2019/03/20 by Martin Zofka · 1 citation
Physics and Astronomy · #gr-qc #msc:83C15 #msc:83C22 #msc:83C50
paper · pdf · doi:10.1103/physrevd.99.044058
published as Phys. Rev. D 99, 044058 (2019) · 3 pages
arxiv created 2019/03/20 · arxiv updated 2019/03/21
We generalize the well-known Bonnor-Melvin solution of the Einstein-Maxwell equations to the case of a non-vanishing cosmological constant. The spacetime is again cylindrically symmetric and static but, unlike the original solution, it truly represents a homogeneous magnetic field.