In this work we study a classically scale-invariant extension of the Standard Model in which the dark matter and electroweak scales are generated through the Coleman-Weinberg mechanism. The extra $SU(3)_X$ gauge factor gets completely broken by the vevs of two scalar triplets. Out of the eight resulting massive vector bosons the three lightest are stable due to an intrinsic $Z_2\times Z_2'$ discrete symmetry and can constitute dark matter candidates. We analyze the phenomenological viability of the predicted multi-Higgs sector imposing theoretical and experimental constraints. We perform a comprehensive analysis of the dark matter predictions of the model solving numerically the set of coupled Boltzmann equations involving all relevant dark...
We examine the impact of the expected reach of the LHC and the XENONIT experiments on the parameter ...
Although the standard model (SM) can explain almost all experimental results obtained until now, the...
The composition of Dark Matter (DM) remains an important open question. The current data do not dist...
We propose a classically scale invariant extension of the Standard Model where the electroweak symme...
We study an extension of the Standard Model featuring a hidden sector that consists of a new scalar...
We analyze a classically scale invariant extension of the Standard Model with a dark gauge U(1) X br...
Abstract We propose a new physics model which has a cold dark matter candidate and can explain the b...
We examine the collider and dark matter phenomenology of the Standard Model extended by a hypercharg...
A dark sector with non-abelian gauge symmetry provides a sound framework to justify stable dark matt...
AbstractExtending the spacetime symmetries of standard model (SM) by scale invariance (SI) may addre...
We studied Dark Matter (DM) phenomenology with multiple DM species consisting of both scalar and vec...
Abstract TeV-scale dark matter is well motivated by notions of naturalness as the new physics thresh...
With the assistance of two extra groups, i.e., an extra hidden gauge group SU(2) D and a global U(1)...
The compelling astrophysical evidence for dark matter on one hand and the experimental evidence for ...
International audienceWe investigate a model with two real scalar fields that minimally generates ex...
We examine the impact of the expected reach of the LHC and the XENONIT experiments on the parameter ...
Although the standard model (SM) can explain almost all experimental results obtained until now, the...
The composition of Dark Matter (DM) remains an important open question. The current data do not dist...
We propose a classically scale invariant extension of the Standard Model where the electroweak symme...
We study an extension of the Standard Model featuring a hidden sector that consists of a new scalar...
We analyze a classically scale invariant extension of the Standard Model with a dark gauge U(1) X br...
Abstract We propose a new physics model which has a cold dark matter candidate and can explain the b...
We examine the collider and dark matter phenomenology of the Standard Model extended by a hypercharg...
A dark sector with non-abelian gauge symmetry provides a sound framework to justify stable dark matt...
AbstractExtending the spacetime symmetries of standard model (SM) by scale invariance (SI) may addre...
We studied Dark Matter (DM) phenomenology with multiple DM species consisting of both scalar and vec...
Abstract TeV-scale dark matter is well motivated by notions of naturalness as the new physics thresh...
With the assistance of two extra groups, i.e., an extra hidden gauge group SU(2) D and a global U(1)...
The compelling astrophysical evidence for dark matter on one hand and the experimental evidence for ...
International audienceWe investigate a model with two real scalar fields that minimally generates ex...
We examine the impact of the expected reach of the LHC and the XENONIT experiments on the parameter ...
Although the standard model (SM) can explain almost all experimental results obtained until now, the...
The composition of Dark Matter (DM) remains an important open question. The current data do not dist...