activity
20202026
most citedPolarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave

4 citations · 6 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2026

Tightening Cosmological Constraints Within and Beyond CDM Using Gamma-Ray Bursts Calibrated with Type Ia Supernovae

Wei Hong, Luca Izzo, Massimo Della Valle +3

Context. Gamma-ray bursts (GRBs) reach redshifts beyond Type Ia supernovae (SNe Ia) and can extend distance measurements into the early Universe, but their use as distance indicato…

gr-qc2026

High Sensitivity Methodologies to Detect Radio Band Gravitational Waves

Wei Hong, Peng He, Tong-Jie Zhang +2

Gravitational waves (GWs) can resonate with magnetic fields through the Gertsenshtein-Zeldovich effect, producing electromagnetic signals at the same frequency. In pulsar magnetosp…

astro-ph.CO2025

Exploring the Cosmological Model Degeneracy with a new evaluate factor G

Yuan-bo Xie, Yun-dong Wu, Wei Hong +1

In the context of fitting cosmological models, parameter degeneracy remains a central issue. This paper critically examines traditional methods for constraining parameters and focu…

astro-ph.CO2025★ 4 cited

Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave

Jian-Kang Li, Wei Hong, Tong-Jie Zhang

Electromagnetic waves (EMWs) can be generated by gravitational waves (GWs) within a magnetic field via the Gertsenshtein effect. The conversion probability between GWs and EMWs can…

astro-ph.HE2024★ 2 cited

Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field

Wei Hong, Zhen-Zhao Tao, Peng He +1

Gravitational waves (GWs) can convert into electromagnetic waves in the presence of a magnetic field via the Gertsenshtein-Zeldovich (GZ) effect. The characteristics of the magneti…

astro-ph.CO2024

Cosmic Dynamics in Einstein-Cartan Theory: Analysing Hubble Tension through Curvature and Torsion field

Yun-Dong Wu, Wei Hong, Tong-Jie Zhang

The Hubble tension refers to the significant discrepancy in the Hubble constant obtained from two different measurement methods in cosmology. One method derives data from t…