Classical defects in higher-dimensional Einstein gravity coupled to nonlinear $\sigma$-models
Ilham Prasetyo, Handhika S. Ramadhan

TL;DR
This paper constructs and analyzes higher-dimensional black hole solutions coupled with nonlinear sigma-model defects, revealing unique horizon structures, asymptotic behaviors, and conditions for extremal solutions in various cosmological constant scenarios.
Contribution
It introduces noncanonical kinetic terms in higher-dimensional sigma-model coupled gravity, generalizing known monopole solutions and exploring their black hole and factorized spacetime configurations.
Findings
Existence of black hole solutions with deficit angles and multiple horizons.
Classification of extremal black holes in different dimensions and cosmological constants.
Identification of factorized solutions with product topologies.
Abstract
We construct solutions of higher-dimensional Einstein gravity coupled to nonlinear -model with cosmological constant. The -model can be perceived as exterior configuration of a spontaneously-broken global higher-codimensional "monopole". Here we allow the kinetic term of the -model to be noncanonical; in particular we specifically study a quadratic-power-law type. This is some possible higher-dimensional generalization of the Bariola-Vilenkin (BV) solutions with -global monopole studied recently. The solutions can be perceived as the exterior solution of a black hole swallowing up noncanonical global defects. Even in the absence of comological constant its surrounding spacetime is asymptotically non-flat; it suffers from deficit solid angle. We discuss the corresponding horizons. For in there can exist three extremal conditions (the…
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