The axino and the gravitino are extremely weakly interacting candidates for the lightest supersymmetric particle (LSP). We demonstrate that either of them could provide the right amount of cold dark matter. Assuming that a charged slepton is the next-to-lightest supersymmetric particle (NLSP), we discuss how NLSP decays into the axino/gravitino LSP can provide evidence for axino/gravitino dark matter at future colliders. We show that these NLSP decays will allow us to estimate the value of the Peccei–Quinn scale and the axino mass if the axino is the LSP. In the case of the gravitino LSP, we illustrate that the gravitino mass can be determined. This is crucial for insights into the mechanism of supersymmetry breaking and can lead to a micro...
We consider supergravity with a gravitino lightest supersymmetric particle. The next-to-lightest sup...
AbstractMotivated by specific connections to dark matter signatures, we study the prospects of obser...
In view of the recent interest in the pMSSM with light third generation squarks, we consider a hithe...
AbstractThe axino and the gravitino are well-motivated candidates for the lightest supersymmetric pa...
Gravitinos and axinos produced in the late decays of other supersymmetric particles are well-motivat...
The identification of dark matter in our particle physics model is still an open question. Here, we ...
The gravitino is a promising candidate for cold dark matter. We study cosmological constraints on sc...
In supersymmetric extensions of the Standard Model, the lightest neutralino, the gravitino, and the ...
SuperWeakly-Interacting Massive Particles (superWIMPs) produced in the late decays of other particle...
We investigate supergravity models in which the lightest supersymmetric particle (LSP) is a stable g...
Considering scenarios in which the gravitino is the lightest supersymmetric particle and a charged s...
We investigate phenomenological consequences of locally supersymmetric extensions of the Standard Mo...
We review the case of gravitino Dark Matter for stop, neutralino and sneutrino Next-to-Lightest Supe...
Axino and gravitino are promising candidates to solve the dark matter (DM) problem in the framework ...
We show that axinos produced in the early Universe in the decay of the lightest neutralinos are a na...
We consider supergravity with a gravitino lightest supersymmetric particle. The next-to-lightest sup...
AbstractMotivated by specific connections to dark matter signatures, we study the prospects of obser...
In view of the recent interest in the pMSSM with light third generation squarks, we consider a hithe...
AbstractThe axino and the gravitino are well-motivated candidates for the lightest supersymmetric pa...
Gravitinos and axinos produced in the late decays of other supersymmetric particles are well-motivat...
The identification of dark matter in our particle physics model is still an open question. Here, we ...
The gravitino is a promising candidate for cold dark matter. We study cosmological constraints on sc...
In supersymmetric extensions of the Standard Model, the lightest neutralino, the gravitino, and the ...
SuperWeakly-Interacting Massive Particles (superWIMPs) produced in the late decays of other particle...
We investigate supergravity models in which the lightest supersymmetric particle (LSP) is a stable g...
Considering scenarios in which the gravitino is the lightest supersymmetric particle and a charged s...
We investigate phenomenological consequences of locally supersymmetric extensions of the Standard Mo...
We review the case of gravitino Dark Matter for stop, neutralino and sneutrino Next-to-Lightest Supe...
Axino and gravitino are promising candidates to solve the dark matter (DM) problem in the framework ...
We show that axinos produced in the early Universe in the decay of the lightest neutralinos are a na...
We consider supergravity with a gravitino lightest supersymmetric particle. The next-to-lightest sup...
AbstractMotivated by specific connections to dark matter signatures, we study the prospects of obser...
In view of the recent interest in the pMSSM with light third generation squarks, we consider a hithe...