collaborators

7 papers

astro-ph.CO2026

How Dilatation Invariance Suppresses Loop Corrections to Curvature Perturbations on CMB Scales

Danilo Artigas, Shi Pi, Takahiro Tanaka +1

Departures from standard slow-roll (SR) inflation have attracted increasing interest in recent years. In particular, scenarios that strongly enhance the power spectrum of the curva…

hep-ph2026

On the survival of strong nuggets in the early Universe

Haoyang Qi, Wen-Li Yuan, Yudong Luo +3

Strong nuggets with a baryon number of could be able to survive from the cosmic separation of the QCD phases, provided the transition from strange quark matter t…

astro-ph.CO2026

Inflationary relics from an Ultra-Slow-Roll plateau

Albert EscrivÃ, Jaume Garriga, Shi Pi

We investigate the formation of primordial black holes (PBHs) in inflationary scenarios featuring an ultra-slow-roll (USR) plateau with a sharp transition to slow roll. We focus on…

astro-ph.CO2025

Non-Gaussianities and Primordial Black Holes

Shi Pi

The most promising mechanism of generating PBHs is by the enhancement of power spectrum of the primordial curvature perturbation, which is usually accompanied by the the enhancemen…

astro-ph.CO2025

Extended formalism: Nonspatially Flat Separate Universe Approach

Danilo Artigas, Shi Pi, Takahiro Tanaka

The formalism is a powerful approach to compute non-linearly the large-scale evolution of the comoving curvature perturbation . It assumes a set of FLRW patches that evol…

astro-ph.CO2025

Primordial black holes and induced gravitational waves from logarithmic non-Gaussianity

Ryoto Inui, Cristian Joana, Hayato Motohashi +3

We investigate the formation of primordial black hole (PBH) based on numerical relativity simulations and peak theory as well as the corresponding scalar induced gravitational wave…