Cosmological constant, brane tension and large hierarchy in a generalized Randall-Sundrum braneworld scenario

Details Cosmological constant, brane tension and large hierarchy in a generalized Randall-Sundrum braneworld scenario Cosmological constant, brane tension and large hierarchy in a generalized Randall-Sundrum braneworld scenario

2007-11-12

arxiv.org/abs/0711.1744v2

JHEP0805:042,2008

Physics

High Energy Physics

High Energy Physics - Theory

5 pages, 2 figures, Revtex

Scientific paper

10.1088/1126-6708/2008/05/042

We consider a generalized Randall Sundrum (RS) brane world scenario with a cosmological constant $\Omega$ induced on the visible brane. We show that for $\Omega<0$, resolution of the hierarchy problem requires an upper bound on the magnitude of $\Omega$. The corresponding tension on the visible brane can be positive or negative. On the other hand, there is no such bound for $\Omega>0$. However, in this case, the resolution of the hierarchy problem along with the tuning of the value of the cosmological constant to its observed value closed to $+10^{-124}$ (in Planck units) naturally lead to the tuning of the modulus to a small value of inverse Planck length as estimated in the original RS scenario.

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