Nanohertz gravitational waves from NEC violation in the early universe
Hiroaki W. H. Tahara, Tsutomu Kobayashi

TL;DR
This paper explores how quantum fluctuations during an NEC-violating phase in the early universe can produce nanohertz gravitational waves detectable by pulsar timing arrays, proposing a model compatible with BBN constraints.
Contribution
It introduces a stable NEC-violating model within cubic Horndeski theory that generates observable gravitational wave spectra consistent with recent NANOGrav results.
Findings
Gravitational wave spectra with spectral indices 0.8, 0.9, 0.95 fit NANOGrav data.
The model evades BBN constraints while producing detectable signals.
Different inflationary durations affect the peak frequency of gravitational waves.
Abstract
We study nanohertz gravitational waves relevant to pulsar timing array experiments from quantum fluctuations in the early universe with null energy condition (NEC) violation. The NEC violation admits accelerated expansion with the scale factor (), which gives the tensor spectral index . To evade the constraint from Big Bang nucleosynthesis (BBN), we connect the NEC-violating phase to a subsequent short slow-roll inflationary phase which ends with standard reheating, and thereby reduce the high frequency part of the spectrum. An explicit model is constructed within the cubic Horndeski theory which allows for stable violation of the NEC. We present numerical examples of the background evolution having the different maximal Hubble parameters (which determine the peak amplitude of gravitational waves), the different inflationary Hubble parameters…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
