{2} (kT)^2</math>
 
==2.) MC calculation of Pi==
 
==2.) MC calculation of Pi==
  

Revision as of 21:06, 27 September 2007

Homework 1

1.) Mawell Boltzmann

Given the Maxwell -Boltzmann Distribution

[math]N(v) = 4 \pi \left ( \frac{m}{2\pi kT}\right)^{3/2} v^2 e^{-\frac{mv^2}{2kT}}[/math]

a.) Show <v>

Show that

[math]\lt v\gt = 4/pi \left ( \frac{m}{2 \pi kT}\right )^{3/2} \left( \frac{2kT}{m}\right)^2 \frac{\Gamma(2)}{2}[/math]

b.) Energy Fluctuation

Show that the energy fluctuation is

[math]\frac{1}{4} m \lt \left ( v - \lt v\gt \right)^2\gt = \frac{3}{2} (kT)^2[/math]

2.) MC calculation of Pi

Calculate \pi using the Monte Carlo method described in the Notes

3.) Histograms using ROOT

Homework 2

Homework 3

Homework 4

Back to Notes