Status of self - bound structures in hydrostatic equilibrium The actual meaning of exterior Schwarzschild solution
نویسنده
چکیده
We show that regular structures governed by an equation of state (EOS) or density variation such that the density at the surface does not vanish together with pressure (also known as self-bound regular structures) can not exist in the state of hydrostatic equilibrium. The only configuration which could exist in this regard is governed by homogeneous density distribution. Other structures which can fulfill the requirement set up by exterior Schwarzschild solution (and, therefore, can exist in hydrostatic equilibrium) would always be governed by a singular solution (that is, the pressure and density both become infinity at the centre), and in this sense can not be considered regular.
منابع مشابه
Hydrostatic Equilibrium of Insular, Static, Spherically Symmetric, Perfect Fluid Solutions in General Relativity
An analysis of insular solutions of Einstein’s field equations for static, spherically symmetric, source mass, on the basis of exterior Schwarzschild solution is presented. Following the analysis, we demonstrate that the regular solutions governed by a self-bound (that is, the surface density does not vanish together with pressure) equation of state (EOS) or density variation can not exist in t...
متن کاملStatus of Self-bound Structures in Hydrostatic Equilibrium
We show that regular structures governed by an equation of state (EOS) or density variation such that the density at the surface does not vanish together with pressure (also known as self-bound regular structures) can not exist in the state of hydrostatic equilibrium. The only configuration which could exist in this regard is governed by homogeneous density distribution. Other structures which ...
متن کاملStellar Equilibrium in 2 + 1 Dimensions
The hydrostatic equilibrium of a 2+1 dimensional perfect fluid star in asymptotically anti-de Sitter space is discussed. The interior geometry matches the exterior 2+1 black-hole solution. An upper mass limit is found, analogous to Buchdahl’s theorem in 3+1, and the possibility of collapse is discussed. The case of a uniform matter density is solved exactly and a new interior solution is presen...
متن کاملExact Solutions of Einstein’s Field Equations
We examine various well known exact solutions available in the literature to investigate the recent criterion obtained in ref. [20] which should be fulfilled by any static and spherically symmetric solution in the state of hydrostatic equilibrium. It is seen that this criterion is fulfilled only by (i) the regular solutions having a vanishing surface density together with the pressure, and (ii)...
متن کاملDynamical stability of strange quark stars
The necessary and sufficient condition for dynamical stability is worked out for the sequences of relativistic star models corresponding to the well defined and causal values of adiabatic sound speed, √ (dP/dE)0 = v0, at the centre. On the basis of these conditions, we show that the mass-radius (M −R) relation corresponding to the MIT bag models of strange quark matter (SQM) and the models obta...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2002