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: Black Holes: A Laboratory for Testing Strong Gravity; Cosimo Bambi Textbook 2017 Springer Nature Singapore Pte Ltd. 2017 textbook black ho

[復(fù)制鏈接]
樓主: 領(lǐng)口
31#
發(fā)表于 2025-3-27 00:02:10 | 只看該作者
Testing the Kerr Paradigm with X-Ray ObservationsThe chapter briefly reviews current attempts to test the Kerr metric around astrophysical black holes with the continuum-fitting method, X-ray reflection spectroscopy, and quasi-periodic oscilations.
32#
發(fā)表于 2025-3-27 02:10:07 | 只看該作者
Tests with Other ApproachesThe chapter briefly reviews current/future attempts to test the Kerr metric around astrophysical black holes with SgrA., precise measurements in the weak gravitational field of black holes, and with gravitational waves.
33#
發(fā)表于 2025-3-27 06:51:34 | 只看該作者
Cosimo BambiProvides the mathematical tools to compute some key-features in the X-ray spectrum of black holes.Contains calculations and analytical details in the appendix.Offers exercises and examples for student
34#
發(fā)表于 2025-3-27 11:45:17 | 只看該作者
35#
發(fā)表于 2025-3-27 16:18:40 | 只看該作者
https://doi.org/10.1007/978-981-10-4524-0textbook black holes; Continuum-Fitting Method; Iron Line Method; Quasi-Periodic Oscillations; Kerr Para
36#
發(fā)表于 2025-3-27 18:45:17 | 只看該作者
978-981-13-5158-7Springer Nature Singapore Pte Ltd. 2017
37#
發(fā)表于 2025-3-28 00:54:03 | 只看該作者
38#
發(fā)表于 2025-3-28 03:14:15 | 只看該作者
39#
發(fā)表于 2025-3-28 09:37:57 | 只看該作者
Thin Accretion Disksholes, pointing out its assumptions. It also describes the transfer function for thin accretion disks and how the transfer function can be calculated in a stationary and axisymmetric spacetime and in the Kerr metric in particular. Last, the chapter discusses possible deviations from the Kerr backgro
40#
發(fā)表于 2025-3-28 10:37:34 | 只看該作者
Imaging Black Holeslity of imaging astrophysical black holes is mainly motivated by the special situation of SgrA., because it is widely thought that sub-mm VLBI facilities will be soon able to image this black hole and detect its shadow.
 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|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-12 23:51
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
溧水县| 田阳县| 元朗区| 都匀市| 闽侯县| 南澳县| 陇川县| 靖远县| 都兰县| 玛曲县| 太白县| 潜江市| 于都县| 肥西县| 和平区| 潞城市| 大兴区| 万盛区| 林口县| 安康市| 利川市| 镇远县| 巴彦县| 汉源县| 兰考县| 中宁县| 田林县| 台南县| 凤阳县| 姚安县| 宝清县| 丁青县| 杭州市| 铜梁县| 大兴区| 利津县| 长阳| 宣化县| 嘉鱼县| 河东区| 望都县|