標題: Titlebook: Astroparticle Physics: Theory and Phenomenology; Günter Sigl Book 2017 Atlantis Press and the author(s) 2017 High Energy Astroparticle Phy [打印本頁] 作者: fitful 時間: 2025-3-21 16:58
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書目名稱Astroparticle Physics: Theory and Phenomenology讀者反饋學科排名
作者: 玩笑 時間: 2025-3-21 20:51 作者: 輕率的你 時間: 2025-3-22 01:23
Atlantis Studies in Astroparticle Physics and Cosmologyhttp://image.papertrans.cn/b/image/163667.jpg作者: BOAST 時間: 2025-3-22 06:53 作者: floaters 時間: 2025-3-22 10:55
2.3.7 Drilling, completion and production,energy astrophysics. More comprehensive reviews on electromagnetic processes can be found in standard textbooks, e.g. Refs.?[230, 528], and also in Ref.?[529]. In the second part we will apply this to the main scenarios and models of .ray sources, separated into Galactic and extragalactic sources.作者: QUAIL 時間: 2025-3-22 14:17
https://doi.org/10.2991/978-94-6239-243-4High Energy Astroparticle Physics; Early Universe Cosmology; Cosmic Rays, Gamma-rays and Neutrinos; Gra作者: collagenase 時間: 2025-3-22 20:57 作者: 搖曳的微光 時間: 2025-3-22 23:56
2.2 Oil exploitation technologies,lopment. Special emphasize will be put on neutrino physics since it plays an important role in high energy astroparticle physics as will be developed in detail in part IV. At this occasion we will also develop and summarize some general concepts in particle physics such as quantum fields and represe作者: 北極熊 時間: 2025-3-23 04:02
2.3.7 Drilling, completion and production,f these interactions in a broader and more formal context together with the other known fundamental interactions. We start with general aspects of divergences in the effective description of the electroweak interactions and their relation to renormalization in quantum field theory. We then turn to t作者: JOT 時間: 2025-3-23 07:43 作者: AWL 時間: 2025-3-23 12:28 作者: Reclaim 時間: 2025-3-23 15:26
2.4 CO2 removal and deposition,ncludes the development of the most relevant aspects of air shower physics. The second part then summarizes the current experimental situation and the main open questions, roughly separated for cosmic radiation of Galactic and extragalactic origin. The following chapters will then provide the theore作者: 心胸開闊 時間: 2025-3-23 21:41
2.3.7 Drilling, completion and production,ies observed in the cosmic radiation arriving at Earth, and possibly beyond. We start with an overview of the main acceleration mechanisms and then discuss the maximal energy that can be reached by these processes. In the last section we then apply this to Galactic and extragalactic source models. T作者: Folklore 時間: 2025-3-23 23:39 作者: AGGER 時間: 2025-3-24 04:33 作者: thyroid-hormone 時間: 2025-3-24 09:00
2.4 CO2 removal and deposition, such as the production of neutral pions and their subsequent decays into .-rays, high energy extraterrestrial neutrinos are unique messengers of hadronic acceleration processes because they can only be produced by the decay of charged pions or heavier mesons which can not be produced electromagneti作者: anticipate 時間: 2025-3-24 12:44 作者: 鳥籠 時間: 2025-3-24 17:33
2.4 CO2 removal and deposition,ion of neutrino oscillations in the laboratory. The central third part of this chapter describes how neutrino oscillations are influenced by the presence of matter. This includes both ordinary matter made up of electrons and nuclei, and the role of self-interactions of neutrinos which becomes releva作者: 弓箭 時間: 2025-3-24 19:15 作者: tenosynovitis 時間: 2025-3-24 23:28 作者: Harness 時間: 2025-3-25 06:40 作者: 吹牛大王 時間: 2025-3-25 11:20 作者: 放逐某人 時間: 2025-3-25 13:37 作者: 榮幸 時間: 2025-3-25 19:44 作者: 支架 時間: 2025-3-25 22:02 作者: Munificent 時間: 2025-3-26 01:28
1879-6923 ly Universe such as primordial magnetic fields and gravitational waves. It also contains exercises and thus will be suitable for both introductory and advanced courses in astroparticle physics.978-94-6239-243-4Series ISSN 1879-6923 Series E-ISSN 1879-6931 作者: Camouflage 時間: 2025-3-26 07:49
The Fundamental Gauge Interactions and Their Descriptione chapter closes with a brief discussion of several possible extensions of the Standard Model, including Grand Unified Theories of the non-gravitational interactions, supersymmetry, extra dimensions and quantum effects in gravity.作者: poliosis 時間: 2025-3-26 11:27 作者: Synthesize 時間: 2025-3-26 14:04 作者: elucidate 時間: 2025-3-26 20:28 作者: indicate 時間: 2025-3-26 21:14
Electroweak Interactions and Neutrinoslopment. Special emphasize will be put on neutrino physics since it plays an important role in high energy astroparticle physics as will be developed in detail in part IV. At this occasion we will also develop and summarize some general concepts in particle physics such as quantum fields and represe作者: 使混合 時間: 2025-3-27 03:23
The Fundamental Gauge Interactions and Their Descriptionf these interactions in a broader and more formal context together with the other known fundamental interactions. We start with general aspects of divergences in the effective description of the electroweak interactions and their relation to renormalization in quantum field theory. We then turn to t作者: tangle 時間: 2025-3-27 07:00
