26,187 research outputs found
Lepton Flavor Violation in B Decays?
The LHCb Collaboration's measurement of R_K = B(B+ -> K+ mu+ mu-)/B(B+ -> K+
e+e-) lies 2.6 sigma below the Standard Model prediction. Several groups
suggest this deficit to result from new lepton non-universal interactions of
muons. But non-universal leptonic interactions imply lepton flavor violation in
B decays at rates much larger than are expected in the Standard Model. A simple
model shows that these rates could lie just below current limits. An
interesting consequence of our model, that B(B_s -> mu+ mu-)_{exp}/B(B_s -> mu+
mu-)_{SM} = R_K = 0.75, is compatible with recent measurements of these rates.
We stress the importance of searches for lepton flavor violations, especially
for B -> K mu e, K mu tau and B_s -> mu e, mu tau.Comment: 8 pages. Discussion of P'5 added; some discussion sharpened;
discussion of decays with tau's modified; references adde
A new method to find the potential center of N-body systems
We present a new and fast method to nd the potential center of an N-body
distribution. The method uses an iterative algorithm which exploits the fact that
the gradient of the potential is null at its center: it uses a smoothing radius to
avoid getting trapped in secondary minima. We have tested this method on several
random realizations of King models (in which the numerical computation of this
center is rather dicult, due to the constant density within their cores), and com-
pared its performance and accuracy against a more straightforward, but computer
intensive method, based on cartesian meshes of increasing spatial resolution. In all
cases, both methods converged to the same center, within the mesh resolution, but
the new method is two orders of magnitude faster.
We have also tested the method with one astronomical problem: the evolu-
tion of a 105 particle King model orbiting around a xed potential that represents
our Galaxy. We used a spherical harmonics expansion N-body code, in which the
potential center determination is crucial for the correct force computation. We
compared this simulation with another one in which a method previously used to
determine the expansion center is employed (White 1983). Our routine gives better
results in energy conservation and mass loss.Fil: Aguilar, L. A.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; MéxicoFil: Cruz, F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; MéxicoFil: Carpintero, Daniel Diego. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentin
Voronoi Cell Patterns: theoretical model and applications
We use a simple fragmentation model to describe the statistical behavior of
the Voronoi cell patterns generated by a set of points in 1D and in 2D. In
particular, we are interested in the distribution of sizes of these Voronoi
cells. Our model is completely defined by two probability distributions in 1D
and again in 2D, the probability to add a new point inside an existing cell and
the probability that this new point is at a particular position relative to the
preexisting point inside this cell. In 1D the first distribution depends on a
single parameter while the second distribution is defined through a
fragmentation kernel; in 2D both distributions depend on a single parameter.
The fragmentation kernel and the control parameters are closely related to the
physical properties of the specific system under study. We use our model to
describe the Voronoi cell patterns of several systems. Specifically, we study
the island nucleation with irreversible attachment, the 1D car parking problem,
the formation of second-level administrative divisions, and the pattern formed
by the Paris M\'etro stations.Comment: 12 pages, 9 figure
Experiencia de enseñanza de la Geometría con NeoTrie VR
The possibilities of using the new software of virtual reality NeoTrie VR (or Neotrie) to teach geometry to children aged 11- 14 years old are presented. This software is tested for the first time as a part of math lessons at a School in Żernica (Poland). The use of Neotrie has made it easier to eliminate some of the problems faced by the pupils in the early stages of geometry learning. Moreover, the participating students solve geometric tasks more quickly, compared with previous years, especially those that require spatial imagination and those with a higher degree of difficulty. Since the program has been implemented, pupils are more active and prone to cooperation, and to formulate conclusions. Neotrie turns out to be a useful tool for teaching Geometry, it helps students to better organize their geometric knowledge in a ludic way, to increase their spatial reasoning and creativity
Analyzing Capture Zone Distributions (CZD) in Growth: Theory and Applications
We have argued that the capture-zone distribution (CZD) in submonolayer
growth can be well described by the generalized Wigner distribution (GWD)
, where is the CZ area divided by its average
value. This approach offers arguably the best method to find the critical
nucleus size , since . Various analytical and numerical
investigations, which we discuss, show that the simple GWD expression is
inadequate in the tails of the distribution, it does account well for the
central regime , where the data is sufficiently large to be
reliably accessible experimentally. We summarize and catalog the many
experiments in which this method has been applied.Comment: 6 pages, 3 figures, conference paper for 17th International
Conference on Crystal Growth and Epitaxy (ICCGE-17), Warsaw, Poland, Aug.
11-16, 2013, submitted for publication in different forma
The evolution of the bi-modal colour distribution of galaxies in SDSS groups
We analyse colour distributions for several samples of galaxies in
groups drawn from the Fourth Data Release of the Sloan Digital Sky Survey. For
all luminosity ranges and environments considered the colour distributions are
well described by the sum of two Gaussian functions. We find that the fraction
of galaxies in the red sequence is an increasing function of group virial mass.
We also study the evolution of the galaxy colour distributions at low redshift,
in the field and in groups for galaxies brighter than
, finding significant evidence of recent evolution in the
population of galaxies in groups. The fraction of red galaxies monotonically
increases with decreasing redshift, this effect implies a much stronger
evolution of galaxies in groups than in the field.Comment: 7 pages, 6 figures, submited to MNRAS after minor revisio
Sporopollenin, the least known yet toughest natural biopolymer
© 2015 Mackenzie, Boa, Diego-Taboada, Atkin and Sathyapalan. Sporopollenin is highly cross-linked polymer composed of carbon, hydrogen, and oxygen that is extraordinarily stable and has been found chemically intact in sedimentary rocks some 500 million years old. It makes up the outer shell (exine) of plant spores and pollen and when extracted it is in the form of an empty exine or microcapsule. The exines resemble the spores and pollen from which they are extracted, in size and morphology. Also, from any one plant such characteristics are incredible uniform. The exines can be used as microcapsules or simply as micron-sized particles due to the variety of functional groups on their surfaces. The loading of a material into the chamber of the exine microcapsule is via multi-directional nano-diameter sized channels. The exines can be filled with a variety of polar and non-polar materials. Enzymes can be encapsulated within the shells and still remain active. In vivo studies in humans have shown that an encapsulated active substance can have a substantially increased bioavailability than if it is taken alone. The sporopollenin exine surface possesses phenolic, alkane, alkene, ketone, lactone, and carboxylic acid groups. Therefore, it can be derivatized in a number of ways, which has given rise to applications in areas, such as solid supported for peptide synthesis, catalysis, and ion-exchange chromatography. Also, the presence of the phenolic groups on sporopollenin endows it with antioxidant activity
Global soil moisture bimodality in satellite observations and climate models
A new diagnostic metric based on soil moisture bimodality is developed in order to examine and compare soil moisture from satellite observations and Earth System Models. The methodology to derive this diagnostic is based on maximum likelihood estimator encoded into an iterative algorithm, which is applied to the soil moisture probability density function. This metric is applied to satellite data from the Advanced Microwave Scanning Radiometer for the Earth Observing System and global climate models data from the Coupled Model Intercomparison Project Phase 5 (CMIP5). Results show high soil moisture bimodality in transitional climate areas and high latitudes, potentially associated with land-atmosphere feedback processes. When comparing satellite versus climate models, a clear difference in their soil moisture bimodality is observed, with systematically higher values in the case of CMIP5 models. These differences appear related to areas where land-atmospheric feedback may be overestimated in current climate models
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