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The curved spacetime couterpart of γ matrices is γµ =eµ αγα and also satisfies, {γµ,γν} = 2gµν

Fermionic field in Covariant form In the curved spacetime, Lagrangian density for fermionic field [47] is written as L = ei 2 ( ˜ψγµDµψ−Dµ ˜ψγµψ)−eM ˜ψψ, (3

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RGUP Corrections to Scalar and Fermionic Fields

gr-qc · 2025-04-22 · reject · novelty 4.0

The RGUP field-theory corrections collapse to trivial constant rescalings of kinetic terms, and the fermionic correction vanishes identically.

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  • RGUP Corrections to Scalar and Fermionic Fields gr-qc · 2025-04-22 · reject · none · ref 1

    The RGUP field-theory corrections collapse to trivial constant rescalings of kinetic terms, and the fermionic correction vanishes identically.