球体上粒子的渐近量子化

Q2 Physics and Astronomy
J. L. Romero, A. Klimov
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引用次数: 0

摘要

态紧密分布于若干不变子空间(可变自旋系统)的量子系统可以用在大平均角动量极限下的四维相空间T * S2中的分布来描述。余切束T * S2也是具有适当固定卡西密算子的E(3)对称群系统的经典流形。这允许我们使用适合于变量(整数)自旋系统的星积的渐近形式来发展一个在二维球体上运动的粒子的变形量化方案,其可观测值是e(3)代数的元素,相应的相空间是T * S2。我们证明了从相应的经典泊松括号中恢复了e(3)代数的标准对易关系,并得到了一些量化的经典可观测值(如角动量算子及其平方)的特征值和特征函数的显式表达式。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Asymptotic Quantization of a Particle on a Sphere
Quantum systems whose states are tightly distributed among several invariant subspaces (variable spin systems) can be described in terms of distributions in a four-dimensional phase-space T∗S2 in the limit of large average angular momentum. The cotangent bundle T∗S2 is also the classical manifold for systems with E(3) symmetry group with appropriately fixed Casimir operators. This allows us to employ the asymptotic form of the star-product proper for variable (integer) spin systems to develop a deformation quantization scheme for a particle moving on the two-dimensional sphere, whose observables are elements of e(3) algebra and the corresponding phase-space is T∗S2. We show that the standard commutation relations of the e(3) algebra are recovered from the corresponding classical Poisson brackets and the explicit expressions for the eigenvalues and eigenfunctions of some quantized classical observables (such as the angular momentum operators and their squares) are obtained.
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来源期刊
Quantum Reports
Quantum Reports Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
3.30
自引率
0.00%
发文量
33
审稿时长
10 weeks
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