Exact correspondence maps Einstein-scalar-Maxwell solutions to gauged Skyrme-Maxwell-Einstein solutions with baryonic charge, illustrated by a Kerr-Newman-like example where baryonic charge quantization enforces quantization of the Kerr rotation parameter.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
gr-qc 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Numerical non-perturbative stationary vacuum ring wormhole solutions invariant under throat reflections, with slow-rotation M ~ J^2, fast-rotation J = M^2, and limits mimicking extremal Kerr.
citing papers explorer
-
Generation of gravitating solutions with Baryonic charge from Einstein-Scalar-Maxwell seeds
Exact correspondence maps Einstein-scalar-Maxwell solutions to gauged Skyrme-Maxwell-Einstein solutions with baryonic charge, illustrated by a Kerr-Newman-like example where baryonic charge quantization enforces quantization of the Kerr rotation parameter.
-
Stationary generalizations for the vacuum ring wormhole
Numerical non-perturbative stationary vacuum ring wormhole solutions invariant under throat reflections, with slow-rotation M ~ J^2, fast-rotation J = M^2, and limits mimicking extremal Kerr.