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pro vyhledávání: '"CAPUANO A"'
Autor:
Everaldo Batista da Costa
Publikováno v:
Patryter, Vol 5, Iss 10 (2022)
Esta entrevista integra el vol. 5, núm. 10 de PatryTer, que rinde homenaje al profesor Francisco Capuano Scarlato por su dedicación y aportación a la Geografía desde el año de 1964, o sea, cumplirán seis décadas junto a la Facultad de Filosof
Externí odkaz:
https://doaj.org/article/06ddb2ca0d9941f0a97cd0c2b550044e
Autor:
Shank, Michael H.
Publikováno v:
Early Science and Medicine, 2009 Jan 01. 14(1/3), 290-315.
Externí odkaz:
https://www.jstor.org/stable/20617787
Akademický článek
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Autor:
CAPUANO, CAMILLA, MOFFA, CARMELA
Publikováno v:
Pasticceria Internazionale. feb2024, Vol. 47 Issue 352, p56-58. 3p.
A posteriori analysis based upon a recently proposed non-dissipative large-eddy simulation framework for transcritical wall-bounded turbulence has been carried out. Due to the complexities arisen in such flows, the discretization requires kinetic-ene
Externí odkaz:
http://arxiv.org/abs/2410.22279
Autor:
Messuti, Giovanni, Amoroso, ortensia, Napolitano, Ferdinando, Falanga, Mariarosaria, Capuano, Paolo, Scarpetta, Silvia
Deep learning models have demonstrated remarkable success in various fields, including seismology. However, one major challenge in deep learning is the presence of mislabeled examples. Additionally, accurately estimating model uncertainty is another
Externí odkaz:
http://arxiv.org/abs/2410.06120
Mixing and heat transfer rates are typically enhanced when operating at high-pressure transcritical turbulent flow regimes. The rapid variation of thermophysical properties in the vicinity of the pseudo-boiling region can be leveraged to significantl
Externí odkaz:
http://arxiv.org/abs/2409.17310
The effects of kinetic-energy preservation errors due to Runge-Kutta (RK) temporal integrators have been analyzed for the case of large-eddy simulations of incompressible turbulent channel flow. Simulations have been run using the open-source solver
Externí odkaz:
http://arxiv.org/abs/2409.08851
We provide the most complete analysis so far of quasinormal modes of rotating black holes in a general higher-derivative extension of Einstein's theory. By finding the corrections to the Teukolsky equation and expressing them in a simple form, we are
Externí odkaz:
http://arxiv.org/abs/2409.04517