Standard

Comparison of magnetic flux tube and cosmic string behavior in Kerr metric. / Dyadechkin, S. A.; Semenov, V. S.; Biernat, H. K.; Penz, T.

в: Advances in Space Research, Том 42, № 3, 05.08.2008, стр. 565-571.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Dyadechkin, SA, Semenov, VS, Biernat, HK & Penz, T 2008, 'Comparison of magnetic flux tube and cosmic string behavior in Kerr metric', Advances in Space Research, Том. 42, № 3, стр. 565-571. https://doi.org/10.1016/j.asr.2007.06.065

APA

Dyadechkin, S. A., Semenov, V. S., Biernat, H. K., & Penz, T. (2008). Comparison of magnetic flux tube and cosmic string behavior in Kerr metric. Advances in Space Research, 42(3), 565-571. https://doi.org/10.1016/j.asr.2007.06.065

Vancouver

Dyadechkin SA, Semenov VS, Biernat HK, Penz T. Comparison of magnetic flux tube and cosmic string behavior in Kerr metric. Advances in Space Research. 2008 Авг. 5;42(3):565-571. https://doi.org/10.1016/j.asr.2007.06.065

Author

Dyadechkin, S. A. ; Semenov, V. S. ; Biernat, H. K. ; Penz, T. / Comparison of magnetic flux tube and cosmic string behavior in Kerr metric. в: Advances in Space Research. 2008 ; Том 42, № 3. стр. 565-571.

BibTeX

@article{021e6c094458420a8c6546dee9811c45,
title = "Comparison of magnetic flux tube and cosmic string behavior in Kerr metric",
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. It turns out that the cosmic string behavior at an early stage copies the flux tube movement in some degree. Involved in differential rotation, the central part of the cosmic string starts to lose energy and angular momentum due to string braking. Stretching and twisting around the event horizon, the central part of the string gains negative energy in the ergosphere. To compensate these losses, positive energy is subsequently generated and apparently can be extracted from the ergosphere as in the flux tube case. Because of an increase of the numerical errors the code breaks down near the event horizon and only initial stages of the negative energy creation can be observed. In comparison with the cosmic string, further simulations of the flux tube behavior clearly demonstrate an energy extraction process which is attended by relativistic jet forming. Consequently, within the frame of direct analogy, we consider our result as the very beginning of cosmic string jet formation in Kerr geometry.",
keywords = "Cosmic string, Kerr black hole, Magnetic flux tube, Relativistic jet",
author = "Dyadechkin, {S. A.} and Semenov, {V. S.} and Biernat, {H. K.} and T. Penz",
year = "2008",
month = aug,
day = "5",
doi = "10.1016/j.asr.2007.06.065",
language = "English",
volume = "42",
pages = "565--571",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "3",

}

RIS

TY - JOUR

T1 - Comparison of magnetic flux tube and cosmic string behavior in Kerr metric

AU - Dyadechkin, S. A.

AU - Semenov, V. S.

AU - Biernat, H. K.

AU - Penz, T.

PY - 2008/8/5

Y1 - 2008/8/5

N2 - 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. It turns out that the cosmic string behavior at an early stage copies the flux tube movement in some degree. Involved in differential rotation, the central part of the cosmic string starts to lose energy and angular momentum due to string braking. Stretching and twisting around the event horizon, the central part of the string gains negative energy in the ergosphere. To compensate these losses, positive energy is subsequently generated and apparently can be extracted from the ergosphere as in the flux tube case. Because of an increase of the numerical errors the code breaks down near the event horizon and only initial stages of the negative energy creation can be observed. In comparison with the cosmic string, further simulations of the flux tube behavior clearly demonstrate an energy extraction process which is attended by relativistic jet forming. Consequently, within the frame of direct analogy, we consider our result as the very beginning of cosmic string jet formation in Kerr geometry.

AB - 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. It turns out that the cosmic string behavior at an early stage copies the flux tube movement in some degree. Involved in differential rotation, the central part of the cosmic string starts to lose energy and angular momentum due to string braking. Stretching and twisting around the event horizon, the central part of the string gains negative energy in the ergosphere. To compensate these losses, positive energy is subsequently generated and apparently can be extracted from the ergosphere as in the flux tube case. Because of an increase of the numerical errors the code breaks down near the event horizon and only initial stages of the negative energy creation can be observed. In comparison with the cosmic string, further simulations of the flux tube behavior clearly demonstrate an energy extraction process which is attended by relativistic jet forming. Consequently, within the frame of direct analogy, we consider our result as the very beginning of cosmic string jet formation in Kerr geometry.

KW - Cosmic string

KW - Kerr black hole

KW - Magnetic flux tube

KW - Relativistic jet

UR - http://www.scopus.com/inward/record.url?scp=44849097529&partnerID=8YFLogxK

U2 - 10.1016/j.asr.2007.06.065

DO - 10.1016/j.asr.2007.06.065

M3 - Article

AN - SCOPUS:44849097529

VL - 42

SP - 565

EP - 571

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 3

ER -

ID: 52654747