標(biāo)題: Titlebook: Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators; Silvia Celli Book 2019 Springer Nature Switzerland AG 2019 The Orig [打印本頁] 作者: 貪吃的人 時(shí)間: 2025-3-21 20:07
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書目名稱Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators讀者反饋學(xué)科排名
作者: Cocker 時(shí)間: 2025-3-21 22:33
Grundlagen, Kompetenzen und Rollen,unequivocally explain the observations [119, 182, 255]. To address this issue, it has been proposed by Zirakashvili and Aharonian [255] (and later on investigated by [118, 143]) that the very hard energy spectrum at low energies could result also from hadronic emission if the SNR is expanding inside a clumpy medium.作者: 馬籠頭 時(shí)間: 2025-3-22 02:21 作者: nostrum 時(shí)間: 2025-3-22 07:13 作者: 嚴(yán)峻考驗(yàn) 時(shí)間: 2025-3-22 10:46 作者: Onerous 時(shí)間: 2025-3-22 13:28 作者: Onerous 時(shí)間: 2025-3-22 19:00 作者: 高貴領(lǐng)導(dǎo) 時(shí)間: 2025-3-23 00:30
Book 2019 and radiation of particles in supernova remnants; (2) very high energy neutrinos from the Galactic Center; and (3) the potential held by the next-generation gamma-ray and neutrino detectors CTA and KM3NeT for studying extended non-thermal sources in the Galaxy. The topics are intrinsically connecte作者: MAOIS 時(shí)間: 2025-3-23 02:32
2190-5053 for Galactic cosmic-ray sources.Presents technical descriptiThis book addresses three “hot” topics concerning the general problem of the origin of Galactic cosmic rays, namely (1) the acceleration, propagation, and radiation of particles in supernova remnants; (2) very high energy neutrinos from the作者: 針葉樹 時(shí)間: 2025-3-23 05:42
Personalpsychologie im Projektmanagement in order to provide the reader with a complete picture concerning the current understanding of the physical processes responsible for the formation of the cosmic-ray (CR) flux observed at Earth and the detection principles of their secondary emission.作者: Abjure 時(shí)間: 2025-3-23 12:46
Grundlagen, Kompetenzen und Rollen,nerally done on a case by case basis. The case of RX?J1713.7-3946?is of special interest in this respect. This remnant has been considered for long time the best candidate for an efficient acceleration scenario, mainly due to its high gamma-ray flux. The detection of gamma-ray emission in the energy作者: 遵循的規(guī)范 時(shí)間: 2025-3-23 15:21
Einleitung. Die Ausnutzung der Atomenergie,ee [126] for an extensive review). It is now in a state of relative inactivity [201] but it might well be a non-stationary source. For instance, there are interesting hints of a much stronger emission few hundreds years ago [154]; on the timescale of .?years, major variability episodes are expected 作者: octogenarian 時(shí)間: 2025-3-23 20:33
https://doi.org/10.1007/978-3-662-64847-6d by the H.E.S.S. [83], MAGIC [50], VERITAS [139] and HAWC [17] Collaborations. Recently, success has been reported also in neutrino astronomy by the detection of a diffuse flux of multi-TeV neutrinos of ‘extra-terrestrial origin’? by the IceCube Collaboration [2]. In the feasible future, the upgrad作者: 原告 時(shí)間: 2025-3-23 23:34
Angewandte Regressionsanalyse mit SPSSand VHE gamma-ray and neutrino astronomy. This comes as a result of the fact that the sources of CRs are also expected to be bright VHE gamma-ray and neutrino emitters, due to the decay of neutral and charged pions produced in the interactions between the accelerated particles and the gas surroundin作者: 大炮 時(shí)間: 2025-3-24 04:12
978-3-030-33126-9Springer Nature Switzerland AG 2019作者: PRISE 時(shí)間: 2025-3-24 10:20 作者: gastritis 時(shí)間: 2025-3-24 13:57
Angewandte Psychologie im UnternehmenUnderstanding the escape mechanism?of accelerated particles is a key ingredient to establishing a connection between SNRs and the origin of CRs.作者: 靈敏 時(shí)間: 2025-3-24 16:58
