Journal articles: 'Binary energy'

1

Mashud Hyder, Md, and Kaushik Mahata. "Reconfiguration of distribution system using a binary programming model." AIMS Energy 4, no. 3 (2016): 461–80. http://dx.doi.org/10.3934/energy.2016.3.461.

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Fang, Yingping, Gota Kikugawa, Hiroki Matsubara, Takeshi Bessho, Seiji Yamashita, and Taku Ohara. "108 Molecular Thermal Energy Transfer in Binary Mixture of Simple Liquids." Proceedings of Conference of Tohoku Branch 2016.51 (2016): 15–16. http://dx.doi.org/10.1299/jsmeth.2016.51.15.

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Changyuan Xu, Changyuan Xu, Cheng Zhan Changyuan Xu, Jingrui Liao Cheng Zhan, and Bin Zeng Jingrui Liao. "UAV-Enabled Mobile Edge Computing with Binary Computation Offloading and Energy Constraints." 網際網路技術學刊 23, no. 5 (September 2022): 947–54. http://dx.doi.org/10.53106/160792642022092305003.

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Mobile edge computing (MEC) has been considered to provide computation services near the edge of mobile networks, while the unmanned aerial vehicle (UAV) is becoming an important integrated component to extend service coverage. In this paper, we consider a UAV-enabled MEC with binary computation offloading and energy constraints, where an energy-limited UAV is employed as an aerial edge server and each task of devices is either executing locally or offloading to the aerial edge server as a whole. To provide fairness among different ground devices, we aim to maximize the minimum computation throughput among all devices via the joint design of computing mode selection and UAV trajectory as well as resource allocation. The optimization problem is formulated as a mixed-integer non-linear problem consisting of binary variables, which is difficult to tackle. By employing deductive penalty function to penalize the effect of non-binary solution, we develop an efficient iterative algorithm to obtain a suboptimal solution via leveraging the penalty successive convex approximation (P-SCA) method and difference of two convex (D.C.) optimization framework, where the algorithm is guaranteed to converge. Extensive simulations are conducted and the results with different system parameters show that the proposed joint design algorithm can improve the computation throughput by about 40% compared to other benchmark schemes.

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Luo, Chao, Jun Zhao, Yulie Gong, Yongzhen Wang, and Weibin Ma. "Energy efficiency comparison between geothermal power systems." Thermal Science 21, no. 6 Part A (2017): 2633–42. http://dx.doi.org/10.2298/tsci151225074l.

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The geothermal water which can be considered for generating electricity with the temperature ranging from 80? to 150? in China because of shortage of electricity and fossil energy. There are four basic types of geothermal power systems: single flash, double flash, binary cycle, and flash-binary system, which can be adapted to geothermal energy utilization in China. The paper discussed the performance indices and applicable conditions of different power system. Based on physical and mathematical models, simulation result shows that, when geofluid temperature ranges from 100? to 130?, the net power output of double flash power is bigger than flash-binary system. When the geothermal resource temperature is between 130? and 150?, the net power output of flash-binary geothermal power system is higher than double flash system by the maximum value 5.5%. However, the sum water steam amount of double flash power system is 2 to 3 times larger than flash-binary power system, which will cause the bigger volume of equipment of power system. Based on the economy and power capacity, it is better to use flash-binary power system when the geofluid temperature is between 100? and 150?.

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5

Odusote, Y. A., and A. I. Popoola. "Thermodynamic Prediction of the Free Energy of Mixing and Activities of some Goldbased Binary Liquid Alloys." Nigeria Journal of Pure and Applied Physics 9, no. 1 (April 21, 2020): 11–16. http://dx.doi.org/10.4314/njpap.v9i1.3.

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The free energy of mixing and activities of gold in selected six Au-based binary liquid Au-Cu, Au-Zn, Au-Pb, Au-Ni, Au-Sn and Al-Au alloys at different working temperatures have been studied using the quasi-chemical approximation model (QCAM). The predicted free enegry of mixing and activities results were compared with available experimental values. The predicted results are in reasonable agreement with reported experimental data and confirms that the model is reliable and, thus should serve as an alternative for the prediction of thermodynamic properties of binary liquid alloys. Keywords: free energy of mixing, activities, Au, Binary liquid alloys, concentration

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6

Bhat, Pradeep G., and Sabitha D'Souza. "Minimum Covering Energy of Binary Labeled Graph." International Journal of Mathematics and Soft Computing 4, no. 2 (July 13, 2014): 153. http://dx.doi.org/10.26708/ijmsc.2014.2.4.16.

