Differential yeast populations in grape musts from different Vitis species in a shared terroir

The study of indigenous microbial communities in V. vinifera L. ecosystems constitutes a major research area in oenology. Few studies, however, consider the yeast communities present in non-vinifera Vitis ecosystems. Moreover, there are no comparative studies concerning yeast communities in V. vinifera L. and non-vinifera Vitis ecosystems in a shared terroir.Fil: Raymond Eder, María Laura. Universidad Católica de Córdoba. Instituto de Investigaciones en Recursos Naturales y Sustentabilidad José Sanchez Labrador S. J. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Investigaciones en Recursos Naturales y Sustentabilidad José Sanchez Labrador S. J.; Argentina. Universidad Católica de Córdoba; ArgentinaFil: Conti, Francisco. Universidad Católica de Córdoba; ArgentinaFil: Rosa, Alberto Luis. Universidad Católica de Córdoba; Argentina. Universidad Católica de Córdoba. Instituto de Investigaciones en Recursos Naturales y Sustentabilidad José Sanchez Labrador S. J. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Investigaciones en Recursos Naturales y Sustentabilidad José Sanchez Labrador S. J.; ArgentinaLIV Reunión Anual de la Sociedad Argentina de Investigación Bioquímica y Biología MolecularParanáArgentinaConsejo Nacional de Investigaciones Científicas y TécnicasFondo para la Investigación Científica y Tecnológic

SLIDES: Overview of Colorado Aquifer Systems

Presenter: Christopher J. Sanchez, P.G., BBA Water Consultants, Bishop-Brogden Associates, Inc. 28 slide

The Cold War: Living Under Its Shadow featuring guest Dr. Michael J. Devine

Video recording from The Cold War: Living Under Its Shadow series featuring host Armando F. Sanchez and his guest Dr. Michael J. Devine

Technical note on using the movement velocity to estimate the relative load in resistance exercises – Letter to the Editor

AbstractThe studies by Sanchez-Medina et al. (Sports Medicine International Open, 1(02), E80-E88. 2017) and Gonzalez-Badillo and Sanchez-Medina (Int J Sports Med, 31, 347–52. 2010) attempted to provide a good estimation of relative load from movement velocity measured in bench press and full squat. However, both aforementioned studies contain methodological issues concerning the predicted equations used to address load-velocity relationship that coaches should be aware of.</jats:p

Self-Gravitating Phase Transitions: Point Particles, Black Holes and Strings

We compute the quantum string entropy S_s(m,j) of the microscopic string states of mass m and spin j in two physically relevant backgrounds: Kerr (rotating) black holes and de Sitter (dS) space-time. We find a new formula for the quantum gravitational entropy S_{sem} (M, J), as a function of the usual Bekenstein-Hawking entropy S_{sem}^(0)(M, J). We compute the quantum string emission by a black hole in de Sitter space-time (bhdS). In all these cases: (i) strings with the highest spin, and (ii) in dS space-time, (iii) quantum rotating black holes, (iv) quantum dS regime, (v) late bhdS evaporation, we find a new gravitational phase transition with a common distinctive universal feature: A square root branch point singularity in any space-time dimensions. This is the same behavior as for the thermal self-gravitating gas of point particles (de Vega-Sanchez transition), thus describing a new universality class.Comment: Invited lecture at `Statistical Mechanics of Non-Extensive Systems', Observatoire de Paris, 24-25 October 2005, to be published in a Special issue of `Les Comptes rendus de l'Academie des sciences', Elsevie

Concert recording 2019-04-22

[Track 1]. El shing-a-ling / Poncho Sanchez arranged by Fernando Valencia -- [Track 2]. Mambo Inn / Mario Bauza arranged by Fernando Valencia -- [Track 3]. We don\u27t talk anymore / Charlie Puth J. Kasher adapted by Fernando Valencia -- [Track 4]. Song for Chano / Ray Barretto -- [Track 5]. Our love is here to stay / George Gershwin arranged by Fernando Valencia -- [Track 6]. Macumbia / Francisco Zumaque adapted by Fernando Valencia -- [Track 7]. Coco my my / Poncho Sanchez -- [Track 8]. Fly me to the moon / Bart Howard arranged by Fernando Valencia -- [Track 9]. Hasta que te concoci / Juan Gabriel adapted by Fernando Valencia

First report of Tomato torrado virus on weed hosts in Spain

Alfaro Fernández, AO.; Córdoba-Sellés, C.; Cebrián, M.; Herrera-Vásquez, J.; Sanchez Navarro, JA.; Juárez, M.; Espino, A.... (2088). First report of Tomato torrado virus on weed hosts in Spain. Plant Disease. 92(5):831-831. https://doi.org/10.1094/pdis-92-5-0831b83183192

Semiclassical (QFT) and Quantum (String) Rotating Black Holes and their Evaporation: New Results

Combination of both quantum field theory (QFT) and string theory in curved backgrounds in a consistent framework, the string analogue model, allows us to provide a full picture of the Kerr-Newman black hole and its evaporation going beyond the current picture. We compute the quantum emission cross section of strings by a Kerr-Newmann black hole (KNbh). It shows the black hole emission at the Hawking temperature T_{sem} in the early evaporation and the new string emission featuring a Hagedorn transition into a string state of temperature T_ s at the last stages. New bounds on the angular momentum J and charge Q emerge in the quantum string regime. The last state of evaporation of a semiclassical KNbh is a string state of temperature T_s, mass M_s, J = 0 = Q, decaying as a quantum string into all kinds of particles.(There is naturally, no loss of information, (no paradox at all)). We compute the microscopic string entropy S_s(m, j) of mass m and spin mode j. (Besides the usual transition at T_s), we find for high j, (extremal string states) a new phase transition at a temperature T_{sj} higher than T_s. We find a new formula for the Kerr black hole entropy S_{sem}, as a function of the usual Bekenstein-Hawking entropy . For high angular momentum, (extremal J = GM^2/c), a gravitational phase transition operates and the whole entropy S_{sem} is drastically different from the Bekenstein-Hawking entropy. This new extremal black hole transition occurs at a temperature T_{sem J} higher than the Hawking temperature T_{sem}.Comment: New articl

Angelica, Mother; Arias Sanchez, Oscar; St. Laurent, Louis; Salazar, António.

Contributions by Howard J. Bromberg to Great Lives from History: The Twentieth Centur