Hot, vibrating neutron stars.
Thermal and vibrational energy in neutron star after creation in supernova explosion, considering dissipative effect of neutrino producing reactions
Engineering topics
Publications and source records attributed to Wolf, R. A..
Thermal and vibrational energy in neutron star after creation in supernova explosion, considering dissipative effect of neutrino producing reactions
Surface magnetic field variations in early stars, suggesting mechanism for magnetic energy transfer from convective core to surface
Solar wind flow behind moon where magnetic field parallels flow, noting severe recompression near boundary
Thermal, and vibrational energy calculations for neutron star during supernova explosion
Properties of neutron star at absolute zero temperature, discussing ground state, particle models and energy spectrum
Neutrino producing cooling reaction rates indicate that discrete X-ray sources located in direction of galactic center are not neutron stars
Neutron star cooling tested by photon flux measurements indicative of effective temperature change
Nuclear reaction rates between nuclei vibrating about adjacent lattice sites in highly dense stars from solving Schroedinger equation
Neutron star properties and structure at absolute zero temperature
Neutron stars - neutrino cooling and observability
Stellar temperature and density effects on proton- proton chain termination and endoergic electron- capture reaction rate
Rate of nuclear reactions in stars calculated using solid state method
Causes of impact injury in automobile accidents