Relevant bibliographies by topics / Binary energy

Academic literature on the topic 'Binary energy'

Author: Grafiati
Published: 10 December 2022
Last updated: 28 January 2023

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Journal articles on the topic "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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<p>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.</p> <p>&nbsp;</p>
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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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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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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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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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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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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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Dissertations / Theses on the topic "Binary energy"

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Dickinson, Hugh John. "Very high energy gamma-rays from binary systems." Thesis, Durham University, 2010. http://etheses.dur.ac.uk/290/.

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This thesis presents a study of the very high energy (VHE) gamma-ray emission from X-ray binary systems using the H.E.S.S. imaging atmospheric Cherenkov array. The historical background and basic principles of ground-based gamma-ray astronomy are briefly reviewed and an overview of the design and capabilities of the H.E.S.S. telescope system is presented. The broadband observational properties of X-ray binary systems and their relevance in a broader astrophysical context is also discussed. A review of the radiative emission mechanisms which relate to VHE gamma-ray emission in X-ray binaries is presented, with emphasis given to the leptonic emission processes of synchrotron radiation and inverse-Compton scattering. Intrinsic absorption processes which act to attenuate the emitted flux of VHE gamma-rays are also discussed. Three computer models are introduced which simulate aspects of the gamma-ray emission and absorption in X-ray binary systems. A detailed analysis of the VHE gamma-ray emission from the X-ray binary LS 5039 is presented and the relevant procedures for data selection, gamma-hadron separation and background estimation are discussed in some detail. Methods for the determination of detection significance and the calculation of gamma-ray fluxes are also reviewed and results are derived which apply specifically to LS 5039. A detailed temporal analysis of the gamma-ray signal from LS 5039 is presented, applying tests for secular, excess and periodic variability. Strong evidence is found for modulation of the observed gamma-ray flux on the orbital period of ~3.9 days. Following a brief discussion of the procedures required for spectral analysis of VHE gamma-ray data, results are presented for LS 5039 which reveal evidence for spectral variability which is correlated with the observed gamma-ray flux and therefore, the orbital phase of the binary system. The spectral and temporal characteristics of LS 5039 are then compared with the predictions of theoretical models in an attempt to explain the observed behaviour. Contemporaneous X-ray and VHE gamma-ray observations of three galactic microquasars using the Rossi X-ray Timing Explorer and H.E.S.S. are presented. Although no gamma-ray detections are reported, the observations permit the derivation of upper limits to the VHE gamma-ray flux which correspond to episodes of known X-ray behaviour. The X-ray characteristics of each target are compared with pre-existing observational data to infer the presence or otherwise of relativistic outflows at the H.E.S.S. observation epochs. The implications of the gamma-ray non-detections are then discussed in the context of these inferred system properties. The results of a survey of the VHE gamma-ray emission associated with the positions of 125 known X-ray binaries are presented. Although no conclusive detections were obtained, tentative indications were found for a population of faint, spectrally hard gamma-ray sources associated with high-mass X-ray binary systems. The inferred characteristics of the indicated population show broad agreement with the measured properties of known gamma-ray-emitting X-ray binary systems like LS 5039.
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Chu, Chiang-Kai. "Energy Redistribution with Controllable Binary State Latch Element." Thesis, Virginia Tech, 2017. http://hdl.handle.net/10919/78336.

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An application of binary state latch device with proper real-time control algorithm for energy redistribution application is introduced in this thesis. Unlike traditional tuned vibration absorber, the latch device can be viewed as variable semi-active dampers such as magnetorheological (MR) and piezoelectric friction dampers. The distinct difference between other semi-active dampers and our latch device is that other semi-active dampers can provide continuous resistance according to the amount of input current, however, the binary latch device can only provide two different values of resistance - either the maximum or no resistance at all. This property brings the latch possibly having higher maximum and minimum ratio of resistance than MR dampers. As for the operating structure, the mechanism of latch element is nearly the same as the piezoelectric friction dampers which the resistance force is provided according to the normal force acting on two rough plates. Nonetheless, because of the characteristic of the binary states output of the latch element, this make it very different from the ordinary variable dampers. Since it is either being turned on or turned off, a novel control law is required for shifting energy. Also, because of the simplicity of the binary states output, it is very accessible to implement the controller on Field Programmable Gate Array (FPGA). With this accessibility, it is promising to apply plenty of latch elements in the same time for large scale application, such as multi-agent networks. In this thesis, an energy-based analytic solution is proposed to illustrate the universal latch-off condition. And a latch-on condition under ideal situations is discussed. At the end, a control law under nonideal condition is being suggested for real-time periodically excited system. We found that energy redistribution is achievable by using the proper control law under fairly broad conditions.
Master of Science
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Vancea, Anisoara. "Energy and electron transfer on titania-silica binary oxides." Thesis, Loughborough University, 2013. https://dspace.lboro.ac.uk/2134/12152.

