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Similar

A. Kandus, K. E. Kunze and C. G. Tsagas, “Primordial magnetogenesis,” Phys. Rept. 505
Original
2011
Cited alongside, same era.
C. Deffayet, X. Gao, D. A. Steer and G. Zahariade, “From k-essence to generalised Galileons,” Phys. Rev. D 84
Original
2011
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T. Fujita and S. Mukohyama, “Universal upper limit on inflation energy scale from cosmic magnetic field,” JCAP 1210
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2012
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2012
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T. Kahniashvili, A. Brandenburg, L. Campanelli, B. Ratra and A. G. Tevzadze, “Evolution of inflation-generated magnetic field through phase transitions,” Phys. Rev. D 86

Then

P. A. R. Ade et al
Original
2014
Later among the works it cites.
W. Chen, J. H. Buckley and F. Ferrer, “Search for GeV γ \gamma -Ray Pair Halos Around Low Redshift Blazars,” Phys. Rev. Lett. 115
Original
2015
Later among the works it cites.
G. Tasinato, “A scenario for inflationary magnetogenesis without strong coupling problem,” JCAP 1503
Original
2015
Later among the works it cites.
T. Fujita, R. Namba, Y. Tada, N. Takeda and H. Tashiro, “Consistent generation of magnetic fields in axion inflation models,” JCAP 1505
Original
2015
Later among the works it cites.
K. Subramanian, “The origin, evolution and signatures of primordial magnetic fields,” Rept. Prog. Phys. 79

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2016

Stealth magnetic field in de Sitter spacetime

Mukohyama, Shinji

Understand

In the context of a U(1) gauge theory non-minimally coupled to scalar-tensor gravity, we find a cosmological attractor solution that represents a de Sitter universe with a homogeneous magnetic field.

The solution fully takes into account backreaction of the magnetic field to the geometry and the scalar field.
Such a solution is made possible by scaling-type global symmetry and fine-tuning of two parameters of the theory.
If the fine-tuning is relaxed then the solution is deformed to an axisymmetric Bianchi type-I universe with constant curvature invariants, a homogeneous magnetic field and a homogeneous electric field.