activity
20242026
collaborators

9 papers

astro-ph.CO2026

Inverse-k Primordial Oscillations from a Symbolic Regression Search

Ze-Yu Peng, Qing-Yu Lan, Yun-Song Piao

Oscillatory features in the primordial power spectrum, potential signatures of new physics in the early universe, are usually searched for using fixed templates. In this work, we p…

astro-ph.CO2026

DeepInflation: an AI agent for research and model discovery of inflation

Ze-Yu Peng, Hao-Shi Yuan, Qi Lai +4

We present DeepInflation, an AI agent designed for research and model discovery in inflationary cosmology. Built upon a multi-agent architecture, DeepInflation integrates Large Lan…

astro-ph.CO2026

Single field slow-roll inflation with step uplift to

Hao-Shi Yuan, Ze-Yu Peng, Yun-Song Piao

The early dark energy resolution of Hubble tension seems to be suggesting a scale-invariant Harrison-Zeldovich spectrum of primordial scalar perturbation, i.e. ($|n_s-1|\si…

astro-ph.HE2026

The environmental dependence of mid-IR luminous dusty Supernovae

Lin Xiao, Zeyue Peng, Lluis Galbany +10

Using the Spitzer and WISE images, we discovered 42 mid-IR luminous dusty supernovae with local integral-field spectroscopy data. The observed mid-IR emission indicates the presenc…

astro-ph.CO2025

Testing in light of the latest ACT and SPT data

Ze-Yu Peng, Jun-Qian Jiang, Hao Wang +1

It is commonly recognized that the primordial scalar spectral index is approximately , depending on the dataset. However, this view is being completely altered by…

astro-ph.CO2025

Hint of after DESI DR2 ?

Hao Wang, Ze-Yu Peng, Yun-Song Piao

In the report by BICEP/Keck collaborations, the tensor-to-scalar ratio is (95\% C.L.). However, recent datasets have preferred the evolving dark energy, which thus…