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(76) For case II with n = 3, ϵII n=3 ≈ 4M b − Λb3 6M − α · 560M 3b5

Case II with n = 2, 3 In exactly the same manner as above, one can calculate the deflection angles for Case II with n = 2, 3, to find the following results: For case II with n = 2

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Solar system tests in covariant f(Q) gravity

gr-qc · 2024-12-23 · conditional · novelty 5.0

Solar system data bound the parameter α in f(Q)=Q+αQ^n-2Λ gravity, with limits that depend strongly on the chosen affine connection.

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  • Solar system tests in covariant f(Q) gravity gr-qc · 2024-12-23 · conditional · none · ref 3

    Solar system data bound the parameter α in f(Q)=Q+αQ^n-2Λ gravity, with limits that depend strongly on the chosen affine connection.