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.
%0 Journal Article
%1 Cardoso2012NRHEP
%A Cardoso, Vitor
%A Gualtieri, Leonardo
%A Herdeiro, Carlos
%A Sperhake, Ulrich
%A Chesler, Paul M.
%A Lehner, Luis
%A Park, Seong C.
%A Reall, Harvey S.
%A Sopuerta, Carlos F.
%A Alic, Daniela
%A Dias, Oscar J. C.
%A Emparan, Roberto
%A Ferrari, Valeria
%A Giddings, Steven B.
%A Godazgar, Mahdi
%A Gregory, Ruth
%A Hubeny, Veronika E.
%A Ishibashi, Akihiro
%A Landsberg, Greg
%A Lousto, Carlos O.
%A Mateos, David
%A Moeller, Vicki
%A Okawa, Hirotada
%A Pani, Paolo
%A Parker, M. Andy
%A Pretorius, Frans
%A Shibata, Masaru
%A Sotani, Hajime
%A Wiseman, Toby
%A Witek, Helvi
%A Yunes, Nicolas
%A Zilhao, Miguel
%D 2012
%K 4d\_bhs, 5d-bhs, arxiv, black-string, blackring, lectures
%T NR/HEP: roadmap for the future
%U http://arxiv.org/abs/1201.5118
%X 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.
@article{Cardoso2012NRHEP,
abstract = {{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.}},
added-at = {2019-02-26T10:37:35.000+0100},
archiveprefix = {arXiv},
author = {Cardoso, Vitor and Gualtieri, Leonardo and Herdeiro, Carlos and Sperhake, Ulrich and Chesler, Paul M. and Lehner, Luis and Park, Seong C. and Reall, Harvey S. and Sopuerta, Carlos F. and Alic, Daniela and Dias, Oscar J. C. and Emparan, Roberto and Ferrari, Valeria and Giddings, Steven B. and Godazgar, Mahdi and Gregory, Ruth and Hubeny, Veronika E. and Ishibashi, Akihiro and Landsberg, Greg and Lousto, Carlos O. and Mateos, David and Moeller, Vicki and Okawa, Hirotada and Pani, Paolo and Parker, M. Andy and Pretorius, Frans and Shibata, Masaru and Sotani, Hajime and Wiseman, Toby and Witek, Helvi and Yunes, Nicolas and Zilhao, Miguel},
biburl = {https://www.bibsonomy.org/bibtex/2db263cd3278c0e2f2a319b9f8a65ad97/acastro},
citeulike-article-id = {10272140},
citeulike-linkout-0 = {http://arxiv.org/abs/1201.5118},
citeulike-linkout-1 = {http://arxiv.org/pdf/1201.5118},
day = 24,
eprint = {1201.5118},
interhash = {716324f11a0f4d88229a0263971c6179},
intrahash = {db263cd3278c0e2f2a319b9f8a65ad97},
keywords = {4d\_bhs, 5d-bhs, arxiv, black-string, blackring, lectures},
month = jan,
posted-at = {2012-01-26 13:03:19},
priority = {2},
timestamp = {2019-02-26T10:37:35.000+0100},
title = {{NR/HEP: roadmap for the future}},
url = {http://arxiv.org/abs/1201.5118},
year = 2012
}