A new proof for non-occurrence of trapped surfaces in spherical collapse
نویسنده
چکیده
We present here a very simple, short and new proof which shows that no trapped surface is ever formed in spherical gravitational collapse of isolated bodies. Although this derivation is of purely mathematical nature and without any assumption, it is shown, in the Appendix, that, physically, trapped surfaces do not form in order that the 3 speed of the fluid as measured by an observer at a fixed circumference coordinate R (a scalar), is less than the speed of light c. The consequence of this result is that, mathematically, even if there would be Schwarzschild Black Holes, they would have unique gravitational mass M = 0. Recall that Schwazschild BHs may be considered as a special case of rotating Kerr BHs with rotation parameter a = 0. If one would derive the Boyer-Lindquist metric [1] in a straight forward manner by using the Backlund transformation[2], one would obtain a = M sinφ where φ is the azimuth angle. This relation demands that BHs have unique massM = 0 (along with a = 0) which in turn confirms that there cannot be any trapped surface in realistic gravitational collapse where the fluid has real pressure and density. Since there is no trapped surface and horizon, there is no Information Paradox in the first place. When a self-gravitating fluid undergoes gravitational contraction, by virtue of Virial Theorem, part of the gravitational energy must be radiated out. Thus the total mass energy, M , (c = 1) of a body decreases as its radius R decreases. But in Newtonian regime (2M/R ≪ 1, G = 1), M is almost fixed and the evolution of the ratio, 2M/R, is practically dictated entirely by R. If it is assumed that even in the extreme general relativistic case 2M/R would behave in the same Newtonian manner, then for sufficiently small R, it would be possible to have 2M/R > 1, i.e, trapped surfaces would form[3,4].
منابع مشابه
A new proof for non-occurrence of trapped surfaces and information paradox
We present here a very simple, short and new proof which shows that no trapped surface is ever formed in spherical gravitational collapse of isolated bodies. Although this derivation is of purely mathematical nature and without any assumption, it is shown, in the Appendix, that, physically, trapped surfaces do not form in order that the 3 speed of the fluid as measured by an observer at a fixed...
متن کاملNon-occurrence of Trapped Surfaces and Black Holes in Spherical Gravitational Collapse: An Abridged Version
By using the most general form of Einstein equations for General Relativistic (GTR) spherical collapse of an isolated fluid having arbitrary equation of state and radiation transport properties, we show that they obey a Global Constraint, 2GM(r, t)/R(r, t)c2 ≤ 1, where R is the “invariant circumference radius”, t is the comoving time, and M(r, t) is the gravitational mass enclosed within a como...
متن کاملA new security proof for FMNV continuous non-malleable encoding scheme
A non-malleable code is a variant of an encoding scheme which is resilient to tampering attacks. The main idea behind non-malleable coding is that the adversary should not be able to obtain any valuable information about the message. Non-malleable codes are used in tamper-resilient cryptography and protecting memories against tampering attacks. Many different types of non-malleability have alre...
متن کاملCosmic Walls and Filaments Formation in Modied Chaplygin Gas Cosmology
We want to study the perturbation growth of an initial seed of an ellipsoidal shape in Top-Hat collapse model of the structure formation in the Modied Chaplygin gas cosmology. Considering reasonable values of the constants and the parameters of the model under study, we can show that a very small deviation from spherical symmetry (ellipsoidal geometry) in the initial seed leads to a nal highly ...
متن کاملTrapped surfaces and the Penrose inequality in spherically symmetric geometries.
We demonstrate that the Penrose inequality is valid for spherically symmetric geometries even when the horizon is immersed in matter. The matter field need not be at rest. The only restriction is that the source satisfies the weak energy condition outside the horizon. No restrictions are placed on the matter inside the horizon. The proof of the Penrose inequality gives a new necessary condition...
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 2004