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NR/HEP: roadmap for the future

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arxiv 1201.5118 v1 pith:FYHTC5IN submitted 2012-01-24 hep-th astro-ph.HEgr-qchep-ph

classification hep-thastro-ph.HEgr-qchep-ph
keywords fieldphysicsnumericalphenomenaprocessesunderstandyearsaccurate
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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.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Thermalization dynamics of finite-size quantum critical systems

    hep-th 2025-09 conditional novelty 7.0 of 10

    Finite-size quantum critical systems thermalize in three regimes: recurrent non-equilibrium steady states, long-lived confined shock waves, or oscillatory decay, with near-complete energy swapping between the two sides.

  2. Nonlinear Stability of Kerr-Sen Black Holes in Merging Binaries

    gr-qc 2026-06 unverdicted novelty 4.0 of 10

    Head-on binary black hole simulations in EMDA theory show dilaton and axion fields persist through merger, indicating nonlinear stability of Kerr-Sen black holes and scalarization of initially unscalarized solutions.

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