Gravitational waves in vacuum spacetimes with cosmological constant. II. Deviation of geodesics and interpretation of non-twisting type N solutions
J. Bicak, J. Podolsky

TL;DR
This paper analyzes the behavior of gravitational waves in vacuum spacetimes with a cosmological constant, focusing on non-twisting type N solutions, and interprets their effects as exact transverse waves propagating on various backgrounds.
Contribution
It provides a detailed analysis of non-twisting type N vacuum solutions with cosmological constant, interpreting them as exact gravitational waves with specific polarization modes.
Findings
Non-twisting type N solutions behave as exact transverse gravitational waves.
Solutions with positive Lambda illustrate the cosmic 'no-hair' conjecture.
Explicit coordinate forms and properties of these solutions are derived.
Abstract
In a suitably chosen essentially unique frame tied to a given observer in a general spacetime, the equation of geodesic deviation can be decomposed into a sum of terms describing specific effects: isotropic (background) motions associated with the cosmological constant, transverse motions corresponding to the effects of gravitational waves, longitudinal motions, and Coulomb-type effects. Conditions under which the frame is parallelly transported along a geodesic are discussed. Suitable coordinates are introduced and an explicit coordinate form of the frame is determined for spacetimes admitting a non-twisting null congruence. Specific properties of all non-twisting type N vacuum solutions with cosmological constant Lambda (non-expanding Kundt class and expanding Robinson-Trautman class) are then analyzed. It is demonstrated that these spacetimes can be understood as exact transverse…
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