the_pulp
- 206
- 9
What makes it more "gravity-wavy" than the fi or psi scalar of the vector perturbations? (Im talking about metric perturbations)
Thanks!
Thanks!
The discussion revolves around the representation of gravity waves by the h tensor in the context of metric perturbations in general relativity. Participants explore the distinctions between scalar, vector, and tensor perturbations, and the implications of these classifications for understanding gravity waves.
Participants do not reach a consensus on the reasons behind the classification of the h tensor as representative of gravity waves, and multiple competing views on the nature of gravity waves and metric perturbations remain present.
There are limitations in understanding the definitions and implications of scalar, vector, and tensor perturbations, as well as the specific conditions under which gravitational waves are produced. The discussion reflects varying levels of comprehension and interpretation of these concepts.
the_pulp said:What makes it more "gravity-wavy" than the fi or psi scalar of the vector perturbations? (Im talking about metric perturbations)
Thanks!
dextercioby said:Can you first figure out why you need to perturb the metric tensor? Then, if you write [itex]g_{\mu\nu} = \eta_{\mu\nu} + \mbox{first order perturbation}[/itex], how do you balance the indices?
the_pulp said:What makes it more "gravity-wavy" than the fi or psi scalar of the vector perturbations? (Im talking about metric perturbations)