1,034 research outputs found
Improved 3D thinning algorithms for skeleton extraction
In this study, we focused on developing a novel 3D Thinning algorithm to extract one-voxel wide skeleton from various 3D objects aiming at preserving the topological information. The 3D Thinning algorithm was testified on computer-generated and real 3D reconstructed image sets acquired from TEMT and compared with other existing 3D Thinning algorithms. It is found that the algorithm has conserved medial axes and simultaneously topologies very well, demonstrating many advantages over the existing technologies. They are versatile, rigorous, efficient and rotation invariant.<br /
Sodium and potassiumvapor Faraday filters re-visited: Theory and applications
A complete theory describing the transmission of atomic vapor Faraday filters is developed. The dependence of the filter transmission on atomic density and external magnetic field strength, as well as the frequency dependence of transmission, are explained in physical terms. As examples, applications of the computed results to ongoing research to suppress sky background, thus allowing Na lidar operation under sunlit conditions, and to enable measurement of the density of mesospheric oxygen atoms are briefly discussed
Search for Light Weakly-Interacting-Massive-Particle Dark Matter by Annual Modulation Analysis with a Point-Contact Germanium Detector at the China Jinping Underground Laboratory
We present results on light weakly interacting massive particle (WIMP)
searches with annual modulation (AM) analysis on data from a 1-kg mass -type
point-contact germanium detector of the CDEX-1B experiment at the China Jinping
Underground Laboratory. Datasets with a total live time of 3.2 yr within a 4.2
yr span are analyzed with analysis threshold of 250 eVee. Limits on
WIMP-nucleus (-) spin-independent cross sections as function of WIMP
mass () at 90\% confidence level (C.L.) are derived using the dark
matter halo model. Within the context of the standard halo model, the 90\% C.L.
allowed regions implied by the DAMA/LIBRA and CoGeNT AM-based analysis are
excluded at 99.99\% and 98\% C.L., respectively. These results correspond to
the best sensitivity at 6 among WIMP AM
measurements to date.Comment: 5 pages, 4 figure
Constraints on Spin-Independent Nucleus Scattering with sub-GeV Weakly Interacting Massive Particle Dark Matter from the CDEX-1B Experiment at the China Jin-Ping Laboratory
We report results on the searches of weakly interacting massive particles
(WIMPs) with sub-GeV masses () via WIMP-nucleus spin-independent
scattering with Migdal effect incorporated. Analysis on time-integrated (TI)
and annual modulation (AM) effects on CDEX-1B data are performed, with 737.1
kgday exposure and 160 eVee threshold for TI analysis, and 1107.5
kgday exposure and 250 eVee threshold for AM analysis. The sensitive
windows in are expanded by an order of magnitude to lower DM masses
with Migdal effect incorporated. New limits on at
90\% confidence level are derived as 1010
for TI analysis at 50180 MeV/, and
1010 for AM analysis at
75 MeV/3.0 GeV/.Comment: 5 pages, 4 figure
Supersymmetric Intersecting Branes on the Waves
We construct a general family of supersymmetric solutions in time- and
space-dependent wave backgrounds in general supergravity theories describing
single and intersecting p-branes embedded into time-dependent dilaton-gravity
plane waves of an arbitrary (isotropic) profile, with the brane world-volume
aligned parallel to the propagation direction of the wave. We discuss how many
degrees of freedom we have in the solutions. We also propose that these
solutions can be used to describe higher-dimensional time-dependent "black
holes", and discuss their property briefly.Comment: 12 pages, LaTe
A Note on Noncommutative Brane Inflation
In this paper, we investigate the noncommutative KKLMMT D3/anti-D3 brane
inflation scenario in detail. Incorporation of the brane inflation scenario and
the noncommutative inflation scenario can nicely explain the large negative
running of the spectral index as indicated by WMAP three-year data and can
significantly release the fine-tuning for the parameter . Using the WMAP
three year results (blue-tilted spectral index with large negative running), we
explore the parameter space and give the constraints and predictions for the
inflationary parameters and cosmological observables in this scenario. We show
that this scenario predicts a quite large tensor/scalar ratio and what is more,
a too large cosmic string tension (assuming that the string coupling is
in its likely range from 0.1 to 1) to be compatible with the present
observational bound. A more detailed analysis reveals that this model has some
inconsistencies according to the fit to WMAP three year results.Comment: 20 pages, 5 figures; accepted for publication in JCA
Bottleneck effects in turbulence: Scaling phenomena in r- versus p-space
We (analytically) calculate the energy spectrum corresponding to various
experimental and numerical turbulence data analyzed by Benzi et al.. We find
two bottleneck phenomena: While the local scaling exponent of the
structure function decreases monotonically, the local scaling exponent
of the corresponding spectrum has a minimum of
at and a maximum
of at . A physical
argument starting from the constant energy flux in p--space reveals the general
mechanism underlying the energy pileups at both ends of the p--space scaling
range. In the case studied here, they are induced by viscous dissipation and
the reduced spectral strength on the scale of the system size, respectively.Comment: 9 pages, 3figures on reques
A Matrix Model for the Null-Brane
The null-brane background is a simple smooth 1/2 BPS solution of string
theory. By tuning a parameter, this background develops a big crunch/big bang
type singularity. We construct the DLCQ description of this space-time in terms
of a Yang-Mills theory on a time-dependent space-time. Our dual Matrix
description provides a non-perturbative framework in which the fate of both
(null) time, and the string S-matrix can be studied.Comment: 26 pages, LaTeX; references adde
Non-escaping frost tolerant QTL linked genetic loci at reproductive stage in six wheat DH populations
Reproductive stage frost poses a major constraint for wheat production in countries such as Australia. However, little progress has been made in identifying key genes to overcome the constraint. In the present study, a severe frost event hit two large-scale field trials consisting of six doubled haploid (DH) wheat populations at reproductive stage (young microspore stage) in Western Australia, leading to the identification of 30 robust frost QTL on 17 chromosomes. The major 18 QTL with the phenotype variation over 9.5% were located on 13 chromosomes including 2A, 2B, 2D, 3A, 4A, 4B, 4D, 5A, 5D, 6D, 7A, 7B and 7D. Most frost QTL were closely linked to the QTL of anthesis, maturity, Zadok stages as well as linked to anthesis related genes. Out of those, six QTL were repetitively detected on the homologous regions on 2B, 4B, 4D, 5A, 5D, 7A in more than two populations. Results showed that the frost damage is associated with alleles of Vrn-A1a, Vrn-D1a, Rht-B1b, Rht-D1b, and the high copy number of Ppd-B1. However, anthesis QTL and anthesis related genes of Vrn-B1a and TaFT3-1B on chromosomes 5B and 1B did not lead to frost damage, indicating that these early-flowering phenotype related genes are compatible with frost tolerance and thus can be utilised in breeding. Our results also indicate that wild-type alleles Rht-B1a and Rht-D1a can be used when breeding for frost-tolerant varieties without delaying flowering time
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