Neutron star models including the effects of hyperon formation
Neutron star matter equations of state involving hyperon formation effects for maximal stable mass models, tabulating moments of inertia
Cameron, A. G. W.↗
Engineering topics
Cameron, A. G. W.
Publications and source records attributed to Cameron, A. G. W..
Evidence for a collapsar in the binary system epsilon Aur
Black hole model accounting for epsilon Aur eclipsing binary secondary component observations
Cameron, A. G. W.↗
Pre-main sequence stellar evolution with mass loss
Pre-main sequence /T Tauri/ stellar evolution, discussing mass loss rates and star formation by interstellar cloud violent hydrodynamic compression
Cameron, A. G. W.↗
Stellar evolution
Stellar evolution, discussing mass loss to interstellar medium, galactic distances determination and supernova explosions
Cameron, A. G. W.↗
Physics of the neutron star
Neutron star models, discussing crystalline crust, particle superfluid properties, rotational vortices and relation to Crab Nebula pulsar
Cameron, A. G. W.↗
Supernova explosions.
The recent history of theoretical investigations of the supernova mechanism is considered, giving attention also to a number of nuclear physical problems which have yet to be solved in connection with the thermonuclear detonation. A variety of different processes of nucleo-synthesis are expected to occur in association with the supernova explosions. Aspects of the chemical evolution of the galaxy are discussed including the cosmic ray production of lithium, beryllium, and boron in the interstellar medium. Various hypotheses to account for the very large amount of light that comes from a supernova explosion are also examined.
Cameron, A. G. W.↗
The role of neutron stars in the acceleration of cosmic rays.
Two cases of cosmic ray acceleration are considered, including the acceleration of the material from the surface of a neutron star and the acceleration of the material in an EM wave interaction with the supernova ejecta. It is assumed that the neutron star mass would probably be somewhat less than the limiting mass of white dwarf stars, 1.4 solar masses. It is found that neutron stars may be effective in accelerating helium and iron to the highest cosmic ray energies, and that at lower energies they may accelerate supernova debris into the cosmic ray fluxes throughout the galaxy.
Cameron, A. G. W.↗
The Jovian turbopause probe. Part 1 - The scientific requirements for the Jovian turbopause probe
Mission planning for Jovian turbopause probe
Axford, W. I.↗
Formation of the earth-moon system
Earth-moon system formation theory, discussing condensation from terrestrial hot extended silicate atmosphere
Cameron, A. G. W.↗
URCA shells in dense stellar interiors
Stellar thermal and vibrational energy losses due to URCA shells in interiors
Cameron, A. G. W.↗
The galactic halo
Galactic halo origin and evolution postulated from chemical evolution assuming stellar evolution details
Cameron, A. G. W.↗
Neutron star models based on an improved equation of state
Neutron star models based on equation of state for cold degenerate matter, taking into account nuclear forces and clustering
Cameron, A. G. W.↗
Neutron stars
Neutron stars, discussing equations of state and stellar interiors, models, atmosphere, cooling, vibration, rotation and magnetic fields
Cameron, A. G. W.↗
Rotational properties of neutron star models
Rotational properties of neutron star models for Crab Nebula energy source, using expressions for angular momentum and rotational kinetic energy
Cameron, A. G. W.↗
Supernovae, neutron stars, and pulsars
Pulsars pulse duration and shape as key to neutron stars linkage with supernova explosions
Cameron, A. G. W.↗
An equation of state at subnuclear densities
Equation of state for neutron, proton and electron gas mixture associated with cold matter above white dwarf densities and below nuclear density
Cameron, A. G. W.↗
Equilibrium theory of the nuclear symmetry energy of infinite nuclear matter.
Symmetry energy of infinite nuclear matter calculated for cases of constant density and minimum saturation energy by density variation, considering finite compressibility effects
Cameron, A. G. W.↗
Equilibrium theory of the symmetry energy of finite nuclei.
Nonequilibrium and equilibrium schemes studies of nuclear symmetry energy of finite nuclei, discussing binding energy of nuclei with neutron excess
Cameron, A. G. W.↗