amjad-sh said:
Here where I get confused, as dk means nothing physically.
1) If you read again my answer, I didn't say that dk has not a physical meaning. I said instead that dk is
not related to the spacing between the states
Be careful: the \mathbf{k}-space is a
vector space. Your variable \mathbf{k} = k_x \mathbf{x} + k_y \mathbf{y} + k_z \mathbf{z}, is in fact a
vector. It is defined by its components along the \mathbf{x}, \mathbf{y} and \mathbf{z} axes. The space between the allowed states is \pi / L for each component of \mathbf{k}, as you stated in your first post. So, the
density of the allowed states in
this vector space is (L / \pi)^3.
2) When you deal with g(k), you are
no more dealing with the vector \mathbf{k}, but just with its modulus: the real number k = | \mathbf{k} | = \sqrt{k_x^2 + k_y^2 + k_z^2}. You take a sphere of radius
k = | \mathbf{k} | = \sqrt{k_x^2 + k_y^2 + k_z^2}, then you take a sphere of radius k + dk = | \mathbf{k} | = \sqrt{k_x^2 + k_y^2 + k_z^2} + dk and you want to count
how many states of the vector space are present in the
shell between the two spheres. And correctly you make the multiplication of your first post. Now you are only interested in the radii k and k + dk of the spheres, and you are
no more interested in the \mathbf{k} vectors.
It is convenient for you to say that the number of the states in the shell is not just a number n, but a quantity g(k)dk, that is: (\mathrm{density\ per\ unit\ length}) \times \mathrm{length}.
The density per unit length is g(k), density per unit length of k: note that this variable k is
new for you. It is the
modulus of the vectors \mathbf{k}, not the vector \mathbf{k} itself. The length is dk: it is a linear length, because k is a real variable and it can be represented as an horizontal axis, just like x. You were dealing with spheres, but
because you are only interested in their radius, you are basically dealing with
a real number. You now can forget the spheres: you simply have a function g(k) to integrate, just like in Calculus you had a function f(x).
Why not considering a finite length \Delta k? You can. No problem. But this in general doesn't allow you to solve an integral:
\displaystyle \int_{k = k_1}^{k = k_2} g(k) \Delta k
is not correct. In order to solve an integral (and you
will have to solve it, when dealing with energy) you need an infinitesimal length dk:
\displaystyle \int_{k = k_1}^{k = k_2} g(k) dk
is correct and practicable.
So, the physical meaning of dk is the following. The states in \mathbf{k}-space are fixed and you know them pretty well. In order to solve this integral, now you must wonder: how many states are enclosed between two spherical shells whose radii are respectively k and k + dk? The outer sphere must have a radius infinitesimally longer than the first, in order to write g(k) dk. That is: how many states I enclose if I consider a real (not vector) variable k and I increase it by an infinitesimal quantity? This is how to proceed in Calculus courses when you deal with derivatives and integrals.
So, if you hoped dk has a practical, evident meaning, the answer is no: it doesn't. But you can draw two concentric spheres in the \mathbf{k} space, reduce the outer one to almost overlap the inner one, and measure the distance between them. dk is roughly that distance.
You are interested in k and not in \mathbf{k} because energy is a function of k only (k^2 to be more clear). Now you can write k as a function of E and dk in terms of k and dE and solve the integral, to find the density of states with respect to energy.