commotion
发表于 2025-3-21 19:16:46
书目名称Scalar Fields in Numerical General Relativity影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0861068<br><br> <br><br>书目名称Scalar Fields in Numerical General Relativity读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0861068<br><br> <br><br>
acclimate
发表于 2025-3-21 22:06:12
2190-5053 lating spacetimes using numerical relativity (NR), ideal for.This book explores the use of numerical relativity (NR) methods to solve cosmological problems, and describes one of the first uses of NR to study inflationary physics. NR consists in the solution of Einstein’s Equation of general relativi
暂时别动
发表于 2025-3-22 04:16:29
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HILAR
发表于 2025-3-22 06:52:34
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parallelism
发表于 2025-3-22 09:23:59
Book 2018flationary physics. NR consists in the solution of Einstein’s Equation of general relativity, which governs the evolution of matter and energy on cosmological scales, and in systems where there are strong gravitational effects, such as around black holes. To date, NR has mainly been used for simulat
发怨言
发表于 2025-3-22 12:53:02
Technical Background evolution, and the background to the specific problems studied. Discussion of the implementation aspects of the numerical evolution are left to the following chapter in which the code which was developed is described. As in Chap. ., we divide this chapter into three sections, GR, NR and Scalar Fiel
粗俗人
发表于 2025-3-22 19:46:29
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圆柱
发表于 2025-3-22 22:21:52
Inhomogeneous Inflation223, 1982, [.], Starobinsky, Phys Lett B 91:99–102, 1980, [.]) is thought to provide a solution to several problems in standard Big Bang theory by dynamically driving a “generic” initial state to a flat, homogeneous and isotropic Universe, while generating a nearly scale-invariant power spectrum of
OASIS
发表于 2025-3-23 02:04:40
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易发怒
发表于 2025-3-23 07:51:30
Conclusions and Further Work code based on the BSSN/CCZ4 evolution scheme. It supports Berger-Collela type AMR evolution with Berger-Rigoutsos block structured grid generation and is fully parallelised via the Message Passing Interface. Time evolution is via standard 4th order Runge–Kutta time-stepping.