Comparison of magnetic flux tube and cosmic string behavior in Kerr metric |
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Authors: | SA Dyadechkin VS Semenov HK Biernat T Penz |
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Institution: | 1. Institute of Physics, State University St. Petersburg, St. Petersburg 198504, Russia;2. Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, A–8042 Graz, Austria;3. Institute of Physics, University of Graz, Universitätsplatz 5, A–8010 Graz, Austria;4. INAF–Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy |
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Abstract: | Cosmic strings are topological defects which were generated at a transition phase of the very early Universe and are probably responsible for large-scale structure forming. However, they may pull through all history and exist in the recent epoch. Thus, they can have influence for the recent Universe interacting with different objects. We consider the cosmic string behavior in the vicinity of a spinning black hole by means of a numerical simulation. Here we present preliminary results of this work via a comparison of cosmic string and magnetic flux tube behavior in the Kerr metric. Such an approach follows from the similarity of the equations which describe these objects. Therefore, many aspects of this behavior may be comparable. |
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Keywords: | Magnetic flux tube Cosmic string Kerr black hole Relativistic jet |
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