# 53rd Rencontres de Moriond - EW 2018

10-17 March 2018
Europe/Paris timezone

## Extra Dimensions are Dark

14 Mar 2018, 17:40
15m

### Speaker

Dr Thomas Rizzo (SLAC)

### Description

Extra dimensions (ED) can provide a useful tool for model-building. In this paper we introduce a single, flat ED extension of the kinetic-mixing/dark photon (DP) portal for dark matter (DM)
interactions with the Standard Model (SM) assuming a compactification `radius' of order $R^{-1}\sim10-1000$ MeV and examine the resulting modifications to and augmentation of the
usual DP phenomenology. In the present scenario, both the DP and DM experience the full 5-D while the SM fields are constrained to lie on a 4-D brane at the boundary of the ED. Such a
setup can naturally yield the observed value of the DM relic density and explain the required rough degeneracy of the DM and DP masses needed to obtain it. Gauge symmetry breaking can
occur via boundary conditions without the introduction of an additional singlet Higgs scalar thus avoiding all constraints associated with the coupling of such a field to the usual SM Higgs
field in 5-D. The self-consistency of the field redefinitions that map the gauge fields into a canonical basis and thus removing the kinetic mixing terms is found to lead to a strong model building
constraint on the ED setup involving a brane localized kinetic term for the 5-D gauge field on the SM brane. Multiple variations of this scenario are found to be possible which are consistent with
all current experimental constraints but which predict very different phenomenologies. In this paper, after setting up the general model formalism, we discuss in detail the case of a complex
scalar 5-D DM field, consistent with constraints arising from the CMB, which may or may not obtain a vacuum expectation value (vev). The resulting Kaluza-Klein (KK) towers of both the DM
and DP fields are found to yield interesting and distinctive signatures while simultaneously being constrained by a wide array of existing measurements but with the details being dependent
upon the specifics of the KK spectrum and the presence or absence of this 5-D scalar vev.

### Primary author

Dr Thomas Rizzo (SLAC)

### Presentation Materials

 Moriond18.pdf Rizzo.tar.gz