Transformations of Operators and Symmetry

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Quantum Mechanics A
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Schrödinger Equation
The most fundamental equation of quantum mechanics; given a Hamiltonian , it describes how a state evolves in time.
Basic Concepts and Theory of Motion
UV Catastrophe (Black-Body Radiation)
Photoelectric Effect
Stability of Matter
Double Slit Experiment
Stern-Gerlach Experiment
The Principle of Complementarity
The Correspondence Principle
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Brief Derivation of Schrödinger Equation
Relation Between the Wave Function and Probability Density
Stationary States
Heisenberg Uncertainty Principle
Some Consequences of the Uncertainty Principle
Linear Vector Spaces and Operators
Commutation Relations and Simultaneous Eigenvalues
The Schrödinger Equation in Dirac Notation
Transformations of Operators and Symmetry
Time Evolution of Expectation Values and Ehrenfest's Theorem
One-Dimensional Bound States
Oscillation Theorem
The Dirac Delta Function Potential
Scattering States, Transmission and Reflection
Motion in a Periodic Potential
Summary of One-Dimensional Systems
Harmonic Oscillator Spectrum and Eigenstates
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Coherent States
Charged Particles in an Electromagnetic Field
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The Heisenberg Picture: Equations of Motion for Operators
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Angular Momentum as a Generator of Rotations in 3D
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Feynman Path Integrals
The Free-Particle Propagator
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Differential Cross Section and the Green's Function Formulation of Scattering
Central Potential Scattering and Phase Shifts
Coulomb Potential Scattering

Transformations of Operators

In the previous section, we discussed operators as transformations of vectors. In many cases, however, we will be interested in how operators, observables in particular, will transform under the action of another operator. Given an operator and a transformation we define the transformed operator as follows. Given the relation,

between two vectors and , the operator is the operator giving the relation between and i.e.,

To find let us first act on both sides of the original relation with

We now introduce the identity between and in the form,

Using the above definitions of and we may write this as

We see then that the transformed operator In matrix form, this would simply correspond to a similarity transformation of

Of particular importance is the case in which is unitary and is an observable. This is because, in addition to preserving the normalization of the state vectors, as mentioned in the previous section, they also preserve the Hermitian nature of

Symmetry and its Role in Quantum Mechanics

Having discussed the transformation of operators, we will now apply our results to discuss symmetries of the Hamiltonian, a very important topic. As alluded to in the previous section, identifying the symmetries of the Hamiltonian will allow us to greatly simplify the problem at hand. In addition, in both classical and quantum mechanics, symmetry transformations become important due to their relation to conserved quantities via Noether's Theorem. Moreover, in quantum mechanics, the importance of symmetries is further enhanced by the fact that measurements of conserved quantities can be exact in spite of the probabilistic nature of quantum predictions.

Given a unitary transformation we say that it is a symmetry of the Hamiltonian if it leaves the Hamiltonian invariant; i.e., if We will now show that, if a transformation is a symmetry of the Hamiltonian, then it commutes with the Hamiltonian. To see this, let us take the relation,

and act on both sides with

Now, if is a symmetry of the Hamiltonian, then it must also be true that

Subtracting these two equations, we see that, because is arbitrary, the Hamiltonian commutes with the transformation operator; i.e.,

Problem on symmetry

Commutators & symmetry

We can define an operator called the parity operator, which does the following:

The parity operator commutes with the Hamiltonian if the potential is symmetric, . Since the two commute, the eigenfunctions of the Hamiltonian can be chosen to be eigenfunctions of the parity operator. This means that if the potential is symmetric, the solutions can be chosen to have definite parity (even and odd functions).