论文标题
量子真空摩擦的能量学。 II:偶极子波动和场波动
Energetics of quantum vacuum friction. II: Dipole fluctuations and field fluctuations
论文作者
论文摘要
作为与Arxiv串联的第二篇论文:2108.01539,我们在这里讨论在本质上耗散粒子上的量子真空摩擦。摩擦不仅源于场的波动,而且还来自偶极子的固有性。结果,耗散粒子可以从失去或获得内部能量的非平衡稳态(NESS)中脱离。只有当粒子的温度等于特殊的温度时,粒子才会处于ness中。我们首先得出了将粒子温度与辐射温度的函数和粒子速度的函数得出的NES条件。施加NESS条件,我们获得了NESS中量子真空摩擦的表达。 NESS量子真空摩擦始终是负定的,因此是真正的阻力。对于各种模型,计算了NESS温度和量子真空摩擦。在NESS之外,即使量子真空摩擦力在辐射的其余框架中不再具有确定的迹象,我们发现保持粒子移动所需的外力必须与粒子运动的运动相同。然后,这排除了制造永久运动机的可能性,该机器可以将真空能量转换为有用的机械工作。此外,我们发现粒子温度偏离其NES的温度会导致粒子损失或获得内部能量,以使粒子在偏离粒子后会恢复到NESS。这使得对这些量子真空摩擦效应的可行签名实现了实验测量。
As a second paper in series with arXiv:2108.01539, we discuss here quantum vacuum friction on an intrinsically dissipative particle. The friction arises not only from the field fluctuations but also from the dipole fluctuations intrinsic to the particle. As a result, the dissipative particle can be out of the nonequilibrium steady state (NESS), where it loses or gains internal energy. Only if the temperature of the particle equals a special NESS temperature will the particle be in NESS. We first derive the NESS conditions which give the NESS temperature of the particle as a function of the radiation temperature and the velocity of the particle. Imposing the NESS conditions, we then obtain an expression for the quantum vacuum friction in NESS. The NESS quantum vacuum friction is shown to be always negative definite, therefore a true drag. The NESS temperature and quantum vacuum friction are calculated numerically for various models. Out of NESS, even though the quantum vacuum frictional force no longer has a definite sign in the rest frame of the radiation, we find the external force needed to keep the particle moving must be in the same direction as the motion of the particle. This then excludes the possibility of making a perpetual motion machine, which could convert the vacuum energy into useful mechanical work. In addition, we find that the deviation of the temperature of the particle from its NESS temperature causes the particle to lose or gain internal energy in such a way that the particle would return to NESS after deviating from it. This enables experimental measurements of the NESS temperature of the particle to serve as a feasible signature for these quantum vacuum frictional effects.