Year: 2025
Type: article
Abstract: In this paper, we construct an exact solution of the S U ( N ) Einstein-Skyrme model in D = 4 space-time dimensions describing a charged and rotating black hole with toroidal horizon. Rotation is added by applying an improper coordinate transformation to the known static toroidal black hole with Skyrme hair, while the electric charge is supplemented by considering a U ( 1 ) gauge field interacting with Einstein gravity. We perform the thermal analysis in the grand canonical ensemble, explicitly showing the role that the flavor number plays. Some discussions about stability are also considered.
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Awards: G2463242031, G2949202400, THERMODYNAMIC PROPERTIES OF NUCLEAR PASTA PHASES IN THE LOW-ENERGY LIMIT OF QCD AT EQUILIBRIUM, G4377445928, FORTALECIMIENTO DE LA INVESTIGACION EN EL AREA DE GRAVITACION Y COSMOLOGIA Y LA DOCENCIA DE LA FACULTAD DE INGENIERIA DE LA UCSC, G6105535391, CONSERVATION LAWS IN GRAVITY UNDER FRAME TRANSFORMATIONS DUAL DIFFEOMORPHISMS AND NEW APPLICATIONS, CONSTRUCTING AND STABILIZING EXTENDED BLACK OBJECTS THROUGH MATTER FIELDS AND LIE GROUPS, ON THE SOLUTIONS AND ASYMPTOTIC STRUCTURE OF EXTENDED (SUPER)GRAVITY THEORIES WITH AND WITHOUT TORSION
OpenAlex ID: W4410121651