Roberto Capuzzo Dolcetta (57 results)

Hardcover. Condition: Très bon. Ancien livre de bibliothèque. Edition 2000. Ammareal reverse jusqu'à 15% du prix net de cet article à des organisations caritatives. ENGLISH DESCRIPTION Book Condition: Used, Very good. Former library book. Edition 2000. Ammareal gives back up to 15% of this item's net price to charity organizations.…

Hardcover. Condition: Très bon. Edition 2000. Ammareal reverse jusqu'à 15% du prix net de cet article à des organisations caritatives. ENGLISH DESCRIPTION Book Condition: Used, Very good. Edition 2000. Ammareal gives back up to 15% of this item's net price to charity organizations.

Hardcover. Condition: Très bon. Légères traces d'usure sur la couverture. Edition 2000. Ammareal reverse jusqu'à 15% du prix net de cet article à des organisations caritatives. ENGLISH DESCRIPTION Book Condition: Used, Very good. Slight signs of wear on the cover. Edition 2000. Ammareal gives back up to 15% of this item's net price to charity organizations.…

Condition: New.

Paperback or Softback. Condition: New. Physical Processes in Fragmentation and Star Formation: Proceedings of the Workshop on 'Physical Processes in Fragmentation and Star Formation', Held. Book.

Condition: New.

Condition: leido. Bravo. 1ª ed., 1ª imp. edición. rústica. 94.

Condition: Good. 1990th Edition. Former library copy. Pages intact with minimal writing/highlighting. The binding may be loose and creased. Dust jackets/supplements are not included. Includes library markings. Stock photo provided. Product includes identifying sticker. Better World Books: Buy Books. Do Good. …

Hardcover. Condition: Very Good. No Jacket. May have limited writing in cover pages. Pages are unmarked. ~ ThriftBooks: Read More, Spend Less.

Condition: New.

Condition: New. In English.

Condition: As New. Unread book in perfect condition.

Gr.-8°, Original Hardcover. 1. ed. Numerous illustr., XVII, 469 p. Shelfmark on spine, stamp on title, otherwise very fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Condition: Used: Like New. libro nuovo. Attenzione la copertina è leggermente rovinata a causa della giacenza su scaffale. Adesivo non removibile sul piatto anteriore. Consegna in 24/48 h. 56 p6.

Condition: New. pp. 492.

Hardcover. Condition: new. Hardcover. This book offers a readily comprehensible introduction to classical Newtonian gravitation and potential theory, which are fundamental for understanding classical mechanics and particularly relevant to astrophysics. This enlarged and updated second edition introduces two new chapters, various newly developed exercises, and a comprehensive index. The opening chapter reviews essential elements of vector calculus and analysis, providing the formalism used in subsequent chapters. In Chapter 2, the theory of classical Newtonian gravity for a single point mass and a generic number N of point masses is presented and discussed, extending naturally to the continuous case. Chapter 3 addresses the paradigmatic case of spherical symmetry in mass density distribution (central force), introducing the useful tool of qualitative motion analysis. Chapter 4 deals with astrophysical applications, like, for instance the Jeans theory of gravitational instability. The following chapter discusses the general case of non-symmetric mass density distribution and develop classical potential theory, incorporating elements of harmonic theory, which is essential for understanding the series development of the gravitational potential. Finally, Chapter 6 discusses some relevant differences between Newtonian and relativistic gravitation. Examples and exercises throughout the book clarify various aspects of the theory presented in the book.The book is aimed at those progressing beyond an initial bachelors degree toward a masters degree and a Ph.D. It is also a valuable resource for postgraduates and active researchers in the field. The following chapter discusses the general case of non-symmetric mass density distribution and develop classical potential theory, incorporating elements of harmonic theory, which is essential for understanding the series development of the gravitational potential. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.…

Paperback. Condition: Brand New. 492 pages. 9.25x6.10x1.11 inches. In Stock.

Condition: New.

Condition: Wie Neu. Zustandsbeschreibung: leicht berieben/slightly rubbed. XII,136 Seiten mit 19 Farb- und 7 s/w-Abb., gebunden (UNITEXT for Physics/Springer-Verlag 2023). Statt EUR 85,59. Gewicht: 375 g - Gebunden/Gebundene Ausgabe.

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Recent years have witnessed the expansion and multiplication of the observations of star formation and fragmentation accompanied by a consequent growth in the study of the underlying physical processes, the chemistry, the sites, the times, etc. Moreover, recent studies have shown that the formation of stars is likely to share many features with the formation of other self-gravitating objects. The present volume, therefore, discusses the formation of such objects in a systematic and comparative manner. …

Hardcover. Condition: new. Hardcover. This book is exceptional in providing an up-to-date, but compact, introduction to the field of hydrodynamics and fluid dynamics that is both sufficiently comprehensive and easy to read. It covers all the elements of compressible and incompressible fluid dynamics, from the basic concepts through to the constituent equations and their applications. Fluid flows in different environments are thoroughly discussed, and specific aspects such as dissipation, turbulence, shock waves, and blast waves receive detailed attention. The book contains many exercises and draws attention to numerical solutions to specific problems. The book is ideal for undergraduate and graduate students and young researchers in physics, astrophysics, mathematics (pure and applied), and engineering. As this book is intended for a wide audience, the mathematical prerequisites are kept to a low level. This book is exceptional in providing an up-to-date, but compact, introduction to the field of hydrodynamics and fluid dynamics that is both sufficiently comprehensive and easy to read. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.…

