6,616 research outputs found
Phenomenological implications of sterile neutrinos in the SSM and dark matter
We analyze the role of sterile neutrinos in the framework of the SSM,
where the presence of right-handed neutrinos provides a simultaneous solution
to - and -problems in supersymmetry. We adopt a minimalistic
approach, reproducing light neutrino masses and mixing angles at tree level
using just two right-handed neutrinos as part of the seesaw mechanism. A third
right-handed neutrino does not contribute significantly to the mass of the
three active ones, behaving as a sterile neutrino with a mass in the range
keVMeV. Furthermore, a sterile neutrino of about keV can be a good
candidate for dark matter with a lifetime larger than the age of the Universe.
In particular, the three-body decay to active neutrinos gives the dominant
contribution to its lifetime. The one-loop decay to gamma and active neutrino
is subdominant, but relevant for observations such as astrophysical X-rays. We
find regions of the parameter space of the SSM, with different values
of the sterile neutrino mass, fulfilling not only these constraints but also
collider constraints from the Higgs sector.Comment: Version published in Astroparticle Physics. Discussion improved
including one figure. 24 pages, 7 figures, 2 table
Computational Ego Level: Large Data and New Methods Illuminate the Construct of Ego Development
Seeing double with K2: Testing re-inflation with two remarkably similar planets around red giant branch stars
Despite more than 20 years since the discovery of the first gas giant planet
with an anomalously large radius, the mechanism for planet inflation remains
unknown. Here, we report the discovery of EPIC228754001.01, an inflated gas
giant planet found with the NASA K2 Mission, and a revised mass for another
inflated planet, K2-97b. These planets reside on ~9 day orbits around host
stars which recently evolved into red giants. We constrain the irradiation
history of these planets using models constrained by asteroseismology and
Keck/HIRES spectroscopy and radial velocity measurements. We measure planet
radii of 1.31 +\- 0.11 Rjup and and 1.30 +\- 0.07 Rjup, respectively. These
radii are typical for planets receiving the current irradiation, but not the
former, zero age main sequence irradiation of these planets. This suggests that
the current sizes of these planets are directly correlated to their current
irradiation. Our precise constraints of the masses and radii of the stars and
planets in these systems allow us to constrain the planetary heating efficiency
of both systems as 0.03% +0.03%/-0.02%. These results are consistent with a
planet re-inflation scenario, but suggest the efficiency of planet re-inflation
may be lower than previously theorized. Finally, we discuss the agreement
within 10% of stellar masses and radii, and planet masses, radii, and orbital
periods of both systems and speculate that this may be due to selection bias in
searching for planets around evolved stars.Comment: 18 pages, 15 figures, accepted to AJ. Figures 11, 12, and 13 are the
key figures of the pape
Evaluación mediante teledetección del efecto de canalizaciones sobre el humedal del Saladillo, Argentina
Los humedales son ecosistemas naturales cuya dinámica está determinada principalmente por la presencia de agua. Generalmente se los identifica como áreas que se inundan temporariamente donde el agua subterránea aflora en la superficie, o con áreas con suelos de baja permeabilidad que permanecen cubiertos por agua poco profunda. El agua, por lo tanto, juega un rol fundamental en la determinación de su estructura y funciones ecológicas. Los datos provistos por imágenes satelitales son una herramienta apropiada para analizar humedales y los cambios ocurridos en ellos a lo largo del tiempo. Los Bañados del Saladillo son un complejo de humedales en el centro de Argentina, de gran importancia para la preservación de aves acuáticas. Estos bañados han sufrido profundos cambios por el avance de la agricultura y las canalizaciones realizadas para mitigar el efecto de inundaciones en el sudeste de la provincia de Córdoba de este paÃs. El objetivo del trabajo fue conocer la condición histórica y presente de los Bañados del Saladillo, y analizar los efectos de las canalizaciones sobre los mismos. Se estudiaron 6 imágenes satelitales que se clasificaron con ENVI 4.8 (ITT, 2010), representando la estación seca y húmeda en tres perÃodos: previo a las canalizaciones (1996); posterior a las canalizaciones (2004-2006); perÃodo reciente (2010-2011). Éstas fueron seleccionadas de acuerdo a las precipitaciones acumuladas en 6 meses previos para que fueran comparables. El área de lagunas se redujo entre un 70% (estación húmeda) y un 33% (estación seca). Los mayores cambios observados en la estación húmeda se reflejaron también en la reducción del número de lagunas (40%), la variabilidad de su tamaño (66%), el perÃmetro de las mismas (28%) y el incremento de la distancia entre ellas. Más allá de la mitigación de las inundaciones, las canalizaciones favorecieron el avance de la agricultura sobre áreas históricamente inundadas en la estación lluviosa, poniendo en riesgo la persistencia de este importante humedal del sudeste