Triply efficient shadow tomography
Given copies of a quantum state $\rho$, a shadow tomography protocol aims to learn all expectation values from a fixed set of observables, to within a given precision $\epsilon$. We say that a shadow tomography protocol is triply efficient if it is sample- and time-efficient, and only employs measur...
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Zusammenfassung: | Given copies of a quantum state $\rho$, a shadow tomography protocol aims to
learn all expectation values from a fixed set of observables, to within a given
precision $\epsilon$. We say that a shadow tomography protocol is triply
efficient if it is sample- and time-efficient, and only employs measurements
that entangle a constant number of copies of $\rho$ at a time. The classical
shadows protocol based on random single-copy measurements is triply efficient
for the set of local Pauli observables. This and other protocols based on
random single-copy Clifford measurements can be understood as arising from
fractional colorings of a graph $G$ that encodes the commutation structure of
the set of observables. Here we describe a framework for two-copy shadow
tomography that uses an initial round of Bell measurements to reduce to a
fractional coloring problem in an induced subgraph of $G$ with bounded clique
number. This coloring problem can be addressed using techniques from graph
theory known as chi-boundedness. Using this framework we give the first triply
efficient shadow tomography scheme for the set of local fermionic observables,
which arise in a broad class of interacting fermionic systems in physics and
chemistry. We also give a triply efficient scheme for the set of all $n$-qubit
Pauli observables. Our protocols for these tasks use two-copy measurements,
which is necessary: sample-efficient schemes are provably impossible using only
single-copy measurements. Finally, we give a shadow tomography protocol that
compresses an $n$-qubit quantum state into a $\text{poly}(n)$-sized classical
representation, from which one can extract the expected value of any of the
$4^n$ Pauli observables in $\text{poly}(n)$ time, up to a small constant error. |
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DOI: | 10.48550/arxiv.2404.19211 |