Gravity is perhaps the most intuitive and familiar of nature’s fundamental interactions. Despite significant progress over the past 300 years, a complete description of gravity remains elusive.
Our research focuses on gravitational physics, particularly phenomena involving compact objects such as black holes, regular black holes, and hairy black holes. These objects exhibit extreme gravitational effects, making them ideal laboratories for testing gravitational theories. In strong-gravity regions—such as those near neutron stars, black holes, or their singularities—existing models of gravity are pushed to their limits. By studying these environments, we aim to uncover new insights or identify deviations from current theoretical frameworks.
Current active research topics include:
Our research focuses on gravitational physics, particularly phenomena involving compact objects such as black holes, regular black holes, and hairy black holes. These objects exhibit extreme gravitational effects, making them ideal laboratories for testing gravitational theories. In strong-gravity regions—such as those near neutron stars, black holes, or their singularities—existing models of gravity are pushed to their limits. By studying these environments, we aim to uncover new insights or identify deviations from current theoretical frameworks.
Current active research topics include:
Black holes
- Black hole solutions and their interactions with fundamental particles
- Quasinormal modes, greybody factor and superradiance
- Spontaneous scalarization
- Black hole shadow
- Black hole and dark matter
- Gravitational wave echoes