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Steady state reflectance and emission characteristics of anthracene adsorbed on silica gel and titania-silica mixed oxides have been investigated as a function of sample loading. Titania-silica mixed oxides with 1, 3, 5 and 10 wt. % TiO2 were prepared by two different methods: a dropwise method and a sol-gel route. Ground state diffuse reflectance and fluorescence emission spectra of anthracene adsorbed on titania-silica surfaces show a dependence on titania content. The absorption peaks of anthracene are difficult to resolve at higher titania content due to the increasing red-shift of the titania absorption edge. The absorption edge of titania is shifted to longer wavelengths and the band gap energy decreases with increasing the titania loading. Diffuse reflectance laser flash photolysis at 355 nm produces both the triplet and radical cation of anthracene and gives relevant information regarding the photochemical transients and the kinetics details of the surface photochemical processes. Energy dependence studies confirm the monophotonic nature of the triplet production, whereas the anthracene radical cation is formed by monophoton or multiphoton ionisation in the mixed titania-silica systems. Energy and electron transfer reactions of anthracene co-adsorbed with azulene as electron donor on silica sol-gel and titania-silica mixed oxides prepared by the sol-gel method with different titania content have been studied using the time-resolved diffuse reflectance laser flash photolysis technique. The fluorescence of excited anthracene adsorbed on silica sol-gel is quenched by the addition of azulene, while co-adsorption of azulene on titania-silica mixed oxides resulted in a decrease in the fluorescence intensity of the adsorbed anthracene due to the formation, at the same time, of anthracene radical cation and Ti3+ species on the titania-silica surface. Triplet-triplet energy transfer from the excited anthracene to ground state azulene and electron transfer from azulene to the anthracene radical cation have been investigated using a time-resolved diffuse reflectance laser flash photolysis technique following laser excitation at 355 nm. Bimolecular rate constants for energy and electron transfer between anthracene and azulene have been obtained. Kinetic analysis of the decay of the anthracene triplet state and radical cation show that the kinetic parameters depend on the titania content of the sample and the azulene concentration. This indicates that the rate of energy and electron transfer reactions increases as a function of azulene concentration and decreases with increasing titania content in titania-silica mixed oxides, whereas the observed rate of reaction on silica sol-gel is predominantly governed by the rate of diffusion of azulene. Electron transfer reactions in a ternary system using azulene for hole transfer between 9-anthracenecarboxylic acid radical cation as electron acceptor and perylene as electron donor were also studied in order to demonstrate the mobility of radical cations on the silica sol-gel and titania-silica surfaces. The co-adsorption of azulene as a molecule shuttle with 9-anthracenecarboxylic acid and perylene on both silica sol-gel and titania-silica systems has been shown to enhance the rate of electron transfer in this ternary system. Activation energies for energy and electron transfer on photoinduced bimolecular and termolecular processes on silica sol-gel and titania-silica mixed oxides have been measured. In bimolecular anthracene / azulene systems, at higher azulene loadings, the activation energies and the pre-exponential factors on titania-silica surfaces are the same for both energy and electron transfer and are comparable with the parameters extracted for azulene diffusion on silica Davisil suggesting that azulene diffuses across the silica Davisil and titania-silica mixed oxides surfaces, while at lower azulene loadings, ion-electron recombination dominates and the activation energy extracted is for this process. In a ternary 9-anthracenecarboxylic acid / azulene / perylene system, the activation energy for perylene diffusion is higher than that observed for the anthracene / azulene system, reflecting the lower mobility of the perylene molecule. In this study, a series of titania-silica samples with different loadings of titania (1 10 wt. %) prepared by the sol-gel method and also the pure TiO2 P25 Degussa have been used to study the photocatalytic degradation of 4-chlorophenol in aqueous solution under UV light irradiation. The absorption peak of 4-chlorophenol at 280 nm decreases with increasing titania content and finally disappeared suggesting that titania has a positive influence on the degradation of 4-chlorophenol. The investigated titania-silica mixed oxides prepared by the sol-gel method are less efficient photocatalysts for the degradation of 4-chlorophenol than TiO2 P25.
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Sinjab, Issam Musleh. "Energy transfer in W Ursae Majoris type contact binary stars." Thesis, University of Sussex, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.543317.

