The entropy of entanglement (or entanglement entropy) is a measure of the degree of quantum entanglement between two subsystems constituting a two-part composite quantum system. Given a pure bipartite quantum state of the composite system, it is possible to obtain a reduced density matrix describing knowledge of the state of a subsystem. The entropy of entanglement is the Von Neumann entropy of the reduced density matrix for any of the subsystems. If it is non-zero, it indicates the two subsystems are entangled.
More mathematically; if a state describing two subsystems A and B
|\PsiAB\rangle=|\phiA\rangle|\phiB\rangle
\rhoA=\operatorname{Tr}B|\PsiAB\rangle\langle\PsiAB|=|\phiA\rangle\langle\phiA|
Suppose that a quantum system consists of
N
A
B
k
l
k+l=N
The bipartite von Neumann entanglement entropy
S
\rhoAB=|\Psi\rangle\langle\Psi|AB
l{S}(\rhoA)=-\operatorname{Tr}[\rhoA\operatorname{log}\rhoA]=-\operatorname{Tr}[\rhoB\operatorname{log}\rhoB]=l{S}(\rhoB)
where
\rhoA=\operatorname{Tr}B(\rhoAB)
\rhoB=\operatorname{Tr}A(\rhoAB)
The entanglement entropy can be expressed using the singular values of the Schmidt decomposition of the state. Any pure state can be written as
|\Psi\rangle=\sumim\alphai|ui\rangleA ⊗ |vi\rangleB
|ui\rangleA
|vi\rangleB
A
B
This form of writing the entropy makes it explicitly clear that the entanglement entropy is the same regardless of whether one computes partial trace over the
A
B
Many entanglement measures reduce to the entropy of entanglement when evaluated on pure states. Among those are:
Some entanglement measures that do not reduce to the entropy of entanglement are:
The Renyi entanglement entropies
l{S}\alpha
\alpha\geq0
l{S}\alpha(\rhoA)=
1 | |
1-\alpha |
\operatorname{log}\operatorname{tr}
\alpha) | |
(\rho | |
A |
=l{S}\alpha(\rhoB)
Note that in the limit
\alpha → 1
Consider two coupled quantum harmonic oscillators, with positions
qA
qB
pA
pB
2 | |
H=(p | |
A |
+
2)/2 | |
p | |
B |
+
2 | |
\omega | |
1 |
(
2 | |
q | |
A |
+
2)/{2} | |
q | |
B |
+{
2 | |
\omega | |
2 |
(qA-
2}/{2} | |
q | |
B) |
With
2 | |
\omega | |
\pm |
=
2 | |
\omega | |
1 |
+
2 | |
\omega | |
2 |
\pm
2 | |
\omega | |
2 |
\rhoAB=|0\rangle\langle0|
\langleqA,qB|\rhoAB|qA',qB'\rangle\propto\exp\left(-{\omega+(qA+
2}/{2} | |
q | |
B) |
-{\omega-(qA-
2}/{2} | |
q | |
B) |
-{\omega+(q'A+
2}/{2} | |
q' | |
B) |
-{\omega-(q'A-
2}/{2} | |
q' | |
B) |
\right)
\langleqA|\rhoA|qA'\rangle\propto\exp\left(
| |||||||||||||||||||
8(\omega++\omega-) |
\right)
Since
\rhoA
\omega\equiv\sqrt{\omega+\omega-}
T
\omega/kBT=\cosh-1\left(
| |||||||||||||
|
\right)
kB
\rhoA
λn=
-\omega/kBT | |
(1-e |
-n\omega/kBT | |
)e |
n
-\sumnλnln(λn)=
\omega/kBT | ||||||
|
-
-\omega/kBT | |
ln(1-e |
)
Similarly the Renyi entropy
S\alpha(\rhoA)=
| |||||||
|
/(1-\alpha)
A quantum state satisfies an area law if the leading term of the entanglement entropy grows at most proportionally with the boundary between the two partitions.Area laws are remarkably common for ground states of local gapped quantum many-body systems. This has important applications, one such application being that it greatly reduces the complexity of quantum many-body systems. The density matrix renormalization group and matrix product states, for example, implicitly rely on such area laws.[3]