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: Astrophysical Sources of High Energy Particles and Radiation; Maurice M. Shapiro,Todor Stanev,John P. Wefel Book 2001 Springer Science+Bus

[復(fù)制鏈接]
樓主: SCOWL
41#
發(fā)表于 2025-3-28 16:12:43 | 只看該作者
Galactic Clues About the High-Energy Processes in BL Lac (AGN) Jets formed, and how they are related to the central massive black hole (BH) and its accompanying accretion flow. Understanding this coupling, as well as the overall system energetics, is not possible without knowing the jet content (i.e., pure leptonic or hadronic). Unfortunately, this is still a matter of significant debate in the community.
42#
發(fā)表于 2025-3-28 19:15:01 | 只看該作者
Theory of Cosmic Ray and High-Energy Gamma-Ray Production in Supernova Remnants rays (CRs) originates in supernova remnants (SNRs). Theoretically progress in the solution of this problem has been due to the development of the theory of diffusive shock acceleration (see, for example, reviews [1–3]). Although still incomplete, the theory is able to explain the main characteristi
43#
發(fā)表于 2025-3-29 00:33:23 | 只看該作者
44#
發(fā)表于 2025-3-29 06:28:29 | 只看該作者
Electron Acceleration by Quasi-Parallel Shock Wavestabilities induced by protons in the transition region inside the shock plays the main role in the electron heating and their injection to the first order Fermi acceleration mechanism. The electron distribution function in the vicinity of the shock front can be calculated in our model. The model is
45#
發(fā)表于 2025-3-29 09:02:56 | 只看該作者
46#
發(fā)表于 2025-3-29 11:55:44 | 只看該作者
Supernovae, Superbubbles, Nonthermal Emission & Light Element Nucleosynthesis in the Galaxy with molecular clouds, superbubbles created by massive starformation regions, and high-velocity clouds. We discuss hard continuum and the 511 keV annihilation line emission from that objects. Multiwavelength spectra of extended and compact sources are used to constrain the nonthermal particle gener
47#
發(fā)表于 2025-3-29 18:03:50 | 只看該作者
Cosmic Ray Interactions in the Galactic Center RegionIt is usually assumed that these gamma-rays arise from the interactions of cosmic ray nuclei with ambient matter. Cosmic Ray particles have been observed up to 310. eV, with many arguments suggesting, that up to about 3 10. eV they are of Galactic origin. Cosmic ray particles get injected by their s
48#
發(fā)表于 2025-3-29 22:19:50 | 只看該作者
Dark Matter Halo of Our Galaxyd cosmology on the one hand and with nuclear and particle physics on the other. Dark matter particles are the only relicts that still servive to-day from epochs prior to the primordial helium synthesis which took place at about 400s after the big bang. The first clues pointing to the presence of hid
49#
發(fā)表于 2025-3-30 03:08:59 | 只看該作者
A New Model for the Thermal X-Ray Composites and the Proton Origin γ-Rays from Supernova Remnantslectrons are accelerated on SNR shocks up to the energy ~ 10. eV. We have no direct observational confirmations about proton acceleration by SNR. Different models of γ-emission from SNRs predict different emission mechanisms as dominating. Only π° decays created in proton-nucleon interactions allow
50#
發(fā)表于 2025-3-30 06:28:22 | 只看該作者
 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, 2025-10-11 22:15
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
城市| 江华| 高唐县| 龙里县| 尤溪县| 宽甸| 峡江县| 望城县| 永川市| 南漳县| 灯塔市| 鹤壁市| 凉城县| 股票| 古浪县| 聂拉木县| 全州县| 临漳县| 独山县| 崇礼县| 铁岭市| 丰县| 紫金县| 京山县| 从化市| 榆树市| 威海市| 九龙坡区| 礼泉县| 西宁市| 武乡县| 象山县| 进贤县| 神农架林区| 敦煌市| 卓资县| 调兵山市| 曲周县| 山阳县| 嘉峪关市| 临桂县|