- Source: Laughlin wavefunction
In condensed matter physics, the Laughlin wavefunction is an ansatz, proposed by Robert Laughlin for the ground state of a two-dimensional electron gas placed in a uniform background magnetic field in the presence of a uniform jellium background when the filling factor of the lowest Landau level is
ν
=
1
/
n
{\displaystyle \nu =1/n}
where
n
{\displaystyle n}
is an odd positive integer. It was constructed to explain the observation of the
ν
=
1
/
3
{\displaystyle \nu =1/3}
fractional quantum Hall effect (FQHE), and predicted the existence of additional
ν
=
1
/
n
{\displaystyle \nu =1/n}
states as well as quasiparticle excitations with fractional electric charge
e
/
n
{\displaystyle e/n}
, both of which were later experimentally observed. Laughlin received one third of the Nobel Prize in Physics in 1998 for this discovery.
Context and analytical expression
If we ignore the jellium and mutual Coulomb repulsion between the electrons as a zeroth order approximation, we have an infinitely degenerate lowest Landau level (LLL) and with a filling factor of 1/n, we'd expect that all of the electrons would lie in the LLL. Turning on the interactions, we can make the approximation that all of the electrons lie in the LLL. If
ψ
0
{\displaystyle \psi _{0}}
is the single particle wavefunction of the LLL state with the lowest orbital angular momenta, then the Laughlin ansatz for the multiparticle wavefunction is
⟨
z
1
,
z
2
,
z
3
,
…
,
z
N
∣
n
,
N
⟩
=
ψ
n
,
N
(
z
1
,
z
2
,
z
3
,
…
,
z
N
)
=
D
[
∏
N
⩾
i
>
j
⩾
1
(
z
i
−
z
j
)
n
]
∏
k
=
1
N
exp
(
−
∣
z
k
∣
2
)
{\displaystyle \langle z_{1},z_{2},z_{3},\ldots ,z_{N}\mid n,N\rangle =\psi _{n,N}(z_{1},z_{2},z_{3},\ldots ,z_{N})=D\left[\prod _{N\geqslant i>j\geqslant 1}\left(z_{i}-z_{j}\right)^{n}\right]\prod _{k=1}^{N}\exp \left(-\mid z_{k}\mid ^{2}\right)}
where position is denoted by
z
=
1
2
l
B
(
x
+
i
y
)
{\displaystyle z={1 \over 2{\mathit {l}}_{B}}\left(x+iy\right)}
in (Gaussian units)
l
B
=
ℏ
c
e
B
{\displaystyle {\mathit {l}}_{B}={\sqrt {\hbar c \over eB}}}
and
x
{\displaystyle x}
and
y
{\displaystyle y}
are coordinates in the x–y plane. Here
ℏ
{\displaystyle \hbar }
is the reduced Planck constant,
e
{\displaystyle e}
is the electron charge,
N
{\displaystyle N}
is the total number of particles, and
B
{\displaystyle B}
is the magnetic field, which is perpendicular to the xy plane. The subscripts on z identify the particle. In order for the wavefunction to describe fermions, n must be an odd integer. This forces the wavefunction to be antisymmetric under particle interchange. The angular momentum for this state is
n
ℏ
{\displaystyle n\hbar }
.
True ground state in FQHE at ν = 1/3
Consider
n
=
3
{\displaystyle n=3}
above: resultant
Ψ
L
(
z
1
,
z
2
,
z
3
,
…
,
z
N
)
∝
Π
i
<
j
(
z
i
−
z
j
)
3
{\displaystyle \Psi _{L}(z_{1},z_{2},z_{3},\ldots ,z_{N})\propto \Pi _{i
is a trial wavefunction; it is not exact, but qualitatively, it reproduces many features of the exact solution and quantitatively, it has very high
overlaps with the exact ground state for small systems. Assuming Coulomb repulsion between any two electrons, that
ground state
Ψ
E
D
{\displaystyle \Psi _{ED}}
can be determined using exact diagonalisation and the
overlaps have been calculated to be close to one. Moreover, with short-range interaction (Haldane pseudopotentials for
m
>
3
{\displaystyle m>3}
set to zero),
Laughlin wavefunction becomes exact,
i.e.
⟨
Ψ
E
D
|
Ψ
L
⟩
=
1
{\displaystyle \langle \Psi _{ED}|\Psi _{L}\rangle =1}
.
