Energy fluctuations in canonical ensemble

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SUMMARY

The discussion centers on energy fluctuations in a canonical ensemble of particles with two energy states, where the ground state energy is zero and the energy difference is denoted as ##\delta##. It is established that even when the thermal energy ##k_BT## is less than the energy gap, particles can still be found in the excited state due to energy fluctuations. The partition function is calculated as ##Z = 1 + e^{-\delta/k_BT}##, leading to a probability of approximately 0.12 for finding a particle in the excited state. The fluctuations in energy are shown to be proportional to ##\frac{1}{\sqrt{N}}##, indicating that individual particle fluctuations do not depend on the number of particles in the system.

PREREQUISITES
  • Understanding of canonical ensemble theory
  • Familiarity with partition functions in statistical mechanics
  • Knowledge of Boltzmann distribution and its applications
  • Basic concepts of energy fluctuations in thermodynamics
NEXT STEPS
  • Study the derivation of the partition function in canonical ensembles
  • Explore the implications of the Boltzmann factor in statistical mechanics
  • Investigate energy fluctuations in systems with varying degrees of freedom
  • Learn about the thermodynamic limit and its effects on particle systems
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Students and researchers in statistical mechanics, physicists studying thermodynamic systems, and anyone interested in the behavior of particles in energy states within canonical ensembles.

lampCable
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Homework Statement


Consider an ensamble of particles that can be only in two states with the difference ##\delta## in energy, and take the ground state energy to be zero. Is it possible to find the particle in the excited state if ##k_BT=\delta/2##, i.e. if the thermal energy is lower than the gap between the energy levels? If so, explain why.

Homework Equations

The Attempt at a Solution



We calculate the partition function which becomes ##Z = 1+e^{-\delta/k_BT} = 1+e^{-2}## and so the probability for finding a particle in the excited state is ##P(excited) = \frac{e^{-\delta/k_BT}}{Z} = \frac{e^{-2}}{1+e^{-2}} \approx 0.12##. So we can therefore expect to find particles in the excited state.

Since the thermal energy ##k_BT## is too small to put particles in the excited state there must be something else going on. The solution to the problem says that it is due to energy fluctuations for a system in thermal contact with a reservoir of constant temperature. Now, it is possible to show that the fluctuations in the energy in the canonical ensamble is $$\frac{\Delta E}{E} \propto \frac{1}{\sqrt{N}},$$ where ##E## is the energy, ##\Delta E## is the standard deviation in ##E## and ##N## is the number of particles. But in the thermodynamic limit, i.e. when the number of particles is so big that the fluctuations are in principle zero, how can this be the reason?
 
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lampCable said:
Now, it is possible to show that the fluctuations in the energy in the canonical ensamble is $$\frac{\Delta E}{E} \propto \frac{1}{\sqrt{N}},$$ where ##E## is the energy, ##\Delta E## is the standard deviation in ##E## and ##N## is the number of particles. But in the thermodynamic limit, i.e. when the number of particles is so big that the fluctuations are in principle zero, how can this be the reason?
That is the fluctuation in the total energy of the system of N particles. The fluctuation in the energy of a single particle in that system doesn't depend on the number of particles and is exactly what is given by the Boltzmann distribution.
 
Okay, I think I understand. So when we talk about fluctuations in energy of a single particle in the system, we essentially talk about fluctuations in speed of that particle?
 
lampCable said:
Okay, I think I understand. So when we talk about fluctuations in energy of a single particle in the system, we essentially talk about fluctuations in speed of that particle?
Only for a free particle without any internal structure. Otherwise, energy is distributed among all degrees of freedom.
 
I see. But the Boltzmann distribution is only related to the translational degrees of freedom, so if we talk about fluctuations in say rotational energy then how is that described?
 
lampCable said:
I see. But the Boltzmann distribution is only related to the translational degrees of freedom, so if we talk about fluctuations in say rotational energy then how is that described?
I'm not talking about the Maxwell-Boltzmann distribution of speed, but the Boltzmann factor used to calculate the probability in the canonical ensemble.
 

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