Derives background-hierarchy bounds on the two free parameters of Type 3 NGR to ensure linear cosmological perturbation theory remains viable around flat FLRW.
On the duality of massive Kalb-Ramond and Proca fields
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Stueckelberg restoration converts deformed Abelian reducible gauge theories to invariant form, enabling ghost quantization and one-loop effective action computation for massive fermionic tensor fields in AdS as functional determinants of Dirac operators.
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Gauge-invariant cosmological perturbations in Type 3 New General Relativity and background-hierarchy bounds
Derives background-hierarchy bounds on the two free parameters of Type 3 NGR to ensure linear cosmological perturbation theory remains viable around flat FLRW.
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On a quantization of deformed reducible gauge theories
Stueckelberg restoration converts deformed Abelian reducible gauge theories to invariant form, enabling ghost quantization and one-loop effective action computation for massive fermionic tensor fields in AdS as functional determinants of Dirac operators.