235,021 research outputs found

    Biodegradable Polylactic Acid (PLA) Microstructures for Scaffold Applications

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    In this research, we present a simple and cost effective soft lithographic process to fabricate PLA scaffolds for tissue engineering. In which, the negative photoresist JSR THB-120N was spun on a glass subtract followed by conventional UV lithographic processes to fabricate the master to cast the PDMS elastomeric mold. A thin poly(vinyl alcohol) (PVA) layer was used as a mode release such that the PLA scaffold can be easily peeled off. The PLA precursor solution was then cast onto the PDMS mold to form the PLA microstructures. After evaporating the solvent, the PLA microstructures can be easily peeled off from the PDMS mold. Experimental results show that the desired microvessels scaffold can be successfully transferred to the biodegradable polymer PLA.Comment: Submitted on behalf of EDA Publishing Association (http://irevues.inist.fr/EDA-Publishing

    Nonlinear response and scaling law in the vortex state of d-wave superconductors

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    We study the field dependence of the quasi-particle density of states, the thermodynamics and the transport properties in the vortex state of d-wave superconductors when a magnetic field is applied perpendicular to the conducting plane, specially for the low field and the low temperature compared to the upper critical field and transition temperature, respectively, H/Hc2ā‰Ŗ1H/H_{c2} \ll 1 and T/Tcā‰Ŗ1T/T_c \ll 1. Both the superfluid density and the spin susceptibility exhibit the characteristic H\sqrt{H}-field dependence, while the nuclear spin lattice relaxation rate T1āˆ’1_1^{-1} and the thermal conductivity are linear in field HH. With increasing temperature, these quantities exhibit the scaling behavior in T/HT/\sqrt{H}. The present theory applies to 2D ff-wave superconductor as well; a possible candidate of the superconductivity in Sr2_2RuO4_4.Comment: 11 pages, 4 figure

    Automatic Brain Tumor Segmentation using Convolutional Neural Networks with Test-Time Augmentation

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    Automatic brain tumor segmentation plays an important role for diagnosis, surgical planning and treatment assessment of brain tumors. Deep convolutional neural networks (CNNs) have been widely used for this task. Due to the relatively small data set for training, data augmentation at training time has been commonly used for better performance of CNNs. Recent works also demonstrated the usefulness of using augmentation at test time, in addition to training time, for achieving more robust predictions. We investigate how test-time augmentation can improve CNNs' performance for brain tumor segmentation. We used different underpinning network structures and augmented the image by 3D rotation, flipping, scaling and adding random noise at both training and test time. Experiments with BraTS 2018 training and validation set show that test-time augmentation helps to improve the brain tumor segmentation accuracy and obtain uncertainty estimation of the segmentation results.Comment: 12 pages, 3 figures, MICCAI BrainLes 201

    An unexpectedly low-redshift excess of Swift gamma-ray burst rate

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    Gamma-ray bursts (GRBs) are the most violent explosions in the Universe and can be used to explore the properties of high-redshift universe. It is believed that the long GRBs are associated with the deaths of massive stars. So it is possible to use GRBs to investigate the star formation rate (SFR). In this paper, we use Lynden-Bell's cāˆ’c^- method to study the luminosity function and rate of \emph{Swift} long GRBs without any assumptions. We find that the luminosity of GRBs evolves with redshift as L(z)āˆg(z)=(1+z)kL(z)\propto g(z)=(1+z)^k with k=2.43āˆ’0.38+0.41k=2.43_{-0.38}^{+0.41}. After correcting the redshift evolution through L0(z)=L(z)/g(z)L_0(z)=L(z)/g(z), the luminosity function can be expressed as Ļˆ(L0)āˆL0āˆ’0.14Ā±0.02\psi(L_0)\propto L_0^{-0.14\pm0.02} for dim GRBs and Ļˆ(L0)āˆL0āˆ’0.70Ā±0.03\psi(L_0)\propto L_0^{-0.70\pm0.03} for bright GRBs, with the break point L0b=1.43Ɨ1051Ā ergĀ sāˆ’1L_{0}^{b}=1.43\times10^{51}~{\rm erg~s^{-1}}. We also find that the formation rate of GRBs is almost constant at z<1.0z<1.0 for the first time, which is remarkably different from the SFR. At z>1.0z>1.0, the formation rate of GRB is consistent with the SFR. Our results are dramatically different from previous studies. Some possible reasons for this low-redshift excess are discussed. We also test the robustness of our results with Monte Carlo simulations. The distributions of mock data (i.e., luminosity-redshift distribution, luminosity function, cumulative distribution and logā”Nāˆ’logā”S\log N-\log S distribution) are in good agreement with the observations. Besides, we also find that there are remarkable difference between the mock data and the observations if long GRB are unbiased tracers of SFR at z<1.0z<1.0.Comment: 33 pages, 10 figures, 1 table, accepted by ApJ
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