The Universe Between Today and First Light after the big bang, when it was smaller than today by a factor ., and today, in roughly inverse chronological order. We start with the physics of the observable sources, namely stars which are powered by nuclear fusion, and objects powered by the accretion of gas onto compact objects such as neutro作者: Melanocytes 時間: 2025-3-27 12:15 作者: 不確定 時間: 2025-3-27 14:15
Detection Techniques and Experimental Resultsncludes the development of the most relevant aspects of air shower physics. The second part then summarizes the current experimental situation and the main open questions, roughly separated for cosmic radiation of Galactic and extragalactic origin. The following chapters will then provide the theore作者: 起波瀾 時間: 2025-3-27 20:08 作者: FLACK 時間: 2025-3-27 22:19 作者: 他很靈活 時間: 2025-3-28 03:56
Electromagnetic Radiation in Astrophysicsenergy astrophysics. More comprehensive reviews on electromagnetic processes can be found in standard textbooks, e.g. Refs.?[230, 528], and also in Ref.?[529]. In the second part we will apply this to the main scenarios and models of .ray sources, separated into Galactic and extragalactic sources.作者: Aesthete 時間: 2025-3-28 09:00 作者: 無王時期, 時間: 2025-3-28 12:48
Neutrino Propertiesigenstates, the so-called neutrino mixing, and how the transition rates behave under . and . transformations. We also discuss the so far open question whether neutrinos are identical to their antiparticles or not, and thus whether they are Majorana or Dirac fermions. This has a strong influence on t作者: 溫和女人 時間: 2025-3-28 16:50 作者: 鉤針織物 時間: 2025-3-28 20:24 作者: medium 時間: 2025-3-29 02:00
Weak Gravitational Fields and Gravitational Wavesussing their production by moving masses and deriving the relevant formulae from Einstein’s equation (.), we then estimate their strength for the most relevant astrophysical sources. We discuss the recent first direct detection of gravitational waves emitted from a binary black hole merger by the gr作者: 離開可分裂 時間: 2025-3-29 03:51
Dark Mattere Coma cluster from the virial theorem in 1933 [806]. Together with the cosmological evidence for the existence of some form of dark energy, dark matter forms one of the central unsolved problems of modern cosmology. The present chapter starts with reviewing the astrophysical and cosmological eviden作者: 把手 時間: 2025-3-29 08:32
1879-6923 he market. Other works typically focus on subtopics such as This books aims at giving an overview over theoretical and phenomenological aspects of particle astrophysics and particle cosmology. To be of interest for both students and researchers in neighboring fields of physics, it keeps a balance be作者: 紅潤 時間: 2025-3-29 12:28
2.4 CO2 removal and deposition, main open questions, roughly separated for cosmic radiation of Galactic and extragalactic origin. The following chapters will then provide the theoretical and phenomenological fundamentals required to understand the observations and find solutions to the open questions.作者: 地牢 時間: 2025-3-29 18:08 作者: amygdala 時間: 2025-3-29 23:23
Detection Techniques and Experimental Results main open questions, roughly separated for cosmic radiation of Galactic and extragalactic origin. The following chapters will then provide the theoretical and phenomenological fundamentals required to understand the observations and find solutions to the open questions.作者: ARCHE 時間: 2025-3-30 01:25
Neutrino Properties and Their Role in Astrophysics and Cosmologyd the production of neutrinos of high energy neutrinos by the interactions of primary cosmic rays in the Earth atmosphere, the so-called atmospheric neutrinos. We also cover the flavor composition of high energy neutrinos from astrophysical sources, the role of neutrinos as hot dark matter and in lepto- and baryogenesis.作者: CODA 時間: 2025-3-30 05:33
Electroweak Interactions and Neutrinosntations of the group of space-time symmetries. A more formal discussion of all known interactions will follow in the next chapter. The aspects of strong and electromagnetic interactions relavant to astroparticle physics will mostly be discussed in Chaps.?., . and?..作者: 口音在加重 時間: 2025-3-30 10:38
Cosmic Ray Sources and Accelerationhe physics relevant for cosmic ray interactions and propagation within and between the sources and the observer at Earth will be the subject of Chap.?. whereas processes relevant for secondary .-rays will be discussed in Chap.?..作者: MORT 時間: 2025-3-30 14:53
Book 2017aboratory and in high energy cosmic radiation, axion-like particles, and relics of the early Universe such as primordial magnetic fields and gravitational waves. It also contains exercises and thus will be suitable for both introductory and advanced courses in astroparticle physics.作者: lethargy 時間: 2025-3-30 17:42
2.1 Coal exploitation technologies, aspects of magnetized plasmas which play an important role both in high energy astroparticle physics and in the early Universe, subjects that will developed in later chapters. We end with an introduction to gravitational lensing which is an important probe of the large scale structure of the Universe.作者: 價值在貶值 時間: 2025-3-30 23:51
