Antisymmetric tensor fields in a generalized Randall–Sundrum scenario

@article{Das2010AntisymmetricTF,
  title={Antisymmetric tensor fields in a generalized Randall–Sundrum scenario},
  author={Ashmita Das and Soumitra Sengupta},
  journal={Physics Letters B},
  year={2010},
  volume={698},
  pages={311-318}
}

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References

SHOWING 1-10 OF 61 REFERENCES

Bulk antisymmetric tensor fields in a Randall-Sundrum model

We consider bulk antisymmetric tensor fields of various ranks in a Randall-Sundrum scenario. We show that, rank 2 onwards, the zero-modes of the projections of these fields on the (3+1)-dimensional

Bulk fields in the Randall-Sundrum compactification scenario

Recently, Randall and Sundrum proposed a solution to the hierarchy problem where the background spacetime is five dimensional. There are two 3-branes, and the mass scale for fields that propagate on

Gravitational redshift in Einstein-Kalb-Ramond spacetime and Randall-Sundrum scenario

It is shown that the gravitational redshift as predicted by Einstein's theory is modified in the presence of a second-rank antisymmetric tensor (Kalb-Ramond) field in a string-inspired background

Does a randall-sundrum scenario create the illusion of a torsion-free universe?

This work considers spacetime with torsion in a Randall-Sundrum scenario where torson, identified with the rank-2 Kalb-Ramond field, exists in the bulk together with gravity and finds that an additional exponential suppression comes for the torsions zero-mode on the visible brane.

Universal torsion-induced interaction from large extra dimensions

Using a global fit to Z-pole observables, the 3sigma bound on the scale of quantum gravity is found to be 28 TeV for n = 2.

Torsion Effects in Braneworld Scenarios

We present gravitational aspects of braneworld models endowed with torsion terms both in the bulk and on the brane. In order to investigate a conceivable and measurable gravitational effect, arising

Phenomenology of the randall-sundrum gauge hierarchy model

We explore the phenomenology of the localized gravity model of Randall and Sundrum where a 5-dimensional nonfactorizable geometry generates the gauge hierarchy by an exponential function called a
...