淡江大學機構典藏:Item 987654321/104577
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    Please use this identifier to cite or link to this item: https://tkuir.lib.tku.edu.tw/dspace/handle/987654321/104577


    Title: Noise kernel near the horizon of de Sitter space
    Authors: Jason D. Bates;H. T. Cho;Paul R. Anderson;B. L. Hu
    Keywords: COORDINATES;CORRELATION FUNCTIONS;DE SITTER SPACE;KERNELS;SCALAR FIELDS;SPACE-TIME;SYMMETRY
    Date: 2014-01-21
    Issue Date: 2016-01-06 11:03:47 (UTC+8)
    Abstract: 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.
    Relation: Classical and Quantum Gravity 31(2), 025015(18 pages)
    DOI: 10.1088/0264-9381/31/2/025015
    Appears in Collections:[Graduate Institute & Department of Physics] Journal Article

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