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.
"synopsis" may belong to another edition of this title.
Seller: Grand Eagle Retail, Bensenville, IL, U.S.A.
Paperback. Condition: 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. Seller Inventory # 9786209860522
Seller: California Books, Miami, FL, U.S.A.
Condition: New. Seller Inventory # I-9786209860522
Seller: PBShop.store UK, Fairford, GLOS, United Kingdom
PAP. Condition: New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000. Seller Inventory # L0-9786209860522
Quantity: Over 20 available
Seller: PBShop.store US, Wood Dale, IL, U.S.A.
PAP. Condition: New. New Book. Shipped from UK. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000. Seller Inventory # L0-9786209860522
Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany
Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware 212 pp. Englisch. Seller Inventory # 9786209860522
Seller: preigu, Osnabrück, Germany
Taschenbuch. Condition: 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: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu Print on Demand. Seller Inventory # 135194346
Seller: CitiRetail, Stevenage, United Kingdom
Paperback. Condition: 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. Seller Inventory # 9786209860522
Quantity: 1 available
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 212 pp. Englisch. Seller Inventory # 9786209860522
Seller: AHA-BUCH GmbH, Einbeck, Germany
Taschenbuch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering. Seller Inventory # 9786209860522
Seller: Books Puddle, New York, NY, U.S.A.
Condition: New. Seller Inventory # 26406575739