Classical and Quantum Statistics

There are 3 (or maybe 3 and a half?) distributions that we shall look at : Maxwell-Boltzmann distribution, Fermi-Dirac distribution and Bose-Einstein distribution.

Boltzmann distribution concerns distinguishable particles. Its half-cousin is the Maxwell-Boltzmann distribution, which applies to  dilute gases. They resemble one another so much that many people don’t even care to make a distinction between them.

statistical-thermodynamics-boltzmann-distribution

Maxwell-Boltzmann statistics simply takes away the N! factor from w, which makes no difference to the partition function and the distribution function. Hence the two distributions are often taken to be the same.

Fermi-Dirac particles are loners – they cannot share the same quantum states with each other, i.e., they obey Pauli’s exclusion principle.

statistical-thermodynamics-fermi-dirac-distribution

Bose-Einstein particles are social animals, they prefer staying together than being left alone.

Statistical Thermodynamics - Bose-Einstein distribution.png

 

Coupled pendulum

A coupled pendulum is a simple 2- state system. One way to make such a system is to attach a light spring between two pendulums. Starting with one of the pendulums swinging while the other one at rest, soon the oscillations of the one that moves first reduce in amplitude while the other one’s amplitude builds up. Then the cycle repeats itself and we get a continuous back-and-forth pouring of energy between the two pendulums.

The mathematics behind this interesting behaviour begins with a set of differential equations :

coupled-pendulum-de

To solve these differential equations, we assume that their solutions are in the form as given below :

coupled-pendulum-gs

Plugging them back to the original differential equations and we now can solve for the unknown A and B :

Coupled Pendulum - two solutions.png

The first solution simply have the two pendulums swinging together in unison : each keeps its own energy and nothing transfers between them, in other words nothing really fun to look at. The second solution is the one corresponding to the start-stop behaviour that sees alternately one pendulum with dying and the other pendulum with growing oscillations, definitely more gratifying when watched.

Hermite polynomials

After struggling for many years to understand harmonic oscillator, I’m finally making some headway.

To remember this happy moment, let’s also remember 4 nice formula related to Hermite polynomials.

hermite-polynomial

“Any serious student of quantum mechanics must have a thorough understanding of the harmonic oscillator.”    –  J.J. Sakurai.

Euler angles

A rotation in 3-dimension space about any axis passing through the origin can be made equivalent to the combined effect of 3 successive rotations. Euler proved this theorem and the angles associated with the 3 rotations were named Euler angles, in particular, α, β and γ.

First a rotation about the z axis by an angle α results in new orientations for the original x and y axes, let’s call them x′ and y′. Then a rotation about the x′ axis by an angle β  turns y′ and z′ to two new directions : y″ and z″. Finally a rotation about the z″ axis by an angle γ brings the body to a final orientation (referenced by XYZ axes in red below) coinciding with that obtained by rotating about the initial prescribed axis.

pictorial-representation-of-euler-angles-a-b-and-y

This sequence of rotation can be represented as an algebraic operation of matrix multiplication :
euler-angles

Learning about Euler angles can help us form up the transformation matrix in passing from one representation to another when spin-half particles are filtered by 2 Stern-Gerlach apparatus oriented differently with respect to one another.

Complex Refractive Index

In working out the formula for the refractive index of a piece of material, we considered the oscillations of an electron, being impinged upon by the electric field carried by the incoming electromagnetic wave. In the end a complex number inadvertently creeped out. This is due to the inclusion of the drag force acting on the oscillator, which translated into absorption of the electromagnetic energy by the material as the electrons shake about.

complex-refractive-index

The real part of the complex number gives the ordinary re-radiated wave (with a phase shift) ; the imaginary part will cause a drop in the amplitude of the wave as it penetrates deeper into the material.

absorption-coefficient

We note the attenuation of the amplitude of the E field upon passing into the material. The coefficient of absorption β is deduced.

Another interesting observation we can make is that the index of refraction can be less than 1 ! But that doesn’t mean the wave speed is really higher than c. We need to make a distinction between phase speed and group speed, the speed of the carrier and the speed of the signal. The signal speed will not surpass c.

A few other useful quantities can be derived upon further considerations.

In a conductor the conduction electrons are unbounded, so we can ignore the natural frequency in the above formula. Also, by bringing in other electrical characteristics of the material, such as the conductivity and the characteristic time, the refractive index of metals is presented in a new form :

conductor-refractive-index

At low frequencies, we simplify the above expression by taking away 1 and the second order term in omega, then the skin-depth is deduced.

skin-depth

At high frequencies, we can simplify the denominator by ignoring the first order term in omega. Then we obtain the plasma frequency, which is related to the density oscillations of free electrons.

plasma frequency.png

Negative temperature

Can temperature go lower than absolute zero kelvin ? It’s possible with statistical thermodynamics.

Consider a two-level system, for example magnetic dipoles in a magnetic field. Some of the dipoles may be aligned with the magnetic field while the rest are aligned opposite to the field. Those aligned with the field are at a lower energy level and those aligned opposite are at a higher energy level.

We can relate the number of dipoles of each type with energy and temperature this way :

negative temperature

So if there are more dipoles in the upper level than the lower level, we will have a negative thermodynamic temperature !

Electron radius, fine structure constant and HEC

Here’s a way to remember the formula for the Bohr radius, the classical electron radius and the fine structure constant : HEC (in French this acronym means Hautes Etudes Commerciales).

Bohr radius is the quantum mechanical radius for electron and it can be calculated by the ratio between Planck’s reduced constant squared and the product of the mass of an electron and its reduced charge squared.

Bohr radius

The classical electron radius is the ratio of the square of the reduced electronic charge to the product of the mass of an electron and the square of the speed of light.

classical electron radius

The ratio of Bohr radius to classical electron radius is about 137², and it’s the square of the reciprocal of the fine structure constant.

alpha

 

 

 

Jones vectors and matrices

As a plane-polarised electromagnetic wave propagates in the z-direction, the electric field vector may be oscillating either linearly or elliptically in the x-y plane. The vector can be decomposed into an x-component and a y-component. The phase relation between the two components determines the type of polarisation.

Here are some examples of the Jones vectors corresponding to the various types of polarisation :

Jones vectors.png

The action by a polariser can be represented with a matrix. Upon passing through the polariser, the original orientation of the polarised light will be modified. By carrying out matrix multiplication, the emerging light polarisation direction can be deduced.

jones matrices

The convention follows that employed in optics : right hand polarised means when looking towards the source, the electric vector rotates clockwise.

Two integrals (to be memorised)

These two integrals are said (by Richard Feynman) to be so commonly encountered in statistical mechanics that it is worthwhile memorising them :

2 integrals

They are useful because they are needed to make Fourier transforms between momentum representation and position representation.