A cosmologically motivated reference formulation of numerical relativity
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Publication:4605305
DOI10.1088/1361-6382/aa8af9zbMath1380.83019arXiv1704.04307OpenAlexW3101090763WikidataQ63354504 ScholiaQ63354504MaRDI QIDQ4605305
James B. Mertens, Glenn D. Starkman, John T. jun. Giblin
Publication date: 22 February 2018
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1704.04307
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Exact solutions to problems in general relativity and gravitational theory (83C15) Computational methods for problems pertaining to relativity and gravitational theory (83-08)
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Cites Work
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- \(3+1\) formalism in general relativity. Bases of numerical relativity.
- Covariant formulations of Baumgarte, Shapiro, Shibata, and Nakamura and the standard gauge
- Evolution of three-dimensional gravitational waves: Harmonic slicing case
- Numerical integration of Einstein’s field equations
- Implementation of standard testbeds for numerical relativity
- A numerical relativity scheme for cosmological simulations
- How does the cosmic large-scale structure bias the Hubble diagram?
- Relativistic Cosmology
- Introduction to 3+1 Numerical Relativity
- Evolution of a family of expanding cubic black-hole lattices in numerical relativity