Rescuing the concept of swimming in curved spacetime
arXiv:1611.06183 · doi:10.1103/PhysRevD.94.121502
Abstract
It has been argued that an extended, quasi-rigid body evolving freely in curved spacetime can deviate from its natural trajectory by simply performing cyclic deformations. More interestingly, in the limit of rapid cycles, the amount of deviation, per cycle, would depend on the sequence of deformations but not on how fast they are performed -- like the motion of a swimmer at low Reynolds number. Here, however, we show that the original analysis which supported this idea is inappropriate to investigate the motion of extended bodies in the context of general relativity, rendering its quantitative results invalid and casting doubts on the reality of this swimming effect. We illustrate this by showing that the original analysis leads to a non-zero deviation even in a scenario where no swimming can possibly occur. Notwithstanding, by applying a fully covariant, local formalism, we show that swimming in curved spacetime is indeed possible and that, in general, its magnitude can be of the same order as (fortuitously) anticipated -- although it is highly suppressed in the particular scenario where it was originally investigated.
arXiv comment6 pages. To appear in Phys. Rev. D as a Rapid Communication
References in corpus (3)
- Trouble with the Lorentz law of force: Incompatibility with special relativity and momentum conservation
- Comment on "Trouble with the Lorentz law of force: Incompatibility with special relativity and momentum conservation"
- Comment on "Trouble with the Lorentz Law of Force: Incompatibility with Special Relativity and Momentum Conservation"
Cited by in corpus (5)
- Extended-body motion in black hole spacetimes: What is possible?
- How to glide in Schwarzschild spacetime
- Chaotic dynamics of a spinless axisymmetric extended body around a Schwarzschild black hole
- Extended-body effects and rocket-free orbital maneuvering
- Free-falling motion of an elastic rigid rod towards a Schwarzschild black hole