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Computational Cosmology: from the Early Universe to the Large Scale Structure.

Peter Anninos¹

¹Lawrence Livermore National Laboratory, University of California, Livermore, CA 94550 USA.

Living Reviews in Relativity

|February 14, 2017

Summary

This review explores numerical calculations in cosmology, integrating physics disciplines to model the Universe. These simulations test cosmological models against observable data, from the Big Bang to large-scale structures.

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Area of Science:

Cosmology
Astrophysics
Computational Physics

Background:

Comprehensive cosmological models require integrating diverse physics, including gauge theories, baryonic matter hydrodynamics, electromagnetism, and spacetime curvature.
Despite challenges, computational advancements significantly enhance understanding of cosmological models and astrophysical processes.

Purpose of the Study:

To review numerical calculations that address key cosmological issues.
To emphasize testing various cosmological models against observable universe data.

Main Methods:

Numerical simulations and calculations are employed.
Focus on integrating multiple physics disciplines for comprehensive modeling.

Main Results:

Review covers Big Bang singularity dynamics, gravitational wave interactions, quark-hadron phase transitions, and large-scale structure formation.
Simulations provide a means to test cosmological theories against empirical evidence.

Conclusions:

Numerical methods are crucial for advancing cosmological understanding.
Testing models against observations is key to validating cosmological theories.