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標(biāo)題: Titlebook: Quantum Communication Networks; Riccardo Bassoli,Holger Boche,Sajad Saeedinaeeni Book 2021 The Editor(s) (if applicable) and The Author(s) [打印本頁]

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書目名稱Quantum Communication Networks影響因子(影響力)




書目名稱Quantum Communication Networks影響因子(影響力)學(xué)科排名




書目名稱Quantum Communication Networks網(wǎng)絡(luò)公開度




書目名稱Quantum Communication Networks網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Quantum Communication Networks被引頻次




書目名稱Quantum Communication Networks被引頻次學(xué)科排名




書目名稱Quantum Communication Networks年度引用




書目名稱Quantum Communication Networks年度引用學(xué)科排名




書目名稱Quantum Communication Networks讀者反饋




書目名稱Quantum Communication Networks讀者反饋學(xué)科排名





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Riccardo Bassoli,Holger Boche,Christian Deppe,Roberto Ferrara,Frank H. P. Fitzek,Gisbert Janssen,Sajf such simulations represent a good match to the observations. This issue is not entirely straightforward given the complex morphology and hierarchical nature of observed molecular clouds (and also of numerical simulations). For example, the fact that simulations generally produce filamentary and hi
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Riccardo Bassoli,Holger Boche,Christian Deppe,Roberto Ferrara,Frank H. P. Fitzek,Gisbert Janssen,Sajch simulations are informed by observations of the gas in Giant Molecular Clouds (GMCs). We therefore present a brief overview of the properties of GMCs and how these are deduced observationally, focussing in particular on the three inter-related ‘Larson’ relations. We emphasise the dynamical import
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(such as an open or globular cluster), or disperses to join the field stars in the disc of the Galaxy? These questions not only impact understanding of the origins of stars and planetary systems like our own (and the potential for life to emerge that they represent), but also galaxy formation and ev
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Quantum Computing and Programming,are preferably solved with a quantum computer. The goal of this chapter is to provide an understanding of these key quantum ideas that are standard must-do topics in quantum computation and which might find their applications in quantum networks.
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Introduction,ing quantum-mechanical characteristics of nature, future communication networks can achieve unexpected performances in an efficient way. The clarification of such context and the reasons behind the deployment of quantum mechanics in telecommunications are the central theme of this introductory chapter.
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Quantum Information Theory, Regarding the choice of topics treated as well as the methodological approach pursued, one can draw analogies with the material covered in standard classical information theory modules, which are intended for master’s as well as bachelor’s students of electrical engineering and communication scienc
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Quantum Error Correction,of data, because in these conditions noise has had a chance to accumulate over space or time. Otherwise, there is no active error correction in computation because the signal levels are extremely high compared to the noise. Amplification cannot be used to achieve stable qubits because it cannot be d
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Fundamental Background, systems, composite systems, density matrices, entanglement, and quantum measurement models, the discussion next moves to quantum channels, statistical theory and quantum entropy. Finally, we explain the concept of quantum nonlocality and its connection to cooperative games in quantum game theory.
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Riccardo Bassoli,Holger Boche,Christian Deppe,Roberto Ferrara,Frank H. P. Fitzek,Gisbert Janssen,Saj
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Riccardo Bassoli,Holger Boche,Christian Deppe,Roberto Ferrara,Frank H. P. Fitzek,Gisbert Janssen,Sajstribution of gas and stars, the stellar initial mass function (IMF), and clustering and stellar mass segregation. We follow this by applying some of these methods to the simplest class of star cluster formation simulations (termed ‘vanilla’ calculations in these chapters) which contain only the thr
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Riccardo Bassoli,Holger Boche,Christian Deppe,Roberto Ferrara,Frank H. P. Fitzek,Gisbert Janssen,Sajent on a timescale of a few Myr, and therefore cannot be strictly treated as isolated systems. We also review the observational evidence that GMCs are gravitationally bound and conclude that a significant fraction may be (mildly) gravitationally unbound. The implications of these for the star format
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