General thermo questions [Thermal average occupancy]

In summary, the conversation is about the thermal average occupancy, specifically the quantity represented by N. The grand partition function and definitions for <N> are discussed, and the connection between the equations for <N> is questioned.
  • #1
IHateMayonnaise
94
0
Howdy,

Just studying for a test, need to clear something up and I can't find it in any of my books.

My question is in regards to [itex]N[/itex], which to me seems like it is the same as [itex]<N>[/itex] also known as the thermal average occupancy. This quantity represents the thermal average number of the orbitals in the system while in thermal and diffusive contact with a reservoir. In such a domain, we want to use the grand partition function:

[tex]z=\sum_{ASN}e^{-\beta(N\mu-\varepsilon_s)}=\sum_{ASN}\lambda^Ne^{(-\beta\varepsilon_s)}[/tex]

where
[tex]\beta=\frac{1}{K_bT}[/tex], [tex]\lambda=e^{\beta\mu}[/tex]

And the following definitions for [itex]<N>[/itex]:

[tex]<N>=\frac{1}{z}\sum_{ASN}Ne^{-\beta(N\mu-\varepsilon_s)}[/tex]

and

[tex]<N>=\lambda\sum_{S}e^{-\beta\varepsilon_s}[/tex]

My question: What is the connection between the last two equations for [itex]<N>[/itex]? Thanks yall

IHateMayonnaise
 
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  • #2
There are two ways of getting ensemble averages: you can either take an average weighted by the coefficients in the partition function


Say, if

[tex] Z = \sum_{\mathrm{states}} \rho, \hspace{0.5cm} \mathrm{then} \hspace{0.5cm} \langle N \rangle = \frac{1}{Z} \sum_{\mathrm{states}} N \rho. [/tex]

The second way that I know of to calculate averages is to derivate the thermodynamic potential twice. Your second formula looks like it might be something of the sort, but I'm really not very sure.
 

1. What is thermal average occupancy?

Thermal average occupancy is a measure of the average number of particles or molecules in a system at a particular temperature. It takes into account the probability of each possible state of the system and calculates the average number of particles in each state. It is an important concept in thermodynamics and statistical mechanics.

2. How is thermal average occupancy calculated?

Thermal average occupancy is typically calculated using the Boltzmann distribution, which takes into account the energy of each state and the temperature of the system. The formula for thermal average occupancy is:
N = ∑ni e-Ei/kT
Where N is the average occupancy, ni is the number of particles in state i, Ei is the energy of state i, k is the Boltzmann constant, and T is the temperature of the system.

3. What factors can affect thermal average occupancy?

Thermal average occupancy can be affected by several factors, including temperature, energy levels of the system, and the number of particles present. It can also be influenced by external factors such as pressure and volume. Additionally, the type of particles in the system and their interactions with each other can also impact thermal average occupancy.

4. Why is thermal average occupancy important in thermodynamics?

Thermal average occupancy is important in thermodynamics because it helps us understand and predict the behavior of particles in a system. It provides a way to quantify the average number of particles in each state and how that changes with temperature. This information is crucial in understanding the properties of materials and how they respond to changes in temperature and other external factors.

5. How is thermal average occupancy related to entropy?

Thermal average occupancy is closely related to the concept of entropy. Entropy is a measure of the disorder or randomness in a system, and it is directly related to the number of microstates (or possible arrangements) of particles in a system. As thermal average occupancy increases, the number of microstates also increases, leading to an increase in entropy. This relationship is described by the Boltzmann equation: S = k ln W, where S is entropy, k is the Boltzmann constant, and W is the number of microstates.

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