2,996 research outputs found
Multi-particle and High-dimension Controlled Order Rearrangement Encryption Protocols
Based on the controlled order rearrange encryption (CORE) for quantum key
distribution using EPR pairs[Fu.G.Deng and G.L.Long Phys.Rev.A68 (2003)
042315], we propose the generalized controlled order rearrangement encryption
(GCORE) protocols of qubits and qutrits, concretely display them in the
cases using 3-qubit, 2-qutrit maximally entangled basis states. We further
indicate that our protocols will become safer with the increase of number of
particles and dimensions. Moreover, we carry out the security analysis using
quantum covariant cloning machine for the protocol using qutrits. Although the
applications of the generalized scheme need to be further studied, the GCORE
has many distinct features such as great capacity and high efficiency
Compound orbits break-up in constituents: an algorithm
In this paper decomposition of periodic orbits in bifurcation diagrams are
derived in unidimensional dynamics system , being an
unimodal function. We proof a theorem which states the necessary and sufficient
conditions for the break-up of compound orbits in their simpler constituents. A
corollary to this theorem provides an algorithm for the computation of those
orbits. This process closes the theoretical framework initiated in (Physica D,
239:1135--1146, 2010)
An updated catalog of M33 clusters and candidates: photometry, and some statistical results
We present photometry for 392 star clusters and candidates in the
field of M33, which are selected from the most recent star cluster catalog. In
this catalog, the authors listed star clusters' parameters such as cluster
positions, magnitudes and colors in the filters, and so on.
However, a large fraction of objects in this catalog do not have previously
published photometry. Photometry is performed using archival images from the
Local Group Galaxies Survey, which covers 0.8 deg along the major axis of
M33. Detailed comparisons show that, in general, our photometry is consistent
with previous measurements. Positions (right ascension and declination) for
some clusters are corrected here. Combined with previous literature, we
constitute a large sample of M33 star clusters. Based on this cluster sample,
we present some statistical results: none of the M33 youngest clusters ( yr) have masses approaching ; roughly half the star
clusters are consistent with the to mass models; the
continuous distribution of star clusters along the model line indicates that
M33 star clusters have been formed continuously from the epoch of the first
star cluster formation until recent times; there are star clusters
which being overlapped with the Galactic globular clusters on the color-color
diagram, and these clusters are old globular clusters candidates in M33.Comment: Accepted for Publication in AJ, 22 pages, 12 figures and 9 table
Caractérisation physico-chimique de la gomme Sterculia de trois localités de la région de Tambacounda au Sénégal
La gomme sterculia est produite par Sterculia setigera Del. en Afrique. Ses propriétés physicochimiques changent suivant divers facteurs dont l’influence sur sa qualité a été peu étudiée. C’est dans cette perspective que l’humidité, le pH, le pouvoir gonflant et la viscosité de cette gomme ont été évalués au Sénégal (Daoudi, Malem niani et Bala). Les résultats ont montré que son humidité varie en fonction du phénotype (écorce claire ou foncée). Elle a été plus élevée sur la gomme de la période sèche-chaude à Daoudi mais elle n’a pas changé suivant le site après un an de conservation. Son pH a varié en fonction de l’interaction période de saignée- couleur de l’écorce à Malem Niani alors qu’à Daoudi il a varié suivant la période de saignée seulement. A Malem, son gonflement a aussi varié suivant l’interaction période de saignée-couleur de l’écorce. Après un an de conservation (température ambiante), son pouvoir gonflant a diminué dans tous les sites. Sa viscosité a été 3,5 fois plus élevée à Bala qu’à Daoudi et Malem Niani. Ces résultats ont permis d’acquérir de nouvelles connaissances et d’identifier Bala comme ayant la meilleure qualité de gomme par rapport aux deux autres sites.Mots clés: Acidité, Humidité, pouvoir de gonflement, Sterculia setigera Del., Tambacounda, viscosité
Constructions of Semi-regular Relative Difference Sets
AbstractJ. A. Davis, J. Jedwab, and M. Mowbray (1998, Des. Codes Cryptogr.13, 131–146) gave two new constructions for semi-regular relative difference sets (RDSs). They asked if the two constructions could be unified. In this paper, we show that the two constructions are closely related. In fact, the second construction should be viewed as an extension of the first. Furthermore, we generalize the second construction to obtain new RDSs
The M33 Globular Cluster System with PAndAS Data: The Last Outer Halo Cluster?
