Gravitational instabilities in helicity-1 waves propagating through matter in equilibrium
Luis Bento, Jose P. S. Lemos

TL;DR
This paper investigates how helicity-1 gravitational waves interacting with matter in equilibrium can cause new types of instabilities, including a Jeans-like instability with a critical wavelength related to the speed of light.
Contribution
It introduces a novel instability mechanism caused by helicity-1 gravitational waves interacting with matter, differing from traditional Jeans instability.
Findings
Helicity-1 waves induce shear motion in matter.
Instability occurs above a critical wavelength related to the speed of light.
Different from classical Jeans instability, involving transverse shear motions.
Abstract
It is shown that the interaction of helicity-1 waves of gravity and matter in a thin slab configuration produces new types of instabilities. Indeed, a transverse spin-2 helicity-1 mode interacts strongly with the shear motion of matter. This mode is unstable above a critical wavelength which reminds the Jeans wavelength but with the speed of sound interchanged by the speed of light. The two instabilities are of course different. For the case analyzed, a plane parallel configuration, Jeans instability appears through a density wave perturbation, the material collapsing into a set of plane-parallel slabs. On the other hand, the helicity-1 wave instability induces a transverse motion in the fluid that tends to shear in the material along the node of the perturbation.
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