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標(biāo)題: Titlebook: Kinetic Theory and Gas Dynamics; C. Cercignani Book 1988 Springer-Verlag Wien 1988 dynamics.gas.kinetic theory.complexity [打印本頁]

作者: FERAL    時間: 2025-3-21 17:15
書目名稱Kinetic Theory and Gas Dynamics影響因子(影響力)




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書目名稱Kinetic Theory and Gas Dynamics網(wǎng)絡(luò)公開度




書目名稱Kinetic Theory and Gas Dynamics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Kinetic Theory and Gas Dynamics被引頻次




書目名稱Kinetic Theory and Gas Dynamics被引頻次學(xué)科排名




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書目名稱Kinetic Theory and Gas Dynamics年度引用學(xué)科排名




書目名稱Kinetic Theory and Gas Dynamics讀者反饋




書目名稱Kinetic Theory and Gas Dynamics讀者反饋學(xué)科排名





作者: CORD    時間: 2025-3-21 22:45
Kinetic Theory and Gas Dynamics978-3-7091-2762-9Series ISSN 0254-1971 Series E-ISSN 2309-3706
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https://doi.org/10.1007/978-3-7091-2762-9dynamics; gas; kinetic theory; complexity
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covers ultra-luminous infrared galaxies and major mergers and Chapter 5 briefly examines the techniques used for computer simulation results and how increasing computer capacity has affected the development of this field. The following chapter looks at understanding the physical processes of trigger
作者: 詳細(xì)目錄    時間: 2025-3-23 15:02
H. Babovsky,H. Neunzertcovers ultra-luminous infrared galaxies and major mergers and Chapter 5 briefly examines the techniques used for computer simulation results and how increasing computer capacity has affected the development of this field. The following chapter looks at understanding the physical processes of trigger
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J. F. Clarkecovers ultra-luminous infrared galaxies and major mergers and Chapter 5 briefly examines the techniques used for computer simulation results and how increasing computer capacity has affected the development of this field. The following chapter looks at understanding the physical processes of trigger
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作者: CLAN    時間: 2025-3-24 08:30
C. Cercignanihe techniques used for computer simulation results and how increasing computer capacity has affected the development of this field. The following chapter looks at understanding the physical processes of trigger978-0-387-85370-3978-0-387-85371-0
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H. Spohnhe techniques used for computer simulation results and how increasing computer capacity has affected the development of this field. The following chapter looks at understanding the physical processes of trigger978-0-387-85370-3978-0-387-85371-0
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A. Palczewskilaxies, what they might look like, and how cosmic processes might affect life in other solar systems. It will explain crucial stages in the development of physical structure in the universe, and the effect of galaxy scale processes. Professor Struck will explore all the issues surrounding galaxy col
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J. F. Clarkelaxies, what they might look like, and how cosmic processes might affect life in other solar systems. It will explain crucial stages in the development of physical structure in the universe, and the effect of galaxy scale processes. Professor Struck will explore all the issues surrounding galaxy col
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H. Spohnlaxies, what they might look like, and how cosmic processes might affect life in other solar systems. It will explain crucial stages in the development of physical structure in the universe, and the effect of galaxy scale processes. Professor Struck will explore all the issues surrounding galaxy col
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Existence and Uniqueness Theorems for the Boltzmann Equation,e present state of the theory as two such surveys has been written recently (Fiszdon, Lachowicz, Palczewski [12] and Greenberg, Polewczak, Zweifel [17]). We are rather going to present those results which, according to the present author’s opinion, shown to be most fruitful in the further developmen
作者: 吊胃口    時間: 2025-3-26 09:40
Asymptotics of the Boltzmann Equation and Fluid Dynamics,. In these four lectures at CISM in Udine I present an outline of this theory and some of its main results: derivation and validity of the fluid equations using the Hilbert and Chapman-Enskog expansions, description of shock waves, boundary layer solutions, and fluid dynamics of discrete velocity mo
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Asymptotics of the Boltzmann Equation and Fluid Dynamics,ions using the Hilbert and Chapman-Enskog expansions, description of shock waves, boundary layer solutions, and fluid dynamics of discrete velocity models. The objective of these lectures is to present rigorous results with solid physical meaning and to suggest further lines of research.
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