Gravitational waves in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si8.svg" display="inline" id="d1e26"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> non-metric gravity without gauge fixing
Salvatore Capozzıello, Maurizio Capriolo
Abstract
We investigate the polarization modes of gravitational waves in f(Q) non-metric gravity without gauge fixing. The main result of this study is that no further scalar mode appears more than the two standard plus and cross transverse polarizations of massless tensor gravitational radiation, typical of General Relativity. This is because the first-order perturbation of connection does not modify the linearized field equations in vacuum which remain gauge invariant. Then, the world line equations of free point particles, as well as the equations of their deviations, are obtained using only the symmetric teleparallel connection. In f(Q) gravity, test masses follow timelike geodesics and not autoparallel curves. In the proper reference frame, thanks to the geodesic deviation equation of the structure-less bodies in free fall, we prove that, in any gauge, only the metric perturbations hμν, related to tensor modes, survive by exploiting the gauge invariance. Besides, scalar modes disappear. This allows us to conclude that only two degrees of freedom of linearized f(Q) non-metric gravity propagate as in General Relativity and in f(T) teleparallel gravity. The situation is different with respect to f(R) gravity (with f(R)≠R) where a further scalar mode is found.