Room temperature ferromagnetic-like behavior in Mn-implanted and post-annealed InAs layers deposited by Molecular Beam Epitaxy

We report on the magnetic and structural properties of Ar and Mn implanted InAs epitaxial films grown on GaAs (100) by Molecular Beam Epitaxy (MBE) and the effect of Rapid Thermal Annealing (RTA) for 30 seconds at 750C. Channeling Particle Induced X- ray Emission (PIXE) experiments reveal that after Mn implantation almost all Mn atoms are subsbtitutional in the In-site of the InAs lattice, like in a diluted magnetic semiconductor (DMS). All of these samples show diamagnetic behavior. But, after RTA treatment the Mn-InAs films exhibit room-temperature magnetism. According to PIXE measurements the Mn atoms are no longer substitutional. When the same set of experiments were performed with As as implantation ion all of the layers present diamagnetism without exception. This indicates that the appearance of room-temperature ferromagnetic-like behavior in the Mn-InAs-RTA layer is not related to lattice disorder produce during implantation, but to a Mn reaction produced after a short thermal treatment. X-ray diffraction patterns (XRD) and Rutherford Back Scattering (RBS) measurements evidence the segregation of an oxygen deficient-MnO2 phase (nominally MnO1.94) in the Mn-InAs-RTA epitaxial layers which might be on the origin of room temperature ferromagnetic-like response observed.Comment: 16 pages, 5 figures. Acepted in J. Appl. Phy

Caracterización de materiales antiguos de construcción (tapial y adobe) en las iglesias de Cisneros, Villada y Boada de Campos (Palencia)

The aim of this work is to characterize the ancient building materials (mud wall and adobe) of three churches in the province of Palencia. This is the first part of a study which seeks to evaluate how the mud walls of the tower of the church of Cisneros reacted to restoration treatment which consisted of a structural reinforcement made by injecting a highly fluid grout of cement/lime/sand mortar. This treatment implies the introduction of large quantities of water into the fabric. The mud walls of the tower of Cisneros are compositionally and texturally very similar to each other, which indicates that despite their large dimensions, care was taken in the homogeneity of the materials. These mud walls are also very similar to those of the church of Villada. The original raw material is mud with some additives (rubble, ashes, bones, etc.) and some remains of lime used as a stabiliser. Although there is a very high proportion of clay, no effervescing clay has been detected. Hence it is deduced that once the mud wall was built, there were no important changes in volume due to variation in the humidity of the fabric. The characteristics of the adobe of the tower of Boada are logically different form those of the mud walls, being made of less sandy, more clayey mud with a high proportion of straw that the mud walls do not have, and without the addition of bricks, bones, etc.El objetivo de este trabajo es caracterizar los materiales antiguos de construcción (tapial y adobe) de tres iglesias en la provincia de Falencia. El trabajo es la primera parte de un estudio en el que se pretende evaluar el comportamiento de los tapiales de la torre de la iglesia de Cisneros frente al tratamiento de restauración, consistente en un cosido estructural mediante la realización de perforaciones en las que se introduce una barra de acero y donde, posteriormente, se inyecta una lechada muy fluidificada de mortero de cemento/cal/arena. Este tratamiento implica la introducción en las fábricas de grandes cantidades de agua. Los tapiales de la torre de Cisneros son, composicional y texturalmente, muy similares entre sí, lo que indica que, a pesar de sus grandes dimensiones, se cuidó la homogeneidad de los materiales. Estos tapiales guardan una notable similitud con los de la iglesia de Villada. La materia prima original es barro con algunos aditivos (escombro, cenizas, huesos, etc.) y algunos restos de cal empleada como estabilizante. Aunque la proporción de arcilla es muy elevada no se han detectado arcillas hinchables, de lo que se deduce que una vez construido el tapial no se habrían producido importantes cambios de volumen por variaciones de humedad de las fábricas. Las características del adobe de la torre de Boada son lógicamente diferentes de las de los tapiales estando constituido por un barro menos arenoso, más arcilloso, con una elevada proporción de paja que no tienen los tapiales y sin adiciones de ladrillos, huesos, etc

