@article {Br{\"u}gmann366,
author = {Br{\"u}gmann, Bernd},
title = {Fundamentals of numerical relativity for gravitational wave sources},
volume = {361},
number = {6400},
pages = {366--371},
year = {2018},
doi = {10.1126/science.aat3363},
publisher = {American Association for the Advancement of Science},
abstract = {Einstein{\textquoteright}s theory of general relativity affords an enormously successful description of gravity. The theory encodes the gravitational interaction in the metric, a tensor field on spacetime that satisfies partial differential equations known as the Einstein equations. This review introduces some of the fundamental concepts of numerical relativity{\textemdash}solving the Einstein equations on the computer{\textemdash}in simple terms. As a primary example, we consider the solution of the general relativistic two-body problem, which features prominently in the new field of gravitational wave astronomy.},
issn = {0036-8075},
URL = {https://science.sciencemag.org/content/361/6400/366},
eprint = {https://science.sciencemag.org/content/361/6400/366.full.pdf},
journal = {Science}
}