Primordial observables of explicit diffeomorphism violation in gravity
Year: 2026
Type: article
Abstract: We investigate the potential for current and future gravitational-wave detectors to observe imprints of explicit diffeomorphism violation in primordial signals. Starting from a simple model with known effects, we derive the strain amplitude and power spectrum for primordial gravitational waves, both of which are affected by the symmetry breaking. Through this, we directly find predictions for the tensor spectral index and tensor-to-scalar which are different from general relativity. By considering the known sensitivity curves for NANOGrav, SKA, THEIA, μ -ARES, ASTROD-GW, LISA, BBO, DECIGO, CE, AION-km, AEDGE, ET, and aLIGO, we place observability limits on the parameters controlling the diffeomorphism violation. For instance, we find that aLIGO could observe signals for s 00 ≲ − 0.1 , while more sensitive future detectors like LISA and DECIGO could probe violations as small as s 00 ≈ − 5 × 10 − 4 and − 3 × 10 − 3 , respectively. Finally, we consider the existing constraints on the number of relativistic degrees of freedom Δ N eff which is tightly constrained by Big-Bang Nucleosynthesis, where we find that Δ N eff only weakly depends on the symmetry breaking but places a lower bound on the coefficients which is consistent with available bounds from the speed of gravitational waves.
Source: Physics Letters B
Institutions: Khazar University, Damghan University, Institute for Research in Fundamental Sciences, Centre National de la Recherche Scientifique, Université Paris Sciences et Lettres, Observatoire de Paris, Sorbonne Université, Institute for Basic Science, Laboratoire Temps Espace, University of Salerno, Istituto Nazionale di Fisica Nucleare, Gruppo Collegato di Salerno, K. N. Toosi University of Technology
Language: English
Subfield: Statistical and Nonlinear Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: diamond
Awards: G4117354703, G4487476711, G61869192
OpenAlex ID: W4416747248
