activity
20242026
collaborators

5 papers

astro-ph.HE2026

Clumpy Outflows from Super-Eddington Accreting Black Holes I: Radiation Hydrodynamics Simulations and Observational Implications

Haojie Hu, Yuta Asahina, Shogo Yoshioka +2

Recent advances in X-ray spectroscopic observation have enabled researchers to reveal distinct clumpy structures in the super-Eddington outflows from the supermassive black hole in…

astro-ph.GA2026

Back to Normal Again: Possible Destinies of JWST overmassive SMBHs and "Little Red Dots" in the View of Shin-Uchuu Simulation

Haojie Hu, Hiroto Yanagisawa, Moka Nishigaki +3

The James Webb Space Telescope (JWST) has enabled the discovery of hundreds of supermassive black holes (SMBHs) at redshifts . A non-negligible fraction of these SMBH…

gr-qc2026

Microlensing of non-singular black holes at finite size: a ray tracing approach

Jens Boos, Hao Hu

We study the gravitational microlensing of various static and spherically symmetric non-singular black holes (and horizonless, non-singular compact objects of similar size). For po…

gr-qc2025

Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant

Hao Hu, Guoxiong Zhu

This paper investigates the dynamic behavior of static, spherically symmetric black holes within the Einstein-Bumblebee gravity model with a cosmological constant, focusing on scal…

hep-th2024

Forced non-conformal relativistic fluid from the Chamblin-Reall gravity

Chao Wu, Hao Hu, Ruohan Wang +1

The Chamblin-Reall gravity is a remarkable non-conformal platform for the fluid/gravity correspondence to achieve its maximum efficiency. When a probe scalar field that does not ch…