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7

Han, Jin-Hua, Ying-Can Qin, Gang Guo, and Yan-Wen Zhang. "A method of designing binary energy degrader." Acta Physica Sinica 69, no. 3 (2020): 033401. http://dx.doi.org/10.7498/aps.69.20191514.

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8

LAMB, R. C., and T. C. WEEKES. "Very High Energy Gamma-Ray Binary Stars." Science 238, no. 4833 (December 11, 1987): 1528–34. http://dx.doi.org/10.1126/science.238.4833.1528.

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Lazaridis, Mihalis, and Yannis Drossinos. "Energy fluctuations in steady-state binary nucleation." Journal of Physics A: Mathematical and General 30, no. 11 (June 7, 1997): 3847–65. http://dx.doi.org/10.1088/0305-4470/30/11/015.

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10

Frustaci, Fabio, Stefania Perri, Marco Lanuzza, and Pasquale Corsonello. "Energy-efficient single-clock-cycle binary comparator." International Journal of Circuit Theory and Applications 40, no. 3 (July 25, 2010): 237–46. http://dx.doi.org/10.1002/cta.720.

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11

Li, Zhongmu, and Chen Yan. "Modeling of Integrated Spectral Energy Distributions of Stellar Populations with Various Binary Fractions." Journal of Physics: Conference Series 2068, no. 1 (October 1, 2021): 012048. http://dx.doi.org/10.1088/1742-6596/2068/1/012048.

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Abstract Binary stars are common in the universe, but binary fractions are various in different star clusters and galaxies. Studies have shown that binary fraction affects the integrated spectral energy distributions obviously, in particular in the UV band. It affects spectral fitting of many star clusters and galaxies significantly. However, previous works usually take a fixed binary fraction, i.e., 0.5, and this is far from getting accurate results. Therefore, it is important to model the integrated spectral energy distributions of stellar populations with various binary fractions. This work presents a modeling of spectral energy distributions of simple stellar populations with binary fractions of 0.3, 0.7, and 1.0. The results are useful for different kinds of spectral studies.

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12

Kim, Chang-Seob, Sungjin Lee, and Dong-Myeong Ha. "The Measurement of Flash Point for Unflammable-Flammable Binary Mixtures(CCl4+o-Xylene and CCl4+p-Xylene) Using Open Cup Tester." Journal of Energy Engineering 24, no. 4 (December 31, 2015): 18–23. http://dx.doi.org/10.5855/energy.2015.24.4.018.

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13

Wang, Jing. "IS GRAVITATIONAL VACUUM ENERGY RENORMALIZEDIN NEUTRON STAR BINARY?" International Journal of Advanced Research 10, no. 02 (February 28, 2022): 1147–53. http://dx.doi.org/10.21474/ijar01/14324.

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The vacuum energy of fluctuating quantum fields has been intensively studied by analyzing boundary conditions on the objects. By treating the two star components, making up of a wide neutron star (NS) binary with orbital separation of , as two Dirichlet point particles on the radial line, we calculate the quantum vacuum energy of fluctuating gravitational fields, arising from the Newtonian gravitational scalar potential and a gravitational vector potential that leads to the spiral-in orbital motion of the system. It is found that the stress tensor, which is responsible for the fluctuations of gravitational fields, gives rise to a finite quantum vacuum energy inside the binary system, i.e., in the region of . Accordingly, both objects making up of the binary are imposed by an additionally finite and attractive stress of . While outside the system, , the gravitational vacuum energy consists of a divergent term , resulting from the free Greens function without any presence of gravitational sources, and a term of that disappears when the distance is far away from the sources. However, the gravitational Casimir force imposed on NS binary is a finite one, because the fluctuating gravitational fields vanish on the star, on which the stress tensor appears discontinuity.

