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A cosmic string is a hypothetical 1-dimensional topological defect in the fabric of spacetime. Cosmic strings are hypothesized to form when different regions of spacetime undergo phase changes, resulting in domain boundaries between the two regions when they meet. This is somewhat analogous to the boundaries that form between crystal grains in solidifying liquids, or the cracks that form when water freezes into ice.

Cosmic strings, if they exist, would be extremely thin with diameters on the same order as a proton. They would have immense density, however, and so would represent significant gravitational sources. A cosmic string 1.6 kilometers in length would exert more gravity than the Earth. Cosmic strings would form a network of loops in the early universe, and their gravity could have been responsible for the original clumping of matter into galactic superclusters.

A cosmic string's vibrations, which are thought to oscillate near the speed of light, can cause part of the string to snap off, and create a new string of any length. All cosmic strings have a finite lifespan due to decay via gravitational radiation.

Other types of topological defects in spacetime are domain walls, monopoles, and texture s.

External link

http://www.damtp.cam.ac.uk/user/gr/public/cs_interact.html

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Topics: Cosmic String, Cosmic Inflation, Cosmic Background Radiation...

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