Static charged fluid spheres in general relativity: Exact interior solutions

 
9783639260892: Static charged fluid spheres in general relativity: Exact interior solutions
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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 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 Mathematics/Physics and to professional Mathematician/Physicist, with interest in exact interior solutions for charged fluid spheres.

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Kalikkuddy Komathiraj (author)
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Book Description Condition: New. Publisher/Verlag: VDM Verlag Dr. Müller | Exact interior solutions | 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 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 Mathematics/Physics and to professional Mathematician/Physicist, with interest in exact interior solutions for charged fluid spheres. | Format: Paperback | Language/Sprache: english | 162 gr | 112 pp. Seller Inventory # K9783639260892

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Book Description VDM Verlag Jun 2010, 2010. Taschenbuch. Condition: Neu. Neuware - 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 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 Mathematics/Physics and to professional Mathematician/Physicist, with interest in exact interior solutions for charged fluid spheres. 112 pp. Englisch. Seller Inventory # 9783639260892

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Book Description VDM Verlag Jun 2010, 2010. Taschenbuch. Condition: Neu. Neuware - 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 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 Mathematics/Physics and to professional Mathematician/Physicist, with interest in exact interior solutions for charged fluid spheres. 112 pp. Englisch. Seller Inventory # 9783639260892

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Book Description VDM Verlag. Paperback. Condition: New. 112 pages. Dimensions: 8.7in. x 5.9in. x 0.3in.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 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. This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN. Paperback. Seller Inventory # 9783639260892

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Book Description VDM Verlag, Germany, 2010. Paperback. Condition: New. Language: English . Brand New Book ***** Print on Demand *****.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 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 Mathematics/Physics and to professional Mathematician/Physicist, with interest in exact interior solutions for charged fluid spheres. Seller Inventory # AAV9783639260892

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