淡江大學機構典藏:Item 987654321/104577
English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 62830/95882 (66%)
造訪人次 : 4042212      線上人數 : 1007
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library & TKU Library IR team.
搜尋範圍 查詢小技巧:
  • 您可在西文檢索詞彙前後加上"雙引號",以獲取較精準的檢索結果
  • 若欲以作者姓名搜尋,建議至進階搜尋限定作者欄位,可獲得較完整資料
  • 進階搜尋
    請使用永久網址來引用或連結此文件: https://tkuir.lib.tku.edu.tw/dspace/handle/987654321/104577


    題名: Noise kernel near the horizon of de Sitter space
    作者: Jason D. Bates;H. T. Cho;Paul R. Anderson;B. L. Hu
    關鍵詞: COORDINATES;CORRELATION FUNCTIONS;DE SITTER SPACE;KERNELS;SCALAR FIELDS;SPACE-TIME;SYMMETRY
    日期: 2014-01-21
    上傳時間: 2016-01-06 11:03:47 (UTC+8)
    摘要: The symmetric two point correlation function of the stress–energy tensor, also known as the noise kernel, for the conformally invariant scalar field is computed in the static region of de Sitter space in terms of the usual static coordinates. Its behavior near the cosmological horizon is investigated. The exact expression is then compared to an approximate expression derived using a quasi-local expansion in order to test the validity of that expansion in a static spherically symmetric spacetime containing a horizon. This gives insight into the likely range of validity of the quasi-local expansion for the noise kernel in Schwarzschild spacetime which has been previously computed.
    關聯: Classical and Quantum Gravity 31(2), 025015(18 pages)
    DOI: 10.1088/0264-9381/31/2/025015
    顯示於類別:[物理學系暨研究所] 期刊論文

    文件中的檔案:

    檔案 描述 大小格式瀏覽次數
    index.html0KbHTML162檢視/開啟
    Noise kernel near the horizon of de Sitter space.pdf772KbAdobe PDF1檢視/開啟

    在機構典藏中所有的資料項目都受到原著作權保護.

    TAIR相關文章

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