ISSN:
1420-9136
Source:
Springer Online Journal Archives 1860-2000
Topics:
Geosciences
,
Physics
Notes:
Summary In this paper in section I the structure of massive fluid spheres (stars) which are composed of completely degenerate matters is investigated. Equations of equilibrium govering such configurations have been put in convenient forms. In section II a few minimal properties of the stars, such as the maximum (or minimum) central energy density and temperature, etc., have been studied. It has further been shown that for nondegenerate matters the reductions in maximum central energy density and temperature are proportional to 1/K 3 3 c −2 and 1/K 3 respectively (c=2.998×1010 cm/sec andK 3 is assumed to be greater thanK 1(=3.17×1012).
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00875637