Name: Scalar Fields in Numerical General Relativity: Inhomogeneous Inflation and Asymmetric Bubble Collapse (en Inglés)
SKU: 57090644
Price: 1858.65 MXN
Availability: InStock
Author: Clough, Katy
ISBN: 9783030064877

portada Scalar Fields in Numerical General Relativity: Inhomogeneous Inflation and Asymmetric Bubble Collapse (en Inglés)

Scalar Fields in Numerical General Relativity: Inhomogeneous Inflation and Asymmetric Bubble Collapse (en Inglés)

Formato

Libro Físico

Autor

Katy Clough

Editorial

Springer

Idioma

Inglés

N° páginas

197

Encuadernación

Tapa Blanda

Dimensiones

23.4x15.6x1.2 cm

Peso

0.31 kg.

ISBN13

9783030064877

Categorías

Cosmología y el universo
Gravedad
Física matemática

Scalar Fields in Numerical General Relativity: Inhomogeneous Inflation and Asymmetric Bubble Collapse (en Inglés)

Katy Clough (Autor) · Springer · Tapa Blanda

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Reseña del libro "Scalar Fields in Numerical General Relativity: Inhomogeneous Inflation and Asymmetric Bubble Collapse (en Inglés)"

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 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 simulating binary black hole and neutron star mergers like those detected recently by LIGO. Its use as a tool in fundamental problems of gravity and cosmology is novel, but rapidly gaining interest. In this thesis, the author investigates the initial condition problem in early universe cosmology - whether an inflationary expansion period could have "got going" from initially inhomogeneous conditions - and identifies criteria for predicting the robustness of particular models. State-of-the-art numerical relativity tools are developed in order to address this question, which are now publicly available.