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14

Sargsyan, V. V., H. Lenske, G. G. Adamian, and N. V. Antonenko. "From dinuclear systems to close binary stars: Application to source of energy in the universe." International Journal of Modern Physics E 27, no. 11 (November 2018): 1850093. http://dx.doi.org/10.1142/s0218301318500933.

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The evolution of close binary stars in mass asymmetry (transfer) coordinate is considered. The conditions for the formation of stable symmetric binary stars are analyzed. The role of symmetrization of asymmetric binary star in the transformation of potential energy into internal energy of star and the release of a large amount of energy is revealed.

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15

Sargsyan, V. V., H. Lenske, G. G. Adamian, and N. V. Antonenko. "Close Binary Galaxies: Application to Source of Energy and Expansion in Universe." International Journal of Modern Physics E 28, no. 05 (May 2019): 1950031. http://dx.doi.org/10.1142/s0218301319500319.

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Applying the microscopic nuclear physics ideas for fusion reactions to macroscopic galactic systems, we study the evolution of the compact binary galaxy in mass asymmetry (transfer) coordinate. The conditions for the formation of stable symmetric binary galaxy are analyzed. The role of symmetrization of asymmetric binary galaxy in the transformation of gravitational energy into internal energy of galaxies accompanied by the release of a large amount of energy during the symmetrization process is revealed.

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Hagenmuller, Pascal, Guillaume Chambon, Bernard Lesaffre, Frédéric Flin, and Mohamed Naaim. "Energy-based binary segmentation of snow microtomographic images." Journal of Glaciology 59, no. 217 (2013): 859–73. http://dx.doi.org/10.3189/2013jog13j035.

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AbstractX-ray microtomography has become an essential tool for investigating the mechanical and physical properties of snow, which are tied to its microstructure. To allow a quantitative characterization of the microstructure, the grayscale X-ray attenuation coefficient image has to be segmented into a binary ice/pore image. This step, called binary segmentation, is crucial and affects all subsequent analysis and modeling. Common segmentation methods are based on thresholding. In practice, these methods present some drawbacks and often require time-consuming manual post-processing. Here we present a binary segmentation algorithm based on the minimization of a segmentation energy. This energy is composed of a data fidelity term and a regularization term penalizing large interface area, which is of particular interest for snow where sintering naturally tends to reduce the surface energy. The accuracy of the method is demonstrated on a synthetic image. The method is then successfully applied on microtomographic images of snow and compared to the threshold-based segmentation. The main advantage of the presented approach is that it benefits from local spatial information. Moreover, the effective resolution of the segmented image is clearly defined and can be chosen a priori.

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17

Vila, Gabriela S., Daniela Pérez, and Gustavo E. Romero. "High-energy signatures of binary supermassive black holes." EPJ Web of Conferences 61 (2013): 08005. http://dx.doi.org/10.1051/epjconf/20136108005.

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18

Abraham, Sneha Elizabeth, Dwaipayan Chakrabarti, and Biman Bagchi. "Energy landscape view of nonideality in binary mixtures." Journal of Chemical Physics 126, no. 7 (February 21, 2007): 074501. http://dx.doi.org/10.1063/1.2434967.

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19

Jiang, Dengkai, Jiangcheng Wang, Zhanwen Han, Tianyu Jiang, and Lifang Li. "The energy transfer in W UMa binary stars." Proceedings of the International Astronomical Union 4, S252 (April 2008): 433–34. http://dx.doi.org/10.1017/s1743921308023430.

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AbstractThe properties of W UMa binary stars are studied based on the well-determined physical parameters of 132 W UMa systems. It is found that the energy transfer rate has a maximum value at q ~ 0.58. The relation between the energy transfer rate and the temperature deviation is also investigated, and the temperature of the secondary component is related to the energy transfer rate.

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20

Namboodiri, P. M. S., and R. K. Kochhar. "Energy and Angular Momentum Transfer in Binary Galaxies." International Astronomical Union Colloquium 124 (1990): 589–93. http://dx.doi.org/10.1017/s0252921100005698.

