Probing non-Gaussianity during reheating with SIGW in the LISA band

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Perna, Gabriele, Domènech, Guillem
Format: Preprint
Veröffentlicht: 2026
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866910117125947392
author Perna, Gabriele
Domènech, Guillem
author_facet Perna, Gabriele
Domènech, Guillem
contents We analyse the effects of a non-standard evolution of the Universe during the reheating epoch on the spectrum of scalar-induced gravitational waves (SIGWs) accounting for the presence of primordial non-Gaussianity. We show that given values of $w$ and $c_s^2$ leave characteristic features in the spectrum which can be detectable by third generation interferometers like LISA. In addition, we argue that the specific reheating dynamics can suppress or even enhance the spectrum, with crucial consequences for its detectability. We perform a Fisher forecast for different values of $w$ and different scans to assess the detectability of the signal when different values of the amplitude and central frequency are considered.
format Preprint
id arxiv_https___arxiv_org_abs_2604_08493
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Probing non-Gaussianity during reheating with SIGW in the LISA band
Perna, Gabriele
Domènech, Guillem
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
We analyse the effects of a non-standard evolution of the Universe during the reheating epoch on the spectrum of scalar-induced gravitational waves (SIGWs) accounting for the presence of primordial non-Gaussianity. We show that given values of $w$ and $c_s^2$ leave characteristic features in the spectrum which can be detectable by third generation interferometers like LISA. In addition, we argue that the specific reheating dynamics can suppress or even enhance the spectrum, with crucial consequences for its detectability. We perform a Fisher forecast for different values of $w$ and different scans to assess the detectability of the signal when different values of the amplitude and central frequency are considered.
title Probing non-Gaussianity during reheating with SIGW in the LISA band
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2604.08493