© 2020 American Physical Society. We find initial data for numerical relativity simulations of inhomogeneous cosmologies. This involves treating an exceptional case of the general relativity constraint equations. We devise analytic and numerical methods to treat this exceptional case. We apply the analytic method to the standard case of cosmology with a single scalar field. The numerical method is applied to the two-field ekpyrotic cosmology
AbsIraeL We discuss a detailed numerical comparison of the results of two mdes which treat lhe same ...
In numerical relativity simulations with non-trivial matter configurations, one must solve the Hamil...
In this thesis classical relativistic cosmology models based on the Robertson-Walker metric are stud...
In this work numerical methods for solving Einstein's equations are developed and applied to the stu...
Cosmography is the part of cosmology that proceeds by making minimal dynamic assumptions. That is, o...
We perform three-dimensional numerical relativity simulations of homogeneous and inhomogeneous expan...
We consider numerical simulations in general relativity in ADM formalism with cosmological ansatz fo...
Initial data are the starting point for any numerical simulation. In the case of numerical relativit...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
This paper is the first in a series describing a method for evolving planar cosmological models on a...
Advances in our understanding of the origin, evolution, and structure of the universe have long been...
Numerical relativity is concerned with the generation of solutions to Einstein's equations by numeri...
The problem of initial data in cosmology and general relativity is considered by analogy with the Ca...
A new numerical scheme to solve the Einstein field equations based upon the generalized harmonic dec...
The observational approach to cosmology is the endeavour to reconstruct the geometry of the Universe...
AbsIraeL We discuss a detailed numerical comparison of the results of two mdes which treat lhe same ...
In numerical relativity simulations with non-trivial matter configurations, one must solve the Hamil...
In this thesis classical relativistic cosmology models based on the Robertson-Walker metric are stud...
In this work numerical methods for solving Einstein's equations are developed and applied to the stu...
Cosmography is the part of cosmology that proceeds by making minimal dynamic assumptions. That is, o...
We perform three-dimensional numerical relativity simulations of homogeneous and inhomogeneous expan...
We consider numerical simulations in general relativity in ADM formalism with cosmological ansatz fo...
Initial data are the starting point for any numerical simulation. In the case of numerical relativit...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
This paper is the first in a series describing a method for evolving planar cosmological models on a...
Advances in our understanding of the origin, evolution, and structure of the universe have long been...
Numerical relativity is concerned with the generation of solutions to Einstein's equations by numeri...
The problem of initial data in cosmology and general relativity is considered by analogy with the Ca...
A new numerical scheme to solve the Einstein field equations based upon the generalized harmonic dec...
The observational approach to cosmology is the endeavour to reconstruct the geometry of the Universe...
AbsIraeL We discuss a detailed numerical comparison of the results of two mdes which treat lhe same ...
In numerical relativity simulations with non-trivial matter configurations, one must solve the Hamil...
In this thesis classical relativistic cosmology models based on the Robertson-Walker metric are stud...
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