EbookBell.com

Most ebook files are in PDF format, so you can easily read them using various software such as Foxit Reader or directly on the Google Chrome browser.
Some ebook files are released by publishers in other formats such as .awz, .mobi, .epub, .fb2, etc. You may need to install specific software to read these formats on mobile/PC, such as Calibre.

Please read the tutorial at this link: https://ebookbell.com/faq

We offer FREE conversion to the popular formats you request; however, this may take some time. Therefore, right after payment, please email us, and we will try to provide the service as quickly as possible.

For some exceptional file formats or broken links (if any), please refrain from opening any disputes. Instead, email us first, and we will try to assist within a maximum of 6 hours.

EbookBell Team

Relativistic Numerical Hydrodynamics Wilson Jr Mathews Gj

Name: Relativistic Numerical Hydrodynamics Wilson Jr Mathews Gj
SKU: BELL-2048686
Price: 31.00 USD
Availability: InStock
Rating: 4.25 (48 reviews)

SKU: BELL-2048686

$ 31.00 ~~$ 45.00~~ (-31%)

4.3

48 reviews

Relativistic Numerical Hydrodynamics Wilson Jr Mathews Gj instant download after payment.

Publisher: CUP

File Extension: PDF

File size: 2.68 MB

Pages: 233

Author: Wilson J.R., Mathews G.J.

ISBN: 9780521631556, 0521631556

Language: English

Year: 2003

Product desciption

Relativistic Numerical Hydrodynamics Wilson Jr Mathews Gj by Wilson J.r., Mathews G.j. 9780521631556, 0521631556 instant download after payment.

Calculations of relativistic hydrodynamics are crucial to several areas of current research in the physics of supernovae and stellar collapse. This book provides an overview of the computational framework in which such calculations have been developed, with examples of applications to real physical systems. Beginning with the development of the equations and differencing schemes for special relativistic hydrodynamics, the book stresses the viability of the Euler-Lagrange approach to most astrophysical problems. It details aspects of solving the Einstein equations together with the fluid dynamics for various astrophysical systems in one, two and three dimensions.