How Does Room Temperature Affect Electron States in an Energy Band?

V = 1.684*10^9*(KT)^3Therefore, in summary, the number of states per unit volume within a small energy range KT about the centre of the band at room temperature is equal to 1.684*10^9*(KT)^3.
  • #1
nadeemo
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Homework Statement



Given the width of an energy band of electrons is typically ~10eV, calculate the number of states per unit volume within a small energy range KT about the centre of the band at room temperature.

K is boltzmanss constant = 8.617*10^-5 eV/K

Homework Equations



volume of a sphere = 4*pi*(p^2)*dp

p^2 = 2mE

g(E) dE = 2*B*(m^3/2)*sqrt E* dE

p is momentum, E is energy, m is mass, B is some constant (not given)


The Attempt at a Solution



so I've let E = 10eV, and m as the mass of an electron, but we still don't know B, and how room temp plays into the equation...my relevant equations may be wrong, also if you solve for E = p^2 / 2m, and plug it into volume and solve for g(E) dE you get, B/(4*pi)
 
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  • #2
* (m^3/2) * (2m/KT)^3/2, and then you can multiply by the small energy range dE, but I'm not sure if this is correct.

Thank you for your question. To calculate the number of states per unit volume within a small energy range KT about the centre of the band at room temperature, we can use the density of states formula:

g(E) = (2*m^3/2)/sqrt(2*pi*h^3)*(E)^(1/2)

Where m is the mass of an electron and h is Planck's constant. We can then integrate this formula over the energy range KT to get the total number of states within that range.

g(KT) = (2*m^3/2)/sqrt(2*pi*h^3)*∫(E)^(1/2)dE from 0 to KT

Simplifying this integral, we get:

g(KT) = (2*m^3/2)/sqrt(2*pi*h^3)*(2/3)*(KT)^(3/2)

Substituting in the given values for m, h, and K, we get:

g(KT) = (2*(9.109*10^-31)^3/2)/sqrt(2*pi*(6.626*10^-34)^3)*(2/3)*(8.617*10^-5)^(-3/2)*(KT)^(3/2)

g(KT) = 4.258*10^47*(KT)^(3/2)

To get the number of states per unit volume, we divide this value by the volume of a sphere with radius p = √(2mE):

g(KT)/V = 4.258*10^47*(KT)^(3/2)/(4*pi*(√(2mE))^3)

g(KT)/V = 2.129*10^47*(KT)^3/(8*pi*(m^3)*E^(3/2))

Substituting in the given value for E = 10eV and the mass of an electron, we get:

g(KT)/V = 2.129*10^47*(KT)^3/(8*pi*(9.109*10^-31)^3*(10*1.602*10^-19)^(3/2))

g(KT
 

1. What is Statistical Mechanics?

Statistical Mechanics is a branch of physics that uses statistical methods to explain and predict the behavior of large systems of particles. It is based on the fundamental principles of thermodynamics and statistical probability.

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Statistical Mechanics is closely related to thermodynamics, as it provides a microscopic understanding of the macroscopic behavior of thermodynamic systems. It helps to explain how energy is distributed among particles in a system and how this affects the overall properties of the system.

3. What are the key concepts in Statistical Mechanics?

The key concepts in Statistical Mechanics include the concept of ensembles, which are collections of possible states of a system, and the Boltzmann distribution, which describes the probability of a system being in a particular state. Other important concepts include entropy, temperature, and the partition function.

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