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arXiv 0810.3893quant-ph
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耗散相空间量子力学中的Wigner函数和阻尼星积

On Wigner functions and a damped star product in dissipative phase-space quantum mechanics

B. Belchev, M. A. Walton

摘要:

Dito和Turrubiates最近介绍了相空间中阻尼谐振子耗散量子力学的一个有趣模型。它的关键成分是一个非厄米变形的Moyal星产品的阻尼常数作为变形参数。我们比较了Dito-Turrubiates方案与基于其他星积的相空间量子力学(或变形量子化),并将其扩展到包含Wigner函数。变形(或阻尼)的星积与复哈密顿量有关,因此需要一个包含复共轭的修正的运动方程。我们发现,这种变化的维格纳函数满足经典的运动方程。这似乎是合适的,因为具有二次哈密顿量的非耗散系统共享此属性。

英文摘要:

Dito and Turrubiates recently introduced an interesting model of the dissipative quantum mechanics of a damped harmonic oscillator in phase space. Its key ingredient is a non-Hermitian deformation of the Moyal star product with the damping constant as deformation parameter. We compare the Dito-Turrubiates scheme with phase-space quantum mechanics (or deformation quantization) based on other star products, and extend it to incorporate Wigner functions. The deformed (or damped) star product is related to a complex Hamiltonian, and so necessitates a modified equation of motion involving complex conjugation. We find that with this change the Wigner function satisfies the classical equation of motion. This seems appropriate since non-dissipative systems with quadratic Hamiltonians share this property.

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