Energy fluctuations of canonical system

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SUMMARY

The discussion focuses on deriving the mean square fluctuation in energy for a canonical system in thermal contact with a reservoir, expressed as < e-U >^2 = t^2*(∂U/∂t). The key equations include U = Σε*exp(-ε/t)/Z and Z = Σexp(-ε/t), where the summation is over all states. Participants emphasize the importance of the partition function in relating energy fluctuations to temperature and derivatives of Z. The challenge lies in expressing <ε2> in terms of the partition function and its derivatives.

PREREQUISITES
  • Understanding of canonical ensembles in statistical mechanics
  • Familiarity with partition functions and their properties
  • Knowledge of thermodynamic derivatives and their applications
  • Basic calculus, particularly differentiation of functions
NEXT STEPS
  • Explore the derivation of the partition function Z for various systems
  • Learn about the statistical interpretation of energy fluctuations in canonical ensembles
  • Investigate the relationship between temperature and energy fluctuations in thermodynamic systems
  • Study the application of derivatives in statistical mechanics, particularly in relation to U and Z
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Students and researchers in statistical mechanics, physicists studying thermodynamic systems, and anyone interested in the mathematical foundations of energy fluctuations in canonical ensembles.

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Homework Statement


Consider a system of fixed volume in thermal contact with a reservoir. Show that the mean square fluctuation in the energy is

< e-U >^2= t^2*(∂U/∂t) where U=<e>

Hint: use the partition function to relate (∂U/∂t) to the mean square flucuation. Also, mulitply out the (...)^2 term. Note: the temperature t of a system is a quantity that by definition does not flucuate in value when the system is in thermal contact with a reservoir.

Homework Equations


[/B]
U=Σε*exp(-ε/t)/Z=t^2*(∂logZ/∂t)
Where the summation is over all states

Z=Σexp(-ε/t)
Where the summation is over all states

The Attempt at a Solution


1. Replace U in the mean square energy flucation term with the definition
<ε-t^2*(∂logZ/∂t)>^2=t^2*(∂U/∂t)

2. (∂logZ/∂t)=(1/z)*(∂Z/∂t)
<ε-t^2*(1/z)*(∂Z/∂t)>^2=t^2*(∂U/∂t)

3. (∂Z/∂t)=∑ε*t^-2*exp(-ε/t)
<ε-t^2*(1/z)*∑ε*t^-2*exp(-ε/t)>^2=t^2*(∂U/∂t)

Not sure where to go from here. My intution says to take the deriviative of U and substitue on the right hand side. But taking the deriviaitve of U (as its defined above) with respect to t introduces a second derivative of logZ and makes the problem a lot more difficult. I feel like there is an easier way?
 
Physics news on Phys.org
Hi. You already know that <ε> =(1/Z) Σε*exp(-ε/t)
Now you need to find out an expression for <ε2>–<ε>2, so:
How would you express <ε2> using the partition function?
What function of the Z and derivatives of Z (with respect to time) would that correspond to?
 

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