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Titlebook: Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste; Keisuke Sugiura Book 2020 The Editor

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發(fā)表于 2025-3-21 18:47:23 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste
編輯Keisuke Sugiura
視頻videohttp://file.papertrans.cn/271/270015/270015.mp4
概述Nominated as an outstanding Ph.D. thesis by the Nagoya University, Japan.Summarizes SPH techniques required for simulations of solid body impacts, helping readers to develop simulation codes using the
叢書名稱Springer Theses
圖書封面Titlebook: Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste;  Keisuke Sugiura Book 2020 The Editor
描述.This book describes numerical simulations of collisions between asteroids, based on a unique numerical code developed by the author. The code accurately solves the elastic dynamic equations and describes the effects of fracture and friction, which makes it possible to investigate the shapes of impact outcomes produced by asteroid collisions and subsequent gravitational accumulation of fragments..The author parallelizes the code with high parallelization efficiency; accordingly, it can be used to conduct high-resolution simulations with the aid of supercomputers and clarify the shapes of small remnants produced through the catastrophic destruction of asteroids. The author demonstrates that flat asteroids can only be produced by impacts involving objects with similar mass and low velocity, which suggests that the flat asteroids in our solar system were created in the planet formation era and have kept their shapes until today. The author also shows that asteroid collisions under certain conditions can produce the extremely elongated shape of an interstellar minor body, 1I/‘Oumuamua. In brief, the book offers a comprehensive investigation of asteroid impacts and shapes, making it a u
出版日期Book 2020
關鍵詞Numerical Simulations of Asteroid Collisions; Asteroid Shapes Formed Through Collisions; High-resoluti
版次1
doihttps://doi.org/10.1007/978-981-15-3722-6
isbn_softcover978-981-15-3724-0
isbn_ebook978-981-15-3722-6Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 21:11:58 | 只看該作者
板凳
發(fā)表于 2025-3-22 03:25:27 | 只看該作者
978-981-15-3724-0The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
地板
發(fā)表于 2025-3-22 07:35:55 | 只看該作者
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Springer Theseshttp://image.papertrans.cn/d/image/270015.jpg
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Erbrecht,such numerical simulations, we need knowledge about not only hydrodynamics but also elastic dynamics for intact rocks, fracturing of rocky materials, and friction of completely damaged rocks. In this chapter, we introduce the detailed methods necessary for numerical simulations of asteroidal collisi
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發(fā)表于 2025-3-22 21:29:32 | 只看該作者
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發(fā)表于 2025-3-23 04:49:38 | 只看該作者
https://doi.org/10.1007/978-3-662-29974-6acts produce spherical and bilobed shapes but they do not produce flat shapes. The impact velocity is strongly affected by the environments of planetary systems such as the existence of gas components or giant planets. Low-velocity impacts are realized in the primordial environment, while high-veloc
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發(fā)表于 2025-3-23 08:53:37 | 只看該作者
https://doi.org/10.1007/978-3-662-29974-6mua was discovered, and its light curve shows that 1I/‘Oumuamua has the size of about 100?m and an extremely elongated shape with the ratio of intermediate to major axis lengths less than 0.3. In this chapter, we introduce results of our simulations that investigate detailed impact conditions to for
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