The effects of nuclear forces on the maximum mass limit of neutron stars
Nuclear forces effects on maximum mass limit of neutron stars models using V gamma type potentials
Engineering topics
Publications and source records attributed to Tsuruta, S..
Nuclear forces effects on maximum mass limit of neutron stars models using V gamma type potentials
Maximum mass limit effects of stable neutron stars on pulsar models
Stellar thermal and vibrational energy losses due to URCA shells in interiors
Nucleon isobars and hyperons carrying off interstellar and intergalactic proton-proton collision energy, discussing high energy gamma ray decay product
Nucleosynthesis by neutron capture on fast time scale in supernova explosion models for dynamics of highly evolved massive star cores
Nucleosynthesis in dynamics of massive star cores, noting element synthesis by neutron capture in supernova explosions
Vibrating neutron stars, discussing damping, heating, energy storage and X-ray emission possibilities at 1000 years range
Rapid neutron capture in supernova explosions
Surface properties, temperature effect, cooling and detectability of neutron stars, using pure iron and pure magnesium compositions
Neutron star structure analysis using composite state equation
Neutron star rotational flattening after formation in supernova implosion
Properties of dense matter in nuclear statistical equilibrium analyzed at high densities and temperatures in connection with stellar evolution
X-ray emission and cooling of neutron stars, combining neutrino emission from interior and photon emission from surface
Effect of three-body nuclear potential and two neutron-neutron potentials on radial oscillation periods of neutron stars
Surface properties, temperature effects, cooling behavior, and observability of neutron stars
Composite equations of state for determining effects of nuclear forces on neutron star models