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pro vyhledávání: '"Valdez, F."'
Autor:
Mayoral-Villa, E., Alvarado-Rodriguez, C. E., Pahuamba-Valdez, F., Klapp, J., Gomez-Torres, A. M., Del Valle-Gallegos, E., Gomez-Villanueva, A.
This article condenses current endeavors and improvements in the expansion of applications of the DualSPHysics code to analyze heat transfer in a nuclear reactor core. This includes the essential conservation equations and certain physical considerat
Externí odkaz:
http://arxiv.org/abs/2108.07430
Autor:
Pahuamba-Valdez, F., Mayoral-Villa, E., Alvarado-Rodriguez, C. E., Klapp, J., Goomez-Torres, A. M., Del Valle-Gallegos, E.
Publikováno v:
Communications in Computer and Information Science, Springer Nature Switzerland AG 2019
Numerical modeling simulations and the use of high-performance computing are fundamental for detailed safety analysis, control and operation of a nuclear reactor, allowing the study and analysis of problems related to thermal-hydraulics, neutronic, a
Externí odkaz:
http://arxiv.org/abs/2108.00884
Publikováno v:
In Applied Animal Science August 2022 38(4):343-349
Publikováno v:
In Applied Animal Science April 2022 38(2):110-117
We present results from models of galactic winds driven by energy injected from nuclear (at the galactic center) and non-nuclear starbursts. The total energy of the starburst is provided by very massive young stellar clusters,which can push the galac
Externí odkaz:
http://arxiv.org/abs/1612.02787
Autor:
Fernández-Trincado, J. G., Robin, A. C., Vieira, K., Moreno, E., Bienaymé, O., Reylé, C., Valenzuela, O., Pichardo, B., Robles-Valdez, F., Martins, A. M. M.
Publikováno v:
A&A 583, A76 (2015)
Using six-dimesional phase-space information from the Fourth Data release of the Radial Velocity Experiment (RAVE) over the range of Galactic longitude 240$^{\circ}< l <$ 360$^{\circ}$ and $V_{LSR} < -239$ kms$^{-1}$, we have computed orbits for 329
Externí odkaz:
http://arxiv.org/abs/1508.02839
We present a chemical evolution model for M31 based on a pronounced inside-out formation scenario. The model reproduces the three main observational constraints of the M31 disk: the radial distributions of the total baryonic mass, the gas mass, and t
Externí odkaz:
http://arxiv.org/abs/1310.1420
We present and discuss results from chemical evolution models for M33. For our models we adopt a galactic formation with an inside-out scenario. The models are built to reproduce three observational constraints of the M33 disk: the radial distributio
Externí odkaz:
http://arxiv.org/abs/1208.4889
Autor:
Character, L.D., Beach, T., Luzzadder-Beach, S, Cook, D., Schank, C., Valdez, F., Mallner, M.
Publikováno v:
Physical Geography; July 2024, Vol. 45 Issue: 4 p416-438, 23p
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