We study gap amplification of the class
QMA+(2) characterized by unentangled quantum proofs whose amplitudes are nonnegative in the computational basis. This class was recently introduced by Jeronimo and Wu (STOC 2023), and its behavior depends sharply on the completeness-soundness gap: although it captures the power of
NEXP for some small constant gap, it is equal to
QMA(2) for larger constant gap. This is in stark contrast to
QMA(2) where strong gap amplification is known due to the product test by Harrow and Montanaro (FOCS 2010, JACM 2013).
In this paper, we prove for every completeness
c and soundness
s with
c−s=1/poly(n),
NEXP=QMA+(2,c,s)=QMA+(2,1−poly(n)1,41+poly(n)1). Our result gives a clean complexity phase transition for
QMA+(2) since we have
QMAR(2)=QMA+(2,1−poly(n)1,41−poly(n)1), where
QMAR(2) denotes
QMA(2) with witnesses restricted to real amplitudes. Our amplification is thus optimal in the sense that a slight improvement of our soundness would have the collapse
QMAR(2)=NEXP.
Our proof combines symmetric-subspace projections with the relation
QMA+(1)=NEXP of Bassirian, Fefferman, and Marwaha (ITCS 2024). The main technical ingredient is a dimension-independent de Finetti theorem in Hilbert-Schmidt norm that applies when the number of registers under consideration grows logarithmically.
We study a variant of QMA where quantum proofs have no relative phase (i.e. non-negative amplitudes, up to a global phase). If only completeness is modified, this class is equal to QMA [arXiv:1410.2882]; but if both completeness and soundness are modified, the class (named QMA+ by Jeronimo and Wu) can be much more powerful. We show that QMA+ with some constant gap is equal to NEXP, yet QMA+ with some *other* constant gap is equal to QMA. One interpretation is that Merlin's ability to "deceive" originates from relative phase at least as much as from entanglement, since QMA(2)
⊆ NEXP.
We find a modification to QMA where having one quantum proof is strictly less powerful than having two unentangled proofs, assuming EXP
= NEXP. This gives a new route to prove QMA(2) = NEXP that overcomes the primary drawback of a recent approach [arXiv:2402.18790 , arXiv:2306.13247] (QIP 2024). Our modification endows each proof with a form of *multipartite* unentanglement: after tracing out one register, a small number of qubits are separable from the rest of the state.
We study the limitations of black-box amplification in the quantum complexity class Q M A . Amplification is known to boost any inverse-polynomial gap between completeness and soundness to exponentially small error, and a recent result (Jeffery and Witteveen, 2025) shows that completeness can in fact be amplified to be doubly exponentially close to 1. We prove that this is optimal for black-box procedures: we provide a quantum oracle relative to which no Q M A verification procedure using polynomial resources can achieve completeness closer to 1 than doubly exponential, or a soundness which is super-exponentially small. This is proven by making the oracle separation from (Aaronson, 2009) between Q M A and Q M A 1 quantitative, using techniques from complex approximation theory.
We consider restricted versions of
postBQP where postselection probabilities can be efficiently calculated by classical or quantum computers. We show that such restricted
postBQP classes are in
AWPP(⊆PP=postBQP). This result suggests that postselecting an event with an exponentially small probability does not necessarily boost
BQP to PP. The best upperbound of
BQP is
AWPP, and therefore restricted
postBQP classes are other examples of complexity classes slightly above
BQP. In [C. M. Lee and J. Barrett, arXiv:1412.8671], it was shown that the computational capacity of a general probabilistic theory which satisfies the tomographic locality is in
AWPP. Our result therefore implies that quantum physics with restricted postselections is an example of a super quantum theory which seems to be outside of their general probabilistic theory but its computational capacity is also in
AWPP. Although it is physically natural to expect that such restricted
postBQP classes are not equivalent to BQP, we show that
UP∩coUP, which is unlikely to be in BQP, is contained in the restricted
postBQP classes. Finally, we also consider another restricted class of
postBQP, where the postselected probability depends only on the size of inputs. We show that this restricted version is contained in
APP, where
AWPP⊆APP⊆PP=postBQP.