We investigate the phenomenology of a simplified model with a Majorana fermion as dark matter candidate which interacts with Standard Model quarks via a colour-charged coannihilation partner. Recently it has been realized that non-perturbative dynamics, including the Sommerfeld effect, bound state formation/dissociation and thermal corrections, play an important role in coannihilations with coloured mediators. This calls for a careful analysis of thermal freeze-out and a new look at the experimental signatures expected for a thermal relic. We employ a state of the art calculation of the relic density which makes use of a non-relativistic effective theory framework and calculate the effective annihilation rates by solving a plasma-modified S...
Dark matter may be a thermal relic whose abundance is set by mutual annihilations among multiple spe...
Motivated by UV explanations of the B-physics anomalies, we study a dark sector containing a Majoran...
We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM par...
We investigate the phenomenology of a simplified model with a Majorana fermion as dark matter candid...
We investigate the phenomenology of a simplified model with a Majorana fermion as dark matter candid...
We analyse the phenomenology of a simplified model for a real scalar dark matter candidate interacti...
Nonthermal dark matter generation is an appealing alternative to the standard paradigm of thermal WI...
Abstract In thermal dark matter models, allowing the dark matter candidate to coannihilate with anot...
The annihilation cross section of thermal relic dark matter determines both its relic density and in...
We present a general classification of simplified models that lead to dark matter (DM) coannihilatio...
The first part of this thesis deals with refined theoretical predictions of the thermal relic abunda...
Recently many investigations have considered Majorana dark matter co-annihilating with bound states ...
We perform a general study of the relic density and LHC constraints on simplified models where the d...
Abstract In this work, we present UV completions of the recently proposed numbe...
We describe the evolution of Dark Matter (DM) abundance from the very onset of its creation from inf...
Dark matter may be a thermal relic whose abundance is set by mutual annihilations among multiple spe...
Motivated by UV explanations of the B-physics anomalies, we study a dark sector containing a Majoran...
We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM par...
We investigate the phenomenology of a simplified model with a Majorana fermion as dark matter candid...
We investigate the phenomenology of a simplified model with a Majorana fermion as dark matter candid...
We analyse the phenomenology of a simplified model for a real scalar dark matter candidate interacti...
Nonthermal dark matter generation is an appealing alternative to the standard paradigm of thermal WI...
Abstract In thermal dark matter models, allowing the dark matter candidate to coannihilate with anot...
The annihilation cross section of thermal relic dark matter determines both its relic density and in...
We present a general classification of simplified models that lead to dark matter (DM) coannihilatio...
The first part of this thesis deals with refined theoretical predictions of the thermal relic abunda...
Recently many investigations have considered Majorana dark matter co-annihilating with bound states ...
We perform a general study of the relic density and LHC constraints on simplified models where the d...
Abstract In this work, we present UV completions of the recently proposed numbe...
We describe the evolution of Dark Matter (DM) abundance from the very onset of its creation from inf...
Dark matter may be a thermal relic whose abundance is set by mutual annihilations among multiple spe...
Motivated by UV explanations of the B-physics anomalies, we study a dark sector containing a Majoran...
We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM par...