z13asbybztqxcf5fn23evt15kkerubq5c04 [Virialsatz] Virialsatz 117292786997707803818 12.02.2015 09.03.2015 Google+ Öffentlich Permalink #Calculations of the #StellarStructure of so-called degenerate stars using a new pressure function. ... #Calculations of the #StellarStructure of so-called degenerate stars using a new pressure function. https://www.dropbox.com/s/py2natda0vuzaq3/ calc_o_stell_struc.pdf?dl=0 ABSTRACT: Masses and radii of degenerate stars were calculated using a pressure function which significantly deviates from the usual one based on the Fermi energy of free electrons. Assuming only a central number density the calculations yield masses between those of Jupiter and the sun. The masses were found to be a function of the composition of the elements. The maximum masses and the comsic abundance of the elements are correlated. The radii are equal to those of pulsars at high central densities, while at low densities they are equal to those of white dwarfs. The period lenghts of shock waves in dense stars are calculated, the results being in agreement with the observed period lengths of pulsars. A proposal for interpreting quasi-stellar objects is made assuming matter composed of electrons and protons. To put it in a nutshell, and to explain that image with the many dots. #Calculations of the #StellarStructure of so-called degenerate stars using a new pressure function. https://www.dropbox.com/s/py2natda0vuzaq3/calc_o_stell_struc.pdf?dl=0 ABSTRACT: Masses and radii of degenerate stars were calculated using a pressure function which significantly deviates from the usual one based on the Fermi energy of free electrons. Assuming only a central number density the calculations yield masses between those of Jupiter and the sun. The masses were found to be a function of the composition of the elements. The maximum masses and the comsic abundance of the elements are correlated. The radii are equal to those of pulsars at high central densities, while at low densities they are equal to those of white dwarfs. The period lenghts of shock waves in dense stars are calculated, the results being in agreement with the observed period lengths of pulsars. A proposal for interpreting quasi-stellar objects is made assuming matter composed of electrons and protons. To put it in a nutshell, and to explain that image with the many dots. article calc_o_stell_struc.pdf [Shared with Dropbox] [Shared with Dropbox] Shared with Dropbox ‎