Quantum sensors hold great promise for achieving better sensitivity in the measurement of physical quantities compared to their classical counterparts. However, the conditions under which quantum advantage in sensing can be achieved are rather restrictive, and most quantum enhancements in sensing are lost in the presence of noise, errors, or a poorly calibrated system. To overcome these limitations, we are motivated to import ideas from fault-tolerant quantum computing to quantum sensing. Specifically, we consider a qubit noise model where the probability of phase-flip errors is exponentially smaller (in qubit number) compared to the probability of bit-flip errors that occur with probability
p. For this noise structure, we demonstrate that, given a total sensing time
T, Heisenberg scaling can be attained for times up to
T∝1/p(N+1)/2 for a
N-qubit repetition code, in contrast with
T∝1/p without using a fault-tolerant sensing protocol.
The algorithms discussed in Chapter 21 rely on having isolated systems to store information. In practical applications this is not possible, and the environment interacts with the systems causing decoherence. Suppose the data is contained in the state |x〉, and the environment is described by |E〉. The initial state of the entire system is described by the tensor product of the states |X〉⊗|E〉, which evolves according to some unitary operation U. The state |x〉 evolves according to the unitary operation U x which describes the algorithm. In classical error correction codes, all that needs to be corrected are bit flips (see Chapter 10). In the quantum case errors such as bit flips, phase changes and rotations complicate the error correction techniques. Since arbitrary errors in an encoding of information cannot be corrected, only certain types of errors are assumed to occur (this was also the case in classical error correction, where an upper bound in the number of bits that could be flipped in a transmission was assumed). The types of errors depend on the implementation. For example, suppose the types of errors (which we assume are distinguishable due to an encoding) are described by the unitary basis E 1,...E n , so that all errors are a linear combination [138] E = al.E 1 + ... + a n E n ,...E † E = I.
How much quantum information must a sequential optical test retain, and how reliably must that information survive between source preparations? This paper gives preparation budgets and impossibility bounds that distinguish useful quantum storage from regimes where the classical sample order is unavoidable. Optical source and fully counted memory A fixed unknown normal state supplies independent, identical preparations on
m bosonic modes. The null consists of all pure Gaussian states with total mean photon number at most one. Alternatives have half trace distance at least
1/32 from every pure Gaussian state; neither their energy nor the comparison family's energy is capped. Mixed states and infinite photon tails are included. Each visit accesses one entire original once. The total quantum dimension retained between visits is at most
D, while classical records and computation are unrestricted. At every actual waiting interval, the entire register independently survives unchanged with known probability
a, or is erased with a classical flag. The quantity
ka(D,m) is the smallest deterministic original-preparation cap achieving worst-case error at most
1/3. Failed preparations, discarded trials and reserved positions are all charged. A retained register of
q qubits has
D=2q. An exact threshold for statistical advantage Without retained quantum information, the optimal sample order is
Θ(m). Along arbitrary growing-mode sequences, the precise criterion for improving that order is
ka(D,m)=o(m)⟺am→∞ and maD→∞. The two conditions express separate capacity and survival requirements. Arbitrarily large storage cannot reduce the linear sample order when
a=O(1/m), yet a survival probability tending to zero can still permit an advantage. Let
A=max{1,m2/D}. At the fixed energy and separation above, constants
c,C>0, independent of
m,D,a, give
cmin{m,A/a}≤ka(D,m)≤Cmin{m,A/a+min(a−2,m2/3)},0<a≤1. At
a=0, the sample cost is
Θ(m). For ideal memory the complete rate is
k1(D,m)=Θ(min{m,max(1,m2/D)}). With loss, the bounds match whenever
A≥min{a−1,am2/3}. For example,
a=m−1/6 and
D=⌈m11/6⌉ give
Θ(m1/3) preparations. The existence of sublinear advantage is fully characterized even where its optimal exponent remains bracketed: for
D≥m2,
a=m−1/2, the stated bounds are
Ω(m1/2) and
O(m2/3). Why the construction and converse fit the same resources A physical completely positive contraction combines first- and second-moment information before the next wait. Although the temporary pair output has order
m2 labels, only a positive register of dimension
m+1 is retained. The three-visit route requires
D≥m+1 and pays two actual survival events; a classical alternative handles the centering statistics. The converse covers arbitrary adaptive instruments and persistent noncommuting memory. Erasure removes the coherent prediction contribution while preserving information already learned in the full classical history. Unflagged noise and applicability For a fixed memoryless channel on the entire retained register with a physical reset decomposition
N=aΨ+(1−a)Rτ, where
Ψ is CPTP and
Rτ(X)=Tr(X)τ, an exact flagged-erasure simulation gives
kN(D,m)≥ka(D,m). The established positive quantum Doeblin coefficient optimizes this lower obstruction. Whole-register depolarizing noise with unchanged fraction
1−q=O(1/m) therefore forces
Θ(m) samples for every memory dimension. General unflagged noise inherits a converse, not the flagged model's complete achievability guarantees. The results quantify asymptotic preparation and persistent-memory resources under ideal visit-local control. Temporary auxiliary systems and gate complexity have no imposed budget, and the explicit sufficient finite-sample constants are conservative. The task is pure Gaussianity testing, rather than membership in the full family of mixed Gaussian states. The single integrated PDF contains the short main text, full proofs, four figures and precise resource accounting.
How long quantum information survives can matter more than how many samples a receiver processes at once. We establish this distinction for detecting optical squeezing with an unknown source and noisy direction records. At fixed five-percent errors, mean input photon number at most 0.006 and transmissivity in [0.1, 0.2], a receiver with a fixed-width persistent register attains weak-signal sample coefficient 7.35. Arbitrary adaptive receivers that erase all quantum information between blocks sublinear in the total sample budget require at least 7.7216; one-copy measurements with unlimited classical feedback require at least 10.3. The separation persists for a disclosed Gaussian thermal source: the reset-block lower bound is 7.5486, still above the persistent construction. Source uncertainty is governed by a separate exact energy boundary. With noisy direction records, coherence and excess photon population together determine a matched sample-order law. The constructive receiver has 4096 active memory levels, a deterministic non-Gaussian interface, and explicit trial and cumulative memory-noise budgets. Thus growing temporary measurement blocks cannot replace persistent quantum storage at the demonstrated detection cost. The results specify when control records are essential and when receiver design must preserve quantum information across a macroscopic fraction of the acquisition.