The fact that the mass of the visible stars could not account for the gravitational cohesion of the galaxies was the first sign of non-visible (i.e. dark) matter in the Universe. Since then, many observational evidences tell us that most of the matter is indeed dark. The nature of this dark matter is still unknown. There are good reasons to think that most of it is not composed of normal matter. These lectures will review the experimental methods, which have been developed to unravel this mystery and will compare their results with theoretical predictions
The search for dark matter is a very wide and active field of research. Many potential hints of dark...
Astrophysical observations on a wide range of scales indicate that the majority of matter in our Uni...
The dark matter constituting approximately 85% of the mass is an integral part of our universe. As m...
The dark matter problem is almost a century old. Since the 1930s evidence has been growing that our ...
Astronomers can measure the mass of a galaxy by directly observing the galaxy’s visible matter or by...
Contribution from the students of the 4th CERNCLAF School of High-Energy Physics who participated in...
The universe is pervaded by non-luminous matter. Observations at many wavelengths, and on many lengt...
Dark matter is hypothetical matter which does not interact with electromagnetic radiation. The exist...
Astronomical and cosmological observations of the past 80 years build solid evidence that atomic mat...
Over the past decade, a consensus picture has emerged in which roughly a quarter of the universe con...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: ...
We know now that 5/6 of the matter in the Universe is made up of some mysterious material that we ca...
The study of dark matter, in both astrophysics and particle physics, has emerged as one of the most ...
The observational evidence for dark matter on progressively larger cosmic scales is reviewed in a ra...
License, which permits unrestricted use, distribution, and reproduction in any medium, provided the ...
The search for dark matter is a very wide and active field of research. Many potential hints of dark...
Astrophysical observations on a wide range of scales indicate that the majority of matter in our Uni...
The dark matter constituting approximately 85% of the mass is an integral part of our universe. As m...
The dark matter problem is almost a century old. Since the 1930s evidence has been growing that our ...
Astronomers can measure the mass of a galaxy by directly observing the galaxy’s visible matter or by...
Contribution from the students of the 4th CERNCLAF School of High-Energy Physics who participated in...
The universe is pervaded by non-luminous matter. Observations at many wavelengths, and on many lengt...
Dark matter is hypothetical matter which does not interact with electromagnetic radiation. The exist...
Astronomical and cosmological observations of the past 80 years build solid evidence that atomic mat...
Over the past decade, a consensus picture has emerged in which roughly a quarter of the universe con...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: ...
We know now that 5/6 of the matter in the Universe is made up of some mysterious material that we ca...
The study of dark matter, in both astrophysics and particle physics, has emerged as one of the most ...
The observational evidence for dark matter on progressively larger cosmic scales is reviewed in a ra...
License, which permits unrestricted use, distribution, and reproduction in any medium, provided the ...
The search for dark matter is a very wide and active field of research. Many potential hints of dark...
Astrophysical observations on a wide range of scales indicate that the majority of matter in our Uni...
The dark matter constituting approximately 85% of the mass is an integral part of our universe. As m...