Particle Escape from Supernova Remnants,Understanding the escape mechanism?of accelerated particles is a key ingredient to establishing a connection between SNRs and the origin of CRs.作者: lavish 時(shí)間: 2025-3-24 20:46
Silvia CelliNominated as an outstanding Ph.D. thesis by the Gran Sasso Science Institute, L’Aquila, Italy.Provides a comprehensive review of the search for Galactic cosmic-ray sources.Presents technical descripti作者: 門窗的側(cè)柱 時(shí)間: 2025-3-24 23:29
Personalpsychologie im Projektmanagement in order to provide the reader with a complete picture concerning the current understanding of the physical processes responsible for the formation of the cosmic-ray (CR) flux observed at Earth and the detection principles of their secondary emission.作者: 未完成 時(shí)間: 2025-3-25 03:20 作者: 脫水 時(shí)間: 2025-3-25 11:19 作者: tolerance 時(shí)間: 2025-3-25 13:43 作者: Confound 時(shí)間: 2025-3-25 16:19
https://doi.org/10.1007/978-3-030-33124-5The Origin of Cosmic Rays; Galactic Cosmic-Ray Pevatrons; Supernova Remnants; The Galactic Center regio作者: Anterior 時(shí)間: 2025-3-25 20:19
2190-5053 and numerical simulations, which are formulated and presented in a straightforward format that can be readily used in the interpretations of gamma-ray and neutrino observations, as well as for confident predictions for future measurements.978-3-030-33126-9978-3-030-33124-5Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: obligation 時(shí)間: 2025-3-26 01:37
Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators作者: 動(dòng)脈 時(shí)間: 2025-3-26 07:08 作者: META 時(shí)間: 2025-3-26 10:10
Propagation and Radiation of Accelerated Particles in Supernova Remnants with Clumpy Structures,nerally done on a case by case basis. The case of RX?J1713.7-3946?is of special interest in this respect. This remnant has been considered for long time the best candidate for an efficient acceleration scenario, mainly due to its high gamma-ray flux. The detection of gamma-ray emission in the energy作者: paradigm 時(shí)間: 2025-3-26 13:06
The Galactic Center Region,ee [126] for an extensive review). It is now in a state of relative inactivity [201] but it might well be a non-stationary source. For instance, there are interesting hints of a much stronger emission few hundreds years ago [154]; on the timescale of .?years, major variability episodes are expected 作者: 單片眼鏡 時(shí)間: 2025-3-26 19:03 作者: 狗舍 時(shí)間: 2025-3-26 21:39
Summary and Conclusions,and VHE gamma-ray and neutrino astronomy. This comes as a result of the fact that the sources of CRs are also expected to be bright VHE gamma-ray and neutrino emitters, due to the decay of neutral and charged pions produced in the interactions between the accelerated particles and the gas surroundin作者: AFFIX 時(shí)間: 2025-3-27 04:50
Book 1995 (Germany) in 1991, Liege (Belgium) again in 1992 and Grenoble (France) in 1994. HPN‘95 is the sixth event of the series sponsored by IFIP WG 6.4 and will be held at the Arxiduc Lluis Salvador building on the campus of the University of the Balearic Islands in Palma de Mallorca (Spain) from September 13 to 15.作者: organism 時(shí)間: 2025-3-27 06:03
Edgar Baumgartner,Peter Sommerfeldsm enjoyed in certain Western intellectual circles at the time. By creating Eastern Buddhism, a new category, they aimed to attach to the Mahāyāna Buddhism of Japan all that the West admired of “Pure Buddhism” , the orientalist construct resulting from the philological study of the Pāli texts of The作者: 媽媽不開心 時(shí)間: 2025-3-27 13:24 作者: 競選運(yùn)動(dòng) 時(shí)間: 2025-3-27 15:51 作者: FOLD 時(shí)間: 2025-3-27 21:24 作者: 險(xiǎn)代理人 時(shí)間: 2025-3-27 21:59 作者: 無瑕疵 時(shí)間: 2025-3-28 05:21
