Journal Article10.1103/PHYSREVD.34.944
Superconducting cosmic strings
106
TL;DR: In this article, the authors proposed a string model for two recently discovered radio sources, the ''thread'' in the galactic center and the source G357.7-0.1, and predict that the filaments in these sources should move at relativistic speeds.
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Abstract: Superconducting loops of string formed in the early Universe, if they are relatively light, can be an important source of relativistic particles in the Galaxy. They can be observed as sources of synchrotron radiation at centimeter wavelengths. We propose a string model for two recently discovered radio sources, the ``thread'' in the galactic center and the source G357.7-0.1, and predict that the filaments in these sources should move at relativistic speeds. We also consider superheavy superconducting strings, and the possibility that they be observed as extragalactic radio sources.
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Citations
Cosmic strings
M. B. Hindmarsh,T. W. B. Kibble +1 more
- 19 Nov 1994
TL;DR: Cosmic strings provide a bridge between the physics of the very small and the very large They are predicted by some unified theories of particle interactions If they exist, they may help to explain some of the largest-scale structures seen in the Universe today as mentioned in this paper.
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Ultra-High-Energy Cosmic Rays
TL;DR: In this article, the authors review the important progress made in recent years towards understanding the experimental data on ultra-high-energy (E ≳ 1 0 9 GeV ) cosmic rays.
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A Radio Polarimetric Study of the Galactic Center Threads
TL;DR: In this article, the authors used the very large array (VLA) to carry out a multifrequency, polarimetric study of the non-thermal filaments (NTFs), G0.08+0.15, and G359.09, also known as the Northern and Southern Threads (Morris & Yusef-Zadeh 1985).
142
The physics of vortex superconductivity. II
Richard L. Davis,E. P. S. Shellard +1 more
Abstract: The effect of charge on a vortex world-sheet is examined. The relationship between world-sheet charge, winding number, and the flow of momentum along the vortex is illuminated. Full solutions for bosonic field and current profiles are obtained numerically. Both the string energy per unit length and tension are calculated. As an application stationary circular string solutions are studied. We find that except possibly for extreme cases rings stabilized by winding number alone do not exist. The role of angular momentum in stabilizing a ring is then discussed, emphasizing its model independent nature, and it is shown that in this case stationary spinning ring solutions, called vortons, are easily found. In a cosmological setting this can lead to a massive overdensity of vortons equivalent to a monopole problem.
137
Duality relation between charged elastic strings and superconducting cosmic strings
TL;DR: In this article, the mechanical properties of macroscopic electromagnetically coupled string models in a flat or curved background are treated using a covariant formalism allowing the construction of a duality transformation that relates the category of uniform “electric” string models, constructed as the (nonconducting) charged generalisation of ordinary uncoupled (violin type) elastic strings, to a category of “magnetic" string models comprising recently discussed varieties of superconducting cosmic strings.
121
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George B. Rybicki,Alan P. Lightman +1 more
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TL;DR: Inverse square law for a uniformly bright sphere as discussed by the authors is used to define specific intensity and its moments, which is defined as the specific intensity or brightness of a sphere in terms of specific intensity.
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TL;DR: The formation, physical properties and the cosmological evolution of various defects are reviewed, including the string scenario of galaxy formation and possible observational effects of strings.
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Roman Jackiw,Paolo Rossi +1 more
TL;DR: In this paper, the authors suggest that a complete description of the fermion-vortex system should include a fermanion-scalar field interaction. And they show that an index theorem exists for this Dirac equation on the non-compact space R 2.
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