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
21#
發(fā)表于 2025-3-25 05:40:21 | 只看該作者
Erforderliche ZeichenmaterialienThe 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.
22#
發(fā)表于 2025-3-25 07:55:03 | 只看該作者
23#
發(fā)表于 2025-3-25 13:25:52 | 只看該作者
24#
發(fā)表于 2025-3-25 18:46:35 | 只看該作者
Motion Around Black HolesThe chapter reviews the geodesic motion of massless and massive particles in stationary, axisymmetric, and asymptotically flat spacetimes and in the particular case of the Kerr metric.
25#
發(fā)表于 2025-3-25 21:24:36 | 只看該作者
Astrophysical Black HolesThe chapter reviews the astrophysical observations of stellar-mass black holes, intermediate mass black holes, supermassive black holes, the observations supporting the idea that these objects are indeed black holes, and the spectral state classification.
26#
發(fā)表于 2025-3-26 02:52:33 | 只看該作者
27#
發(fā)表于 2025-3-26 05:55:11 | 只看該作者
Continuum-Fitting MethodThe chapter reviews the continuum-fitting method, namely the technique to fit the thermal spectrum of a geometrically thin and optically thick accretion disk of a black hole to probe the metric close to the compact object.
28#
發(fā)表于 2025-3-26 12:00:12 | 只看該作者
X-Ray Reflection SpectroscopyX-ray reflection spectroscopy is the study of the reflection spectrum of a thin accretion disk. The reflection spectrum has some emission lines and the most prominent one is usually the iron K. line. The reflection spectrum is generated in the inner part of the accretion disk and it can be employed to probe the metric close to the black hole.
29#
發(fā)表于 2025-3-26 16:41:55 | 只看該作者
30#
發(fā)表于 2025-3-26 17:44:49 | 只看該作者
Gravitational WavesThe chapter briefly reviews gravitational waves from black hole coalescences, gravitational waves from extreme-mass ratio inspirals, and quasi-normal modes from black holes.
 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 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 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
新干县| 玉环县| 股票| 漳州市| 遂平县| 嘉黎县| 台州市| 西城区| 丹凤县| 岳阳市| 资溪县| 宁城县| 海晏县| 庆城县| 寿光市| 孙吴县| 海阳市| 论坛| 凤庆县| 延庆县| 抚顺县| 雅安市| 邻水| 滕州市| 普兰店市| 龙游县| 屯留县| 若羌县| 旺苍县| 盐城市| 通道| 湘潭市| 玉山县| 定陶县| 沛县| 泊头市| 灵山县| 黄冈市| 乌审旗| 聊城市| 报价|