Download You are going to read the chapter at home.

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Bell's theorem wikipedia , lookup

Light-front quantization applications wikipedia , lookup

Coherent states wikipedia , lookup

Hidden variable theory wikipedia , lookup

Path integral formulation wikipedia , lookup

Hartree–Fock method wikipedia , lookup

Renormalization group wikipedia , lookup

Quantum field theory wikipedia , lookup

Compact operator on Hilbert space wikipedia , lookup

Schrödinger equation wikipedia , lookup

Quantum state wikipedia , lookup

History of quantum field theory wikipedia , lookup

Tight binding wikipedia , lookup

Dirac equation wikipedia , lookup

Self-adjoint operator wikipedia , lookup

Scalar field theory wikipedia , lookup

Atomic theory wikipedia , lookup

Propagator wikipedia , lookup

Ensemble interpretation wikipedia , lookup

Bohr–Einstein debates wikipedia , lookup

Bra–ket notation wikipedia , lookup

Coupled cluster wikipedia , lookup

Probability amplitude wikipedia , lookup

Double-slit experiment wikipedia , lookup

Copenhagen interpretation wikipedia , lookup

Relativistic quantum mechanics wikipedia , lookup

Matter wave wikipedia , lookup

Elementary particle wikipedia , lookup

Wave–particle duality wikipedia , lookup

Symmetry in quantum mechanics wikipedia , lookup

Identical particles wikipedia , lookup

Second quantization wikipedia , lookup

Theoretical and experimental justification for the Schrödinger equation wikipedia , lookup

Wave function wikipedia , lookup

Canonical quantization wikipedia , lookup

Transcript
Chapter 1 : SECOND QUANTIZATION
Readings and lectures ...
You are going to read the chapter at
home.
I will go over some of the calculations in
class, but not all of them.
The purpose of the lectures is to
understand the results, but not always to
derive them in detail.
You should read the material before the
ΑΒΓΔΕΖΗΘΙΚΛΜΝΞΟΠΡΣΤΥΦΧΨΩ
lecture so that you will know the
αβγδεζηθικλμνξοπρςστυφχψω
notations.
+<=>±×⁄←↑→↓⇒⇔∇∏∑−∓∙√∞
≤≥≪≫∫∲ ∂≠〈〉ħ
1. THE SCHROEDINGER EQUATION IN FIRST AND
SECOND QUANTIZATION
Many body theory in first quantization
Start with
H = ∑Nk=1 T(xk) + ½ ∑’ Nk,l=1 V(xk,xl) ;
then find iħ (∂f/∂t) where f is the amplitude
for occupation numbers
fN ( n 1 n2 … n i … n∞ ) .
Notation
∑’ : here the prime means l ≠k
The first quantized theory
To Solve: iħ ∂Ψ/ ∂t = H Ψ
where Ψ = Ψ(x1 x2 x3 … xk … xN)
Introduce a complete set of time-independent
single-particle wave functions
Completeness: We can expand the Nparticle wave function as a product of
single-particle wave functions __
So far, this is simple. Now comes the
hard part: the N particles are identical
particles.
1a. Bosons .
Ψ(x1 … xN ; t ) must be symmetric with
respect to interchange of any two
coordinates; i.e.,
Ψ( … xk … xl … ; t ) = + Ψ( … xl … xk … ; t )
Then also,
C( … Ek … El … ; t ) = + C( … El … Ek … ; t )
for any case of k and l
“standard order”
(Lecture Jan 14)
Summary so far -- the quantum manyparticle problem in first quantized form …
◼ understand that the symmetry of the wave
function (for bosons) implies that the
basis states depend only on the list of
occupation numbers;
◼ expand Ψ( {x} ,t ) in occupation number
basis states;
◼ the Schroedinger equation for the
occupation number amplitude (eq. 1.25);
1b. The many-particle Hilbert space (a.k.
a. Fock space); creation and annihilation
operators; SECOND QUANTIZATION
bosons
H = ∑ij bi+< i |T| j > bj + ½ ∑ij bi+ bj+ < ij |V| kl > bl bk
Proof
1/2
Simplify the notation:
ψi(x) means ψEi(x);
i.e., the single particle wave
function with quantum
numbers Ei .
1/2
The final result is
equivalent to Eq. (1.25).
Q.E.D.
1c. Fermions
Start again with the first quantized Nbody Hamiltonian ,
Now add the antisymmetry of the of the
wave function Ψ(x1 x2 … xk … xN ; t) ,
Ψ( … xk … xk … ; t)
= − Ψ( … xl … xk … ; t)
for any case of k and k , for fermions.
**Exchange includes spin indices, suppressed
here.
Fermions are easier than bosons because
the occupation numbers are more limited:
for any single-particle state i,
ni can only be 0 or 1.
That’s the Pauli exclusion principle.
It is a consequence of the antisymmetry of
the wave function.
… ψE (xk) … ψE’ (xl) …
must be equal to
− … ψE (xl) … ψE’ (xk) …
If E’ = E then the N-body wave function
could only be 0; not possible.
Annihilation and creation operators for
fermions.
Use notation ci and ci☨ for fermions.
FOR FERMIONS, THE DEFINING
COMMUTATION RELATIONS ARE
ANTI COMMUTATION RELATIONS.
{ c i , c j } = c i cj + c j ci = 0
{ ci☨ , cj☨ } = ci☨ cj☨ + cj☨ ci☨ = 0
{ ci , cj☨ } = ci cj☨ + cj☨ ci = δij .
Another notation for the anticommutator:
{A,B} = [A,B]
+
The interpretation of fermionic operators
(ci and ci ☨ ) is the same as for bosonic
operators (bi and bi ☨ ):
ci = annihilation operator; annihilates a
particle in the state Ei ;
ci☨ = creation operator; creates a particle in
the state Ei ;
ci☨ ci = occupation number operator for the
state Ei .
Note that this automatically satisfies the
Pauli exclusion principle:
A state with two particles would be
ci ☨cj☨ |0〉;
but if i = j then we would have ci ☨ci☨ ; but
this is 0 by the second A.C. relation. So two
particles cannot occupy the same s.p. state.
Antisymmetry of the wave
function
Theorem.
The anti commutation
relations of the creation and
annihilation operators
imply that the N-body wave
function will be
antisymmetric.
∴ |000...1...1…0> = ½ (ca+cb+ - cb+ca+) |0>