43 research outputs found

    Borici-Creutz fermions on 2-dim lattice

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    Minimally doubled fermion proposed by Creutz and Borici is a promising chiral fermion formulation on lattice. In this work, we present excited state mass spectroscopy for the meson bound states in Gross-Neveu model using Borici-Creutz fermion. We also evaluate the effective fermion mass as a function of coupling constant which shows a chiral phase transition at strong coupling. The lowest lying meson in 2-dimensional QED is also obtained using Borici-Creutz fermion.Comment: 7 pages, 12 figure. arXiv admin note: text overlap with arXiv:1511.0767

    Estimation of collision centrality in terms of the number of participating nucleons in heavy-ion collisions using deep learning

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    The deep learning technique has been applied for the first time to investigate the possibility of centrality determination in terms of the number of participants (NpartN_{\mathrm{part}}) in high-energy heavy-ion collisions. For this purpose, supervised learning using both deep neural network (DNN) and convolutional neural network (CNN) is performed with labeled data obtained by modeling relativistic heavy-ion collisions utilizing A Multi-phase Transport Model (AMPT). Event-by-event distributions of pseudorapidity and azimuthal angle of charged hadrons weighted by their transverse momentum are used as input to train the DL models. The DL models did remarkably well in predicting NpartN_{\mathrm{part}} values with CNN slightly outperforming the DNN model. The Mean Squared Logarithmic Error (MSLE) for the CNN model (Model-4) is determined to be 0.0592 for minimum bias collisions and 0.0114 for 0-60\% centrality class, indicating that the model performs better for semi-central and central collisions. Furthermore, the studied DL model is proven to be robust to changes in energy as well as model parameters of the input. The current study demonstrates that the data-driven technique has a distinct potential for determining centrality in terms of the number of participants in high-energy heavy-ion collision experiments.Comment: 13 pages, and 7 figure

    Estimating centrality in heavy-ion collisions using Transfer Learning technique

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    In this study, we explore the applicability of Transfer Learning techniques for estimating collision centrality in terms of the number of participants (NpartN_{\rm part}) in high-energy heavy-ion collisions. In the present work, we leverage popular pre-trained CNN models such as VGG16, ResNet50, and DenseNet121 to determine NpartN_{\rm part} in Au+Au collisions at s=200\sqrt{s}=200 GeV on an event-by-event basis. Remarkably, all three models achieved good performance despite the pre-trained models being trained for databases of other domains. Particularly noteworthy is the superior performance of the VGG16 model, showcasing the potential of transfer learning techniques for extracting diverse observables from heavy-ion collision data.Comment: 14 pages, 10 figure

    Prompt emission polarimetry of Gamma Ray Bursts with ASTROSAT CZT-Imager

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    X-ray and Gamma-ray polarization measurements of the prompt emission of Gamma-ray bursts (GRBs) are believed to be extremely important for testing various models of GRBs. So far, the available measurements of hard X-ray polarization of GRB prompt emission have not significantly constrained the GRB models, particularly because of the difficulty of measuring polarization in these bands. The CZT Imager (CZTI) onboard {\em AstroSat} is primarily an X-ray spectroscopic instrument that also works as a wide angle GRB monitor due to the transparency of its support structure above 100 keV. It also has experimentally verified polarization measurement capability in the 100 - 300 keV energy range and thus provides a unique opportunity to attempt spectro-polarimetric studies of GRBs. Here we present the polarization data for the brightest 11 GRBs detected by CZTI during its first year of operation. Among these, 5 GRBs show polarization signatures with \gtrapprox3σ\sigma, and 1 GRB shows \>2σ\sigma detection significance. We place upper limits for the remaining 5 GRBs. We provide details of the various tests performed to validate our polarization measurements. While it is difficult yet to discriminate between various emission models with the current sample alone, the large number of polarization measurements CZTI expects to gather in its minimum lifetime of five years should help to significantly improve our understanding of the prompt emission.Comment: Accepted for Publication in ApJ ; a figure has been update

    A Low-Voltage, Low-Power 4-bit BCD Adder, designed using the Clock Gated Power Gating, and the DVT Scheme

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    This paper proposes a Low-Power, Energy Efficient 4-bit Binary Coded Decimal (BCD) adder design where the conventional 4-bit BCD adder has been modified with the Clock Gated Power Gating Technique. Moreover, the concept of DVT (Dual-vth) scheme has been introduced while designing the full adder blocks to reduce the Leakage Power, as well as, to maintain the overall performance of the entire circuit. The reported architecture of 4-bit BCD adder is designed using 45 nm technology and it consumes 1.384 {\mu}Watt of Average Power while operating with a frequency of 200 MHz, and a Supply Voltage (Vdd) of 1 Volt. The results obtained from different simulation runs on SPICE, indicate the superiority of the proposed design compared to the conventional 4-bit BCD adder. Considering the product of Average Power and Delay, for the operating frequency of 200 MHz, a fair 47.41 % reduction compared to the conventional design has been achieved with this proposed scheme.Comment: To appear in the proceedings of 2013 IEEE International Conference on Signal Processing, Computing and Control (ISPCC,13

    Violation of synchrotron line of death by the highly polarized GRB 160802AGRB~160802A

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    GRB 160802AGRB~160802A is one of the brightest gamma-ray bursts (GRBs) observed with FermiFermi Gamma-ray Burst Monitor (GBM) in the energy range of 10  100010~-~1000 keV, while at the same time it is surprisingly faint at energies 2\gtrsim2 MeV. An observation with AstroSatAstroSat/CZT Imager (CZTI) also provides the polarisation which helps in constraining different prompt emission models using the novel joint spectra-polarimetric data. We analyze the FermiFermi/GBM data, and find two main bursting episodes that are clearly separated in time, one particularly faint in higher energies and having certain differences in their spectra. The spectrum in general shows a hard-to-soft evolution in both the episodes. Only the later part of the first episode shows intensity tracking behaviour corresponding to multiple pulses. The photon index of the spectrum is hard, and in over 90 per cent cases, cross even the slow cooling limit (α=2/3\alpha=-2/3) of an optically thin synchrotron shock model (SSM). Though such hard values are generally associated with a sub-dominant thermal emission, such a component is not statistically required in our analysis. In addition, the measured polarisation in 100--300\,keV is too high, π=85±29%\pi=85\pm29\%, to be accommodated in such a scenario. Jitter radiation, which allows a much harder index up to α=+0.5\alpha=+0.5, in principle can produce high polarisation but only beyond the spectral peak, which in our case lies close to 200  300200~-~300 keV during the time when most of the polarisation signal is obtained. The spectro-polarimetric data seems to be consistent with a subphotospheric dissipation process occurring within a narrow jet with a sharp drop in emissivity beyond the jet edge, and viewed along its boundary
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