AbstractRevealing the nature of dark matter is one of the most interesting tasks in astrophysics. Measuring the distribution of recoil angles is said to be one of the most reliable methods to detect a positive signature of dark matter. We focused on measurements via spin-dependent interactions, and studied the feasibility with carbon tetrafluoride (CF4) gas, while taking into account the performance of an existing three-dimensional tracking detector. We consequently found that it is highly possible to detect a positive signature of dark matter via spin-dependent interactions
Several phenomenological aspects of dark matter detection are examined, involving both MACHO and WIM...
We study how the combined observation of dark matter in various direct detection experiments can be ...
An overview of non-directional direct detection methods is given. The currently leading experiments ...
AbstractRevealing the nature of dark matter is one of the most interesting tasks in astrophysics. Me...
AbstractWe developed a three-dimensional gaseous tracking device and performed a direction-sensitive...
International audienceWe study the prospects for detecting weakly interacting massive particles (WIM...
Directional detection can provide unambiguous observation of Dark Matter interactions even in presen...
The nature of dark matter remains one of the biggest questions in physics today. Weakly Interacting ...
Direct detection of dark matter with directional sensitivity is a promising concept for improving th...
The DRIFT (Directional Recoil Identification From Tracks) collaboration operates a 1m3 low pressure ...
If dark matter has spin 0, only two WIMP-nucleon interaction operators can arise as leading operator...
We report a systematic study on the directional sensitivity of a direct dark matter detector that de...
Scientists have postulated the existence of invisible \u27dark matter\u27 since the 1930?s. This con...
For the last 10 years, the search for dark matter (DM) was carried out taking into account the fact ...
An overview of non-directional direct detection methods is given. The currently leading experiments ...
Several phenomenological aspects of dark matter detection are examined, involving both MACHO and WIM...
We study how the combined observation of dark matter in various direct detection experiments can be ...
An overview of non-directional direct detection methods is given. The currently leading experiments ...
AbstractRevealing the nature of dark matter is one of the most interesting tasks in astrophysics. Me...
AbstractWe developed a three-dimensional gaseous tracking device and performed a direction-sensitive...
International audienceWe study the prospects for detecting weakly interacting massive particles (WIM...
Directional detection can provide unambiguous observation of Dark Matter interactions even in presen...
The nature of dark matter remains one of the biggest questions in physics today. Weakly Interacting ...
Direct detection of dark matter with directional sensitivity is a promising concept for improving th...
The DRIFT (Directional Recoil Identification From Tracks) collaboration operates a 1m3 low pressure ...
If dark matter has spin 0, only two WIMP-nucleon interaction operators can arise as leading operator...
We report a systematic study on the directional sensitivity of a direct dark matter detector that de...
Scientists have postulated the existence of invisible \u27dark matter\u27 since the 1930?s. This con...
For the last 10 years, the search for dark matter (DM) was carried out taking into account the fact ...
An overview of non-directional direct detection methods is given. The currently leading experiments ...
Several phenomenological aspects of dark matter detection are examined, involving both MACHO and WIM...
We study how the combined observation of dark matter in various direct detection experiments can be ...
An overview of non-directional direct detection methods is given. The currently leading experiments ...