Suppose that a quantum system consists of ${\displaystyle N}$ particles. A bipartition of the system is a partition which divides the system into two parts ${\displaystyle A}$  and ${\displaystyle B}$ , containing ${\displaystyle k}$  and ${\displaystyle l}$  particles respectively with ${\displaystyle k+l=N}$ . Bipartite entanglement entropy is defined with respect to this bipartition.

Von Neumann entanglement entropy edit

The bipartite von Neumann entanglement entropy ${\displaystyle S}$  is defined as the von Neumann entropy of either of its reduced states, since they are of the same value (can be proved from Schmidt decomposition of the state with respect to the bipartition); the result is independent of which one we pick. That is, for a pure state ${\displaystyle \rho _{AB}=|\Psi \rangle \langle \Psi |_{AB}}$ , it is given by:

${\displaystyle {\mathcal {S}}(\rho _{A})=-\operatorname {Tr} [\rho _{A}\operatorname {log} \rho _{A}]=-\operatorname {Tr} [\rho _{B}\operatorname {log} \rho _{B}]={\mathcal {S}}(\rho _{B})}$ 

where ${\displaystyle \rho _{A}=\operatorname {Tr} _{B}(\rho _{AB})}$  and ${\displaystyle \rho _{B}=\operatorname {Tr} _{A}(\rho _{AB})}$  are the reduced density matrices for each partition.

The entanglement entropy can be expressed using the singular values of the Schmidt decomposition of the state. Any pure state can be written as ${\displaystyle |\Psi \rangle =\sum _{i=1}^{m}\alpha _{i}|u_{i}\rangle _{A}\otimes |v_{i}\rangle _{B}}$  where ${\displaystyle |u_{i}\rangle _{A}}$  and ${\displaystyle |v_{i}\rangle _{B}}$  are orthonormal states in subsystem ${\displaystyle A}$  and subsystem ${\displaystyle B}$  respectively. The entropy of entanglement is simply:

${\textstyle -\sum _{i}\alpha _{i}^{2}\log(\alpha _{i}^{2})}$ 

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 ${\displaystyle A}$  or ${\displaystyle B}$  subsystem.

Many entanglement measures reduce to the entropy of entanglement when evaluated on pure states. Among those are:

• Distillable entanglement
• Entanglement cost
• Entanglement of formation
• Relative entropy of entanglement
• Squashed entanglement

Some entanglement measures that do not reduce to the entropy of entanglement are:

• Negativity
• Logarithmic negativity
• Robustness of entanglement^[1]

Renyi entanglement entropies edit

The Renyi entanglement entropies ${\displaystyle {\mathcal {S}}_{\alpha }}$  are also defined in terms of the reduced density matrices, and a Renyi index ${\displaystyle \alpha \geq 0}$ . It is defined as the Rényi entropy of the reduced density matrices:

${\displaystyle {\mathcal {S}}_{\alpha }(\rho _{A})={\frac {1}{1-\alpha }}\operatorname {log} \operatorname {tr} (\rho _{A}^{\alpha })={\mathcal {S}}_{\alpha }(\rho _{B})}$ 

Note that in the limit ${\displaystyle \alpha \rightarrow 1}$ , The Renyi entanglement entropy approaches the Von Neumann entanglement entropy.

Consider two coupled quantum harmonic oscillators, with positions ${\displaystyle q_{A}}$  and ${\displaystyle q_{B}}$ , momenta ${\displaystyle p_{A}}$  and ${\displaystyle p_{B}}$ , and system Hamiltonian

${\displaystyle H=(p_{A}^{2}+p_{B}^{2})/2+\omega _{1}^{2}(q_{A}^{2}+q_{B}^{2})/{2}+{\omega _{2}^{2}(q_{A}-q_{B})^{2}}/{2}}$ 

With ${\displaystyle \omega _{\pm }^{2}=\omega _{1}^{2}+\omega _{2}^{2}\pm \omega _{2}^{2}}$ , the system's pure ground state density matrix is ${\displaystyle \rho _{AB}=|0\rangle \langle 0|}$ , which in position basis is ${\displaystyle \langle q_{A},q_{B}|\rho _{AB}|q_{A}',q_{B}'\rangle \propto \exp \left(-{\omega _{+}(q_{A}+q_{B})^{2}}/{2}-{\omega _{-}(q_{A}-q_{B})^{2}}/{2}-{\omega _{+}(q'_{A}+q'_{B})^{2}}/{2}-{\omega _{-}(q'_{A}-q'_{B})^{2}}/{2}\right)}$ . Then ^[2]

${\displaystyle \langle q_{A}|\rho _{A}|q_{A}'\rangle \propto \exp \left({\frac {2(\omega _{+}-\omega _{-})^{2}q_{A}q_{A}'-(8\omega _{+}\omega _{-}+(\omega _{+}-\omega _{-})^{2})(q_{A}^{2}+q_{A}'^{2})}{8(\omega _{+}+\omega _{-})}}\right)}$ 

Since ${\displaystyle \rho _{A}}$  happens to be precisely equal to the density matrix of a single quantum harmonic oscillator of frequency ${\displaystyle \omega \equiv {\sqrt {\omega _{+}\omega _{-}}}}$  at thermal equilibrium with temperature ${\displaystyle T}$  ( such that ${\displaystyle \omega /k_{B}T=\cosh ^{-1}\left({\frac {8\omega _{+}\omega _{-}+(\omega _{+}-\omega _{-})^{2}}{(\omega _{+}-\omega _{-})^{2}}}\right)}$  where ${\displaystyle k_{B}}$  is the Boltzmann constant), the eigenvalues of ${\displaystyle \rho _{A}}$  are ${\displaystyle \lambda _{n}=(1-e^{-\omega /k_{B}T})e^{-n\omega /k_{B}T}}$  for nonnegative integers ${\displaystyle n}$ . The Von Neumann Entropy is thus

${\displaystyle -\sum _{n}\lambda _{n}\ln(\lambda _{n})={\frac {\omega /k_{B}T}{e^{\omega /k_{B}T}-1}}-\ln(1-e^{-\omega /k_{B}T})}$ .

Similarly the Renyi entropy ${\displaystyle S_{\alpha }(\rho _{A})={\frac {(1-e^{-\omega /k_{B}T})^{\alpha }}{1-e^{-\alpha \omega /k_{B}T}}}/(1-\alpha )}$ .

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]

• Janzing, Dominik (2009). "Entropy of Entanglement". In Greenberger, Daniel; Hentschel, Klaus; Weinert, Friedel (eds.). Compendium of Quantum Physics. Springer. pp. 205–209. doi:10.1007/978-3-540-70626-7_66. ISBN 978-3-540-70626-7.