368 research outputs found
Verifying the Identity of High-Redshift Massive Galaxies Through the Clustering of Lower Mass Galaxies Around Them
Massive high-redshift galaxies form in over-dense regions where the
probability of forming other galaxies is also strongly enhanced. Given an
observed flux of a galaxy, the inferred mass of its host halo tends to be
larger as its inferred redshift increases. As the mass and redshift of a galaxy
halo increase, the expected clustering of other galaxies around it gets
stronger. It is therefore possible to verify the high-redshift identity of a
galaxy (prior to an unambiguous spectral identification) from the clustering of
other galaxies around it. We illustrate this method for the massive galaxy
suggested by Mobasher et al. (2005) to be at redshift z~6.5. If this galaxy
were to exist at z~6.5, there should have been a mean of ~10 galaxies larger
than a hundredth of its mass and having z-band magnitudes less than ~25
detected as i-dropouts in the HUDF. We calculate an approximate probability
distribution for neighbor galaxies and determine that there is less than a
~0.3% chance of detecting no massive neighbor galaxies. The lack of other
massive z~6.5 galaxies in the HUDF image argues that the Mobasher et al. (2005)
galaxy is instead a low redshift interloper. We generalize our results to other
galaxy masses and redshifts.Comment: 7 pages, 5 figures. Typos correcte
Formation in-situ of metallic nanoclusters of Mn interlayered into bentonite previously pillared with Al
Hasta el momento, el crecimiento de agregados polinucleares en el espacio interlaminar de diferentes aluminosilicatos por reacción en el estado sólido requiere de tiempos prolongados de contacto (alrededor de 4 meses). En consecuencia, en el presente trabajo se ha evaluado una metodologÃa novedosa para llevar a cabo tal sÃntesis, especÃficamente para el crecimiento in-situ de MnS en el espacio interlaminar de una bentonita que involucra un tiempo aproximado de 10 horas de reacción. Sin embargo, los resultados han evidenciado que hay varias condiciones que se deben controlar por cuanto afectan la estabilidad de los clusters; entre estos factores están el tratamiento quÃmico, térmico, el tipo de atmósfera empleado en la calcinación y la densidad de los pilares de Al
In-situ growing of MnS and FeS nanoclusters at the interlayer of Al-pillared bentonite
Introduction Since formation of metal nanoclusters is thermodynamically unstable and difficult to control, in this work it has been explored the in-situ growing of either MnS or FeS nanoclusters in the interlayer space of a bentonite by means of a pretty short process taking only around 12 h. The interlayered polynuclear sulfidized metal clusters were prepared by cationic exchange of either Mn 2+ or Fe 2+ on the bentonite previously interlayered/pillared with aluminium under different conditions. These metal sulfidized nanomaterials have attracted substantial interests due to their unique optical and electrical properties and wide variety of potential applications in electroluminescence 1 and nonlinear optical devices 2. Since the main physical and optical properties of such metal sulfides primarily depend on their shape and size, the immobilization of metal sulfide nanoparticles in a spatially confined environment is a way to control the photo-physical and photo-chemical properties which result in very interesting strategy of morphological control
Understanding the Observed Evolution of the Galaxy Luminosity Function from z=6-10 in the Context of Hierarchical Structure Formation
Recent observations of the Lyman-break galaxy (LBG) luminosity function (LF)
from z~6-10 show a steep decline in abundance with increasing redshift.
