fRevolution— relativistic cosmological simulations in f(R) gravity. Part I. Methodology
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Publication:5025402
DOI10.1088/1475-7516/2019/07/035OpenAlexW2946266979MaRDI QIDQ5025402
Publication date: 1 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1905.07345
Related Items (4)
GRAMSES: a new route to general relativistic N-body simulations in cosmology. Part I. Methodology and code description ⋮ Asevolution: a relativistic N-body implementation of the (a)symmetron ⋮ fRevolution ⋮ Does relativistic cosmology software handle emergent volume evolution?
Uses Software
Cites Work
- \(f(R)\) theories
- Klassische Runge-Kutta-Formeln vierter und niedrigerer Ordnung mit Schrittweiten-Kontrolle und ihre Anwendung auf Wärmeleitungsprobleme
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- Singularity Problem with<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Models for Dark Energy
- Modified Gravity Models of Dark Energy
- General relativistic weak-field limit and Newtonian N-body simulations
- Relativistic initial conditions for N-body simulations
- A new approach to cosmological structure formation with massive neutrinos
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