Physics:Entropy of entanglement

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Short description: Concept in quantum physics

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.

Mathematically, if a state describing two subsystems A and B |ΨAB=|ϕA|ϕB is a product state, then the reduced density matrix ρA=TrB|ΨABΨAB|=|ϕAϕA| is a pure state. Thus, the entropy of the state is zero; similarly, the density matrix of B would also have zero entropy. If the entropy of the reduced density matrix is nonzero, the reduced density matrix is a mixed state, which indicates that the subsystems A and B are entangled.

Entanglement entropy was first proposed by Sorkin as a source for black hole entropy,[1][2] and remains a candidate.[3] It is thought to have connections to gravity, and the possibility of induced gravity, following the work of Jacobson,[4] and ideas of Sakharov.[5]

Bipartite entanglement entropy

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

Von Neumann entanglement entropy

The bipartite von Neumann entanglement entropy 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 ρAB=|ΨΨ|AB, it is given by:

𝒮(ρA)=Tr[ρAlogρA]=Tr[ρBlogρB]=𝒮(ρB)

where ρA=TrB(ρAB) and ρB=TrA(ρAB) 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 |Ψ=i=1mαi|uiA|viB where |uiA and |viB are orthonormal states in subsystem A and subsystem B respectively. The entropy of entanglement is simply:

iαi2log(αi2)

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 or B subsystem.

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:

Renyi entanglement entropies

The Rényi entanglement entropies 𝒮α are defined in terms of the reduced density matrices and a Rényi index α0. They are given as the Rényi entropy of the reduced density matrices:

𝒮α(ρA)=11αlogtr(ρAα)=𝒮α(ρB)

Note that in the limit α1, the Rényi entanglement entropy approaches the Von Neumann entanglement entropy.

Example with coupled harmonic oscillators

Consider two coupled quantum harmonic oscillators, with positions qA and qB, momenta pA and pB, and system Hamiltonian

H=(pA2+pB2)/2+ω12(qA2+qB2)/2+ω22(qAqB)2/2

With ω±2=ω12+ω22±ω22, the system's pure ground state density matrix is ρAB=|00|, which in position basis is qA,qB|ρAB|qA,qBexp(ω+(qA+qB)2/2ω(qAqB)2/2ω+(q'A+q'B)2/2ω(q'Aq'B)2/2). Then [7]

qA|ρA|qAexp(2(ω+ω)2qAqA(8ω+ω+(ω+ω)2)(qA2+qA'2)8(ω++ω))

Since ρA happens to be precisely equal to the density matrix of a single quantum harmonic oscillator of frequency ωω+ω at thermal equilibrium with temperature T ( such that ω/kBT=cosh1(8ω+ω+(ω+ω)2(ω+ω)2) where kB is the Boltzmann constant), the eigenvalues of ρA are λn=(1eω/kBT)enω/kBT for nonnegative integers n. The Von Neumann Entropy is thus

nλnln(λn)=ω/kBTeω/kBT1ln(1eω/kBT).

Similarly the Renyi entropy Sα(ρA)=(1eω/kBT)α1eαω/kBT/(1α).

Area law of bipartite entanglement entropy

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.[8]

References

  1. Sorkin RD (2014). "1983 paper on entanglement entropy: "On the Entropy of the Vacuum outside a Horizon"". arXiv:1402.3589 [gr-qc].
  2. "Quantum source of entropy for black holes". Physical Review D 34 (2): 373–383. July 1986. doi:10.1103/PhysRevD.34.373. PMID 9957156. Bibcode1986PhRvD..34..373B. 
  3. "Entanglement Entropy of Black Holes". Living Reviews in Relativity 14 (1). December 2011. doi:10.12942/lrr-2011-8. PMID 28179833. Bibcode2011LRR....14....8S. 
  4. "Thermodynamics of spacetime: The Einstein equation of state". Physical Review Letters 75 (7): 1260–1263. August 1995. doi:10.1103/PhysRevLett.75.1260. PMID 10060248. Bibcode1995PhRvL..75.1260J. 
  5. "Vacuum Fluctuations in Curved Space and the Theory of Gravitation.". Doklady Akademii Nauk SSSR 177: 64–66. 1968. doi:10.1142/9789812815941_0006. ISBN 978-981-02-3606-9. https://www.worldscientific.com/doi/abs/10.1142/9789812815941_0006. 
  6. "Robustness of entanglement". Physical Review A 59 (1): 141–155. 1999. doi:10.1103/PhysRevA.59.141. Bibcode1999PhRvA..59..141V. 
  7. "Entropy and area.". Physical Review Letters 71 (5): 666–669. 1993. doi:10.1103/PhysRevLett.71.666. PMID 10055336. Bibcode1993PhRvL..71..666S. 
  8. "Colloquium: Area laws for the entanglement entropy". Reviews of Modern Physics 82 (1): 277–306. February 2010. doi:10.1103/RevModPhys.82.277. Bibcode2010RvMP...82..277E. 

Further reading