We use CFHT/MegaCam data to search for outer halo star clusters in M33 as
part of the Pan-Andromeda Archaeological Survey (PAndAS). This work extends
previous studies out to a projected radius of 50 kpc and covers over 40 square
degrees. We find only one new unambiguous star cluster in addition to the five
previously known in the M33 outer halo (10 kpc <= r <= 50 kpc). Although we
identify 2440 cluster candidates of various degrees of confidence from our
objective image search procedure, almost all of these are likely background
contaminants, mostly faint unresolved galaxies. We measure the luminosity,
color and structural parameters of the new cluster in addition to the five
previously-known outer halo clusters. At a projected radius of 22 kpc, the new
cluster is slightly smaller, fainter and redder than all but one of the other
outer halo clusters, and has g' ~ 19.9, (g'-i') ~ 0.6, concentration parameter
c ~ 1.0, a core radius r_c ~ 3.5 pc, and a half-light radius r_h ~ 5.5 pc. For
M33 to have so few outer halo clusters compared to M31 suggests either tidal
stripping of M33's outer halo clusters by M31, or a very different, much calmer
accretion history of M33.Comment: 37 pages, 9 figures. Accepted by the Astrophysical Journa
Age and mass studies for young star clusters in M31 from SEDs-fit
In this paper, we present photometry for young star clusters in M31, which
are selected from Caldwell et al. These star clusters have been observed as
part of the Beijing--Arizona--Taiwan--Connecticut (BATC) Multicolor Sky Survey
from 1995 February to 2008 March. The BATC images including these star clusters
are taken with 15 intermediate-band filters covering 3000--10000 \AA. Combined
with photometry in the {\sl GALEX} far- and near-ultraviolet, broad-band
, SDSS , and infrared of Two Micron All Sky Survey,
we obtain their accurate spectral energy distributions (SEDs) from 1538-20000
\AA. We derive these star clusters' ages and masses by comparing their SEDs
with stellar population synthesis models. Our results are in good agreement
with previous determinations. The mean value of age and mass of young clusters
( Gyr) is about 385 Myr and , respectively. There
are two distinct peaks in the age distribution, a highest peak at age 60
Myr and a secondary peak around 250 Myr, while the mass distribution shows a
single peak around . A few young star clusters have two-body
relaxation times greater than their ages, indicating that those clusters have
not been well dynamically relaxed and therefore have not established the
thermal equilibrium. There are several regions showing aggregations of young
star clusters around the 10 kpc ring and the outer ring, indicating that the
distribution of the young star clusters is well correlated with M31's
star-forming regions. The young massive star clusters (age Myr and
mass ) show apparent concentration around the ring
splitting region, suggesting a recent passage of a satellite galaxy (M32)
through M31 disk.Comment: Accepted for Publication in AJ, 15 pages, 14 figures and 4 table
Probabilistic degenerate Fubini polynomials associated with random variables
Let Y be a random variable such that the moment generating function of Y
exists in a neighborhood of the origin. The aim of this paper is to study
probabilistic versions of the degenerate Fubini polynomials and the degenerate
Fubini polynomials of order , namely the probabilisitc degenerate Fubini
polynomials associated with Y and the probabilistic degenerate Fubini
polynomials of order r associated with Y. We derive some properties, explicit
expressions, certain identities and recurrence relations for those polynomials.Comment: 1
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