Knysh Sergey, Smelyanskiy Vadim N
ELORET Corporation, NASA Ames Research Center, MS 229-1, Moffett Field, California 94035-1000, USA.
Phys Rev E Stat Nonlin Soft Matter Phys. 2008 Dec;78(6 Pt 1):061128. doi: 10.1103/PhysRevE.78.061128. Epub 2008 Dec 24.
We study the quantum version of the random K -satisfiability problem in the presence of an external magnetic field Gamma applied in the transverse direction. We derive the replica-symmetric free-energy functional within the static approximation and the saddle-point equation for the order parameter: the distribution P[h(m)] of functions of magnetizations. The order parameter is interpreted as the histogram of probability distributions of individual magnetizations. In the limit of zero temperature and small transverse fields, to leading order in Gamma magnetizations m approximately 0 become relevant in addition to purely classical values of m approximately +/-1 . Self-consistency equations for the order parameter are solved numerically using a quasi-Monte Carlo method for K=3 . It is shown that for an arbitrarily small Gamma quantum fluctuations destroy the phase transition present in the classical limit Gamma=0 , replacing it with a smooth crossover transition. The implications of this result with respect to the expected performance of quantum optimization algorithms via adiabatic evolution are discussed. The replica-symmetric solution of the classical random K -satisfiability problem is briefly reexamined. It is shown that the phase transition at T=0 predicted by the replica-symmetric theory is of continuous type with atypical critical exponents.
我们研究了在横向施加外磁场Γ的情况下随机K -可满足性问题的量子版本。我们在静态近似下推导了复制对称自由能泛函以及序参量的鞍点方程:磁化强度函数的分布P[h(m)]。序参量被解释为各个磁化强度概率分布的直方图。在零温度和小横向场的极限下,除了m约为±1的纯经典值外,m约为0的磁化强度在Γ的主导阶也变得相关。对于K = 3的情况,使用准蒙特卡罗方法数值求解序参量的自洽方程。结果表明,对于任意小的Γ,量子涨落会破坏经典极限Γ = 0时存在的相变,取而代之的是一个平滑的交叉转变。讨论了该结果对通过绝热演化的量子优化算法预期性能的影响。简要重新审视了经典随机K -可满足性问题的复制对称解。结果表明,复制对称理论预测的T = 0时的相变是具有非典型临界指数的连续类型。