Bonnor-Melvin universe with a cosmological constant
Žofka Martin
We generalize the well-known Bonnor-Melvin solution of the Einstein-Maxwell equations to the case of a nonvanishing cosmological constant. The spacetime is again cylindrically symmetric and static but, unlike the original solution, it truly represents a homogeneous magnetic field.
| type: | article |
|---|
| journal: | Phys. Rev. D |
|---|
| volume: | 99 |
|---|
| pages: | 044058 |
|---|
| year: | 2019 |
|---|
| month: | 2 |
|---|
| eprint: | arXiv:1903.08563 |
|---|
| grants: | Sources of strong gravity and their astrophysical meaning, GAČR 17-13525S; 2017-2019; hlavní řešitel: Oldřich Semerák |
|---|