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Chapter
5
Identical
particleTwo-particle
System
201Atoms
210Solids
218Quantum
Statistical
Mechanics
2305.1
Two-particle
SystemsFor
a
single
particle,
is
a
function
of
the
spatialcoordinates
r
and
the
time
t
(here
now
we
ignore
the
spin).The
wave
function
for
a
two-particle
system
is
a
function
ofthe
coordinates
of
particle
one
(r1),
the
coordinates
of
par-ticle
two
(r2),
and
the
time:The
Hamiltonian
for
the
whole
system
is:Its
time
evolution
is
always
determined
by
the
Schr?dingerequation:Normalization:For
time-independent
potentials,
we
obtain
a
complete
set
ofsolutions
by
separation
of
variables:The
time-independent
Schr?dinger
equation:5.1.1
Bosons
and
FermionsQuantum
mechanics
neatly
accommodates
the
E.
Fermiexistence
of
particles
that
are
indistinguishablein
principle:
We
simply
construct
a
wave
functionthat
is
noncommittal
as
to
which
particle
is
inwhich
state.
There
are
actually
two
ways
to
do
it:S.
N.
BoseSuppose
particle
1
is
in
the
(single-particle)
state,
and
particle
2
is
in
the
state .
Inthatcaseis
a
simple
conduct:+:
Bosons;
-:Fermionsones
with
integer
spins
are
bosons
(meson,
photon)ones
with
half-integer
spins
are
fermions
(proton,
electroFurther,
bosons
and
fermions
have
quite
different
statisticalproperties.
The
connection
between
spin
and
“statistics”
canbe
proved
in
relativistic
quantum
mechanics;
in
non-relativisttheory
it
must
be
taken
as
an
axiom.if ,
then:two
identical
fermions
(for
example,
two
electrons)
cannotoccupy
the
same
state,
this
is
the
famous
Pauli
ExclusionPrinciple!solidliquidgasplasmaBose-Einstein
condensationthe
fifth
state
of
matterA
more
general
formulation:define
the
exchange
operator,
P:bosonsfermionsFor
stationary
states:5.1.2
Exchange
Forcestwo
distinguishable
particles
in
one-dimensional
motion:two
identical
bosons:two
identical
fermions:How
about
the
expectation
value
of
the
separation
distancebetween
the
two
particles?Case
1:
distinguishable
particles:Case
2:
Identical
particles:Similarly:whereso:Comparing
the
two
cases,
we
have:This
is
called
exchange
forceP.
A.
M.
Dirac,1928T
h
e
s
y
s
t
e
m
b
e
h
a
v
e
s
a
s
t
h
o
u
g
h
t
h
eo
f
a
t
t
r
a
c
t
i
o
n
”
b
e
t
w
e
e
n
i
d
e
n
t
icc
l
o
s
e
r
t
o
g
e
t
h
e
r
,
a
n
d
a
“
f
o
r
c
e
oi
d
e
n
t
i
c
a
l
f
e
r
m
i
o
n
s
,
p
u
s
h
i
n
g
t
ht
h
a
t
w
e
a
r
e
f
o
r
t
h
e
m
o
m
e
n
t
i
g
n
o
r
a
n
e
x
c
h
a
n
g
e
f
o
r
c
e
,
a
l
t
h
o
u
g
h
i
t
’Hydrogen
moleculeCovalent
bonding
requiresthe
singlet
state!5.2
AtomsA
neutral
atom,
of
atomic
number
Z,
its
Hamiltonian
is:kineticpotential
in
nucleus
mutual
repulsionof
electronsSchr?dinger
equation:Solution
is
antisymmetric
with
respect
to
interchange
of
anytwo
electrons,
no
two
electrons
can
occupy
the
same
state:5.2.1
HeliumAfter
hydrogen,
the
simplest
atom
is
helium,
theHamiltonian
is:If
we
simply
ignore
repulsion
of
two
electrons,
the
solutioncan
be
written
as
products
of
hydrogen
wave
functions:The
total
energy
would
be:Then
the
ground
state
energy
is:The
experimentally
determined
energy
is
78.975eVThe
other
excited
states
are
as: ,
there
are
not
doubleexcited
state
for
helium.In
this
case,
we
can
construct
both
symmetric
and
antisymmetriccombinations,
in
the
usual
way:those
go
with
antisymmetric
spin
configuration
are
paraheliumones
go
with
symmetric
spin
configuration
are
orthohelium.The
parahelium
energiesAre
uniformly
higher
thantheir
orthohelium
ones.But
why
there
is
not
1Striplet
state?5.2.2
The
periodic
tableorbital=1
2
3
4
….n-1m=-
-
+1
…..shelln=1
shell
is
called
Kn=2
shell
is
called
Ln=3
shell
is
called
Mn=4
shell
is
called
Nsubshelll=0
is
called
s
(for
“sharp”)l=1
is
called
p
(for
“principle”)l=2
is
called
d
(for
“diffuse”n)ot
listedl=3
is
called
f
(for
“fundamental”)l=4
is
called
g
(out
of
imagination)l=5
is
called
hl=6
is
called
il=7
is
called
kmagneticTotal
angular
momentum
numberTotal
spin
momentum
numberThe
total
orbital
angular
momentum
numberelectronic
configuration:Pauli
exclusion
principle:Hund’s
RulesHund’s
first
rule:
total
spin
SHund’s
second
rule:
total
orbital
angular
momentum
LHund’s
third
rule:
total
momentum
J√ХF.
