Relationship between k and E when deriving the density of states

In summary, the number of states in a volume of k-space, ##n(k)dk##, is equal to ##\frac{L^3}{\pi^2}dk##. This is derived from the fact that ##n(k)dk = n(E)dE##, and each coordinate in k-space has two associated energy states due to the two directions of polarization.
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Homework Statement
I'm trying to work through the derivation of the density of states function in a Fermi sphere. I understand the derivation except for one part when n(k)dk changes to n(E)dE with the only explanation being "by definition".
Relevant Equations
Volume of k-space per electron energy state = ##\frac{L^3}{4 \pi^3}##
Hence energy states per unit volume is ##\frac{4 \pi^3}{L^3}##
Volume of k-space between spheres of radius ##k## and ##k + dk## is ##4 \pi k^2 dk##.
Number of states in that volume of k-space, ##n(k)dk## is: $$n(k)dk = (\frac{L^3}{4 \pi^3}) \cdot 4 \pi k^2 dk = \frac{L^3}{\pi^2}dk$$.
Then the notes state that by defintion, ##n(k)dk = n(E)dE##, and hence $$n(E)d(E) = \frac{L^3}{\pi^2}dk$$.

I don't quite see why this is true - isn't it the case that each coordinate in k-space has 2 energy states associated with it? Then how is the number of energy states in that volume that same as the number of k states? If someone can clear up my confusion that would be great, thanks!
 
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Related to Relationship between k and E when deriving the density of states

1. What is the relationship between the wave vector k and the energy E when deriving the density of states?

The relationship between k and E is given by the dispersion relation, which describes how the energy of a particle varies with its wave vector. In general, the dispersion relation can vary depending on the system, but it is typically a parabolic relationship for non-interacting particles.

2. How does the density of states depend on the energy of the system?

The density of states is directly proportional to the energy of the system. This means that as the energy of the system increases, the number of available states also increases. This relationship is often described by the density of states function, which is a continuous function that varies with energy.

3. Can the density of states be used to determine the number of particles in a system?

Yes, the density of states can be used to determine the number of particles in a system by integrating over the energy range of interest. This is known as the density of states integral and it provides an estimate of the total number of particles in a given energy range.

4. How does the density of states change with the dimensionality of the system?

The density of states is directly related to the dimensionality of the system. In one-dimensional systems, the density of states is constant, in two-dimensional systems it increases linearly with energy, and in three-dimensional systems it increases quadratically with energy.

5. What is the significance of the density of states in understanding the behavior of a system?

The density of states is a fundamental concept in understanding the behavior of a system, especially in condensed matter physics. It provides information about the available states for particles in a system and is used to calculate various properties such as heat capacity, conductivity, and magnetization. Additionally, it is used in the derivation of many important equations, such as the Fermi-Dirac distribution and the Bose-Einstein distribution.

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