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NR/HEP: roadmap for the future

MPG-Autoren
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Alic,  Daniela
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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1201.5118
(Preprint), 2MB

CQG_29_24_244001.pdf
(beliebiger Volltext), 981KB

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Cardoso, V., Gualtieri, L., Herdeiro, C., Sperhake, U., Chesler, P. M., Lehner, L., et al. (2012). NR/HEP: roadmap for the future. Classical and quantum gravity, 29(24): 244001. doi:10.1088/0264-9381/29/24/244001.


Zitierlink: https://hdl.handle.net/11858/00-001M-0000-0010-0D0B-3
Zusammenfassung
Physics in curved spacetime describes a multitude of phenomena, ranging from astrophysics to high energy physics. 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 high-energy physics processes like 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 guidelines for the next years. This writeup is a summary of the "NR/HEP Workshop" held in Madeira, Portugal from August 31st to September 3rd 2011.