activity
20242026
collaborators

6 papers

astro-ph.IM2026

CWTHF: Subhalo Identification with Continuous Wavelet Transform

Minxing Li, Yun Wang, Ping He

With advances in cosmology and computer science, cosmological simulations now resolve structures in increasingly fine detail. As key tracers of hierarchical structure formation, su…

astro-ph.CO2026

Local Nonlinear Transforms Effectively Extract Cosmological Information From Large-Scale Structure

Yun Wang, Hao-Ran Yu, Yu Yu +1

Extracting cosmological information from nonlinear and non-Gaussian large-scale structure remains a major challenge. We introduce the (Zel'dovich-inspired) ZI transform, a simple o…

astro-ph.CO2026

The dynamical and thermodynamic effects of turbulence on the cosmic baryonic fluid

Yun Wang, Minxing Li, Ping He

Both simulations and observations indicate that the so-called missing baryons reside in the intergalactic medium known as the warm-hot intergalactic medium (WHIM). In this study we…

astro-ph.CO2025

Precision calculation of the EFT likelihood with primordial non-Gaussianities

Ji-Yuan Ke, Yun Wang, Ping He

We perform a precision calculation of the effective field theory (EFT) conditional likelihood for large-scale structure (LSS) using the saddle-point expansion method in the presenc…

hep-ph2025

Calculating the EFT likelihood via saddle-point expansion

Ji-Yuan Ke, Yun Wang, Ping He

In this paper, we extend the functional approach for calculating the EFT likelihood by applying the saddle-point expansion. We demonstrate that, after suitable reformulation, the l…

astro-ph.CO2024

Capturing primordial non-Gaussian signatures in the late Universe by multi-scale extrema of the cosmic log-density field

Yun Wang, Ping He

We construct two new summary statistics, the scale-dependent peak height function (scale-PKHF) and the scale-dependent valley depth function (scale-VLYDF) of matter density, and fo…