The evolution of the universe.
Einstein-Friedmann cosmological model suitability to explain universe beginning and evolution, discussing model features, tests and remaining difficulties
Engineering topics
Publications and source records attributed to Chiu, H.-Y..
Einstein-Friedmann cosmological model suitability to explain universe beginning and evolution, discussing model features, tests and remaining difficulties
Properties of high density matter in intense magnetic fields, presenting equations of state of Fermi gas
Quantum theory of an electron gas with anomalous magnetic moments in intense magnetic fields
Quantum theory of electron gas in magnetic fields caused by gravitational collapse
Cosmological model for universe based on astronomical observations and validity of einstein theory and existing laws of physics
Scalar gravitational fields in pulsating stars, calculating scalar wave radiation rate and star relaxation time
Physical laws of universe, structure and evolution of universe, and cosmological theories of universe
Stellar plasma energy loss due to neutrino emission resulting from electromagnetic interaction between plasma and photon
Photodisintegration of iron into helium and neutrino annihilation process cause hydrostatic and dynamic instabilities that produce star collapse
Plasma neutrino process of Adams, Ruderman and Woo dependent on direct electron-neutrino interaction and connected with stellar evolution
Cosmology models in light of transport equation assuming relativity and conventional physical laws, noting densities inconsistent with closure
Microscopic model of symmetry between particle and antiparticle populations in expanding universe
Plasma neutrino process of Adams, Ruderman and Woo dependent on direct electron-neutrino interaction and connected with stellar evolution
Neutrino processes in stellar evolution, discussing pair annihilation, plasma, photoneutrino, URCA, bremsstrahlung, photo-beta, photon-photon and electron-electron bremsstrahlung processes
Stellar evolution for high temperature, predominantly neutrino processes, noting breakdown of homology relation between density and temperature
Neutron star structure and evolution from presupernovae stars including gravitational collapse and neutrino emission processes