I am now a PhD (in computer science) at the University of Pittsburgh under the supervision of Prof. Junyu Liu.
I got my Master of Philosophy (in physics) degree in 2025 from the Hong Kong University of Science and Technology under the supervision of Prof. Yi Wang and my Bachelor of science (in physics) degree from Nanjing University in 2023.
Now my research covers both theoretical physics and quantum related topics.
1 Quantum Cosmology
This is the main topic of my master thesis, we are trying to understand the quantum features and relics of the primordial fluctuation during the inflation. For more information, please refer my publication.
2 Quantum enhanced search for fundamental physics
Increasing the energy level on the traditional collider has been a trend for several decades. However, we are now facing more and more challenges on energy, environment, and money to build larger collider. On the other hand, collider is also not good at searching some kinds of particles such as axion and axion-like particles (the candidates for dark matter). With developed techniques in quantum metrology and sensing we can have very precise measurement with a tabletop instrument. It is interesting to make use of these knowledges to propose new experiment for beyond Standard Model physics and quantum gravity.
3 Complex system
Cosmological Bell Tests with Decoherence Effects
Abstract: The inflationary universe creates particle pairs, which are entangled in their momenta due to momentum conservation. Operators involving the momenta of the fluctuations can be rewritten into pseudo-spin operators, such as the Gour-Khanna-Mann-Revzen (GKMR) pseudo-spin. Making use of these pseudo-spin operators, cosmological Bell inequalities can be formulated. The violation of these Bell inequalities indicates the quantum nature of primordial fluctuations.
In this work, we focus on primordial curvature perturbations. Since curvature perturbations arise from gravity, their action includes the Gibbons-Hawking-York boundary term. We clarify the role of the boundary term in selecting suitable initial conditions for linear perturbations.
After that, we proceed to the interactions of cosmological perturbations, including the bulk and boundary interaction terms, which introduce decoherence effects. These decoherence effects change the expectation value of the Bell operator, and gradually restore the Bell inequality. We describe this process by a "Bell test curve'', which offers a window around 5 e-folds for testing the quantum origin of cosmological perturbations. We also explore the possibility of extracting the information of the decoherence rate and the structure of primordial interactions from the Bell test curve.
http://arxiv.org/abs/2405.07141
Related Conference talk at Gravity and Cosmology 2024 in Kyoto
Testing scalar decoherence by entangled initial state of cosmic inflation [Slides]