Lecture 3 The Shankar strategy Teach quantum using ...
Transcript of Lecture 3 The Shankar strategy Teach quantum using ...
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Lecture 3
The Shankar strategyTeach quantum using postulatesTeach the math first then the postulates
Okay, but there is a lot of math!What math do we need?
We need the math for the postulatesSo we have the chicken or egg problem
“tell them what you are going to tell them”
Today postulates and the related mathDirac notationphoton polarization
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Math Topics
OperatorsObservable operatorsObservablesHamiltonian operatorPosition operatorMomentum operatorLinear operatorsIdentity operatorHermitean operatorsAntiHermitean operatorsUnitary operatorsProjection operatorsadjoint operation
Vectorsbraketstate vectorinner productouter productbasischange basischaracteristic equationadjoint operationorthogonalnormalorthonormal expansioneigenvalueseigenvectorseigensubspace
MeasurementDirac delta functionTime-dependent Schrodinger equationTime-independent Schrodinger equationDirac notationHilbert Spacediscrete non-degenerate spectrumdiscrete spectrum with degeneracycontinuous non-degenerate spectrum
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Chapter 1
Operator Methods In Quantum
Mechanics
1.1 Introduction
The purpose of the first two lectures is twofold. First, to review the mathematical formalism of
elementary non-relativistic quantum mechanics, especially the terminology. The second purpose is
to present the basic tools of operator methods, commutation relations, shift operators, etc. and
apply them to familiar problems such as the harmonic oscillator. Before we get down to the operator
formalism, let’s remind ourselves of the fundamental postulates of quantum mechanics as covered
in earlier courses. They are:
• Postulate 1: The state of a quantum-mechanical system is completely specified by a function
Ψ(r, t) (which in general can be complex) that depends on the coordinates of the particles
(collectively denoted by r) and on the time. This function, called the wave function or the
state function, has the important property that Ψ∗(r, t)Ψ(r, t) dr is the probability that the
system will be found in the volume element dr, located at r, at the time t.
• Postulate 2: To every observable A in classical mechanics, there corresponds a linear Her-
mitian operator A in quantum mechanics.
• Postulate 3: In any measurement of the observable A, the only values that can be obtained
are the eigenvalues {a} of the associated operator A, which satisfy the eigenvalue equation
AΨa = aΨa
1
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2 CHAPTER 1. OPERATOR METHODS IN QUANTUM MECHANICS
where Ψa is the eigenfunction of A corresponding to the eigenvalue a.
• Postulate 4: If a system is in a state described by a normalised wavefunction Ψ, and the
eigenfunctions {Ψa} of A are also normalised, then the probability of obtaining the value a
in a measurement of the observable A is given by
P (a) =∣∣∣∣∫ ∞
−∞Ψ∗
aΨ dr∣∣∣∣2
(Recall that a function Φ(r) such that∫ ∞
−∞Φ∗Φ dr = 1
is said to be normalised.)
• Postulate 5: As a result of a measurement of the observable A in which the value a is
obtained, the wave function of the system becomes the corresponding eigenfunction Ψa. (This
is sometimes called the collapse of the wave function.)
• Postulate 6: Between measurements, the wave function evolves in time according to the
time-dependent Schrodinger equation∂Ψ∂t
= − i
hHΨ
where H is the Hamiltonian operator of the system.
The justification for the above postulates ultimately rests with experiment. Just as in geometry one
sets up axioms and then logically deduces the consequences, one does the same with the postulates
of QM. To date, there has been no contradiction between experimental results and the outcomes
predicted by applying the above postulates to a wide variety of systems.
We now explore the mathematical structure underpinning quantum mechanics.
1.1.1 Mathematical foundations
In the standard formulation of quantum theory, the state of a physical system is described by a
vector in a Hilbert space H over the complex numbers. The observables and dynamical variables
of the system are represented by linear operators which transform each state vector into another
(possibly the same) state vector. Throughout this course (unless stated otherwise) we will adopt
Dirac’s notation: thus a state vector is denoted by a ket |Ψ〉. This ket provides a complete de-
scription of the physical state. In the next section we will explore the mathematical properties of
the Hilbert space and learn why it plays such a central role in the mathematical formulation of
quantum mechanics.
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