Statistical physics - does total energy matter, or only differences?

  • #1
laser1
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Relevant Equations
Z
In statistical physics, in a two level system, I'll give an example to show what I am talking about:

situation 1) energy 0 and energy E
situation 2) energy E/2 and energy -E/2

Are these two situations equivalent? Computing the partition function for both of them it seems they are different, but I am not sure. Because from my experience when dealing with energies in mechanics only the energy difference is important. Cheers
 
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  • #2
Can you write the two expressions? Why do you think it matters?
 
  • #3
pines-demon said:
Can you write the two expressions? Why do you think it matters?
The two expressions for ##Z##:

1) ##e^{-\beta \epsilon}+1##
2) ##2\cosh\left(\frac{\beta \epsilon}{2}\right)##

I think it matters because they are two different expressions!
 
  • #4
laser1 said:
The two expressions for ##Z##:

1) ##e^{-\beta \epsilon}+1##
2) ##2\cosh\left(\frac{\beta \epsilon}{2}\right)##

I think it matters because they are two different expressions!
Well the partition functions cannot be exactly the same because energies are slightly shifted so it matter for energy-level dependent quantities, for example if you calculate the mean energy ##\overline{E}=-\partial \ln Z/\partial \beta## you get:
  1. ##\epsilon/(e^{\beta \epsilon}+1)##
  2. ##\epsilon \tanh(\beta \epsilon/2)/2##
As ##\beta \to 0##, Eq.1 goes to ##\epsilon/2## and Eq.2 goes to ##0## (the average value) as you would expect because of the choice of energy reference. However if you calculate a quantity that does not depend on the energy reference, for example the energy fluctuations around the mean ##\Delta E^2=\overline {E^2}-\overline{E}^2=\partial^2 \ln Z/\partial \beta^2## you get
$$\Delta E^2=\frac{\epsilon^2 e^{\beta \epsilon}}{(e^{\beta \epsilon}+1)^2}$$
for both. You can try with other energy-independent quantities.
 
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  • #5
Here is another example, imagine that the higher energy state has a magnetic moment ##m## associated to it, and the lower energy state has a moment ##-m##. The average magnetic moment is
$$\overline{m}=m\frac{\exp(-\beta \epsilon)-1}{\exp(-\beta \epsilon)+1}=m\frac{\exp(-\beta \epsilon/2)-\exp(\beta \epsilon/2)}{\exp(-\beta \epsilon/2)+\exp(\beta \epsilon/2)}$$
which is the same value for both.
 
  • #6
Another way to check all of this is to write a system with energies ##-E_0## and ##E-E_0##. If you calculate the mean energy it will depend on ##E_0##, but if you write the other two quantities above, ##E_0## will vanish.
 
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  • #7
pines-demon said:
Well the partition functions cannot be exactly the same because energies are slightly shifted so it matter for energy-level dependent quantities, for example if you calculate the mean energy ##\overline{E}=-\partial \ln Z/\partial \beta## you get:
  1. ##\epsilon/(e^{\beta \epsilon}+1)##
  2. ##\epsilon \tanh(\beta \epsilon/2)/2##
As ##\beta \to 0##, Eq.1 goes to ##\epsilon/2## and Eq.2 goes to ##0## (the average value) as you would expect because of the choice of energy reference.
You can see the shift a little more easily if you rewrite the first partition function ##Z_1## as
$$Z_1 = e^{\beta \epsilon}+1 = e^{\beta \epsilon/2}[\underbrace{2\cosh (\beta \epsilon/2)}_{Z_2}].$$ When you calculate the mean energy, the exponential factor contributes a shift of ##\epsilon/2## to the mean energy you get from the second partition function ##Z_2##.
 
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FAQ: Statistical physics - does total energy matter, or only differences?

1. What is the significance of total energy in statistical physics?

Total energy in statistical physics is significant as it provides a comprehensive description of a system's state. However, in many cases, especially in thermodynamics, only energy differences are relevant because they determine the likelihood of transitions between states and the system's behavior at equilibrium.

2. Why are energy differences often more important than total energy?

Energy differences are more important because they dictate the dynamics of a system, such as the probabilities of state occupancy and transitions. In statistical mechanics, the partition function, which is central to calculating thermodynamic properties, depends on these differences rather than the absolute values of energy.

3. How does the concept of energy differences relate to temperature?

The concept of energy differences is directly related to temperature through the Boltzmann distribution. Temperature is a measure of the average energy per degree of freedom, and it influences the distribution of particles among available energy states, which is determined by the differences in energy levels.

4. Are there situations where total energy is necessary to consider?

Yes, there are situations, such as in the analysis of isolated systems or when considering conservation laws, where total energy is crucial. In these cases, understanding the total energy helps in predicting the system's evolution over time and ensuring that energy conservation principles are upheld.

5. Can you provide an example where only energy differences are relevant?

An example is the calculation of the Helmholtz free energy in a canonical ensemble. The free energy is derived from the logarithm of the partition function, which includes only the differences in energy between states. This approach allows us to determine thermodynamic properties without needing to know the absolute values of the energies involved.

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