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AbstractWe have numerically studied tidal effects of a massive perturber on a satellite galaxy. The model consists of a spherical satellite galaxy and a point mass perturber and the encounter is non-penetrating. A wide range of density ratios and eccentricities of the relative orbits have been considered. The disruption of the satellite galaxy has been observed when the numerical value of the fractional change in the energy is greater than two. The changes in the energy and angular momentum show smooth variation in the case of unbound orbits and irregular variation in the bound orbit cases. It is shown that for a constant pericentric distance, increasing the density ratio decreases the tidal effects; and for a given density ratio an increase in the eccentricity decreases the tidal effects.

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21

Muñoz, Francisco, José Rogan, J. A. Valdivia, A. Varas, and Miguel Kiwi. "Binary cluster collision dynamics and minimum energy conformations." Physica B: Condensed Matter 427 (October 2013): 76–84. http://dx.doi.org/10.1016/j.physb.2013.06.036.

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22

Bhuiyan, G. M., and A. Z. Ziauddin Ahmed. "Energy of formation for and liquid binary alloys." Physica B: Condensed Matter 390, no. 1-2 (March 2007): 377–85. http://dx.doi.org/10.1016/j.physb.2006.08.041.

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23

Menon, V. J., R. K. Dubey, M. Mishra, and B. K. Patra. "Momentum-energy change in elastic relativistic binary collisions." American Journal of Physics 77, no. 5 (May 2009): 447–50. http://dx.doi.org/10.1119/1.3073880.

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24

Follador, M., A. T. Conn, and J. Rossiter. "Bistable minimum energy structures (BiMES) for binary robotics." Smart Materials and Structures 24, no. 6 (May 18, 2015): 065037. http://dx.doi.org/10.1088/0964-1726/24/6/065037.

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25

Parhi, K. K. "Low-energy CSMT carry generators and binary adders." IEEE Transactions on Very Large Scale Integration (VLSI) Systems 7, no. 4 (December 1999): 450–62. http://dx.doi.org/10.1109/92.805752.

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26

Cheng, Yi-Chen, C. J. Wu, and R. C. Chiang. "Free energy of surface segregation in binary alloys." Physical Review B 32, no. 6 (September 15, 1985): 4224–27. http://dx.doi.org/10.1103/physrevb.32.4224.

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27

Van Camp, P. E., and V. E. Van Doren. "Total energy calculations in theDFT on binary compounds." International Journal of Quantum Chemistry 55, no. 4 (August 15, 1995): 339–45. http://dx.doi.org/10.1002/qua.560550405.

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28

Morenov, Valentin, Ekaterina Leusheva, Alexander Lavrik, Anna Lavrik, and George Buslaev. "Gas-Fueled Binary Energy System with Low-Boiling Working Fluid for Enhanced Power Generation." Energies 15, no. 7 (March 31, 2022): 2551. http://dx.doi.org/10.3390/en15072551.

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This article discusses methods of enhanced power generation using a binary power system with low-boiling fluid as an intermediate energy carrier. The binary power system consists of micro-gas and steam power units and is intended for remote standalone power supply. Trifluotrichloroethane was considered as the working agent of the binary cycle. The developed system was modeled by two parts in MATLAB Simulink and Aspen HYSYS. The model in Aspen HYSYS calculates the energy and material balance of the binary energy system. The model in MATLAB Simulink investigates the operation of power electronics in the energy system for quality power generation. The results of the simulation show that the efficiency of power generation in the range of 100 kW in the developed system with micro-turbine power units reaches 50%.

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29

Sweatman, W. L. "Full ionization in binary-binary encounters of equal masses with a small positive total energy." Monthly Notices of the Royal Astronomical Society 377, no. 1 (May 1, 2007): 459–64. http://dx.doi.org/10.1111/j.1365-2966.2007.11628.x.

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Jiang, Yi, Hong Zhou, Yuan Yuan Zu, and Xiao Chen. "Energy Based Dual-Microphone Electronic Speech Segregation." Applied Mechanics and Materials 385-386 (August 2013): 1381–84. http://dx.doi.org/10.4028/www.scientific.net/amm.385-386.1381.

