内容: 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 scatte...
内容: 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 fluctu...
内容: 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...
内容: 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 i...
内容: Most galaxies comparable to or larger than the mass of the Milky Way host hot, X-ray emitting atmospheres and central radio sources. Hot atmospheres and radio jets and lobes are the ingredients...
内容: The idea of primordial black holes (PBHs), first introduced by Stephen Hawking, is not only a possible solution to the dark matter problem, but also a unique tracer of the dynamics of inflatio...