A massless scalar field in Robertson-Walker spacetimes: Adiabatic regularization and Green's function*

被引:8
|
作者
Zhang, Yang [1 ]
Wang, Bo [1 ]
Ye, Xuan [1 ]
机构
[1] Univ Sci & Technol China, Sch Astron & Space Sci, CAS Key Lab Res Galaxies & Cosmol, Dept Astron, Hefei 230026, Peoples R China
关键词
quantum fields in curved spacetimes; inflationary universe; mathematical and relativistic aspects of cosmology; ENERGY-MOMENTUM TENSOR; QUANTUM STRESS TENSOR; CURVED SPACETIME; SITTER SPACE; RENORMALIZATION;
D O I
10.1088/1674-1137/44/9/095104
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We study adiabatic regularization of a coupling massless scalar field in general spatially flat Robertson-Walker (RW) spacetimes. For the conformal coupling, the 2nd-order regularized power spectrum and 4th-order regularized stress tensor are zero, and no trace anomaly exists in general RW spacetimes. This is a new result that exceeds those found in de Sitter space. For the minimal coupling, the regularized spectra are also zero in the radiation-dominant and matter-dominant stages, as well as in de Sitter space. The vanishing of these adiabatically regularized spectra is further confirmed by direct regularization of the Green's function. For a general coupling and general RW spacetimes, the regularized spectra can be negative under the conventional prescription. At a higher order of regularization, the spectra will generally become positive, but will also acquire IR divergence, which is inevitable for a massless field. To avoid the IR divergence, the inside-horizon regularization is applied. Through these procedures, nonnegative UV- and IR-convergent power spectrum and spectral energy density will eventually be achieved.
引用
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页数:16
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