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Speech segregation based on energy has a good performance on dual-microphone electronic speech signal processing. The implication of the binary mask to an auditory mixture has been shown to yield substantial improvements in signal-to-noise-ratio (SNR) and intelligibility. To evaluate the performance of a binary mask based dual microphone speech enhancement algorithm, various spatial noise sources and reverberation test conditions are used. Two compare dual microphone systems based on energy difference and machine learning are used at the same time. Result with SNR and speech intelligibility show that more robust performance can be achieved than the two compare systems.

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31

An, Hongjun. "A model for high-energy emission of the Intrabinary shock in pulsar binaries." EPJ Web of Conferences 168 (2018): 04013. http://dx.doi.org/10.1051/epjconf/201816804013.

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We present our studies of intrabinary shock emission for astrophysical binary systems with a neutron star. We construct a model for the shock emission and compare the model calculation with the light curve and the spectral energy distribution of the gamma-ray binary 1FGL J1018.6-5856. The model assumes a slow and a fast population of particles accelerated in the shock, and computes the high-energy emission spectra and orbital light curves produced by synchrotron, self-Compton and external Compton processes of the high-energy particles in the shock. The model allows one to study plasma properties and to constrain the binary geometry, most importantly the inclination angle (i). We discuss potential use of this model for other pulsar binaries to determine the inclination angle of the binary hence the mass of the neutron star.

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32

Hassan, Said Ali, Prachi Agrawal, Talari Ganesh, and Ali Wagdy Mohamed. "A Novel Discrete Binary Gaining-Sharing Knowledge-Based Optimization Algorithm for the Travelling Counselling Problem for Utilization of Solar Energy." International Journal of Swarm Intelligence Research 13, no. 1 (January 2022): 1–24. http://dx.doi.org/10.4018/ijsir.2022010110.

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This article proposes a novel binary version of recently developed Gaining-Sharing knowledge-based optimization algorithm (GSK) to solve binary optimization problems is proposed. GSK algorithm is based on the concept of how humans acquire and share knowledge during their life span. Discrete Binary version of GSK named novel binary Gaining Sharing knowledge-based optimization algorithm (DBGSK) depends on mainly two binary stages: binary junior gaining sharing stage and binary senior gaining sharing stage with knowledge factor 1. These two stages enable DBGSK for exploring and exploitation of the search space efficiently and effectively to solve problems in binary space.An improved scheduling of the technical counselling process for utilization of the electricity from solar energy power stations is introduced. The scheduling aims at achieving the best utilization of the available day time for the counselling group,n this regard,a new application problem is presented, which is called a Travelling Counselling Problem (TCP).A Nonlinear Binary Model is introduced with a real application

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33

Unno, Wasaburo, Masayoshi Kiguchi, and Masatoshi Kitamura. "Mass and Energy Transfer in Semi-Detached Binary Systems." International Astronomical Union Colloquium 108 (1988): 215–16. http://dx.doi.org/10.1017/s0252921100093854.

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Recently, Kitamura and Nakamura have found that the anomalous gravity darkening occurs in semi-detached binary systems. The exponent of gravity darkening for the secondary components, which is defined by where F is the radiative flux and g is the gravitational accerelation, is significantly greater than the unity as shown in Table 1. We interpret this in terms of the energy transport by the mass outflow from the secondary component filling the Roche-lobe.Table 1.Empirical αc-values and physical quantities of five semi-detached binary systems.From the analysis based on this interpretation, we show that 1) the mass out-flow carries energy if ∇ < ∇ad and 2) the anomalous gravity darkening requires that the flow must originate from deep interior. The mass loss rate can be estimated from the anomalous gravity darkening. Thus, the anomalous gravity darkening can be used not only to estimate the mass transfer rate but also to probe the interior structure and the evolution of the secondary star of the semi-detached binary. This model links Morton’s instability[2] of the secondary with the accretion disk of the primary.

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34

Yong, Jianlin, Simin Ren, Shaoqing Zhang, Guoxiong Wu, Caixia Shao, Haoran Zhao, Xiaolin Yu, Mingkui Li, and Yang Gao. "The Behavior of Moist Potential Vorticity in the Interactions of Binary Typhoons Lekima and Krosa (2019) in with Different High-Resolution Simulations." Atmosphere 13, no. 2 (February 8, 2022): 281. http://dx.doi.org/10.3390/atmos13020281.

