Add to ORKGThere is almost universal agreement among cosmologists that most of the matter in the Universe is dark, and there are very good reasons to believe that most of this dark matter must be nonbaryonic. The two leading candidates for this dark matter are axions and weakly-interacting massive particles (WIMPs), such as the neutralino in supersymmetric extensions of the standard model. I discuss the arguments for these two dark-matter candidates and review techniques for discovery of these dark-matter particles
There is almost universal agreement among astronomers that most of the mass in the Universe and most...
There appear to be three challenges that any theory of dark matter must face: (i) why is $\Omega_{DM...
I will begin by reviewing the evidence for Dark Matter in the Universe, as well as the candidates fo...
I review axions, neutralinos, axinos, gravitinos and super-massive Wimpzillas as dark matter candida...
More than 80 years after its first postulation in modern form, the existence and distribution of dar...
Several lines of evidence suggest that some of the dark matter may be non-baryonic: the non-detectio...
The need for dark matter is briefly reviewed. A wealth of observational information points to the ex...
One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysica...
The status and prospects of the experimental efforts in the detection of Particle Dark Matter is rev...
The most recent observations by the WMAP satellite provided us with data of unprecedented accuracy r...
This report is a brief review of the efforts to explain the nature of non-baryonic dark matter and o...
After a short introduction on some general implications of recent cosmological observations, we disc...
If Weakly Interacting Massive Particles (WIMPs) are the Dark Matter in the Galaxy, they can be detec...
Astrophysical observations indicate that about 23% of the energy density of the universe is in the f...
The emphasis in this review about non-baryonic dark matter will be on experimental approaches to thi...
There is almost universal agreement among astronomers that most of the mass in the Universe and most...
There appear to be three challenges that any theory of dark matter must face: (i) why is $\Omega_{DM...
I will begin by reviewing the evidence for Dark Matter in the Universe, as well as the candidates fo...
I review axions, neutralinos, axinos, gravitinos and super-massive Wimpzillas as dark matter candida...
More than 80 years after its first postulation in modern form, the existence and distribution of dar...
Several lines of evidence suggest that some of the dark matter may be non-baryonic: the non-detectio...
The need for dark matter is briefly reviewed. A wealth of observational information points to the ex...
One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysica...
The status and prospects of the experimental efforts in the detection of Particle Dark Matter is rev...
The most recent observations by the WMAP satellite provided us with data of unprecedented accuracy r...
This report is a brief review of the efforts to explain the nature of non-baryonic dark matter and o...
After a short introduction on some general implications of recent cosmological observations, we disc...
If Weakly Interacting Massive Particles (WIMPs) are the Dark Matter in the Galaxy, they can be detec...
Astrophysical observations indicate that about 23% of the energy density of the universe is in the f...
The emphasis in this review about non-baryonic dark matter will be on experimental approaches to thi...
There is almost universal agreement among astronomers that most of the mass in the Universe and most...
There appear to be three challenges that any theory of dark matter must face: (i) why is $\Omega_{DM...
I will begin by reviewing the evidence for Dark Matter in the Universe, as well as the candidates fo...