Cosmological screening and the phantom braneworld model
Abstract The scalar and vector cosmological perturbations at all length scales of our Universe are studied in the framework of the phantom braneworld model. The model is characterized by the parameter $$\Omega _M\equiv M^3/2m^2H_0$$ ΩM≡M3/2m2H0 , with M and m the five- and four-dimensional Planck sc...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2018-08-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-018-6119-z |