A new haloscope for Axion dark-matter search is under study using in a first step the large bore superconducting magnet in construction at the LNCMI in Grenoble, which will produce 9~T in 812~mm diameter and 1400~mm height. Microwave cavities of high quality factor $Q\sim10^5-10^6$ will be developed at CAPP/IBS in Daejeon. Low-noise microwave amplification of the signal will be ensured by DC superconducting quantum interference devices (SQUID) or/and Josephson parametric amplifiers (JPA) cooled-down to 20~mK by a $^3$He/$^4$He dilution refrigerator. This new haloscope will be designed to probe QCD dark-matter Axions in the mass range of 1-100~$\mu$eV with unprecedented sensitivity
The axion is an hypothetical beyond the Standard Model particle, first introduced in the seventies a...
An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic ...
Abstract. We describe the status of a sensitive search for halo axions with masses in the µeV range....
International audienceA new haloscope for Axion dark-matter search is under study using in a first s...
International audienceA new haloscope for Axion dark-matter search is under study using in a first s...
If axions constitute the dark matter of our galactic halo they can be detected by their conversion i...
The Center for Axion and Precision Physics Research (CAPP) was founded in 2013, with the ambition of...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
We report the first search results for axion dark matter using an 18 T high-temperature superconduct...
The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interacti...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
We report an extended search for the axion dark matter using the CAPP18T haloscope. The CAPP18T expe...
We report an extended search for the axion dark matter using the CAPP18T haloscope. The CAPP18T expe...
The axion is an hypothetical beyond the Standard Model particle, first introduced in the seventies a...
An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic ...
Abstract. We describe the status of a sensitive search for halo axions with masses in the µeV range....
International audienceA new haloscope for Axion dark-matter search is under study using in a first s...
International audienceA new haloscope for Axion dark-matter search is under study using in a first s...
If axions constitute the dark matter of our galactic halo they can be detected by their conversion i...
The Center for Axion and Precision Physics Research (CAPP) was founded in 2013, with the ambition of...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
We report the first search results for axion dark matter using an 18 T high-temperature superconduct...
The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interacti...
The axion emerges in extensions of the Standard Model that explain the absence of CP violation in th...
We report an extended search for the axion dark matter using the CAPP18T haloscope. The CAPP18T expe...
We report an extended search for the axion dark matter using the CAPP18T haloscope. The CAPP18T expe...
The axion is an hypothetical beyond the Standard Model particle, first introduced in the seventies a...
An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic ...
Abstract. We describe the status of a sensitive search for halo axions with masses in the µeV range....