Here is a new representation of the Euler ensemble, leading us to the exact analytic solution below.
We start by replacing independent random variables \( \sigma \) with fixed sum by a Markov process, as suggested in [1]. We start with \( n \) random values of \( \sigma_i = 1 \) and the remaining \( N-n \) values of \( \sigma_i = -1 \). Instead of averaging over all of these values simultaneously, we follow a Markov process of picking \( \sigma_N,\dots, \sigma_1 \) one after another. At each step there will be \( M = N, \dots, 0 \) remaining \( \sigma \). We get a transition \[ n \Rightarrow n-1 \quad \text{with probability } \frac{n}{M} \] and \[ n \Rightarrow n \quad \text{with the complementary probability.} \]
Multiplying these probabilities and summing all histories of the Markov process is equivalent to the computation of the product of the Markov matrices:
This Markov process will be random until \( n=0 \). After that, all remaining \( \sigma_k \) will have negative signs and be taken with probability 1, keeping \( n=0 \).
The expectation value of some function \( \hat{X}(\{\sigma\}) \) reduces to the matrix product
Here \( N_+ = \frac{N + \sum \sigma_l}{2} = \frac{N+qr}{2} \) is the number of positive sigmas. The operator \( \hat{Q}(M) \) sets in \( \hat{X}\lvert n\rangle \) the variable \( \sigma_{M} \) to 1 with probability \( \frac{n}{M} \) and to \(-1\) with complementary probability. The generalization of the Markov matrix \( Q(M) \) to the operator \( \hat{Q}(M) \) will be presented shortly.
Once the whole product is applied to \( \hat{X} \), all the sigma variables in all terms will be specified so that the result is a number.
This Markov process is implemented as a computer code in [2], leading to a fast simulation with \( O(N^0) \) memory requirement.
Now, we observe that quantum Fermi statistics can represent the Markov chain of Ising variables. Let us construct the operator \( \hat{Q}(M) \) with Fermionic creation and annihilation operators, with occupation numbers \[ \nu_k = \frac{1+\sigma_k}{2} = (0,1). \] These operators obey (anti)commutation relations and create/annihilate the \( \sigma=1 \) state as follows (with Kronecker delta \( \delta[n] \equiv \delta_{n,0} \)):
The number \( n(M) \) of positive sigmas, \[ \sum_{l=1}^M \delta[\sigma_l-1], \] coincides with the occupation number of these Fermi particles:
This relation leads to the representation
The variables \( \sigma_l \) can also be expressed in terms of this operator algebra by using
The Wilson loop in \(\eqref{WilsonLoop}\) can now be represented as an average over the small Euler ensemble \( \mathcal{E}(N) \) of a quantum trace expression:
The last component of the vector \( \vec{\mathcal F}_l \) is set to 0 as this component does not depend on \( l \) and yields zero in the sum over the loop \( \sum_l \Delta\vec{C}_l = 0 \).
The proof of equivalence to the combinatorial formula with an average over \( \sigma_l=\pm 1 \) can be given using the following Lemma (obvious for a physicist).
Interchanging indices \( l, n \) shows that both terms are symmetric; hence, \[ \hat{\nu}_l\,\hat{\nu}_n = \hat{\nu}_n\,\hat{\nu}_l. \]
Theorem. The trace formula \(\eqref{trace formula}\) equals the expectation value of the momentum loop ansatz \(\eqref{LoopSol}\), \(\eqref{PFT}\), \(\eqref{Fsol}\) in the big Euler ensemble.
Proof. As all the operators \( \hat{\nu}_l \) commute with each other, the operators \( \hat{Q}(M) \) can be applied in arbitrary order to the states \( \Sigma = \lvert \sigma_1,\dots,\sigma_N \rangle \) involved in the trace. The same is true for individual terms in the circulation in the exponential of the Wilson loop. These terms \( \vec{\mathcal F}_l \) involve the operators \( \hat{\alpha}_l \), which commute with each other and with each \( \hat{Q}(M) \). Thus, we can use the ordered product \[ \hat{G}_l = \hat{Q}(l)\exp\Bigl(i\omega\hat{\sigma}_l + \frac{i\gamma}{\nu}\Delta\vec{C}_l\cdot\vec{\mathcal P}_l(t)\Bigr). \] Each operator \( \hat{G}_l \) acting on an arbitrary state \( \Sigma \) will create two terms with \( \delta[\sigma_l \pm 1] \). The product \(\hat{Z}_l = \prod_{k=1}^l \hat{G}_k\) then produces \( 2^l \) terms in which each \( \sigma_k \) (for \( k\le l \)) is fixed by the Kronecker deltas. Multiplying all the operators \( \hat{G}_M \) yields a superposition \( \hat{\Pi}_N \) of \( 2^N \) terms, each with \( \prod_{M=1}^{N} \delta[\sigma_M-\eta_M] \) for various choices of signs \( \eta_i=\pm 1 \). The product of these deltas projects the total sum over the \( 2^N \) combinations in the trace to a single term corresponding to a particular history \( (\eta_1,\dots,\eta_N) \) of the Markov process. Multiplying by the Markov transition probabilities and by the exponential \[ \exp\Bigl(\frac{i\gamma}{\nu}\sum_l\Delta\vec{C}_l\cdot\hat{\Omega}\cdot\vec{P}_l(t)\Bigr), \] with the operators \( \hat{\sigma} \) replaced by the numbers \( \eta \), reproduces the usual numeric result. Finally, integration over \( \omega \) produces a delta function \[ \delta\Bigl[\sum_l \eta_l - s\Bigr], \] which reduces the trace to the required sum over all histories of the Markov process with fixed \( \sum_l \eta_l \). \(\blacksquare\)
We have found a third vertex of the triangle of equivalent theories: decaying turbulence in three-dimensional space, the fractal curve in complex space, and Fermi particles on a ring. By degrees of freedom, this corresponds to a one-dimensional Fermi gas in the statistical limit \( N\to\infty \). However, there is no local Hamiltonian in this quantum partition function --- only a trace of certain products of operators in Fock space. Thus, an algebraic (or quantum statistical) problem remains: to find the continuum limit of this theory of the Fermion ring.