Pith. sign in

The hyper- angular part is also normalised

ζ 2 0 (58) Energy correction is given by: ⟨Fn|∆ ˆH|Fn⟩=− ℏ2ϵ 2m0 Z ζq ζ0 Z π 2 0 Ψ∗ n(ζ,α)ζ 2∂ζΨn(ζ,α)dζdα ⟨Fn|∆ ˆH|Fn⟩=− ℏ2ϵ 2m0 Z ζq ζ0 Fn(ζ)ζ 2F′ n(ζ)dζ Z π 2 0 |Φ(α)|2dα (59) We have defined thatζ q =ζ 0eqπ/s 0 · 1981

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gr-qc 1

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The effects of the Gravitational Field on the Efimov State

gr-qc · 2025-09-06 · reject · novelty 6.0

The paper derives a first-order gravitational correction to Efimov energy levels in Schwarzschild spacetime, but the correction vanishes because the Schwarzschild Ricci tensor is zero and the equations contain sign errors.

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  • The effects of the Gravitational Field on the Efimov State gr-qc · 2025-09-06 · reject · none · ref 1

    The paper derives a first-order gravitational correction to Efimov energy levels in Schwarzschild spacetime, but the correction vanishes because the Schwarzschild Ricci tensor is zero and the equations contain sign errors.