However, the LF is a convolution of the mass function of dark matter halos
(HMF)--which also declines sharply over this redshift range--and the
galaxy-formation physics that maps halo mass to galaxy luminosity. We consider
the strong observed evolution in the LF from z~6-10 in this context and
determine whether it can be explained solely by the behavior of the HMF. From
z~6-8, we find a residual change in the physics of galaxy formation
corresponding to a ~0.5 dex increase in the average luminosity of a halo of
fixed mass. On the other hand, our analysis of recent LF measurements at z~10
shows that the paucity of detected galaxies is consistent with almost no change
in the average luminosity at fixed halo mass from z~8. The LF slope also
constrains the variation about this mean such that the luminosity of galaxies
hosted by halos of the same mass are all within about an order-of-magnitude of
each other. We show that these results are well-described by a simple model of
galaxy formation in which cold-flow accretion is balanced by star formation and
momentum-driven outflows. If galaxy formation proceeds in halos with masses
down to 10^8 Msun, then such a model predicts that LBGs at z~10 should be able
to maintain an ionized intergalactic medium as long as the ratio of the
clumping factor to the ionizing escape fraction is C/f_esc < 10.Comment: 15 pages, 2 figures; results unchanged; accepted by JCA
Efecto del escalamiento a 10 kg del catalizador Al/Fe-PILC sobre sus propiedades fisicoquÃmicas y catalÃticas en la degradación de fenol
Durante la última década diferentes estudios han demostrado que las arcillas pilarizadas con el sistema mixto Al/Fe presentan una excelente respuesta catalÃtica en la degradación de compuestos orgánicos tóxicos disueltos en agua mediante Peroxidación CatalÃtica en Fase Húmeda (PCFH) [1-3]. Sin embargo,la implementación de ésta tecnologÃa en la descontaminación de aguas a escala real depende fuertemente de la preparación reproducible del catalizador a mayor escala, sin una pérdida significativa de sus propiedades tanto fisicoquÃmicas como catalÃticas.
Este trabajo tiene como objetivo principal determinar el efecto de la preparación del catalizador Al/Fe-PILC en tres diferentes escalas y concentración de sus precursores
Lattice dynamics of mixed semiconductors (Be,Zn)Se from first-principles calculations
Vibration properties of Zn(1-x)Be(x)Se, a mixed II-VI semiconductor
haracterized by a high contrast in elastic properties of its pure constituents,
ZnSe and BeSe, are simulated by first-principles calculations of electronic
structure, lattice relaxation and frozen phonons. The calculations within the
local density approximation has been done with the Siesta method, using
norm-conserving pseudopotentials and localized basis functions; the benchmark
calculations for pure endsystems were moreover done also by all-electron WIEN2k
code. An immediate motivation for the study was to analyze, at the microscopic
level, the appearance of anomalous phonon modes early detected in Raman spectra
in the intermediate region (20 to 80%) of ZnBe concentration. This was early
discussed on the basis of a percolation phenomenon, i.e., the result of the
formation of wall-to-wall --Be--Se-- chains throughout the crystal. The
presence of such chains was explicitly allowed in our simulation and indeed
brought about a softening and splitting off of particular modes, in accordance
with experimental observation, due to a relative elongation of Be--Se bonds
along the chain as compared to those involving isolated Be atoms. The variation
of force constants with interatomic distances shows common trends in relative
independence on the short-range order.Comment: 11 pages, 10 figures, to be published in Phys. Rev.
Crecimiento in-situ de nanoclusters metalicos de Mn intercalados en una bentonita previamente pilarizada con AL
10 kg scaled-up preparation of Al/Fe-pillared clay CWPO catalysts from concentrated precursors
In this work, the significant intensification of a bentonite pillaring process was achieved by using a novel
methodological approach, leading to an intercalating Al/Fe mixed oligomeric precursor, around 100 times more concentrated than usually reported. In addition, the intercalating step was achieved directly on the clay with no previous swelling of the mineral being required; this allowed the successful scaled-up preparation of the Al/Fe-PILC, by a factor of one thousand, from the lab (10 g) to the pilot scale (10 kg).
Intercalating solutions prepared under either oncentrated (13 cm3) or diluted (widely reported, 2.0 dm3) conditions for lab-scale preparations were both translucent, displaying similar final pH values (close to 4.0) typical of highly oligomerized Al-pillaring solutions. The clay modified from concentrated precursors at the 10 g scale reached a high basal spacing (18.3 Å) and specific surface area (198 m2 g−1 ) with very comparable fractions of Fe forming truly mixed Al/Fe pillars in comparison to a reference material (H2-TPR analyses). This promoted high performance in the catalytic wet peroxide oxidation of phenol in aqueous solution as a toxic model organic molecule at very mild temperature (25.0 °C ± 1.0 °C) and
pressure (76 kPa), exhibiting the highest catalytic efficiency as a function of both parameters (full conversion of phenol together with 45.2% of TOC mineralization) with low iron leaching using a very low catalyst concentration (0.25 g dm−3). Particle size refining of the starting clay, the speed of stirring and conditions for the final washing of the interlayered precursor are the main factors influencing successful pillaring at scales higher than 1.0 kg
Uses of droplet-vitrification technique as a long-term storage method and for virus elimination.
Implementation of a cryopreservation system to establish a duplicate of the cassava core collection
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