Polymerase chain reaction detection of rabbit DNA in food and animal feed

[EN] A polymerase chain reaction (PCR) based on oligonucleotide primers targeting the mitochondrial 12S rRNA gene was developed for the specific identification of rabbit DNA (Oryctolagus cuniculus) in food and feedstuffs. The specificity of the primers was verified by PCR analysis of DNA from 32 non-target species including mammals, birds, fish, and plant species. Analysis of experimental mixtures demonstrated the presence of rabbit-derived materials in the range of 0.1-100%. Prolonged heat treatment (up to 133ºC for 20 min at 300 kPa) applied to rabbit muscle/oats binary mixtures did not affect the performance of the method, which could therefore be said to be very useful for the accurate identification of rabbit materials in products submitted to denaturing technologies when other methods are not suitable.This study was supported by Grant Nº. AGL 2007-60077 from the Spanish Ministerio de Educación y Ciencia and the Programa de Vigilancia Sanitaria S-0505/AGR/000265 of the Comunidad de Madrid (Spain). Irene Martín is the recipient of a fellowship from the Universidad Complutense de Madrid (Spain). Violeta Fajardo and María Rojas are recipients of fellowships from the Ministerio de Educación y Ciencia (Spain).Martín, I.; García, T.; Fajardo, V.; Rojas, M.; Pegels, N.; Hernández, P.; González, I.... (2009). Polymerase chain reaction detection of rabbit DNA in food and animal feed. World Rabbit Science. 17(1):27-34. doi:10.4995/wrs.2009.667273417

On the kinematics of the neutron star low mass X-ray binary Cen X-4

We present the first determination of the proper motion of the neutron star low mass X-ray binary {Cen X-4} measured from relative astrometry of the secondary star using optical images at different epochs. We determine the Galactic space velocity components of the system and find them to be significantly different from the mean values that characterize the kinematics of stars belonging to the halo, and the thin and the thick disc of the Galaxy. The high metallicity of the secondary star of the system rules out a halo origin and indicates that the system probably originated in the Galactic disc. A statistical analysis of the galactocentric motion revealed that this binary moves in a highly eccentric ($e\simeq 0.85\pm0.1$) orbit with an inclination of $\simeq 110^\circ$ to the Galactic plane. The large Galactic space velocity components strongly support that a high natal kick as a result of a supernova explosion could have propelled the system into such an orbit from a birth place in the Galactic disc. The high Li abundance in the secondary, comparable to that of stars in star forming regions and young stellar clusters like the Pleiades, may suggest a relatively recent formation of the system. Following the orbit backwards in time, we found that the system could have been in the inner regions of the Galactic disc $\sim$100--200 Myr ago. The neutron star might have formed at that moment. However, we cannot rule out the possibility that the system formed at a much earlier time if a Li production mechanism exists in this LMXB.Comment: 6 pages, 4 figures, accepted for publication in A&

Observational Δν\Delta\nu-ρˉ\bar\rho relation for δ\delta Sct stars using eclipsing binaries and space photometry

Delta Scuti ($\delta$ Sct) stars are intermediate-mass pulsators, whose intrinsic oscillations have been studied for decades. However, modelling their pulsations remains a real theoretical challenge, thereby even hampering the precise determination of global stellar parameters. In this work, we used space photometry observations of eclipsing binaries with a $\delta$ Sct component to obtain reliable physical parameters and oscillation frequencies. Using that information, we derived an observational scaling relation between the stellar mean density and a frequency pattern in the oscillation spectrum. This pattern is analogous to the solar-like large separation but in the low order regime. We also show that this relation is independent of the rotation rate. These findings open the possibility of accurately characterizing this type of pulsator and validate the frequency pattern as a new observable for $\delta$ Sct stars.Comment: 11 pages, including 2 pages of appendix, 2 figures, 2 tables, accepted for publication in ApJ

