Schrödinger Symmetry in Spherically-symmetric Static Mini-superspaces with Matter Fields

Schrödinger symmetry emerged in a "fluid limit" from a full superspace to several mini-superspace models. We consider two spherically-symmetric static mini-superspace models with matter fields and verify the robustness of this emergent symmetry at the classical level: (i) Maxwell field with cosmological constant and (ii) n massless scalar fields. We develop a method based on canonical transformations and show that: for model (i), 3D Schrödinger symmetry emerges, and the solution is the (anti-) de Sitter Reissner-Nordström spacetime, and for model (ii), (2+n)D Schrödinger symmetry appears, and the solution is a generalized Janis-Newman-Winicour spacetime and its "interior", a Kantowski-Sachs type closed universe. In the matter decoupling limit, both cases lead to 2D Schrödinger symmetry in different lapse functions and mini-superspace coordinates, which implies the covariance of Schrödinger symmetry. Finally, we propose a physical interpretation of the symmetry under Hamiltonian constraints H and explain it with examples: Symmetry generators commuting with H map a solution to another one, while those non-commuting with H generate a new theory with the Schrödinger symmetry and the transformed configuration is a solution to the new theory. These support the robustness of the emergence of Schrödinger symmetry and open new possibilities for exploring quantum dynamics of matter and gravity based on the symmetry.