Ciencia

El punto L1, calculado por Lagrange y la superficie de Schwarzschild, son claves de este trabajo. El primero nunca podrá ser un punto de esa superficie, y en este trabajo proponemos aproximarlo a ella. De esta forma estudiaremos que dos agujeros negros podrían no llegar a tocarse, ya que los efectos de la colisión podrían producirse antes del impacto, causando con ello el rechazo o la disolución del menor de los dos. Por último, se aplica este mismo estudio a una estructura ideal, masiva e inestable que podría producir la explosión de la materia oscura.

 J43. Deformation and crack theories of the strong gravitational fields.

The Lagrange point, L1, as well as the Schwarschild surface are both crucial keys all along this work. The former one -the point- shall never be able to belong to that surface, and so the only thing that we thy to do here is to shorten the distance between both or them. In accordance with this we may study the possibility that two black holes may never reach a real contact point between them because the effects of the crash might well appear before the impact, and so, as a consequence, ther would appear a reject between both or them or perhaps the vanishing of the smaller of the two holes. Finally we will apply a similar study to an ideal, mass, unstable structure which could give rise to the blowing up of the dark matter.

Edición Exclusiva.

Bilingüe: Esp.- Ing.

ISBN: 978-84-93723-11-8

Pag. 152.