19โ€“23 Jan 2026
Indian Institute of Technology Madras, Research Park
Asia/Kolkata timezone

Session

Production of Gravitational Waves from Preheating and Tachyonic Instabilities

19 Jan 2026, 15:00
Saha and Sarabhai Auditoriums (Indian Institute of Technology Madras, Research Park)

Saha and Sarabhai Auditoriums

Indian Institute of Technology Madras, Research Park

IITM RESEARCH PARK Kanagam, Tharamani, Chennai, Tamil Nadu 600113

Description

We analyze GW production during preheating for an $\alpha$-attractor
potential terminating in the positive-curvature regime, with energy transfer via
$\phi\chi^{2}$. Linear Floquet analysis and nonlinear simulations show that $\phi$
fluctuations grow by parametric resonance, while $\chi$ undergoes tachyonic
bursts. The GW spectrum features two peaks: a dominant low-frequency peak
from the parametric channel and a subdominant high-frequency peak from the
tachyonic channel. Redshifted to today, the peak reaches $h^{2}\Omega_{\rm GW}^{(0)} \sim 10^{-11}$ at $f_{p} \sim 10^{7}$ Hz. This multi-peak structure is a
characteristic imprint of trilinear preheating in $\alpha$-attractors.

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