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

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Show  that
 
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>
+
:<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
 
Show that the energy fluctuation is

Revision as of 21:06, 27 September 2007

Homework 1

1.) Mawell Boltzmann

Given the Maxwell -Boltzmann Distribution

N(v)=4π(m2πkT)3/2v2emv22kT

a.) Show <v>

Show that

<v>=4π(m2πkT)3/2(2kTm)2Γ(2)2

b.) Energy Fluctuation

Show that the energy fluctuation is

14m<(v<v>)2>=32(kT)2

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