activity
20242026
collaborators

8 papers

gr-qc2026

Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability

Liang Liang, Zhe Luo, Shoulong Li +1

Within general relativity, black holes are widely regarded as the ultimate benchmark for compactness in the Universe. Recently, however, neutron star models have been constructed i…

gr-qc2026

Neutron stars more compact than black holes as a probe of strong-field gravity

Shoulong Li, H. Lü, H. Lü +4

Probing gravity in its strongest regime is a central goal of modern physics, as the nature of the most compact objects reflects fundamental aspects of Einstein's theory of general…

astro-ph.CO2026

Coupled quintessence with a potential from supergravity exhibits sign-changing interaction

Jincheng Wang, Hongwei Yu, Puxun Wu

Quintessence with a potential motivated by supergravity (SUGRA) exhibits several intriguing features. Depending on its initial conditions, it can behave either as dynamical dark en…

gr-qc2026

Black holes and neutron stars in massive Hellings-Nordtvedt theory

Zhe Luo, Liang Liang, Zhong-Xi Yu +3

Hellings-Nordtvedt theory is a vector-tensor theory in which a vector field is nonminimally coupled to curvature through two independent interactions and $A^μ…

gr-qc2026

Quantum gravitodiamagnetic interaction

Di Hao, Jiawei Hu, Hongwei Yu

In the framework of linearized quantum gravity, we investigate the quantum gravitational interaction induced by the gravitodiamagnetic coupling of two massive objects to vacuum flu…

gr-qc2026

Self-consistent neutron stars in a class of massive vector-tensor gravity

Zhe Luo, Shoulong Li, Hongwei Yu

Einstein-bumblebee gravity, as a class of massive non-minimally coupled vector-tensor theories, provides a useful framework for constraining Lorentz symmetry breaking through astro…