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This thesis investigates two problems concerned with contact binary stars: the mechanism of energy transfer and the evolutionary states in the W UMa-type contact binary systems. The observational and theoretical background is first reviewed. This highlights the importance of a proper treatment of energy transfer if W UMa stars are to be understood. Expressions for the ratio of the transferred luminosity to the primary's radiated and centrally generated luminosities are derived. An estimate of the size of the transfer rate in observed unevolved systems is determined. The implications of accurate mass-ratios are briefly discussed. The generalized transport equation is shown to contradict the requirements of the TRO theory. A more general formula is put forward. The sideways convection model is investigated critically and is found to work only in very deep A-type systems. The implications of this result on contact binaries' structure, stability and evolution are discussed. A variety of different energy transfer models are explored. Equilibrium circulation and turbulent conduction models require moderately deep A-type systems. The small- and large-scale models can, respectively, transfer enough energy in the shallow and moderately shallow W-type systems. Webbink's ideas of energy transfer are used to construct numerical contact binary models which for the first time use an explicit mechanism to represent the energy transfer process. The added complications caused by the implementation of such a mechanism rendered the procedure used to build numerical models ineffective. An alternative procedure is briefly discussed. Hazlehurst's dissipation mechanism is simulated numerically. We argue on the basis of our results that this mechanism is unworkable in its present form. We attribute this to a fundamental error in the formulation of the model and sketch a possible reformulation of the model in terms of the theory of thermals. The consequences of strict hydrostatic equilibrium for the overall structure of contact binaries are discussed. It is shown that imposition of strict hydrostatic equilibrium in the envelope requires (1) the observed anomalous M-L relation hold and (2) the contact phenomenon be considered as a single (severely distorted) configuration. A model is proposed which deviates markedly from hydrostatic equilibrium just below the envelope, with accelerating flow through the L, -point and a shock in the secondary component. A substantial amount of energy can be transferred, with conditions in the envelope remaining very close to hydrostatic equilibrium. The model works independently of the overlying envelope structure. We approach the second of our topics by investigating the evolutionary states in 9 A-type systems. Depending on their observed properties the systems are divided into two distinct groups. Group I members are evolved. Group II members belong to a distinct, still problematic category. The W-type system TX Cnc in Praesepe may be a pre-main sequence contact binary system. The implications of these results on the transfer mechanism are discussed.
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Mykhailenko, T. P., and A. H. Omar. "Energy efficienсy of binary cycle power plant for the refinery." Thesis, Видавництво СумДУ, 2012. http://essuir.sumdu.edu.ua/handle/123456789/25763.

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Molina, Lumbreras Edgar. "Modeling and observations of relativistic outflows in high-energy binary systems." Doctoral thesis, Universitat de Barcelona, 2021. http://hdl.handle.net/10803/672686.

