The contraction phase of solar evolution.
Gravitational contraction of stars of one solar mass examined, using Henyey method for calculating stellar evolutionary tracks
Engineering topics
Publications and source records attributed to Cameron, A. G. W..
Gravitational contraction of stars of one solar mass examined, using Henyey method for calculating stellar evolutionary tracks
Properties of dense matter in nuclear statistical equilibrium analyzed at high densities and temperatures in connection with stellar evolution
Systematics of fission based on exponential mass formula, discussing neutron capture
Gas clouds in dense star clusters compared with quasar properties, analyzing possible energy sources like supernova explosions, stellar collisions and star gas interaction
Lunar photometric properties reproducible from surfaces composed of dark randomly-fallen grains, noting density as function of grain geometry and incident angle
Problem of large solar and stellar helium content examined in regard to nucleosynthesis theory that initial composition of galaxy was hydrogen
Parameters of Fermi gas formula using pairing and shell correction energies, noting neutron and protron resonances
X-ray emission and cooling of neutron stars, combining neutrino emission from interior and photon emission from surface
Mass formulas differing in treatment of nuclear symmetry energy with very neutron-rich nuclei being bound in one formula and unbound in other
Cosmic ray production and acceleration by hydromagnetic waves from vibrating neutron stars
Effect of three-body nuclear potential and two neutron-neutron potentials on radial oscillation periods of neutron stars
Discrete X-ray sources associated with neutron or hyperon stars formed during internal collapse which triggers off supernova explosions
Planetary atmospheres origin due to outgassing or capture from primitive solar nebula or solar wind and atmospheric losses due to reverse processes
Fission threshold calculation for systematics of spontaneous fission rates and neutron-fission width ratio
Model sequence calculations of solar evolution extended to varying-G cosmology
Earth and planetary ocean and atmospheric origin, evolution, and composition