Energy of interaction for two particles
The Laughlin wavefunction is the multiparticle wavefunction for quasiparticles. The expectation value of the interaction energy for a pair of quasiparticles is
⟨
V
⟩
=
⟨
n
,
N
∣
V
∣
n
,
N
⟩
,
N
=
2
{\displaystyle \langle V\rangle =\langle n,N\mid V\mid n,N\rangle ,\;\;\;N=2}
where the screened potential is (see Static forces and virtual-particle exchange § Coulomb potential between two current loops embedded in a magnetic field)
V
(
r
12
)
=
(
2
e
2
L
B
)
∫
0
∞
k
d
k
k
2
+
k
B
2
r
B
2
M
(
l
+
1
,
1
,
−
k
2
4
)
M
(
l
′
+
1
,
1
,
−
k
2
4
)
J
0
(
k
r
12
r
B
)
{\displaystyle V\left(r_{12}\right)=\left({2e^{2} \over L_{B}}\right)\int _{0}^{\infty }{{k\;dk\;} \over k^{2}+k_{B}^{2}r_{B}^{2}}\;M\left({\mathit {l}}+1,1,-{k^{2} \over 4}\right)\;M\left({\mathit {l}}^{\prime }+1,1,-{k^{2} \over 4}\right)\;{\mathcal {J}}_{0}\left(k{r_{12} \over r_{B}}\right)}
where
M
{\displaystyle M}
is a confluent hypergeometric function and
J
0
{\displaystyle {\mathcal {J}}_{0}}
is a Bessel function of the first kind. Here,
r
12
{\displaystyle r_{12}}
is the distance between the centers of two current loops,
e
{\displaystyle e}
is the magnitude of the electron charge,
r
B
=
2
l
B
{\displaystyle r_{B}={\sqrt {2}}{\mathit {l}}_{B}}
is the quantum version of the Larmor radius, and
L
B
{\displaystyle L_{B}}
is the thickness of the electron gas in the direction of the magnetic field. The angular momenta of the two individual current loops are
l
ℏ
{\displaystyle {\mathit {l}}\hbar }
and
l
′
ℏ
{\displaystyle {\mathit {l}}^{\prime }\hbar }
where
l
+
l
′
=
n
{\displaystyle {\mathit {l}}+{\mathit {l}}^{\prime }=n}
. The inverse screening length is given by (Gaussian units)
k
B
2
=
4
π
e
2
ℏ
ω
c
A
L
B
{\displaystyle k_{B}^{2}={4\pi e^{2} \over \hbar \omega _{c}AL_{B}}}
where
ω
c
{\displaystyle \omega _{c}}
is the cyclotron frequency, and
A
{\displaystyle A}
is the area of the electron gas in the xy plane.
The interaction energy evaluates to:
To obtain this result we have made the change of integration variables
u
12
=
z
1
−
z
2
2
{\displaystyle u_{12}={z_{1}-z_{2} \over {\sqrt {2}}}}
and
v
12
=
z
1
+
z
2
2
{\displaystyle v_{12}={z_{1}+z_{2} \over {\sqrt {2}}}}
and noted (see Common integrals in quantum field theory)
1
(
2
π
)
2
2
2
n
n
!
∫
d
2
z
1
d
2
z
2
∣
z
1
−
z
2
∣
2
n
exp
[
−
2
(
∣
z
1
∣
2
+
∣
z
2
∣
2
)
]
J
0
(
2
k
∣
z
1
−
z
2
∣
)
=
{\displaystyle {1 \over \left(2\pi \right)^{2}\;2^{2n}\;n!}\int d^{2}z_{1}\;d^{2}z_{2}\;\mid z_{1}-z_{2}\mid ^{2n}\;\exp \left[-2\left(\mid z_{1}\mid ^{2}+\mid z_{2}\mid ^{2}\right)\right]\;{\mathcal {J}}_{0}\left({\sqrt {2}}\;{k\mid z_{1}-z_{2}\mid }\right)=}
1
(
2
π
)
2
2
n
n
!
∫
d
2
u
12
d
2
v
12
∣
u
12
∣
2
n
exp
[
−
2
(
∣
u
12
∣
2
+
∣
v
12
∣
2
)
]
J
0
(
2
k
∣
u
12
∣
)
=
{\displaystyle {1 \over \left(2\pi \right)^{2}\;2^{n}\;n!}\int d^{2}u_{12}\;d^{2}v_{12}\;\mid u_{12}\mid ^{2n}\;\exp \left[-2\left(\mid u_{12}\mid ^{2}+\mid v_{12}\mid ^{2}\right)\right]\;{\mathcal {J}}_{0}\left({2}k\mid u_{12}\mid \right)=}
M
(
n
+
1
,
1
,
−
k
2
2
)
.
{\displaystyle M\left(n+1,1,-{k^{2} \over 2}\right).}
The interaction energy has minima for (Figure 1)
l
n
=
1
3
,
2
5
,
3
7
,
etc.,
{\displaystyle {{\mathit {l}} \over n}={1 \over 3},{2 \over 5},{3 \over 7},{\mbox{etc.,}}}
and
l
n
=
2
3
,
3
5
,
4
7
,
etc.
{\displaystyle {{\mathit {l}} \over n}={2 \over 3},{3 \over 5},{4 \over 7},{\mbox{etc.}}}
For these values of the ratio of angular momenta, the energy is plotted in Figure 2 as a function of
n
{\displaystyle n}
.
References
See also
Landau level
Fractional quantum Hall effect
Coulomb potential between two current loops embedded in a magnetic field
Kata Kunci Pencarian:
- Laughlin wavefunction
- Laughlin
- Robert B. Laughlin
- Landau levels
- Vandermonde matrix
- Fractional quantum Hall effect
- Condensed matter physics
- Composite fermion
- Static forces and virtual-particle exchange
- Index of physics articles (L)
