We construct models with a Kaluza-Klein (KK) parity in a five-dimensional warped geometry, in an attempt to address the little hierarchy problem present in setups with bulk Standard Model fields. The lightest KK particle (LKP) is stable and can play the role of dark matter. We consider the possibilities of gluing two identical slices of AdS 5 in either the UV (IR-UV-IR model) or the IR region (UV-IR-UV model) and discuss the model-building issues as well as phenomenological properties in both cases. In particular, we find that the UV-IR-UV model is not gravitationally stable and that additional mechanisms might be required in the IR-UV-IR model to address flavor issues. Collider signals of the warped KK parity are different from either the conventional warped extra dimension without KK parity, in which the new particles are not necessarily pair-produced, or the KK parity in flat universal extra dimensions, where each KK level is nearly degenerate in mass. Dark matter and collider properties of a TeV mass KK Z gauge boson as the LKP are discussed.Solutions to the hierarchy problem of the Standard Model (SM) invoke new physics (NP) around the TeV scale to cut-off the quadratically divergent quantum corrections to the Higgs mass. Ideally, to avoid too much fine-tuning, the lightest NP states should be present already at the weak (sub-TeV) scale. However, NP induces higher-dimensional operators involving the SM particles which result in a tension with precision tests of the SM, in both the electroweak (EW) and the flavor sector. To be consistent with the EW precision tests, flavor-preserving operators generated by NP typically require the scale of NP to be larger than a few TeV [1] and are difficult to suppress by any known (approximate) symmetries of the SM 1 . This tension is called the little hierarchy problem. Besides, in the presence of O(1) new sources of CP violation, the data on flavor violation in Kaon system requires the NP mass scale to be larger than several thousands TeV. However, it might be possible to address the latter constraints by suitable flavor symmetries.A new symmetry at the TeV scale can ameliorate some of these constraints if at least the lightest NP states, which a priori give the largest electroweak corrections, are charged under this symmetry while the SM particles are neutral [3,4]. In such a case, the charged NP states do not contribute at tree level to the operators constrained by the precision tests since couplings of a single charged state to SM particles are forbidden. NP contributions from these states arise only at loop level. This makes sub-TeV NP states consistent with EW precision data. These NP states may then play the role of cutting-off the Higgs mass divergence without any fine-tuning, thus avoiding the little hierarchy problem. As a spin-off, the new symmetry implies the existence of a new stable particle that can be a dark matter candidate if it is electrically neutral and weakly interacting.The simplest possibility of a new symmetry at the TeV scale is a discrete Z 2 par...