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University of Cambridge > Talks.cam > Theoretical Physics Colloquium > Holography and the self-tuning of the cosmological constant

## Holography and the self-tuning of the cosmological constantAdd to your list(s) Download to your calendar using vCal - Elias Kiritsis, APC Paris and University of Crete
- Wednesday 25 October 2017, 14:15-15:15
- MR2, Centre for Mathematical Sciences.
If you have a question about this talk, please contact David Marsh. We propose a brane-world setup based on gauge/gravity duality in which the four-dimensional cosmological constant is set to zero by a dynamical self-adjustment mechanism. The bulk contains Einstein gravity and a scalar field. We study holographic RG flow solutions, with the standard model brane separating an infinite volume UV region and an IR region of finite volume. For generic values of the brane vacuum energy, regular solutions exist such that the four-dimensional brane is flat. Its position in the bulk is determined dynamically by the junction conditions. Analysis of linear fluctuations shows that a regime of 4-dimensional gravity is possible at large distances, due to the presence of an induced gravity term. The graviton acquires an effective mass, and a five-dimensional regime may exist at large and/or small scales. We show that, for a broad choice of bulk potentials, flat-brane solutions are manifestly stable and free of ghosts. We compute the scalar contribution to the force between brane-localized sources and show that, in certain models, the vDVZ discontinuity is absent and the effective interaction at short distances is mediated by two transverse graviton helicities. This talk is part of the Theoretical Physics Colloquium series. ## This talk is included in these lists:- All CMS events
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