Hund5.3
SolidsIn
the
solid
state,
outermost
valence
electron
become
detachedand
roam
throughout
the
material.
Two
primitive
models:The
electron
gas
theory:Bloch’s
theory:
Periodic
potential5.3.1
The
Free
Electron
Gas
TheoryS
u
p
p
o
s
e
t
h
e
o
b
j
e
c
ti
n
q
u
e
s
ta
r
e
c
t
a
n
g
u
l
a
r
s
o
l
i
d
,w
i
t
hd
i
m
e
n
s
i
o
n
s
l
x
,
l
y
,
l
z
,
a
n
d
i
mt
h
a
t
a
n
e
l
e
c
t
r
o
n
i
n
s
i
d
ee
x
p
e
r
i
e
n
c
e
s
n
o
f
o
r
c
e
s
a
t
a
le
x
c
e
p
t
a
t
t
h
ei
m
p
e
nA.e
Stomrmearfbelld
e81
nominationsThe
Schrodinger
equation:where
k
is
the
magnitude
of
the
wave
vector,
k=(kx,ky,kz).Boundary
condition:Solution
of
wave
function:The
total
energy:If
you
imagine
a
three-dimensional
space,
with
axes
kx,ky,kz,
aplanes
drawn
in
atspace:(kx,ky,kzo)ne
stationary
statone
state
for
every
blockEach
block
in
this
grid,
and
henceeach
state,
occupies
a
volume
in
k-lxlylzSuppose
our
sample
contains
N
atoms,
and
each
atom
contributes
q
free
electronsAvogadro"s
Constant
=
6.0221415
×
1023
mol-1q
is
small
number:
1
or
2If
electrons
were
bosons
(
or
distinguishable
particles),
they
would
all
settlto
the
ground
state, .
But
electrons
are
in
fact
identical
fermions,
subjethe
Pauli
exclusion
principle,
so
only
two
of
them
can
occupy
any
given
state.They
will
fill
up
one
octant
of
a
sphere
in
k-space,
whose
radius,
kF,
is
determby
the
fact
that
each
pair
of
electrons
requires
a
volume
:Volume
of
k-space:Fermi
surfaceVolume
of
all
electron
require:therefore:where:It
is
free
electron
densityThe
boundary
separating
occupied
and
unoccupied
states,
in
k-space,
is
called
the
Fermi
surface
(hence
the
subscript
F).
Thecorresponding
energy
is
called
the
Fermi
energy,
EF;
for
a
freeelectron
gas:Volume
element
in
k-space:Number
of
states
in
v-element:the
energy
which
each
state
carries
is:the
energy
in
the
volume
element:the
total
energy
is:defining
quantum
pressure
P:Degeneracy
pressurePauli
exclusion
pressureElectron-electron
repulsionThermal
motion5.3.2
Band
StructureThe
periodic
potential
here
determines
thequalitative
behavior
of
solids.
Now
we
developthe
simplest
possible
model:
a
one-dimensionalDirac
comb,
consisting
of
evenly
spaced
deltafunction
spikes.F.
Bloch(1).
