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Автор Jian-Pin Wu
Автор Yi Ling
Дата выпуска 2010-05-01
dc.description In this paper we investigate the scalar mode of first-order metric perturbations over spatially flat FRW spacetime when the holonomy correction is taken into account in the semi-classical framework of loop quantum cosmology. By means of the Hamiltonian derivation, the cosmological perturbation equations is obtained in longitudinal gauge. It turns out that in the presence of metric perturbation the holonomy effects influence both background and perturbations, and contribute the non-trivial terms S<sub>h1</sub> and S<sub>h2</sub> in the cosmological perturbation equations.
Формат application.pdf
Издатель Institute of Physics Publishing
Название The cosmological perturbation theory in loop cosmology with holonomy corrections
Тип paper
DOI 10.1088/1475-7516/2010/05/026
Electronic ISSN 1475-7516
Журнал Journal of Cosmology and Astroparticle Physics
Том 2010
Первая страница 26
Последняя страница 026
Выпуск 05

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