Plan estratégico para una alimentación sostenible, adecuada y sana en los escolares de Remedios, Cuba

The work consists of a plan proposed by the University of Remedios, Cuba, to improve the nutritional level of children and young people in the semi-internships of the municipality, to guarantee the variety and sustainability of agricultural products on the table, as well as their consumption. Thanks to this strong educational work, we contributed to improving the nutritional level of the students; For this, the 17 semi-internal centers of the territory and the four farms that guarantee these products in the educational centers were taken as a sample, they belong to the National Association of Small Farmers (ANAP). For the design of the strategic plan, investigative methods were applied, among are observation, survey, interview, and logical history that served to make the initial diagnosis and verify the final results. The work as a whole reveals a sustainable contribution of agricultural products on the table of schoolchildren, achieving a high nutritional level in children, adolescents, and young people of these educational centers with these characteristics of semi-internships from a stable and sustainable consumption of these products since 2020 to 2022 when the strategy was applied.El trabajo consiste en un plan propuesto por la universidad de Remedios, Cuba, para mejorar el nivel nutricional de los niños y jóvenes en los seminternos del municipio, para garantizar la variedad y sostenibilidad de los productos agrícolas en la mesa, así como su consumo. Gracias a este fuerte trabajo educativo se contribuyó a mejorar el nivel nutricional de los educandos; para ello se tomó como muestra a los 17 centros seminternos del territorio y las cuatro fincas que garantizan estos productos en los centros educacionales, las mismas pertenecen a la Asociación Nacional de Agricultores Pequeños (ANAP). Para el diseño del plan estratégico se aplicaron métodos investigativos entre los que se encuentran la observación, la encuesta, la entrevista y el histórico lógico que sirvieron para hacer el diagnóstico inicial y constatar los resultados finales. El trabajo en su conjunto revela una contribución sostenible de productos agrícolas en la mesa de los escolares lográndose un elevado nivel nutricional en los niños, adolescentes y jóvenes de estos centros educacionales con estas características de seminternos a partir de un consumo estable y sostenible de estos productos desde el 2020 hasta el 2022, cuando se aplicó la estrategia.&nbsp

Pre-main sequence stars in the Lagoon Nebula (M8)

We report the discovery of new pre-main sequence (PMS) stars in the Lagoon Nebula (M8) at a distance of 1.25 kpc, based on intermediate resolution spectra obtained with the Boller & Chivens spectrograph at the 6.5-m Magellan I telescope (Las Campanas Observatory, Chile). According to the spectral types, the presence of emission lines and the lithium 6708A absorption line, we are able to identify 27 classical T Tauri stars, 7 weak-lined T Tauri stars and 3 PMS emission objects with spectral type G, which we include in a separated stellar class denominated "PMS Fe/Ge class". Using near-infrared photometry either from 2MASS or from our own previous work we derive effective temperatures and luminosities for these stars and locate them in the Hertzsprung-Russell diagram, in order to estimate their masses and ages. We find that almost all of our sample stars are younger than 3 10^6 years and span over a range of masses between 0.8 and 2.5 Msun. A cross-correlation between our spectroscopic data and the X-ray sources detected with the Chandra ACIS instrument is also presented.Comment: 18 pages, 15 figures, MNRAS, in pres

Toroidal magnetized iron neutrino detector for a neutrino factory

A neutrino factory has unparalleled physics reach for the discovery and measurement of CP violation in the neutrino sector. A far detector for a neutrino factory must have good charge identification with excellent background rejection and a large mass. An elegant solution is to construct a magnetized iron neutrino detector (MIND) along the lines of MINOS, where iron plates provide a toroidal magnetic field and scintillator planes provide 3D space points. In this paper, the current status of a simulation of a toroidal MIND for a neutrino factory is discussed in light of the recent measurements of large θ13. The response and performance using the 10 GeV neutrino factory configuration are presented. It is shown that this setup has equivalent δCP reach to a MIND with a dipole field and is sensitive to the discovery of CP violation over 85% of the values of δCP