Charged gravastars in modified Gauss–Bonnet gravity.

This work probes the influence of charge field on the unique stellar structure, regarded as gravastar, under the corrections of f () theory, i.e. (ℬ) theory, where is named as Gauss–Bonnet invariant. The gravastar has also been recognized as an alternate candidate of black hole structure and is illustrated by three distinct regions termed as (1) the exterior (2) the intermediate thin shell (3) the interior domain. We discussed the mathematical solutions for each of three regions separately with the assistance of different equation-of-states (EoS). The exterior charged vacuum domain is expressed by the Reissner–Nordström solution. The central region is illustrated by the EoS, i.e. a positive pressure of ultra-relativistic matter is equal to the energy density. Whereas, the interior domain reflects that the negative pressure is equal to energy density and manifests a non-attractive force over the central spherical shell. We deduce that in the context of ℬ theory, the nonsingular charged model with distinct physical features, such as energy, length, entropy, is physically viable and consistent. [ABSTRACT FROM AUTHOR]