Conformal and covariant formulation of the Z4 system with constraint-violation damping
By D. Alic, Carles Bona-Casas, C. Bona, Luciano Rezzolla, Carlos Palenzuela. 2011
171 citations recorded by the source corpus.
We present a new formulation of the Einstein equations based on a conformal and traceless decomposition of the covariant form of the Z4 system. This formulation combines the advantages of a conformal decomposition, such as the one used in the BSSNOK formulation (i.e. well-tested hyperbolic gauges, no need for excision, robustness to imperfect boundary conditions) with the advantages of a constraintdamped formulation, such as the generalized harmonic one (i.e. exponential decay of constraint violations when these are produced). We validate the new set of equations through standard tests and by evolving binary black hole systems. Overall, the new conformal formulation leads to a better behavior of the constraint equations and a rapid suppression of the violations when they occur. The changes necessary to implement the new conformal formulation in standard BSSNOK codes are very small as are the additional computational costs.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/0496f8999e14483895779ad85fb368dcbd6ebb37
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
- David Radice
- Luke F. Roberts
- Jonas Lippuner
- Christian D. Ott
- F. Galeazzi
- Luciano Rezzolla
- B. Metzger
- Pau Figueras
In Nuclear and High Energy Physics
- David Radice
- Christian D. Ott
- Luke F. Roberts
- Jonas Lippuner
- Pau Figueras
- Eugene A. Lim
- Luciano Rezzolla
- K. Clough
Citations in the corpus
- GRChombo: Numerical relativity with adaptive mesh refinement (2015, methodology): “As was shown in [29] stability can be achieved by adding in the CCZ4 constraint damping terms GRChombo shows exactly this behaviour (figure 15).”
- Dynamical Mass Ejection from Binary Neutron Star Mergers (2016, background): “Alternatively, the errors in the constraint could be mitigated adopting constraint-damping formulations of the Einstein equations (Bernuzzi & Hilditch 2010; Weyhausen et al. 2012; Alic et al. 2012; Hilditch et al. 2013; Alic et al. 2013; Kastaun et al. 2013).”