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Some binary systems consisting of a compact object, which can be either a neutron star or a black hole, and typically a non-degenerate companion star, have been shown to emit broadband radiation from radio up to gamma-ray frequencies. These systems are normally classified as X-ray or gamma-ray binaries, depending on the frequency at which their emission has its maximum. Unlike with stars, a big part of the observed emission cannot be explained by thermal radiation, and therefore non-thermal radiative processes need to be invoked. The interactions between the star and the compact object may result in the launching of outflows of plasma originating around the compact object position. These outflows can attain speeds close to the speed of light, and be an efficient site for acceleration of charged particles up to relativistic energies. A part of the non-thermal emission observed from X-ray and gamma-ray binaries comes precisely from the non-thermal radiative cooling of these accelerated particles. Additionally, when the companion star is very massive, it produces a strong stellar wind that interacts with the aforementioned relativistic outflows, modifying both their dynamical and radiative evolution. The main theoretical objective of this thesis is the study the interactions between the outflows of X-ray and gamma- ray binary systems and the stellar wind of a massive companion star. For this purpose, we developed versatile semi- analytical models that give a complete view of these interactions for different kinds of systems. The results of the theoretical modeling include broadband spectral energy distributions and light curves that are directly comparable with the observational data. Radio sky maps are also obtained for the large-scale emission of the outflows. The latter allows to directly visualize the dynamical effect of the stellar wind in the outflow trajectory, which acquires a helical or spiral-like pattern. This modified trajectory gives rise to asymmetries in the light curves at different energy ranges, as well as changes in the spectral energy distributions mostly due to variations of angle-dependent processes influencing the outflow emission. From the observational point of view, this thesis focuses on the analysis of the potential very high-energy gamma-ray emission above 100 GeV of the X-ray binary MAXI J1820+070, as seen by the MAGIC telescopes. The analysis is done through a custom software developed by MAGIC, which allows to reconstruct the arrival direction and energy of a gamma ray from the Cherenkov light emitted by the electromagnetic cascade that the gamma ray generates when it enters the atmosphere of the Earth. The observational results consist on a multiwavelength study of MAXI J1820+070 in the form of light curves and spectral energy distributions that use data from a number of telescopes at radio, optical, X-ray and gamma-ray frequencies. The source is not detected in gamma-rays above 100 MeV, and only flux upper limits can be given for those energies. Nevertheless, the obtained upper limits, together with the observed fluxes at other frequencies, are enough to constrain significantly the properties of a potential gamma-ray emitter in MAXI J1820+070. In conclusion, this thesis deepens in our understanding of the interactions between the stellar wind and the outflows of high-energy binary systems. It shows that these interactions must be taken into account in order to properly characterize the subset of those binary systems hosting a massive companion star, in which a powerful stellar wind is present. In this thesis, it is also shown that observations in high-energy and very high-energy gamma rays of X-ray and gamma-ray binary systems allow to set meaningful limits to the outflow properties, even when the sources are not detected and only upper limits in the flux are obtained.
A la nostra Galàxia, existeixen sistemes binaris formats per un objecte compacte i una estrella companya típicament no degenerada que emeten a freqüències des de ràdio fins a raigs gamma. Les interaccions entre l'estrella i l'objecte compacte poden resultar en el llançament d'outflows de plasma originats al voltant de l'objecte compacte, els quals poden adquirir velocitats properes a la de la llum. Quan l'estrella companya és molt massiva, aquesta genera un fort vent estel·lar que interacciona amb els outflows i els afecta tant dinàmicament com radiativa. El principal objectiu d'aquesta tesi des del punt de vista teòric és l'estudi de les interaccions entre els outflows de sistemes binaris i el vent estel·lar d'una companya massiva. Per això, hem desenvolupat una sèrie de models semi- analítics que donen una visió completa d'aquestes interaccions en diferents tipus d'escenaris. Els resultats de la modelització teòrica inclouen prediccions per a les distribucions espectrals d'energia i corbes de llum, així com mapes ràdio per a l'emissió a gran escala dels outflows. En relació a la part observacional, aquesta tesi es focalitza en l'anàlisi de l'emissió potencial de raigs gamma de molt alta energia de la binària MAXI J1820+070, observada amb els telescopis MAGIC. Els resultats observacionals consisteixen en un estudi multifreqüència de la font de ràdia a raigs gamma. Tot i que la font no es detecta per sobre dels 100 MeV, els resultats obtinguts permeten limitar les propietats d'un emissor potencial de raigs gamma a MAXI J1820+070. En conclusió, aquesta tesi profunditza en el coneixement de les interaccions entre el vent estel·lar i els outflows de sistemes binaris d'altes energies. També es conclou que les observacions en raigs gamma de sistemes binaris permeten limitar de manera important les propietats dels outflows, fins i tot quan les fonts no son detectades.
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Snyder, Kenneth A. "Energy localization and transport in binary isotopically disordered Fermi-Pasta-Ulam chains." College Park, Md. : University of Maryland, 2005. http://hdl.handle.net/1903/2643.

