commotion 发表于 2025-3-21 19:16:46

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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.
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查看完整版本: Titlebook: Scalar Fields in Numerical General Relativity; Inhomogeneous Inflat Katy Clough Book 2018 The Editor(s) (if applicable) and The Author(s),