2021/10/09 by Alfredo Herrera–Aguilar, Alfredo Herrera-Aguilar, Joannis E. Paschalis +5 · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #High Energy Physics - Theory (hep-th) #Particle physics theoretical and experimental studies #hep-th
paper · pdf · doi:10.48550/arxiv.2110.04445
12 pages in latex, 4 figures
arxiv created 2021/10/09 · openalex publication_date 2021/10/09 · arxiv updated 2021/10/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We present a novel family of asymptotically Schrodinger hyperscaling violating black holes with a generic dynamical critical exponent and an arbitrary number of spacetime dimensions. This black hole family represents a solution within the Einstein-Maxwell-scalar setup with a self-interaction scalar potential where the Maxwell field is coupled to the scalar field. Through an analysis of the curvature invariants it is observed that this configuration is asymptotically regular for different ranges of the hyperscaling violating exponent. Furthermore, the above mentioned solution constitutes a gravitational candidate for describing field theories with hyperscaling violating Schrodinger symmetry at finite temperature within the framework of the Gravity/Condensed Matter Theory correspondence.