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Magnetism in the Early Universe

Published online by Cambridge University Press:  03 March 2020

Tina Kahniashvili ,
Axel Brandenburg ,
Arthur Kosowsky ,
Sayan Mandal  and
Alberto Roper Pol
Tina Kahniashvili
Affiliation:
Department of Physics, Carnegie Mellon University, USA Abastumani Astrophysical Observatory, Ilia State University, Georgia
Axel Brandenburg
Affiliation:
Department of Physics, Carnegie Mellon University, USA Nordita, KTH Royal Institute of Technology & Stockholm University; Department of Astronomy, Stockholm University, Sweden; and JILA, University of Colorado at Boulder, USA Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, USA
Arthur Kosowsky
Affiliation:
Department of Physics and Astronomy and PITT PACC, University of Pittsburgh, USA
Sayan Mandal
Affiliation:
Department of Physics, Carnegie Mellon University, USA Abastumani Astrophysical Observatory, Ilia State University, Georgia
Alberto Roper Pol
Affiliation:
Abastumani Astrophysical Observatory, Ilia State University, Georgia Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, USA Department of Aerospace Engineering, University of Colorado at Boulder, USA
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Abstract

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Blazar observations point toward the possible presence of magnetic fields over intergalactic scales of the order of up to ∼1 Mpc, with strengths of at least ∼10−16 G. Understanding the origin of these large-scale magnetic fields is a challenge for modern astrophysics. Here we discuss the cosmological scenario, focussing on the following questions: (i) How and when was this magnetic field generated? (ii) How does it evolve during the expansion of the universe? (iii) Are the amplitude and statistical properties of this field such that they can explain the strengths and correlation lengths of observed magnetic fields? We also discuss the possibility of observing primordial turbulence through direct detection of stochastic gravitational waves in the mHz range accessible to LISA.

Keywords

Early UniverseCosmic Magnetic FieldsTurbulenceGravitational Waves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 295 - 298
Copyright
© International Astronomical Union 2020

References

Brandenburg, A., Enqvist, K. & Olesen, P. 1996, Phys. Rev. D, 54, 1291 CrossRefGoogle Scholar
Brandenburg, A. & Kahniashvili, T. 2017, Phys. Rev. Lett., 118, 055102 CrossRefGoogle Scholar
Brandenburg, A. & Dobler, W. 2002, Comput. Phys. Commun., 147, 471 CrossRefGoogle Scholar
Brandenburg, A., Kahniashvili, T., Mandal, M., Roper Pol, A., Tevzadze, A. & Vachaspati, T. 2017, Phys. Rev. D, 96, 123528 CrossRefGoogle Scholar
Caprini, C. & Figueroa, D. G. 2018, Class. Quant. Grav., 35, 163001 CrossRefGoogle Scholar
Cornwall, J. M. 1997, Phys. Rev. D, 56, 6146 CrossRefGoogle Scholar
Christensson, M., Hindmarsh, M. & Brandenburg, A. 2001, Phys. Rev. E, 64, 056405 CrossRefGoogle Scholar
Deryagin, D., Grigoriev, D., Rubakov, V. & Sazhin, M. 1986, Mod. Phys. Lett. A, 1, 593 CrossRefGoogle Scholar
Dimopoulos, K. & Davis, A. C. 1997, Phys. Lett. B, 390, 87 CrossRefGoogle Scholar
Dolag, K., Kachelriess, M., Ostapchenko, S. & Tomas, R. 2011, Astrophys. J., 727, L4 CrossRefGoogle Scholar
Durrer, R. & Neronov, A. 2013, Astron. Astrophys. Rev., 21, 62 Google Scholar
Field, G. B. & Carroll, S. M. 2000, Phys. Rev. D, 62, 103008 CrossRefGoogle Scholar
Giovannini, M. & Shaposhnikov, M. E. 1998, Phys. Rev. D, 57, 2186 CrossRefGoogle Scholar
Giovannini, M. 2000, Phys. Rev. D, 61, 063004 CrossRefGoogle Scholar
Gogoberidze, G., Kahniashvili, T. & Kosowsky, A. 2007, Phys. Rev. D, 76, 083002 CrossRefGoogle Scholar
Jedamzik, K., Katalinic, V. & Olinto, A. V. 1998, Phys. Rev. D, 57, 3264 CrossRefGoogle Scholar
Kahniashvili, T., Kosowsky, A., Gogoberidze, G. & Maravin, Y. 2008, Phys. Rev. D, 78, 043003 CrossRefGoogle Scholar
Kahniashvili, T., Brandenburg, A., Tevzadze, A. G. & Ratra, B. 2010, Phys. Rev. D, 81, 123002 CrossRefGoogle Scholar
Kahniashvili, T. Brandenburg, A., Campanelli, L., Ratra, B. & Tevzadze, A. 2012, Phys. Rev. D, 86, 103005 CrossRefGoogle Scholar
Kahniashvili, T., Brandenburg, A. & Tevzadze, A. 2016, Phys. Scripta, 91, 104008 CrossRefGoogle Scholar
Kahniashvili, T. Brandenburg, A., Durrer, R., Tevzadze, A. & Yin, W. 2017, JCAP, 1712, 002 CrossRefGoogle Scholar
Kamionkowski, M., Kosowsky, A. & Turner, M. S. 1994, Phys. Rev. D, 49, 2837 CrossRefGoogle Scholar
Kosowsky, A., Mack, A. & Kahniashvili, T. 2002, Phys. Rev. D 66, 024030 CrossRefGoogle Scholar
Morrissey, D. E. & Ramsey-Musolf, M. J. 2012, New J. Phys., 14, 125003 CrossRefGoogle Scholar
Neronov, A. & Vovk, I. 2010, Science, 328, 73 CrossRefGoogle Scholar
Roper Pol, A., Brandenburg, A., Kahniashvili, T., Kosowsky, A. & Mandal, S. 2019a, Geophys. Astrophys. Fluid Dynam., arXiv:1807.05479Google Scholar
Roper Pol, A., Mandal, S., Brandenburg, A., Kahniashvili, T., & Kosowsky, A., 2019b, Phys. Rev. Lett. Submitted, arXiv:1903.08585Google Scholar
Smith, T. L. & Caldwell, R. 2017, Phys. Rev. D, 95, 044036 CrossRefGoogle Scholar
Subramanian, K. & Barrow, J. D. 1998, Phys. Rev. Lett., 81, 3575 CrossRefGoogle Scholar
Subramanian, K. 2016, Rept. Prog. Phys., 79, 076901 CrossRefGoogle Scholar
Vachaspati, T. 2001. Phys. Rev. Lett., 87, 251302 CrossRefGoogle Scholar
Vazza, F., Brüggen, M., Gheller, C., Hackstein, S., Wittor, D. & Hinz, P. M. 2017, Class. Quant. Grav., 34, 234001 CrossRefGoogle Scholar