Self-energy in the Gott-Hiscock space-time-Hiscock
cosmic string space-time. The self-energy continuously falls down outward from the
string's center
Particle self-action effects in a gravitational field-thickness
cosmic strings, as well as of a point global monopole are discussed. Some effects related to particle
A remark on bound states in conical spacetime of infinitely thin straight
cosmic string owing to self-interaction forces. It is shown that there are no bound
Static, Cylindrically Symmetric Perfect Fluid Configurations into consideration the types of fluids which are now actively studied in cosmology (dark matter,
cosmic strings Approximate Extension of the Lorentz Symmetry up to Conformal in the Limit of Ultrahigh Energies explanations of this limit without using any kind of so-called “new physics” (e.g., “
cosmic strings” etc
Horizons in matter: Black hole hair versus null big bang between 0 and -1, in particular a gas of disordered
cosmic strings (w = -1/3). If the cosmological
General static black holes in matter/3, the value known for a gas of disordered
cosmic strings. An admixture of 'vacuum matter', characterized by w
Compact and extended objects from self-interacting phantom fields: phantom balls, traversable wormholes, phantom
cosmic strings, and "phantom" domain walls. These four
Particle self-action effects in a gravitational field-thickness
cosmic strings, as well as of a point global monopole are discussed. Some effects related to particle