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
咸丰县| 嵩明县| 莆田市| 裕民县| 赤城县| 依安县| 文山县| 万山特区| 壤塘县| 大宁县| 乌海市| 苍溪县| 章丘市| 库伦旗| 彰武县| 合川市| 红原县| 晋宁县| 泾源县| 通化市| 琼结县| 天津市| 阳谷县| 砚山县| 施甸县| 洪雅县| 通海县| 平安县| 崇义县| 淮阳县| 雅江县| 全州县| 申扎县| 乌鲁木齐县| 乐都县| 沙雅县| 志丹县| 扶沟县| 孙吴县| 长岛县| 泰和县|