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The energetics of quantum vacuum friction: Field fluctuations

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arxiv 2108.01539 v4 pith:WWEF3DGW submitted 2021-08-03 hep-th physics.atom-phquant-ph

classification hep-thphysics.atom-phquant-ph
keywords particlequantumvacuumforcefrictionfrictionalradiationblackbody
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Quantum fluctuations can induce a friction on a neutral but polarizable particle and cause it to radiate energy even if the particle is moving in free space filled with blackbody radiation, and is not in contact with or close to any surface or other object. We explore the energetics of such a particle moving uniformly in vacuum, continuing our previous investigations of quantum friction. The intrinsic polarizability of the particle is considered to be purely real before it is dressed by radiation. The particle is then guaranteed to be in the nonequilibrium steady state (NESS), where it absorbs and emits energy at the same rate. We first calculate the quantum frictional power and force on the particle in the rest frame of the blackbody radiation from first principles, namely the Maxwell-Heaviside equations and the Lorentz force law. Then we provide a simpler method of obtaining the same quantities in the rest frame of the particle by using the principle of virtual work. The equivalence of the two approaches is illustrated. The formulas we derive for quantum vacuum frictional power and force are fully relativistic and applicable to finite temperature. In NESS, the quantum vacuum frictional force on the particle is shown to be a true drag, independent of the model for polarizability and the polarization state of the particle. Finally, we give an estimate of the quantum vacuum friction on a gold atom and comment on the feasibility of detecting such quantum vacuum frictional effects.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Spontaneous Torque on an Inhomogeneous Chiral Body out of Thermal Equilibrium

    quant-ph 2024-12 conditional novelty 6.0 of 10

    A chiral, inhomogeneous body out of thermal equilibrium with its environment experiences a spontaneous second-order quantum vacuum torque, reaching small observable terminal angular velocities.

  2. Perspectives on Quantum Friction, Self-Propulsion, and Self-Torque

    quant-ph 2025-01 conditional novelty 4.0 of 10

    A small chiral object that is hotter or colder than the surrounding vacuum should experience a spontaneous quantum torque and spin with an observable terminal angular velocity.

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