Cardoso, Vitor, Gualtieri, Leonardo, Herdeiro, Carlos, Sperhake, Ulrich, Chesler, Paul M., Lehner, Luis, Park, Seong Chan, Reall, Harvey S., Sopuerta, Carlos F., Alic, Daniela, Dias, Oscar J. C., Emparan, Roberto, Ferrari, Valeria, Giddings, Steven B., Godazgar, Mahdi, Gregory, Ruth, Hubeny, Veronika E., Ishibashi, Akihiro, Landsberg, Greg, Lousto, Carlos O., Mateos, David, Moeller, Vicki, Okawa, Hirotada, Pani, Paolo, Parker, M. Andy, Pretorius, Frans, Shibata, Masaru, Sotani, Hajime, Wiseman, Toby, Witek, Helvi, Yunes, Nicolas and Zilhao, Miguel (2012), "NR/HEP: roadmap for the future", CLASSICAL AND QUANTUM GRAVITY, 29, 24.
Abstract: Physic in curved spacetime describes a multitude of phenomena, ranging
from astrophysics to high-energy physics (HEP). The last few years have
witnessed further progress on several fronts, including the accurate
numerical evolution of the gravitational field equations, which now
allows highly nonlinear phenomena to be tamed. Numerical relativity
simulations, originally developed to understand strong-field
astrophysical processes, could prove extremely useful to understand HEP
processes such as trans-Planckian scattering and gauge-gravity
dualities. We present a concise and comprehensive overview of the
state-of-the-art and important open problems in the field(s), along with
a roadmap for the next years.
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