We show that a recently constructed five-dimensional (5D) model with gauge-Higgs unification and explicit Lorentz symmetry breaking in the bulk, provides a natural dark matter candidate. This is the lightest Kaluza-Klein particle odd under a certain discrete Z(2) symmetry, which has been introduced to improve the naturalness of the model, and resembles KK-parity but is less constraining. The dark matter candidate is the first KK mode of a 5D gauge field and electroweak bounds force its mass above the TeV scale. Its pair annihilation rate is too small to guarantee the correct relic abundance; however coannihilations with colored particles greatly enhance the effective annihilation rate, leading to realistic relic densities
In this paper we analyze a dark matter model inspired by theories with extra dimensions. The dark m...
In this proceeding, the phenomenology of Universal Extra Dimensions (UED), in which all the Standard...
We study for the first time the possibility that Dark Matter (represented by particles with spin 0, ...
We show that a recently constructed five-dimensional (5D) model with gauge-Higgs unification and exp...
We show that a recently constructed five-dimensional (5D) model with gauge-Higgs unification and exp...
In models with universal extra dimensions (UED), the lightest Kaluza-Klein excitation of neutral ele...
In models with universal extra dimensions (UED), the lightest Kaluza-Klein excitation of neutral ele...
International audienceIn extra dimensional models, a Dark Matter candidate can be present thanks to ...
37 pages, 6 figuresWe study the unique 6 dimensional orbifold with chiral fermions where a stable da...
37 pages, 6 figuresWe study the unique 6 dimensional orbifold with chiral fermions where a stable da...
37 pages, 6 figuresWe study the unique 6 dimensional orbifold with chiral fermions where a stable da...
We summarize the main features of several dark matter candidates in extra-dimensional theories. In p...
We construct models with a Kaluza-Klein (KK) parity in a five- dimensional warped geometry, in an at...
We construct models with a Kaluza-Klein (KK) parity in a five- dimensional warped geometry, in an at...
We construct models with a Kaluza-Klein (KK) parity in a five- dimensional warped geometry, in an at...
In this paper we analyze a dark matter model inspired by theories with extra dimensions. The dark m...
In this proceeding, the phenomenology of Universal Extra Dimensions (UED), in which all the Standard...
We study for the first time the possibility that Dark Matter (represented by particles with spin 0, ...
We show that a recently constructed five-dimensional (5D) model with gauge-Higgs unification and exp...
We show that a recently constructed five-dimensional (5D) model with gauge-Higgs unification and exp...
In models with universal extra dimensions (UED), the lightest Kaluza-Klein excitation of neutral ele...
In models with universal extra dimensions (UED), the lightest Kaluza-Klein excitation of neutral ele...
International audienceIn extra dimensional models, a Dark Matter candidate can be present thanks to ...
37 pages, 6 figuresWe study the unique 6 dimensional orbifold with chiral fermions where a stable da...
37 pages, 6 figuresWe study the unique 6 dimensional orbifold with chiral fermions where a stable da...
37 pages, 6 figuresWe study the unique 6 dimensional orbifold with chiral fermions where a stable da...
We summarize the main features of several dark matter candidates in extra-dimensional theories. In p...
We construct models with a Kaluza-Klein (KK) parity in a five- dimensional warped geometry, in an at...
We construct models with a Kaluza-Klein (KK) parity in a five- dimensional warped geometry, in an at...
We construct models with a Kaluza-Klein (KK) parity in a five- dimensional warped geometry, in an at...
In this paper we analyze a dark matter model inspired by theories with extra dimensions. The dark m...
In this proceeding, the phenomenology of Universal Extra Dimensions (UED), in which all the Standard...
We study for the first time the possibility that Dark Matter (represented by particles with spin 0, ...