A major goal of nuclear physics is to quantitively and comprehensively understand the internal dynamics of the nucleon and nuclei described by quantum chromodynamics. Photon and electron scattering fr...
In the past, the quantum-to-classical transition of inflationary cosmological perturbations more focused on explaining today’s classical observations which originate from quantum vacuum fluctuation, ...
Model-based reinforcement learning (MBRL) is widely recognized with the potential to be significantly more sample efficient than model-free reinforcement learning. How an accurate model can be develop...
Cosmic reionization is the last major phase transition that our Universe goes through. In this milestone, the intergalactic medium transitions from primarily neutral, dark, and cold into mainly ionize...
The nature of dark matter remains one of the most interesting problems in physics and astronomy. There are many kinds of candidates of dark matter, which result in big challenges in detecting it exper...
The High-Luminosity upgrade of the LHC and future hadron colliders will present us unprecedented instantaneous luminosities with a much higher pile-up in the collision events than the current LHC. Eff...