Pseudo-conformal Universe: late-time contraction and generation of tensor modes
Sergey Mironov

TL;DR
This paper explores a bouncing Universe model with a contracting phase driven by a complex scalar field, analyzing the resulting tensor mode spectrum which is blue and of small amplitude, providing constraints on model parameters.
Contribution
It introduces a novel bouncing Universe scenario with a complex scalar field and calculates the tensor mode spectrum during contraction.
Findings
Tensor spectrum is blue and small in amplitude
Rapid contraction occurs in the classical evolution
Model parameters face mild observational constraints
Abstract
We consider a bouncing Universe model which explains the flatness of the primordial scalar spectrum via complex scalar field that rolls down its negative quartic potential and dominates in the Universe. We show that in this model, there exists a rapid contraction regime of classical evolution. We calculate the power spectrum of tensor modes in this scenario. We find that it is blue and its amplitude is typically small, leading to mild constraints on the parameters of the model.
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.
