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Автор Alessandro Cerioni
Автор Robert H. Brandenberger
Дата выпуска 2011-08-01
dc.description We consider linear perturbations about a homogeneous and isotropic cosmological background in the projectable version of Hořava-Lifshitz gravity. Starting from the action for cosmological perturbations, we identify the canonically normalized fluctuation variables. We find that - in contrast to what happens in the non-projectable version of the theory - the extra scalar cosmological perturbation mode is already dynamical at the level of linear perturbations and is either ghost-like or tachyonic depending on the value of a free parameter. This indicates a problem for the projectable version of Hořava-Lifshitz gravity.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Cosmological perturbations in the projectable version of Hořava-Lifshitz gravity
Тип paper
DOI 10.1088/1475-7516/2011/08/015
Electronic ISSN 1475-7516
Журнал Journal of Cosmology and Astroparticle Physics
Том 2011
Первая страница 15
Последняя страница 015
Выпуск 08

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