Introduction to 3+1 Numerical Relativity

By M. Alcubierre. 2008

181 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/bd20b3977ea4f640d714c9aac0da0e3e29bc14ab

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Paolo Pani
2. V. Cardoso
3. Carlos A. R. Herdeiro
4. Emanuele Berti
5. Eugen Radu
6. R. Brito
7. L. Gualtieri
8. E. Barausse

In Oceanography

1. N. Wex
2. B. Sathyaprakash
3. Paolo Pani
4. R. O’Shaughnessy
5. Pedro G. Ferreira
6. Hector O. Silva
7. Emanuele Berti
8. Antonio de Felice

Citations in the corpus

• Dynamical boson stars (2012, unknown): “It is therefore more intuitive to instead consider a succession of spacetime geometries, where the evolution of a given slice is given by the Einstein equations (for more detailed treatments see [9, 34, 50, 167]).”
• Testing general relativity with present and future astrophysical observations (2015, background): “The foliation condition of constant (3)R − N−1∆N can be interpreted as the maximal slicing gauge condition common in Numerical Relativity [279], and it is then straightforward to show that the Kerr metric in Boyer-Lindquist coordinates is also a solution of n-DBI gravity [99].”