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Quantum star-graph analogues of pt-symmetric square wells

机译:pt对称方阱的量子星图类似物

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摘要

We recall the solvable pt-symmetric quantum square well on an interval of x ∈ (-L, L) := G~((2)) (with an a-dependent non-Hermiticity given by Robin boundary conditions) and generalize it. In essence, we just replace the support interval G~((2)) (reinterpreted as an equilateral two-pointed star graph with Kirchhoff matching at the vertex x = 0) with a q-pointed equilateral star graph G~((q)) endowed with the simplest complex-rotation-symmetric external a-dependent Robin boundary conditions. The remarkably compact form of the secular determinant is then deduced. Its analysis reveals that (i) at any integer q = 2, 3,..., there exists the same q-independent and infinite subfamily of the real energies, and (ii) at any special q = 2, 6, 10,..., there exists another, additional, q-dependent infinite subfamily of the real energies. In the spirit of the recently proposed dynamical construction of the Hilbert space of a quantum system, the physical bound-state interpretation of these eigenvalues is finally proposed.
机译:我们回想一下在x∈(-L,L):= G〜((2))(具有由Robin边界条件给出的a依赖的非Hermiticity)区间上的可解pt对称量子平方,并对其进行推广。从本质上讲,我们只是将支撑间隔G〜((2))(用在顶点x = 0处具有Kirchhoff匹配的等边两点星形图替换为q点)等边星形图G〜((q) )具有最简单的复杂旋转对称外部a依赖的Robin边界条件。然后推断出世俗行列式的非常紧凑的形式。它的分析表明,(i)在任意整数q = 2、3,...下,存在相同的q独立且无限的实能量子族,并且(ii)在任何特殊q = 2、6、10, ...,存在另一个附加的,q相关的实能量无穷子族。本着最新提出的量子系统希尔伯特空间动力学构造的精神,最后提出了这些特征值的物理束缚态解释。

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