Talk:Kerr–Newman–de–Sitter metric
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More tensors and scalars edit
The covariant, contravariant and mixed tensors as well as the scalars and equations of motion which might be too long for this article can be found here for Boyer Lindquist, here for Null coordinates and here for the transformation between them. This ressource can also be used to easily doublecheck the results since the code is relatively easy to read. --
❇ 19:51, 18 August 2023 (UTC)
Hubble constant vs Hubble parameter edit
@Ra-raisch: - in this edit you changed the Hubble constant to Hubble parameter and linked to the article stating "Though the Hubble constant is constant at any given moment in time, the Hubble parameter varies with time", while in De Sitter universes the H is constant, so I replaced your link with this link. ❇ 16:27, 19 August 2023 (UTC)
Feedback from New Page Review process edit
I left the following feedback for the creator/future reviewers while reviewing this article: Thank you for writing the article on Wikipedia! I genuinely appreciate your efforts in creating the article on Wikipedia and expanding the sum of human knowledge in Wikipedia. Wishing you and your family a great day!
✠ SunDawn ✠ (contact) 04:22, 12 October 2023 (UTC)