We study the dynamics of charged, spherically symmetric dust shells in the presence of a positive cosmological constant. We find generalizations of the well-known solutions in asymptotically flat spacetime, in particular orbits into "parallel universes", but also new solutions corresponding to a "bounce" of the shell before an event horizon has formed. We also discuss "bubble" solutions, in which a charged shell and an oppositely charged singularity are spontaneously created and annihilated.Comment: 16 page2; v2 final versio
Cosmological acceleration is difficult to accommodate in theories of fundamental interactions involv...
We start a systematic investigation of possible isometries of the asymptotically de Sitter solutions...
A thin shell of lightlike dust with its own gravitational field is studied in the special case of sp...
We consider a system representing self-gravitating balls of dust in an expanding Universe. It is dem...
We study the dynamics of a spherically symmetric dust shell separating two spacetime domains, the 'i...
We consider two spatially flat Friedmann-Robertson-Walker spacetimes divided by a timelike thin shel...
Gravitational equilibria of low density dust clouds imbedded in plasma background are studied. These...
Milne-like spacetimes are a class of $k = -1$ FLRW spacetimes which admit continuous spacetime exten...
We analyze the configuration of charged dust in the context of the higher dimensional and higher cur...
We give a comparative description of monopole and electrically charged spherically symmetric dust th...
ABSTRACT. A class of spherical collapsing exact solutions with electromagnetic charge is derived. Th...
Bouncing cosmologies, suggested by string/M-theory, may provide an alternative to standard inflation...
In this note, I derive the Chandrasekhar instability of a fluid sphere in ($N$+1)-dimensional Schwar...
We study the simplest two-body problem in asymptotically anti-de Sitter spacetime: two, infinitely t...
Vacuum decay in de Sitter space is a process of great physical interest, as it allows to rule out co...
Cosmological acceleration is difficult to accommodate in theories of fundamental interactions involv...
We start a systematic investigation of possible isometries of the asymptotically de Sitter solutions...
A thin shell of lightlike dust with its own gravitational field is studied in the special case of sp...
We consider a system representing self-gravitating balls of dust in an expanding Universe. It is dem...
We study the dynamics of a spherically symmetric dust shell separating two spacetime domains, the 'i...
We consider two spatially flat Friedmann-Robertson-Walker spacetimes divided by a timelike thin shel...
Gravitational equilibria of low density dust clouds imbedded in plasma background are studied. These...
Milne-like spacetimes are a class of $k = -1$ FLRW spacetimes which admit continuous spacetime exten...
We analyze the configuration of charged dust in the context of the higher dimensional and higher cur...
We give a comparative description of monopole and electrically charged spherically symmetric dust th...
ABSTRACT. A class of spherical collapsing exact solutions with electromagnetic charge is derived. Th...
Bouncing cosmologies, suggested by string/M-theory, may provide an alternative to standard inflation...
In this note, I derive the Chandrasekhar instability of a fluid sphere in ($N$+1)-dimensional Schwar...
We study the simplest two-body problem in asymptotically anti-de Sitter spacetime: two, infinitely t...
Vacuum decay in de Sitter space is a process of great physical interest, as it allows to rule out co...
Cosmological acceleration is difficult to accommodate in theories of fundamental interactions involv...
We start a systematic investigation of possible isometries of the asymptotically de Sitter solutions...
A thin shell of lightlike dust with its own gravitational field is studied in the special case of sp...