Issue of time in generally covariant theories and the Komar-Bergmann approach to observables in general relativity

Diffeomorphism-induced symmetry transformations and time evolution are distinct operations in generally covariant theories formulated in phase space. Time is not frozen. Diffeomorphism invariants are consequently not necessarily constants of the motion. Time-dependent invariants arise through the choice of an intrinsic time, or equivalently through the imposition of time-dependent gauge fixation conditions. One example of such a time-dependent gauge fixing is the Komar-Bergmann use of Weyl curvature scalars in general relativity. An analogous gauge fixing is also imposed for the relativistic free particle and the resulting complete set time-dependent invariants for this exactly solvable model are displayed. In contrast with the free particle case, we show that gauge invariants that are simultaneously constants of motion cannot exist in general relativity. They vary with intrinsic time.

Soliton collision in general relativity

An exact solution of the Einstein equations in vacuum representing two pairs of gravitational solitons propagating on an expanding universe is given and studied. It is suggested that the solitons evolve from quasiparticles to pure gravitational waves. Two of the four solitons collide and the focusing produced on null rays is studied. Although the spacetime following the collision is highly distorted, null rays do not focus to a singularity.

Anisotropic fluid with SU(2) type structure in general relativity: A model of localized matter

A model of anisotropic fluid with three perfect fluid components in interaction is studied. Each fluid component obeys the stiff matter equation of state and is irrotational. The interaction is chosen to reproduce an integrable system of equations similar to the one associated to self-dual SU(2) gauge fields. An extension of the BelinskyZakharov version of the inverse scattering transform is presented and used to find soliton solutions to the coupled Einstein equations. A particular class of solutions that can be interpreted as lumps of matter propagating in empty space-time is examined.

Conservation laws and variational principles in general relativity /

"April 23, 1962."

Relativity : the special and general theory /

Includes index.

New theories in physics : proceedings of the XI Warsaw Symposium on Elementary Particle Physics, 23-27 May, 1988, Kazimierz, Poland /

Mode of access: Internet.

Relativity in colored pictures.

Cover title.

The theory of general relativity and gravitation.

Mode of access: Internet.

Introduction to Einstein and universal relativity

Mode of access: Internet.

The principle of relativity with applications to physical science /

Mode of access: Internet.

Relativity, the electron theory, and gravitation,

Mode of access: Internet.

Amoroso Costa e o primeiro livro brasileiro sobre a relatividade geral

Em 1922, o físico-matemático brasileiro Amoroso Costa publicou um livro de introdução à Teoria da Relatividade. Este livro, um dos primeiros textos sobre o assunto no mundo, surpreende ainda hoje pela sua limpidez, precisão e concisão. Fazemos uma análise do texto de Amoroso Costa, situando-o no contexto científico mundial e brasileiro.

Implícits filosòfics del convencionalisme en la geometria espaciotemporal

Treball que té com a objectiu, en primer lloc, establir quina possibilitat té el convencionalisme de ser una alternativa a les concepcions realistes de la geometria relativista; en segon lloc, assenyalar les implicacions epistemològiques que en deriven; en tercer lloc, precisar quin tipus de lectura de la hipòtesi inicial hem de fer donat que hi ha un cert marge per a l’ambigüitat i això ha permès diverses propostes; i en quart i darrer lloc, en cas que hom accepti les restriccions que el convencionalisme imposa al nostre coneixement, hem de veure quines conclusions podem extreure en l’àmbit ontològic i fins a quin punt són significatives per a la discussió sobre la relació entre matemàtica i naturalesa

Nuclear curvature energy in relativistic models

The difficulties arising in the calculation of the nuclear curvature energy are analyzed in detail, especially with reference to relativistic models. It is underlined that the implicit dependence on curvature of the quantal wave functions is directly accessible only in a semiclassical framework. It is shown that also in the relativistic models quantal and semiclassical calculations of the curvature energy are in good agreement.