English  |  正體中文  |  简体中文  |  Items with full text/Total items : 60695/93562 (65%)
Visitors : 1051873      Online Users : 32
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library & TKU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
  • Adv. Search
    HomeLoginUploadHelpAboutAdminister Goto mobile version
    Please use this identifier to cite or link to this item: https://tkuir.lib.tku.edu.tw/dspace/handle/987654321/77254

    Title: Quasinormal modes for doubly rotating black holes
    Authors: Cho, H.T.;Doukas, Jason;Naylor, Wade;Cornell, A.S.
    Contributors: 淡江大學物理學系
    Date: 2011-06
    Issue Date: 2012-06-14 09:24:32 (UTC+8)
    Publisher: College Park: American Physical Society
    Abstract: Based on the work of Chen, Lü, and Pope, we derive expressions for the D≥6 dimensional metric for Kerr-anti-de Sitter black holes with two independent rotation parameters and all others set equal to zero: a1≠0, a2≠0, a3=a4=⋯=0. The Klein-Gordon equation is then explicitly separated on this background. For D≥6 this separation results in a radial equation coupled to two generalized spheroidal angular equations. We then develop a full numerical approach that utilizes the asymptotic iteration method to find radial quasinormal modes of doubly rotating flat Myers-Perry black holes for slow rotations. We also develop perturbative expansions for the angular quantum numbers in powers of the rotation parameters up to second order.
    Relation: Physical Review D 83(12), 124034(19pages)
    DOI: 10.1103/PhysRevD.83.124034
    Appears in Collections:[Graduate Institute & Department of Physics] Journal Article

    Files in This Item:

    File Description SizeFormat
    Quasinormal modes for doubly rotating black holes.pdf1235KbAdobe PDF241View/Open

    All items in 機構典藏 are protected by copyright, with all rights reserved.

    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library & TKU Library IR teams. Copyright ©   - Feedback