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Thesis (Ph. D.) -- University of Maryland, College Park, 2005.
Thesis research directed by: Physics. Title from t.p. of PDF. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.
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Schlenker, Stefan. "Very high energy gamma rays from the binary pulsar PSR B1259-63." Doctoral thesis, [S.l. : s.n.], 2005. http://deposit.ddb.de/cgi-bin/dokserv?idn=976502267.

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Edwards, Philip Gregory. "A search for ultra high energy gamma ray emission from binary X-ray systems." Title page, contents and summary only, 1988. http://web4.library.adelaide.edu.au/theses/09PH/09phe266.pdf.

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Chan, Ryan James. "Mean-Field Parameter Study of Radiation-Induced Segregation in a Binary Metal Alloy." Thesis, Virginia Tech, 2020. http://hdl.handle.net/10919/96606.

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The purpose of this thesis is to broaden the tools and knowledge available for understanding the behavior of metals under irradiation to aid in the pursuit of advanced materials for deployment in Generation IV (Gen-IV) nuclear reactor designs. A mean-field study is conducted on a body-centered cubic (BCC) A-B binary metal alloy system. The performance of the simulated metal system is measured by assessing the degree of segregation that occurs at the grain boundary (GB) in the center of the one-dimensional simulation box. This mean-field method was developed using rate theory equations to observe the diffusion of defects and solute atoms in the binary BCC alloy modeled after a section of planes in the <100> direction of α-iron. The method in this thesis is adapted from a previous radiation-induced segregation (RIS) study that was similarly validated against thermal segregation isotherms. This adapted simulation code was used to study RIS by varying the initial values and conditions across ranges relevant to Generation IV reactor designs. The simulations run with this code were centered around segregation energy and the diffusion coefficient relationships between defects and solute atoms. The most influential conditions applied to both the segregation energy and diffusion coefficient relationship test suites were the temperature and dose rate. The interplay of the various segregation energies, manipulated diffusion coefficients, temperatures, and dose rates is explored in this thesis. The code used in this thesis is presented as a modular framework for further parameter study with a clear direction for more complex alloys.
Master of Science
The growing electricity demand for more efficient, safe, reliable, and sustainable means of power generation requires research and subsequent implementation of advanced Generation IV (Gen-IV) nuclear reactor designs. These proposed designs operate under significantly more strenuous conditions from the perspective of materials used in constructing the reactor. Materials inside the reactor will experience temperatures, pressures, and radiation doses greatly exceeding those of previous generations: Gen II through III+. Metals are employed in almost every component inside a reactor and are particularly susceptible to the demanding conditions due to their tendency to lose their ductility under these stressors. This thesis presents a diffusion-based code that models a binary metal alloy under conditions similar to those expected in Gen-IV reactors. The results of the code give insight into the prevalence of a phenomenon known as radiation induced segregation (RIS) in metals under these Gen-IV relevant conditions. The values input into the code have significant effects on the resulting RIS behavior of the metal alloy. This thesis presents correlations between the initial parameters and the amount of segregation this alloy experiences. The results of this thesis allow a sort of mapping of material parameters and operating conditions so that materials can be designed for optimal performance over the lifespan of the next generation of nuclear reactors. The code in this thesis was developed with the expectation that its modularity would be expanded upon to apply to more complex alloys under a broader range of initial conditions.
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Books on the topic "Binary energy"

1

Law, Vincent Hin-Wei. Quasi-static energy recovery binary decision diagram logic (QSBDDL). Ottawa: National Library of Canada, 2003.

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Static Dielectric Constants of Pure Liquids and Binary Liquid Mixtures: Supplement to Volume IV/17. Springer, 2015.

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N, Zhang S., and United States. National Aeronautics and Space Administration., eds. Broadband high-energy observations of the superluminal jet source gro J1655--40 during an outburst. [Washington, DC: National Aeronautics and Space Administration, 1997.

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1936-, Ferrante John, and Lewis Research Center, eds. Equivalent crystal theory of alloys. Washington, D.C: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1991.

