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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

The Cylindrical Symmetric Configurations of the Interacting Scalar and Spinor Fields with Regard of Ideal Fluid used at present in cosmology (dark matter, cosmic strings, domain walls, quintessential, cosmic vacuum

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

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