The particle physics interpretation of the missing-mass, or darkmatter, problem of cosmological and astrophysical nature is going to be posed under deep scrutiny in the next years. From the particle physics side, accelerator physics will deeply test theoretical ideas of new physics beyond the Standard Model, where a particle physics candidate to dark matter is often naturally obtained. From the astrophysical side, many probes are already providing a great deal of independent information on the signals which can be produced by the galactic or extra-galactic dark matter. The ultimate hope is in fact to be able to disentangle a dark matter signal from the various sources of backgrounds and to extract a coherent picture of new physics from th...
In these lectures we first briefly review the main observational facts which imply that most part of...
We review the features of Dark Matter as a particle, presenting some old and new instructive models,...
In this thesis we analyze the consequences of extra spacetime dimensions on the MSSM. We begin by r...
Dark matter has been shown to be extremely abundant in our universe. It comprises about 23 percent o...
Cosmology demands particle physics beyond the Standard Model: we need to explain the nature of dark ...
Cosmology now provides unambiguous, quantitative evidence for new particle physics. I discuss the im...
The most recent observations by the WMAP satellite provided us with data of unprecedented accuracy r...
Contribution from the students of the 4th CERNCLAF School of High-Energy Physics who participated in...
Up to now searches for Dark Matter (DM) detection have not been successful, either because our parad...
Cosmic rays offer an opportunity to search for dark matter, if the latter decays or annihilates into...
Supersymmetry may be discovered at high energy colliders, through low energy precision measurements,...
Dark Matter constitutes more than 80% of the total amount of matter in the Universe, yet almost not...
Observations with the Fermi Large Area Telescope (LAT) indicate an excess in gamma rays originating ...
I will give an update on current status and future prospects in searching for the particle nature ...
The need for dark matter is briefly reviewed. A wealth of observational information points to the ex...
In these lectures we first briefly review the main observational facts which imply that most part of...
We review the features of Dark Matter as a particle, presenting some old and new instructive models,...
In this thesis we analyze the consequences of extra spacetime dimensions on the MSSM. We begin by r...
Dark matter has been shown to be extremely abundant in our universe. It comprises about 23 percent o...
Cosmology demands particle physics beyond the Standard Model: we need to explain the nature of dark ...
Cosmology now provides unambiguous, quantitative evidence for new particle physics. I discuss the im...
The most recent observations by the WMAP satellite provided us with data of unprecedented accuracy r...
Contribution from the students of the 4th CERNCLAF School of High-Energy Physics who participated in...
Up to now searches for Dark Matter (DM) detection have not been successful, either because our parad...
Cosmic rays offer an opportunity to search for dark matter, if the latter decays or annihilates into...
Supersymmetry may be discovered at high energy colliders, through low energy precision measurements,...
Dark Matter constitutes more than 80% of the total amount of matter in the Universe, yet almost not...
Observations with the Fermi Large Area Telescope (LAT) indicate an excess in gamma rays originating ...
I will give an update on current status and future prospects in searching for the particle nature ...
The need for dark matter is briefly reviewed. A wealth of observational information points to the ex...
In these lectures we first briefly review the main observational facts which imply that most part of...
We review the features of Dark Matter as a particle, presenting some old and new instructive models,...
In this thesis we analyze the consequences of extra spacetime dimensions on the MSSM. We begin by r...