| Автор | Corrado Appignani |
| Автор | Roberto Casadio |
| Автор | S. Shankaranarayanan |
| Дата выпуска | 2010-04-01 |
| dc.description | Hořava-Lifshitz theory of gravity with detailed balance is plagued by the presence of a negative bare (or geometrical) cosmological constant which makes its cosmology clash with observations. We argue that adding the effects of the large vacuum energy of quantum matter fields, this bare cosmological constant can be approximately compensated to account for the small observed (total) cosmological constant Λ<sub>OBS</sub>, thus resulting in a self-contained model of gravity and particle physics. Even though we cannot address the fine-tuning problem in this way, we are able to establish a relation between the smallness of Λ<sub>OBS</sub> and the scale ℓ<sub>UV</sub> at which dimension 4 corrections to the Einstein gravity become significant for cosmology. This scale turns out to be ℓ<sub>UV</sub> ≃ 5 ℓ<sub>P</sub> for Λ<sub>OBS</sub> ≃ 0 and we therefore argue that the smallness of Λ<sub>OBS</sub> guarantees that Lorentz invariance is broken only at very small scales. We are also able to provide a first rough estimation for the values of the parameters of the theory μ and Λ<sub>W</sub>. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | The cosmological constant and Hořava-Lifshitz gravity |
| Тип | paper |
| DOI | 10.1088/1475-7516/2010/04/006 |
| Electronic ISSN | 1475-7516 |
| Журнал | Journal of Cosmology and Astroparticle Physics |
| Том | 2010 |
| Первая страница | 6 |
| Последняя страница | 006 |
| Выпуск | 04 |