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Rodrigo, Ibanez-Meier, Ferrante John 1936-, and United States. National Aeronautics and Space Administration., eds. Growth of Au on Ni(110): A semiempirical modeling of surface alloy phases. [Washington, DC]: National Aeronautics and Space Administration, 1995.

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Rodrigo, Ibanez-Meier, Ferrante John 1936-, and United States. National Aeronautics and Space Administration., eds. Growth of Au on Ni(110): A BFS modelling of surface alloy phases. [Washington, DC]: National Aeronautics and Space Administration, 1994.

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1936-, Ferrante John, Rodr £iguez, Agust £in M., and United States. National Aeronautics and Space Administration., eds. Modelling of surfaces. [Washington, DC]: National Aeronautics and Space Administration, 1994.

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1936-, Ferrante John, Rodrʹiguez Agustʹin M, and United States. National Aeronautics and Space Administration., eds. Modelling of surfaces. [Washington, DC]: National Aeronautics and Space Administration, 1994.

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1936-, Ferrante John, Kobistek Robert J, and United States. National Aeronautics and Space Administration., eds. Modelling of surfaces. [Washington, DC: National Aeronautics and Space Administration, 1994.

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1936-, Ferrante John, Kobistek Robert J, and United States. National Aeronautics and Space Administration., eds. Modelling of surfaces. [Washington, DC: National Aeronautics and Space Administration, 1994.

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Book chapters on the topic "Binary energy"

1

Huggins, Robert A. "Binary Electrodes Under Equilibrium or Near-Equilibrium Conditions." In Energy Storage, 161–79. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-21239-5_11.

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Huggins, Robert A. "Binary Electrodes Under Equilibrium or Near-Equilibrium Conditions." In Energy Storage, 161–79. Boston, MA: Springer US, 2010. http://dx.doi.org/10.1007/978-1-4419-1024-0_11.

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Tavani, M. "High-Energy Emission from Binary Pulsars." In The Many Faces of Neutron Stars, 245–57. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-015-9139-3_16.

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Levintov, I. I. "3 P 0 Model of Soft Binary Processes." In High Energy Spin Physics, 566–69. Berlin, Heidelberg: Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-86995-2_72.

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Radhakrishnan, V., and C. S. Shukre. "The Binary Origin of Pulsar Velocities." In High Energy Phenomena Around Collapsed Stars, 271–78. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3823-6_14.

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Schirmer, Pascal A., and Iosif Mporas. "Binary versus Multiclass Deep Learning Modelling in Energy Disaggregation." In Springer Proceedings in Energy, 45–51. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-63916-7_6.

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AbstractThis paper compares two different deep-learning architectures for the use in energy disaggregation and Non-Intrusive Load Monitoring. Non-Intrusive Load Monitoring breaks down the aggregated energy consumption into individual appliance consumptions, thus detecting device operation. In detail, the “One versus All” approach, where one deep neural network per appliance is trained, and the “Multi-Output” approach, where the number of output nodes is equal to the number of appliances, are compared to each other. Evaluation is done on a state-of-the-art baseline system using standard performance measures and a set of publicly available datasets out of the REDD database.
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Trobin, Werner, Thomas Pock, Daniel Cremers, and Horst Bischof. "Continuous Energy Minimization Via Repeated Binary Fusion." In Lecture Notes in Computer Science, 677–90. Berlin, Heidelberg: Springer Berlin Heidelberg, 2008. http://dx.doi.org/10.1007/978-3-540-88693-8_50.

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Matsumoto, Masako, Yu Fujimoto, and Yasuhiro Hayashi. "Energy Disaggregation Based on Semi-Binary NMF." In Machine Learning and Data Mining in Pattern Recognition, 401–14. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-41920-6_31.

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Troncoso, Jacobo. "Chapter 19. Excess Enthalpies for Binary Systems Containing Ionic Liquids." In Enthalpy and Internal Energy, 505–20. Cambridge: Royal Society of Chemistry, 2017. http://dx.doi.org/10.1039/9781788010214-00505.

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Mishra, Krishna Kant, Mukesh Kumar, Ravikant Ravi, Amol Saini, Kunal Salwan, and Mahendra Pal Sharma. "Improving Cold Flow Properties of Biodiesels Using Binary Biodiesel Blends." In Springer Proceedings in Energy, 951–61. Singapore: Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-16-0235-1_73.

