Cosmological Einstein-Skyrme solutions with non-vanishing topological charge
arXiv:1703.04860 · doi:10.1103/PhysRevD.95.065032
Abstract
Time-dependent analytic solutions of the Einstein-Skyrme system --gravitating Skyrmions--, with topological charge one are analyzed in detail. In particular, the question of whether these Skyrmions reach a spherically symmetric configuration for is discussed. It is shown that there is a static, spherically symmetric solution described by the Ermakov-Pinney system, which is fully integrable by algebraic methods. For this spherically symmetric solution is found to be in a "neutral equilibrium" under small deformations, in the sense that under a small squashing it would neither blow up nor dissapear after a long time, but it would remain finite forever (plastic deformation). Thus, in a sense, the coupling with Einstein gravity spontaneously breaks the spherical symmetry of the solution. However, in spite of the lack of isotropy, for (and ) the space time is locally flat and the anisotropy of the Skyrmion only reflects the squashing of spacetime.
arXiv comment12 pages, 6 figures, to appear in Phys. Rev. D
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