Hardcover. Condition: new. Hardcover. This book offers a readily comprehensible introduction to classical Newtonian gravitation and potential theory, which are fundamental for understanding classical mechanics and particularly relevant to astrophysics. This enlarged and updated second edition introduces two new chapters, various newly developed exercises, and a comprehensive index. The opening chapter reviews essential elements of vector calculus and analysis, providing the formalism used in subsequent chapters. In Chapter 2, the theory of classical Newtonian gravity for a single point mass and a generic number N of point masses is presented and discussed, extending naturally to the continuous case. Chapter 3 addresses the paradigmatic case of spherical symmetry in mass density distribution (central force), introducing the useful tool of qualitative motion analysis. Chapter 4 deals with astrophysical applications, like, for instance the Jeans theory of gravitational instability. The following chapter discusses the general case of non-symmetric mass density distribution and develop classical potential theory, incorporating elements of harmonic theory, which is essential for understanding the series development of the gravitational potential. Finally, Chapter 6 discusses some relevant differences between Newtonian and relativistic gravitation. Examples and exercises throughout the book clarify various aspects of the theory presented in the book.The book is aimed at those progressing beyond an initial bachelors degree toward a masters degree and a Ph.D. It is also a valuable resource for postgraduates and active researchers in the field. The following chapter discusses the general case of non-symmetric mass density distribution and develop classical potential theory, incorporating elements of harmonic theory, which is essential for understanding the series development of the gravitational potential. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.…

Taschenbuch. Condition: Neu. Physics of Fluids | Roberto A. Capuzzo Dolcetta | Taschenbuch | UNITEXT for Physics | xii | Englisch | 2025 | Springer | EAN 9783031307522 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. …

Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book offers a readily comprehensible introduction to classical Newtonian gravitation and potential theory, which are fundamental for understanding classical mechanics and particularly relevant to astrophysics. This enlarged and updated second edition introduces two new chapters, various newly developed exercises, and a comprehensive index. The opening chapter reviews essential elements of vector calculus and analysis, providing the formalism used in subsequent chapters. In Chapter 2, the theory of classical Newtonian gravity for a single point mass and a generic number N of point masses is presented and discussed, extending naturally to the continuous case. Chapter 3 addresses the paradigmatic case of spherical symmetry in mass density distribution (central force), introducing the useful tool of qualitative motion analysis. Chapter 4 deals with astrophysical applications, like, for instance the Jeans theory of gravitational instability. The following chapter discusses the general case of non-symmetric mass density distribution and develop classical potential theory, incorporating elements of harmonic theory, which is essential for understanding the series development of the gravitational potential. Finally, Chapter 6 discusses some relevant differences between Newtonian and relativistic gravitation. Examples and exercises throughout the book clarify various aspects of the theory presented in the book.The book is aimed at those progressing beyond an initial bachelor s degree toward a master s degree and a Ph.D. It is also a valuable resource for postgraduates and active researchers in the field.…

Condition: New. 2023rd edition NO-PA16APR2015-KAP.

Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book is exceptional in providing an up-to-date, but compact, introduction to the field of hydrodynamics and fluid dynamics that is both sufficiently comprehensive and easy to read. It covers all the elements of compressible and incompressible fluid dynamics, from the basic concepts through to the constituent equations and their applications. Fluid flows in different environments are thoroughly discussed, and specific aspects such as dissipation, turbulence, shock waves, and blast waves receive detailed attention. The book contains many exercises and draws attention to numerical solutions to specific problems. The book is ideal for undergraduate and graduate students and young researchers in physics, astrophysics, mathematics (pure and applied), and engineering. As this book is intended for a wide audience, the mathematical prerequisites are kept to a low level.…

Condition: New.

Hardcover. Condition: Brand New. reprint edition. 136 pages. 9.25x6.25x0.75 inches. In Stock.

Condition: Sehr gut. Zustand: Sehr gut | Seiten: 492 | Sprache: Englisch | Produktart: Bücher | Recent years have witnessed the expansion and multiplication of the observations of star formation and fragmentation accompanied by a consequent growth in the study of the underlying physical processes, the chemistry, the sites, the times, etc. Moreover, recent studies have shown that the formation of stars is likely to share many features with the formation of other self-gravitating objects. The present volume, therefore, discusses the formation of such objects in a systematic and comparative manner. …

Hardcover. Condition: new. Hardcover. This book offers a readily comprehensible introduction to classical Newtonian gravitation and potential theory, which are fundamental for understanding classical mechanics and particularly relevant to astrophysics. This enlarged and updated second edition introduces two new chapters, various newly developed exercises, and a comprehensive index. The opening chapter reviews essential elements of vector calculus and analysis, providing the formalism used in subsequent chapters. In Chapter 2, the theory of classical Newtonian gravity for a single point mass and a generic number N of point masses is presented and discussed, extending naturally to the continuous case. Chapter 3 addresses the paradigmatic case of spherical symmetry in mass density distribution (central force), introducing the useful tool of qualitative motion analysis. Chapter 4 deals with astrophysical applications, like, for instance the Jeans theory of gravitational instability. The following chapter discusses the general case of non-symmetric mass density distribution and develop classical potential theory, incorporating elements of harmonic theory, which is essential for understanding the series development of the gravitational potential. Finally, Chapter 6 discusses some relevant differences between Newtonian and relativistic gravitation. Examples and exercises throughout the book clarify various aspects of the theory presented in the book.The book is aimed at those progressing beyond an initial bachelors degree toward a masters degree and a Ph.D. It is also a valuable resource for postgraduates and active researchers in the field. The following chapter discusses the general case of non-symmetric mass density distribution and develop classical potential theory, incorporating elements of harmonic theory, which is essential for understanding the series development of the gravitational potential. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.…