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The binary typhoon systems of Lekima and Krosa (2019) have been simulated using the Weather Research and Forecast (WRF) model with 27 km, 9 km, and 3 km resolutions and their behaviors of moist potential vorticity (MPV) in these simulations have been analyzed. All the simulations clearly show that the main sources of instability energy include two parts of MPV—the convective energy from the environmental field (MPV1) and the internal transferring energy between the binary typhoons (MPV2). While typhoons absorb the convective energy from the upper ocean through vortex effects on their periphery as the main external MPV sources, there is an MPV conveying belt at the middle-low layer of the atmosphere in the binary typhoon system, transferring energy between binary typhoons and causing atmospheric baroclinicity changes. While all three-resolution simulations show the fundamental features of MPV and its transferring in the binary typhoon system, the 3 km resolution cloud-resolving simulation yield more detailed and accurate MPV structures inside the individual typhoon, which may have non-negligible feedbacks on the background. Based on the comprehensive characteristics of MPV in binary typhoon interactions, further understanding of the interactions of internal detailed structures inside typhoons and their feedbacks on the background may provide a theoretical basis for improving the forecast of typhoon intensity and track.

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35

Dumitrescu, Ovidiu, and Dorel Radu. "Basicity-Gibbs Free Energy Relationships for Binary Alkali Silicates." Advanced Materials Research 39-40 (April 2008): 169–72. http://dx.doi.org/10.4028/www.scientific.net/amr.39-40.169.

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In present paper there are presented such correlations for the silica-alkali systems (M2O – SiO2) where reliable thermodynamic data exists from the thermal equilibrium diagrams. It was observed that with the saturation of SiO2 tetrahedron with metal ions, the difference in basicity between the reactants is diminished, in the order SiO2 → disilicate → metasilicate → orthosilicate, and that confirms the role of driving force for these reactions of the acid-base interaction between oxides and the intermediate silicates formed. Also, there were proposed some correlations between the standard formation Gibbs free energy, (Gº298), and basicity percentage, pB, for the binary compounds from the same oxide systems. Considering the fact that for a system at equilibrium, reaction constant Kp depends on the reaction free Gibbs energy (rG0 298) and temperature, a correlation between basicity difference through basicity percentage, pB, and rG0 298 is proposed.

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Gao, Jiabao, Qingliang Liu, and Jinmei Lai. "An Approach of Binary Neural Network Energy-Efficient Implementation." Electronics 10, no. 15 (July 30, 2021): 1830. http://dx.doi.org/10.3390/electronics10151830.

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Binarized neural networks (BNNs), which have 1-bit weights and activations, are well suited for FPGA accelerators as their dominant computations are bitwise arithmetic, and the reduction in memory requirements means that all the network parameters can be stored in internal memory. However, the energy efficiency of these accelerators is still restricted by the abundant redundancies in BNNs. This hinders their deployment for applications in smart sensors and tiny devices because these scenarios have tight constraints with respect to energy consumption. To overcome this problem, we propose an approach to implement BNN inference while offering excellent energy efficiency for the accelerators by means of pruning the massive redundant operations while maintaining the original accuracy of the networks. Firstly, inspired by the observation that the convolution processes of two related kernels contain many repeated computations, we first build one formula to clarify the reusing relationships between their convolutional outputs and remove the unnecessary operations. Furthermore, by generalizing this reusing relationship to one tile of kernels in one neuron, we adopt an inclusion pruning strategy to further skip the superfluous evaluations of the neurons whose real output values can be determined early. Finally, we evaluate our system on the Zynq 7000 XC7Z100 FPGA platform. Our design can prune 51 percent of the operations without any accuracy loss. Meanwhile, the energy efficiency of our system is as high as 6.55 × 105 Img/kJ, which is 118× better than the best accelerator based on an NVDIA Tesla-V100 GPU and 3.6× higher than the state-of-the-art FPGA implementations for BNNs.

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37

Basile, Giada, Dario Benedetto, Emanuele Caglioti, and Lorenzo Bertini. "Large deviations for a binary collision model: energy evaporation." Mathematics in Engineering 5, no. 1 (2022): 1–12. http://dx.doi.org/10.3934/mine.2023001.

