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出版商:
Springer
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出版日期:
2023-07-26
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售價:
$3,430
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貴賓價:
9.5 折
$3,259
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語言:
英文
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頁數:
136
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裝訂:
Hardcover - also called cloth, retail trade, or trade
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ISBN:
3031307496
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ISBN-13:
9783031307492
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相關分類:
物理學 Physics
商品描述
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.
商品描述(中文翻譯)
這本書在提供一個最新且簡潔的流體力學和流體動力學領域介紹方面非常出色，內容既全面又易於閱讀。它涵蓋了可壓縮和不可壓縮流體動力學的所有要素，從基本概念到組成方程及其應用。書中詳細討論了不同環境中的流體流動，並對耗散、湍流、衝擊波和爆炸波等特定方面給予了詳細的關注。書中包含許多練習題，並強調針對特定問題的數值解法。這本書非常適合物理學、天體物理學、數學（純數學和應用數學）以及工程學的本科生、研究生和年輕研究人員。由於這本書的讀者範圍廣泛，數學先備知識的要求保持在較低的水平。
作者簡介
Roberto A. Capuzzo Dolcetta has been working for 40 years in the field of Physics and Theoretical Astrophysics. Presently, he is a professor at Sapienza, University of Roma, where he currently teaches Fluid Dynamics for Astrophysics and Theoretical Astrophysics. He also has long experience in teaching Gravitational Physics and Theoretical Mechanics at both undergraduate and graduate levels. In addition, he has taught in the USA, delivering, for instance, the undergraduate course on Extragalactic Astronomy and Cosmology at the University of Washington and Seattle and presenting lectures for graduate students at Boston University. He has several scientific and didactic collaborations with, among the others, the Universities of Heidelberg (DE), of Leiden (NL), and of Prague (CZ). Since May 2010, he has been a scientific reviewer for ISCRA (Italian Super Computing Research Allocation) at CINECA and leader of the panel of Universe Science of the Access Committee of PRACE (the European infrastructure for supercomputing). His research activity is mainly theoretical, in the field of stellar clusters, both galactic and extragalactic. He is an expert in sophisticated numerical methods to deal with large self-gravitating N-body systems also embedded in gaseous cluds. He has obtained important results concerning the evolution and dynamics of the globular cluster systems in galaxies and proposed a new explanation for mass accretion and activity of galactic nuclei, including interpretation of the peculiar dynamics of stars around the Galactic supermassive black hole. He is the author of more than 240 scientific papers in international journals.
作者簡介(中文翻譯)
羅伯托·A·卡普佐·多爾切塔（Roberto A. Capuzzo Dolcetta）在物理學和理論天體物理學領域工作了40年。目前，他是羅馬薩賓納大學（Sapienza, University of Roma）的教授，教授天體物理學流體動力學和理論天體物理學。他在本科和研究生層級教授引力物理學和理論力學方面也有豐富的經驗。此外，他曾在美國授課，例如在華盛頓大學（University of Washington）和西雅圖（Seattle）教授超銀河天文學和宇宙學的本科課程，並在波士頓大學（Boston University）為研究生進行講座。他與海德堡大學（Heidelberg, DE）、萊頓大學（Leiden, NL）和布拉格大學（Prague, CZ）等多所大學有多項科學和教學合作。自2010年5月以來，他一直擔任CINECA的ISCRA（意大利超級計算研究分配）科學審稿人，並擔任PRACE（歐洲超級計算基礎設施）訪問委員會宇宙科學小組的負責人。他的研究活動主要集中在恆星團的理論領域，包括銀河系和超銀河系。他是處理大型自引力N體系統的複雜數值方法的專家，這些系統也嵌入在氣體雲中。他在銀河系的球狀星團系統的演化和動力學方面取得了重要成果，並提出了對銀河核質量吸積和活動的新解釋，包括對圍繞銀河超大質量黑洞的恆星特殊動力學的詮釋。他在國際期刊上發表了超過240篇科學論文。
