Stellar Modelling of Compact Stars: Ultra dense cosmic structures in relativistic gravity - Brossura
Sinossi
The extreme laboratories of the universe demand physics beyond classical limits. This volume rigorously investigates the theoretical modeling of super-dense compact stars. By solving the Einstein Field Equations and their extensions, it constructs observationally consistent models accounting for pressure anisotropy, exotic matter, and modified gravity.Key explorations include:- Dark Energy Stabilization: Uses an embedding class-one formalism to show how repulsive dark energy interacting with baryonic matter acts as a dynamic shield against gravitational collapse.- Electromagnetic Dynamics: Applies a Gaussian density profile to the Einstein-Maxwell equations to model charge accretion, revealing phenomena like spin retardation and force field shifting.- Modified Gravity: Simulates the massive pulsar PSR J0952-0607 using the vanishing complexity condition in f(R,T) gravity, proving matter-geometry coupling allows for denser, stable cores.Verified against fundamental stability criteria, causality bounds, and standard energy conditions, this text provides a robust, physically motivated guide to decoding the densest stellar remnants in the cosmos.
Le informazioni nella sezione "Riassunto" possono far riferimento a edizioni diverse di questo titolo.
Informazioni sull?autore
Theoretical Physicists Dr. Kumar Gaurav Sagar and Dr. Shweta Saklany specialize in Relativistic Astrophysics and Cosmology whereas Dr. Neeraj Pant, HoD is a renowned Mathematician known for his contribution in General Relativity & its applications. All authors are faculty at the prestigious National Defence Academy, Pune.
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Stellar Modelling of Compact Stars
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Paperback. Condizione: new. Paperback. The extreme laboratories of the universe demand physics beyond classical limits. This volume rigorously investigates the theoretical modeling of super-dense compact stars. By solving the Einstein Field Equations and their extensions, it constructs observationally consistent models accounting for pressure anisotropy, exotic matter, and modified gravity.Key explorations include: - Dark Energy Stabilization: Uses an embedding class-one formalism to show how repulsive dark energy interacting with baryonic matter acts as a dynamic shield against gravitational collapse.- Electromagnetic Dynamics: Applies a Gaussian density profile to the Einstein-Maxwell equations to model charge accretion, revealing phenomena like spin retardation and force field shifting.- Modified Gravity: Simulates the massive pulsar PSR J0952-0607 using the vanishing complexity condition in f(R, T) gravity, proving matter-geometry coupling allows for denser, stable cores.Verified against fundamental stability criteria, causality bounds, and standard energy conditions, this text provides a robust, physically motivated guide to decoding the densest stellar remnants in the cosmos. This item is printed on demand. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. Codice articolo 9786209860522
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Stellar Modelling of Compact Stars | Ultra dense cosmic structures in relativistic gravity
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Taschenbuch. Condizione: Neu. Stellar Modelling of Compact Stars | Ultra dense cosmic structures in relativistic gravity | Kumar Gaurav Sagar (u. a.) | Taschenbuch | Englisch | 2026 | LAP LAMBERT Academic Publishing | EAN 9786209860522 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu. Codice articolo 135194346
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Paperback. Condizione: new. Paperback. The extreme laboratories of the universe demand physics beyond classical limits. This volume rigorously investigates the theoretical modeling of super-dense compact stars. By solving the Einstein Field Equations and their extensions, it constructs observationally consistent models accounting for pressure anisotropy, exotic matter, and modified gravity.Key explorations include: - Dark Energy Stabilization: Uses an embedding class-one formalism to show how repulsive dark energy interacting with baryonic matter acts as a dynamic shield against gravitational collapse.- Electromagnetic Dynamics: Applies a Gaussian density profile to the Einstein-Maxwell equations to model charge accretion, revealing phenomena like spin retardation and force field shifting.- Modified Gravity: Simulates the massive pulsar PSR J0952-0607 using the vanishing complexity condition in f(R, T) gravity, proving matter-geometry coupling allows for denser, stable cores.Verified against fundamental stability criteria, causality bounds, and standard energy conditions, this text provides a robust, physically motivated guide to decoding the densest stellar remnants in the cosmos. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. Codice articolo 9786209860522
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Stellar Modelling of Compact Stars : Ultra dense cosmic structures in relativistic gravity
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LAP LAMBERT Academic Publishing, 2026
ISBN 10: 6209860524
ISBN 13: 9786209860522
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ISBN 13: 9786209860522
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