In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few so… mais…
In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity. Bücher, Hörbücher & Kalender / Bücher / Sachbuch / Naturwissenschaften / Mathematik, [PU: VDM Verlag Dr. Müller, Saarbrücken]<
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In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few so… mais…
In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity. Trade Books>Trade Paperback>Science>Mathematics>Mathematics, VDM Verlag Core >1<
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In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few so… mais…
In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity. Bücher / Naturwissenschaften, Medizin, Informatik & Technik / Mathematik, [PU: VDM Verlag Dr. Müller, Saarbrücken]<
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Paperback, [PU: VDM Verlag], In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the … mais…
Paperback, [PU: VDM Verlag], In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity., Mathematics<
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*Mathematics and Physics of Collapsing Stars* / Taschenbuch für 78.99 € / Aus dem Bereich: Bücher, Wissenschaft, Mathematik Medien > Bücher nein Buch (kartoniert) Hardcover;Naturwissensch… mais…
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In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few so… mais…
In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity. Bücher, Hörbücher & Kalender / Bücher / Sachbuch / Naturwissenschaften / Mathematik, [PU: VDM Verlag Dr. Müller, Saarbrücken]<
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In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few so… mais…
In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity. Trade Books>Trade Paperback>Science>Mathematics>Mathematics, VDM Verlag Core >1<
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In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few so… mais…
In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity. Bücher / Naturwissenschaften, Medizin, Informatik & Technik / Mathematik, [PU: VDM Verlag Dr. Müller, Saarbrücken]<
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Paperback, [PU: VDM Verlag], In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the … mais…
Paperback, [PU: VDM Verlag], In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity., Mathematics<
*Mathematics and Physics of Collapsing Stars* / Taschenbuch für 78.99 € / Aus dem Bereich: Bücher, Wissenschaft, Mathematik Medien > Bücher nein Buch (kartoniert) Hardcover;Naturwissensch… mais…
*Mathematics and Physics of Collapsing Stars* / Taschenbuch für 78.99 € / Aus dem Bereich: Bücher, Wissenschaft, Mathematik Medien > Bücher nein Buch (kartoniert) Hardcover;Naturwissenschaften, Medizin, Informatik, Technik;Mathematik, VDM Verlag Dr. Müller<
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In this book, we investigate the issue of the final fate of a gravitationally collapsing massive stars and the associated cosmic censorship problem. When the star is heavier than a few solar masses, it could undergo an endless gravitational collapse without achieving any equilibrium state. This happens when the star has exhausted its internal nuclear fuel which provides the outwards pressure against the inwards pulling gravitational forces. This remains one of the most outstanding open issues (Islam, 1992) in gravitation theory today. We discuss the essential features of spherically symmetric collapse and the final fate of a massive star which undergoes gravitational collapse. It is the spherically symmetric collapse of a homogenous dust cloud, as described by the Oppenheimer-Snyder model (1939), which led to the general concept of trapped surfaces collapsed to singularities. Our objective here is to discuss the above and such other related important questions concerning the global aspects of gravity, and also to discuss some applications of the results which are already available on the global structure of space-time singularity.
Dados detalhados do livro - Mathematics and Physics of Collapsing Stars Md. Haider Ali Biswas Author
EAN (ISBN-13): 9783639221329 ISBN (ISBN-10): 363922132X Livro de bolso Ano de publicação: 2010 Editor/Editora: VDM Verlag Core >1 204 Páginas Peso: 0,321 kg Língua: eng/Englisch
Livro na base de dados desde 2008-01-05T07:47:16-02:00 (Sao Paulo) Página de detalhes modificada pela última vez em 2024-04-17T18:00:42-03:00 (Sao Paulo) Número ISBN/EAN: 363922132X
Número ISBN - Ortografia alternativa: 3-639-22132-X, 978-3-639-22132-9 Ortografia alternativa e termos de pesquisa relacionados: Autor do livro: haider lenauer, oppenheimer Título do livro: when stars look down, the stars, many stars, physics and