Theorem
of
periodic
potential:
Bloch
theoremA
periodic
potential
is
one
that
repeats
itself
aftersome
fixed
distance
a:Let
D
be
the
“displacement”
operator:then
we
are
free
to
choose
eigenfunctions
of
H
that
aresimultaneously
eigenfunctions
of
D:(2).
Band
structureno
real
solid
satisfies
the
condition
of
periodic
potential12N-1However,
for
large
number
ofatoms
containing
in
the
solid,we
can
wrap
the
x-axis
arounda
circle
to
meet
the
periodiccondition
and,
finally,
weimpose
the
following
boundarycondition:12Nthen:Now,
suppose
the
potential
consists
of
a
long
string
ofdelta-function
spikes:In
region
0<x<a
the
potential
is
zero,
sowhere:the
generation
solution:According
to
Bloch’s
theorem,
the
wave
function
in
thecell
immediately
to
the
left
of
the
origin
is:at
x=0,
there
are
two
boundary
condition,
one
is
fromEquation
2.125,
the
other
one
is
continuity:let:The
constant
β
is
a
dimensionless
measure
of
the
“strength”of
the
delta
function.all
values
of
Ka
are
very
closGraph
of
f(z):Graph
of
f(z)
for
β=10,
showing
allowed
bands
(shaded)
separateby
forbidden
gaps
(where
|f(z)|>1).(1)
Electrons
occupation
of
the
band:In
practice
there
will
be
Nq
of
them,
where
q
is
again
the
number
of
“free”
electrons
per
atom.
Because
of
Pauli
exclusion
principle,
only
two
electron
can
occupy
a
given
spatial
state,
so
if
q=1,
they
will
half
fill
the
first
ban
q=2
they
will
completely
fill
the
first
band,
if
q=3
they
half
fill
the
secon
band,
and
so
on——in
the
ground
state.(2)
Conductors,
insulators
and
semiconductorsBand
structure
is
the
signature
of
periodic
potential.If
a
band
is
entirely
filled,
it
takes
a
relatively
large
energy
to
excite
an
electron,
since
it
has
to
jump
across
the
forbidden
zone.
Such
materials
wil
be
electrical
insulators.
On
the
other
hand,
if
a
band
is
only
partly
filled,
takes
very
little
energy
to
excite
an
electron,
and
such
materials
are
typic
conductors.
If
you
dope
an
insulator
with
a
few
atoms
of
larger
or
smaller
q,
this
puts
some
“extra”
electrons
into
the
next
higher
band,
or
creates
som
holes
in
the
previously
filled
one,
allowing
in
either
case
for
weak
electri
currents
to
flow;
such
materials
are
called
semiconductors.5.4
Quantum
Statistical
Mechanics(1).The
fundamental
assumption
of
statistical
mechanicsis
that
in
thermal
equilibrium
every
distinct
state
with
thesame
total
energy,
E,
is
equally
probable!!(2).The
temperature,
T,
is
a
measure
of
the
total
energy
of
asystem
in
thermal
equilibrium
in
classical
mechanics.
Whatis
the
new
in
quantum
mechanics?
How
to
count
the
distinctstates!Problem:
If
we
have
a
large
number
of
N
particles,
inthermal
equilibrium
at
temperature
T
(total
energy
is
E),what
is
the
probability
that
a
particle
would
be
found
tohave
the
specific
energy,
Ej?5.4.1
An
exampleSuppose
we
have
just
have
three
noninteracting
particles,
A,B,
and
C,
(all
of
mass
m)
in
the
one-dimensional
infinitesquare
well.
The
total
energy
is:where
nA,
nB,
and
nC
are
positive
integers.
Now
suppose,
forthe
sake
of
argument,
that
total
energy
is
,which
is
to
say:Then,
there
are
13
combinations
of
three
positive
integers.Thus
(nA,nB,nC
)
can
be
one
of
the
following:configurationnumbercombinations1st1(11,11,11)2nd3(13,13,5),(13,5,13),(5,13,13)3rd3(1,1,19),(19,1,1),(1,19,1)4th6(5,7,17),(5,17,7),(7,5,17)(7,17,5),(17,5,7),(17,7,5)For
example,
(nA,nB,nC
)=(5,7,17)
means
nA=5,
nB=7,
nC=17,If
the
particles
are
distinguishable,
the
three-particle
stateThe
most
important
quantity
is
the
number
of
particles
ineach
state---the
occupation
number,
so
there
are
4configurations:(11,11,11)(13,13,5)(13,5,13)(5,13,13)(1,1,19)(19,1,1)(1,19,1)(5,7,17)(5,17,7)(7,5,17)(7,17,5)(17,5,7)(17,7,5)(1)(3)(3)(6)(1).
