This monograph presents a rigorous analysis of multilayered compact stars within Einstein's gravitational framework, extending beyond isotropic fluid models to incorporate pressure anisotropy, stratified interiors with exotic phases, and baryonic-dark energy coupling, thereby achieving a physically faithful description of supra-nuclear matter.Exact solutions of non-linear field equations are constructed using Tolman-Kuchowicz, Vaidya-Tikekar, Buchdahl-I, and biquadratic geometries, with physical admissibility ensured via Darmois-Israel matching conditions. Stability is systematically examined through the generalized Tolman-Oppenheimer-Volkoff equilibrium, causality bounds, energy conditions, and cracking criteria.Four observationally grounded configurations are developed: dark energy-admixed stars exhibiting enhanced stability and higher mass limits; Karmarkar-constrained models consistent with massive pulsars; a three-layered quark-condensate-neutron structure motivated by phase transitions; and a two-layered core-shell system revealing mesonic interface dynamics.
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Paperback. Etat : new. Paperback. This monograph presents a rigorous analysis of multilayered compact stars within Einstein's gravitational framework, extending beyond isotropic fluid models to incorporate pressure anisotropy, stratified interiors with exotic phases, and baryonic-dark energy coupling, thereby achieving a physically faithful description of supra-nuclear matter.Exact solutions of non-linear field equations are constructed using Tolman-Kuchowicz, Vaidya-Tikekar, Buchdahl-I, and biquadratic geometries, with physical admissibility ensured via Darmois-Israel matching conditions. Stability is systematically examined through the generalized Tolman-Oppenheimer-Volkoff equilibrium, causality bounds, energy conditions, and cracking criteria.Four observationally grounded configurations are developed: dark energy-admixed stars exhibiting enhanced stability and higher mass limits; Karmarkar-constrained models consistent with massive pulsars; a three-layered quark-condensate-neutron structure motivated by phase transitions; and a two-layered core-shell system revealing mesonic interface dynamics. This item is printed on demand. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. N° de réf. du vendeur 9786209783821
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware 196 pp. Englisch. N° de réf. du vendeur 9786209783821
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Taschenbuch. Etat : Neu. Multi-Layered Static Dense Stars in Einstein's Gravity | Applications of general relativity in modelling compact stars | Shweta Saklany (u. a.) | Taschenbuch | Englisch | 2026 | LAP LAMBERT Academic Publishing | EAN 9786209783821 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu Print on Demand. N° de réf. du vendeur 135057069
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -This monograph presents a rigorous analysis of multilayered compact stars within Einstein's gravitational framework, extending beyond isotropic fluid models to incorporate pressure anisotropy, stratified interiors with exotic phases, and baryonic-dark energy coupling, thereby achieving a physically faithful description of supra-nuclear matter.Exact solutions of non-linear field equations are constructed using Tolman-Kuchowicz, Vaidya-Tikekar, Buchdahl-I, and biquadratic geometries, with physical admissibility ensured via Darmois-Israel matching conditions. Stability is systematically examined through the generalized Tolman-Oppenheimer-Volkoff equilibrium, causality bounds, energy conditions, and cracking criteria.Four observationally grounded configurations are developed: dark energy-admixed stars exhibiting enhanced stability and higher mass limits; Karmarkar-constrained models consistent with massive pulsars; a three-layered quark-condensate-neutron structure motivated by phase transitions; and a two-layered core-shell system revealing mesonic interface dynamics.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 196 pp. Englisch. N° de réf. du vendeur 9786209783821
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Paperback. Etat : new. Paperback. This monograph presents a rigorous analysis of multilayered compact stars within Einstein's gravitational framework, extending beyond isotropic fluid models to incorporate pressure anisotropy, stratified interiors with exotic phases, and baryonic-dark energy coupling, thereby achieving a physically faithful description of supra-nuclear matter.Exact solutions of non-linear field equations are constructed using Tolman-Kuchowicz, Vaidya-Tikekar, Buchdahl-I, and biquadratic geometries, with physical admissibility ensured via Darmois-Israel matching conditions. Stability is systematically examined through the generalized Tolman-Oppenheimer-Volkoff equilibrium, causality bounds, energy conditions, and cracking criteria.Four observationally grounded configurations are developed: dark energy-admixed stars exhibiting enhanced stability and higher mass limits; Karmarkar-constrained models consistent with massive pulsars; a three-layered quark-condensate-neutron structure motivated by phase transitions; and a two-layered core-shell system revealing mesonic interface dynamics. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. N° de réf. du vendeur 9786209783821
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