activity
20242026
collaborators

11 papers

gr-qc2026

Learning Boson Star Solution Families with Physics-Informed Neural Networks

Ao Liu, Chen-Hao Hao, Cuihong Wen +2

Computing boson star families traditionally requires repeated solution of nonlinear eigenvalue boundary-value problems and careful numerical continuation through turning points. We…

cs.CV2026

HPSD: Hybrid-Policy Self-Distillation for Text-Image-to-Video Diffusion Models

Jiazi Bu, Pengyang Ling, Yujie Zhou +10

Text-Image-to-Video (TI2V) models are an emerging unified architecture, where a single model simultaneously supports text-to-video (T2V) and image-to-video (I2V) generation. Given…

gr-qc2026

Primordial black hole formation in bulk-viscous cosmology

Zi-Yan Yuwen, Cristian Joana, Shao-Jiang Wang +1

We investigate primordial black hole (PBH) formation in a cosmological background with bulk viscosity. Using numerical simulations, we determine the collapse threshold and the resu…

astro-ph.CO2026

Cosmological intercept tension

Jia-Qi Wang, Shao-Jiang Wang

The long-standing tension in the Hubble constant has motivated extensive explorations of both new physics and observational systematics, for example, the late-time systematic…

astro-ph.CO2026

Nonperturbative stochastic inflation in perturbative dynamical background

Xiao-Quan Ye, Shao-Jiang Wang

Inflationary models that contain a transient ultra-slow-roll phase can exhibit strong non-perturbative dynamics, making the usual perturbative treatment of cosmological fluctuation…

gr-qc2026

Relic gravitational waves from primordial gravitational collapses

Xiang-Xi Zeng, Zhuan Ning, Zi-Yan Yuwen +3

A large primordial density perturbation of the Hubble scale will gravitationally collapse, generating an outgoing sound shell, whether or not a primordial black hole (PBH) is forme…