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Conference papers on the topic "Binary energy"

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Al-Harere, Manal Naji, and Ahmed Abed Ali Omran. "Binary operation graphs." In CURRENT TRENDS IN RENEWABLE AND ALTERNATE ENERGY. Author(s), 2019. http://dx.doi.org/10.1063/1.5095093.

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Tutuncuoglu, Kaya, Omur Ozel, Aylin Yener, and Sennur Ulukus. "Binary energy harvesting channel with finite energy storage." In 2013 IEEE International Symposium on Information Theory (ISIT). IEEE, 2013. http://dx.doi.org/10.1109/isit.2013.6620495.

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Corradi, L., A. M. Stefanini, E. Fioretto, A. Gadea, N. Marginean, G. De Angelis, D. R. Napoli, et al. "Aspects of Low Energy Binary Reactions." In INTERNATIONAL SYMPOSIUM ON EXOTIC NUCLEI. AIP, 2007. http://dx.doi.org/10.1063/1.2746576.

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Pakhomov, Andrew V., Kevin E. Mahaffy, and Andrew V. Pakhomov. "Binary Solid Propellants for Constant Momentum Missions." In BEAMED ENERGY PROPULSION: Fifth International Symposium on Beamed Energy Propulsion. AIP, 2008. http://dx.doi.org/10.1063/1.2931897.

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Raubenheimer, B. C., A. R. North, O. C. de Jager, P. J. Meintjes, C. Brink, H. I. Nel, G. van Urk, B. Visser, and D. O’Donoghue. "TeV gamma-rays from accreting binary systems." In High Energy Gamma−Ray Astronomy. AIP, 1991. http://dx.doi.org/10.1063/1.40325.

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Dabirnia, Mehdi, and Tolga M. Duman. "Code design for binary energy harvesting channel." In 2017 IEEE International Symposium on Information Theory (ISIT). IEEE, 2017. http://dx.doi.org/10.1109/isit.2017.8006704.

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Grad, Johannes, and James E. Stine. "A Multi-Mode Low-Energy Binary Adder." In 2006 Fortieth Asilomar Conference on Signals, Systems and Computers. IEEE, 2006. http://dx.doi.org/10.1109/acssc.2006.355130.

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Paredes, Josep M., Felix A. Aharonian, Werner Hofmann, and Frank Rieger. "Gamma rays from compact binary systems." In HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP, 2008. http://dx.doi.org/10.1063/1.3076631.

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Fox, Allen, J. F. Louis, W. J. Greenlee, and G. H. Parker. "Binary Mercury/Organic Rankine Cycle Power Systems." In 22nd Intersociety Energy Conversion Engineering Conference. Reston, Virginia: American Institute of Aeronautics and Astronautics, 1987. http://dx.doi.org/10.2514/6.1987-9162.

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Nyadzani, Lutendo, and S. Razzaque. "Polarization of Gravitational Waves from Binary Systems." In High Energy Astrophysics in Southern Africa. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.338.0029.

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Reports on the topic "Binary energy"

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Ratmanski, Kiril, and Sergey Vecherin. Resilience in distributed sensor networks. Engineer Research and Development Center (U.S.), October 2022. http://dx.doi.org/10.21079/11681/45680.

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With the advent of cheap and available sensors, there is a need for intelligent sensor selection and placement for various purposes. While previous research was focused on the most efficient sensor networks, we present a new mathematical framework for efficient and resilient sensor network installation. Specifically, in this work we formulate and solve a sensor selection and placement problem when network resilience is also a factor in the optimization problem. Our approach is based on the binary linear programming problem. The generic formulation is probabilistic and applicable to any sensor types, line-of-site and non-line-of-site, and any sensor modality. It also incorporates several realistic constraints including finite sensor supply, cost, energy consumption, as well as specified redundancy in coverage areas that require resilience. While the exact solution is computationally prohibitive, we present a fast algorithm that produces a near-optimal solution that can be used in practice. We show how such formulation works on 2D examples, applied to infrared (IR) sensor networks designed to detect and track human presence and movements in a specified coverage area. Analysis of coverage and comparison of sensor placement with and without resilience considerations is also performed.
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