Static charged fluid spheres in general relativity

✅ In recent years a number of authors have found 🔍️ solutions to the Einstein-Maxwell field 🏑 equations for static gravitational fields 🏑 with isotropic matter. These solutions may be utilized to model a charged relativistic star ⭐️ as they are matchable to the Reissner-Nordstrom exterior at the boundary. It is for this reason that many investigators use a variety of techniques to attain exact solutions. This book 📚️ provides exact solutions to the isotropic Einstein-Maxwell system that model the interior of relativistic stars ⭐️. The field 🏑 equations are transformed to simpler forms; the integration of the system is reduced to solving the condition of pressure isotropy. New 🆕 classes of solutions of linearly independent functions are obtained in terms of special and ➕ elementary functions for different spatial geometries. In addition, two 2️⃣ exact analytical solutions describing the interior of a charged strange quark star ⭐️ are obtained by applying the MIT bag 👜 equation of state. This book 📚️ is addressed to graduate 👨‍🎓️ students 👨‍🎓️ in MathematicsPhysics and ➕ to professional MathematicianPhysicist, with interest in exact interior solutions for charged fluid spheres.

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