Distinguishable
particleIf
the
particles
are
distinguishable,
each
of
these
(nA,nB,nC
)represents
a
distinct
quantum
state,
and
the
fundamentalassumption
of
statistical
mechanics
says
that
in
thermalequilibrium
they
are
all
equally
likely.
Then
what
is
theprobability
(Pn)of
getting
a
specific
(allowed)
energy
En
?(2).
Identical
fermions:For
fermions,
no
two
particles
are
in
thesame
state.
This
antisymmetrizationrequirement
exclude
the
configurationswhere
two
particles
are
in
the
same
state.Only
the
fourth
configuration
isavailable
now!(3).
Identical
bosons:For
bosons,
each
configuration
enables
one
state,
soDiscussion:This
example
shows
that
the
nature
of
the
particlesdetermines
the
counting
properties,
or
the
statisticalproperties!
The
number
of
internal
distinct
states
is
differeand
the
probability
of
getting
specific
energy
is
different
tThis
example
gives
a
system
of
three
particles.
If
thenumber
of
particles
in
huge,
we
can
conclude:
Thedistribution
of
individual
particle
energies,
at
equilibriumsimply
their
distribution
in
the
most
probable
configuration5.4.2
The
General
CaseNow
consider
an
arbitrary
potential,
for
which
one
particleenergies
are:degeneracies
is:Suppose
we
put
N
particles
(all
with
the
same
mass)
intothis
potential;
we
are
interested
in
the
configurationfor
which
there
are
N1
particles
with
energy
E1,
N2
particleswith
energy
E2,
and
so
on.Now
we
consider
general
question:
how
many
distinctstates
correspond
to
this
particular
configuration?The
answer:
The
number
of
the
distinct
states
Q(N1,N2,N3,…)depends
on
whether
the
particles
are
distinguishable,identical
fermions,
or
identical
bosons.(1).
Distinguishable
particles:Choose
N1
from
N
for
energy
bin:
the
binomial
coefficient,
and
then
Arrangement
of
the
N1
particles
within
the
bin
on
the
degenerate
d1
states.
Thus
the
number
of
ways
to
putN1
particles,
selected
from
a
total
population
of
N,
into
a
bin
containing
d1
distinct
option,
is:The
same
goes
for
energy
bin
E2,
of
course,
except
thatthere
are
now
only
N-N1
particles
left
to
work
with:and
so
on,
it
follows:(2).
Identical
fermions:The
particles
are
identical.
The
antisymmetrization
requiresthat
only
one
particle
can
occupy
any
given
state,
so:(3).
Identical
bosons:The
particles
are
identical.
Although
the
wave
function
of
theN-particle
state
is
symmetry,
more
than
one
particles
canoccupy
the
draws
in
certain
bin.Example:
dn=5,
Nn=7Why?5.4.3
The
Most
Probable
ConfigurationIn
thermal
equilibrium,
every
state
with
a
given
totalenergy
E
and
a
given
particle
number
N
is
equally
likely.So
the
most
probable
configuration
(N1,
N2,
N3,
……)
isthe
one
that
particular
configuration
for
whichQ(N1,N2,N3,……..)
is
a
maximum,
subject
to
theconstraints:The
problem
of
maximizing
a
function
F(x1,
x2,
x3,……)
ofseveral
variables,
subject
to
the
constraints
f(x1,
x2,x3,……)=0,
f(x1,
x2,
x3,……)=0,
etc.,
is
most
convenientlyhandled
by
the
method
of
Lagrange
multipliers.
We
introduce
the
new
function:and
set
all
its
derivatives
equal
to
zero:In
our
case
it’s
a
little
easier
to
work
with
the
logarithm
oQ,
instead
of
Q
itself.
So
we
letwhere
α
and
β
are
the
Lagrange
multipliers.
Then:(1).
Distinguishable
particles:Assuming
the
relevant
occupation
numbers
(Nn)
are
large,we
can
invoke
stirling’s
approximation:then:Z=1015.1113.04Z=100364.0360.8Z=100059165912Z=30002103721033....It
follows
that:The
most
probable
occupation
numbers,
for
distinguishableparticles,
are:(
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