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<abstract>We analyze the large deviations for a discrete energy Kac-like walk. In particular, we exhibit a path, with probability exponentially small in the number of particles, that looses energy.</abstract>

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38

Mahmoud, Ra'ad D., and Chris Done. "Modelling the energy dependence of black hole binary flows." Monthly Notices of the Royal Astronomical Society 473, no. 2 (September 13, 2017): 2084–97. http://dx.doi.org/10.1093/mnras/stx2359.

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39

Ikeda, Shuji, Takeshi Kubota, Dan Ohtan Wang, Hiroyuki Yanagisawa, Mizue Yuki, and Akimitsu Okamoto. "Emission control by binary energy transfer processes on oligouridine." Organic & Biomolecular Chemistry 9, no. 19 (2011): 6598. http://dx.doi.org/10.1039/c1ob05869j.

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40

HIJIKATA, Kunio, Nobuhiro HIMENO, Hiroyuki MIYASAKA, Kazuhito SAITO, and Yasuo MORI. "Latent heat thermal energy storage by using binary mixture." Transactions of the Japan Society of Mechanical Engineers Series B 52, no. 479 (1986): 2640–46. http://dx.doi.org/10.1299/kikaib.52.2640.

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41

Yanagida, T., A. J. Matchett, and J. M. Coulthard. "Energy dissipation of binary powder mixtures subject to vibration." Advanced Powder Technology 12, no. 2 (2001): 227–54. http://dx.doi.org/10.1163/15685520052385041.

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42

Kumar, V., G. M. Prasad, and D. Chandra. "Lattice energy and electronic polarizability of binary tetrahedral semiconductors." Journal of Physics and Chemistry of Solids 58, no. 3 (March 1997): 463–65. http://dx.doi.org/10.1016/s0022-3697(96)00141-2.

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43

Degond, Pierre, and Christian Ringhofer. "Binary quantum collision operators conserving mass momentum and energy." Comptes Rendus Mathematique 336, no. 9 (May 2003): 785–90. http://dx.doi.org/10.1016/s1631-073x(03)00185-7.

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44

Spyrou, N. K., and N. Stergioulas. "Evolutionary self-energy-loss effects in compact binary systems." Astronomy & Astrophysics 366, no. 2 (February 2001): 598–604. http://dx.doi.org/10.1051/0004-6361:20000230.

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Kartavtsev, O. I., and A. V. Malykh. "Low-energy three-body dynamics in binary quantum gases." Journal of Physics B: Atomic, Molecular and Optical Physics 40, no. 7 (March 15, 2007): 1429–41. http://dx.doi.org/10.1088/0953-4075/40/7/011.

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Kotti, Margarita, and Konstantinos I. Diamantaras. "Efficient binary classification through energy minimisation of slack variables." Neurocomputing 148 (January 2015): 498–511. http://dx.doi.org/10.1016/j.neucom.2014.07.013.

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47

Huyskens, P. L., M. C. Haulait-Pirson, G. G. Siegel, and F. Kapuku. "Gibbs energy of some binary systems containing hydrogen bonds." Journal of Physical Chemistry 92, no. 23 (November 1988): 6841–47. http://dx.doi.org/10.1021/j100334a067.

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48

Auriemma, G., H. Bilokon, and A. F. Grillo. "High-energy neutrino emission from binary X-ray sources." Il Nuovo Cimento C 9, no. 2 (March 1986): 451–58. http://dx.doi.org/10.1007/bf02514863.

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49

Mengjie, Song, Wan Man Pun, Dubey Swapnil, Pan Dongmei, and Mao Ning. "Thermal stability of organic binary PCMs for energy storage." Energy Procedia 142 (December 2017): 3287–94. http://dx.doi.org/10.1016/j.egypro.2017.12.459.

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50

Matsubara, M., N. Watanabe, and H. Kurimoto. "Binary periodic distillation scheme with enhanced energy conservation—I." Chemical Engineering Science 40, no. 5 (1985): 715–21. http://dx.doi.org/10.1016/0009-2509(85)85024-7.

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Journal articles on the topic 'Binary energy'

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