找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators; Silvia Celli Book 2019 Springer Nature Switzerland AG 2019 The Orig

[復(fù)制鏈接]
樓主: 貪吃的人
11#
發(fā)表于 2025-3-23 12:46:29 | 只看該作者
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
12#
發(fā)表于 2025-3-23 15:21:03 | 只看該作者
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
13#
發(fā)表于 2025-3-23 20:33:55 | 只看該作者
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
14#
發(fā)表于 2025-3-23 23:34:14 | 只看該作者
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
15#
發(fā)表于 2025-3-24 04:12:32 | 只看該作者
978-3-030-33126-9Springer Nature Switzerland AG 2019
16#
發(fā)表于 2025-3-24 10:20:32 | 只看該作者
17#
發(fā)表于 2025-3-24 13:57:07 | 只看該作者
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.
18#
發(fā)表于 2025-3-24 16:58:28 | 只看該作者
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.
19#
發(fā)表于 2025-3-24 20:46:11 | 只看該作者
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
20#
發(fā)表于 2025-3-24 23:29:54 | 只看該作者
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.
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-15 02:22
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
临江市| 香格里拉县| 当雄县| 中卫市| 尼玛县| 富川| 兴仁县| 云和县| 定结县| 秦安县| 新巴尔虎左旗| 舞钢市| 阿拉善左旗| 烟台市| 四子王旗| 重庆市| 浦县| 信阳市| 新乡县| 垣曲县| 邵东县| 新河县| 芦溪县| 临武县| 浦北县| 德阳市| 彩票| 太保市| 荆门市| 乐山市| 英吉沙县| 铁岭县| 武安市| 靖宇县| 和林格尔县| 滦平县| 陇川县| 高密市| 开化县| 武川县| 新疆|