de Córdoba en el centro de Argentina. Los resultados obtenidos representan una herramienta útil al momento de tomar decisiones para el manejo y conservación de estos relictos de hábitat natural y su biodiversidad.Wetlands are natural ecosystems whose dynamics is mainly determined by the presence of water. They are generally identified as temporarily flooded areas where groundwater emerges at the surface, or areas with low permeability soils that remain covered by shallow water. The water, therefore, plays a key role in determining the structure and ecological functions of wetlands. Data provided by satellite images are an appropriate tool for analyzing wetlands and their changes over time. The Saladillo Wetlands are a complex of marshlands in the centre of Argentina, of great importance to the preservation of birds. These marshes have suffered profound changes caused by the advancement of agriculture and channels made to mitigate the effects of flooding in the southeast of the province of Cordoba in this country. The objective of our work was to know the historical and present condition of the Saladillo Wetlands, and to analyze the effects of the channelization on them. We studied six satellite images classified with ENVI 4.8. These images represented the dry and the wet season into three periods: prior to the channelization (1996), after the channelization (2004-2006); and recent period (2010- 2011). They were selected according to the accumulated rainfall during the previous 6 months to make them comparable. The pond area was reduced by 70% (wet season) and 33% (dry season). The major changes observed in the wet season also reflected in the reduction in the number of ponds (40%), the variability of their size (66%), the perimeter of flooded areas (28%) and an increasing the distance between ponds. Beyond the flood mitigation, the channelization favoured the advancement of agriculture on areas historically flooded in the rainy season, threatening the persistence of this important wetland of the southeast of Cordoba in central Argentina. Our results represent a useful tool for the management and conservation of these remnants of natural habitat and biodiversity.Fil: Lopez, C.. Universidad Nacional de Rio Cuarto. Facultad de Ciencias Exactas Fisicoquimicas y Naturales; ArgentinaFil: Brandolin, Pablo Germán. Asociación Civil Amigos para la Conservación de las Aves, Córdoba; ArgentinaFil: Campanella, O. R.. Universidad Nacional de Rio Cuarto. Facultad de Cs.exactas Fisicoquimicas y Naturales. Departamento de Geologia; ArgentinaFil: Martino, A. L.. Universidad Nacional de Rio Cuarto. Facultad de Ciencias Exactas Fisicoquimicas y Naturales; ArgentinaFil: de Angelo, Carlos Daniel. Universidad Nacional de Misiones. Facultad de Ciencias Forestales. Instituto de Biologia Subtropical - Sede Puerto Iguazu; Argentin
Microduplication 10q24.31 in a Spanish girl with scoliosis and myopathy:the critical role of LBX
Multi-task multiple kernel machines for personalized pain recognition from functional near-infrared spectroscopy brain signals
Currently there is no validated objective measure of pain. Recent
neuroimaging studies have explored the feasibility of using functional
near-infrared spectroscopy (fNIRS) to measure alterations in brain function in
evoked and ongoing pain. In this study, we applied multi-task machine learning
methods to derive a practical algorithm for pain detection derived from fNIRS
signals in healthy volunteers exposed to a painful stimulus. Especially, we
employed multi-task multiple kernel learning to account for the inter-subject
variability in pain response. Our results support the use of fNIRS and machine
learning techniques in developing objective pain detection, and also highlight
the importance of adopting personalized analysis in the process.Comment: International Conference on Pattern Recognition (ICPR
All Six Planets Known to Orbit Kepler-11 Have Low Densities
The Kepler-11 planetary system contains six transiting planets ranging in
size from 1.8 to 4.2 times the radius of Earth. Five of these planets orbit in
a tightly-packed configuration with periods between 10 and 47 days. We perform
a dynamical analysis of the system based upon transit timing variations
observed in more than three years of \ik photometric data. Stellar parameters
are derived using a combination of spectral classification and constraints on
the star's density derived from transit profiles together with planetary
eccentricity vectors provided by our dynamical study. Combining masses of the
planets relative to the star from our dynamical study and radii of the planets
relative to the star from transit depths together with deduced stellar
properties yields measurements of the radii of all six planets, masses of the
five inner planets, and an upper bound to the mass of the outermost planet,
whose orbital period is 118 days. We find mass-radius combinations for all six
planets that imply that substantial fractions of their volumes are occupied by
constituents that are less dense than rock. The Kepler-11 system contains the
lowest mass exoplanets for which both mass and radius have been measured.Comment: 39 pages, 10 figure
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