Cosmological screening and the phantom braneworld model

dc.contributor.author	Bhattacharya, S.
dc.contributor.author	Kousvos, S.R.
dc.contributor.author	Romanopoulos, S.
dc.contributor.author	Tomaras, T.N.
dc.date.accessioned	2018-12-29T06:32:38Z
dc.date.available	2018-12-29T06:32:38Z
dc.date.issued	2018-12-29
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/1129
dc.description.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 M ≡ M3/2m2H0, with M and m the five- and four-dimensional Planck scales, respectively, and H0 the Hubble parameter today, while M → 0 recovers the CDM model. Ignoring the backreaction due to the peculiar velocities and also the bulk cosmological constant, allows the explicit computation of the gravitational potentials, and . They exhibit exponentially decreasing screening behaviour characterized by a screening length which is a function of the quasidensity parameter M .	en_US
dc.language.iso	en_US	en_US
dc.title	Cosmological screening and the phantom braneworld model	en_US
dc.type	Article	en_US