Annotation
The parameters of general-relativistic superdense configurations are calculated on the basis of numerical integration of the hydrostatic equilibrium equations of GTR jointly with a number of possible variants on he equation of state of the superdense matter. The possible form of the equilibrium-configuration curve is analyzed in the density range 10^13 <ρ> 10^40 g/cm^3.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
D.D. Ivanenko and N.I. Maksyukov
Department of Theoretical Physics
Department of Theoretical Physics
Science News of the Faculty of Physics, Lomonosov Moscow State University
This new information publication, which is intended to convey to the staff, students and graduate students, faculty colleagues and partners of the main achievements of scientists and scientific information on the events in the life of university physicists.