One way to proof or exclude the existence of axion like particles is a microwave light shining through the wall experiment. In this publication we will emphasize on the engineering aspects of such a setup, currently under development at CERN. One critical point, to achieve meaningful results, is the electromagnetic shielding between axion-emitter and -receiver cavity, which needs to be in the order of 300 dB to improve over existing experimental bounds. The RF leakage or electromagnetic crosstalk between both cavities must be well controlled and quantified during the complete duration of the experiment. A very narrow band (in the 10^-6 Hz range) homodyne detection method is used to reveal the axion signal from background thermal noise. The ...
The CASCADE experiment is a "light shining through a wall" (LSW) experiment consisting of microwave ...
An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic ...
Experimental methods to search for the ``invisible axion`` (f{sub a} {much_gt} 250 GeV) are reviewed...
One way to proof or exclude the existence of axion like particles is a microwave light shining throu...
"Light Shining Through the Wall" experiments can probe the existence of "axion like particles" throu...
To detect or exclude the existence of hidden sector photons or axion like particles, a table-top "mi...
Using microwave cavities one can build a resonant microwave-shining-throughwalls experiment to searc...
For the microwave equivalent of “light shining through the wall” (LSW) experiments, a sensitive micr...
Using microwave cavities one can build a resonant “light-shining-through-walls” experiment to search...
The nature of dark matter remains one of the preeminent mysteries in physics and cosmology. It appea...
We discuss an improved detection scheme for a light-shining-through-wall (LSW) experiment for axion-...
The elegant solutions to the strong CP problem predict the existence of a particle called axion. Thu...
We propose, design and construct a variant of the conventional axion haloscope concept that could be...
Abstract We propose an experimental setup to search for Axion-like particles (ALPs) using two superc...
Joint ILIAS-CAST-CERN Axion Training - Cavity Microwave Searches for Cosmological Axione - The topic...
The CASCADE experiment is a "light shining through a wall" (LSW) experiment consisting of microwave ...
An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic ...
Experimental methods to search for the ``invisible axion`` (f{sub a} {much_gt} 250 GeV) are reviewed...
One way to proof or exclude the existence of axion like particles is a microwave light shining throu...
"Light Shining Through the Wall" experiments can probe the existence of "axion like particles" throu...
To detect or exclude the existence of hidden sector photons or axion like particles, a table-top "mi...
Using microwave cavities one can build a resonant microwave-shining-throughwalls experiment to searc...
For the microwave equivalent of “light shining through the wall” (LSW) experiments, a sensitive micr...
Using microwave cavities one can build a resonant “light-shining-through-walls” experiment to search...
The nature of dark matter remains one of the preeminent mysteries in physics and cosmology. It appea...
We discuss an improved detection scheme for a light-shining-through-wall (LSW) experiment for axion-...
The elegant solutions to the strong CP problem predict the existence of a particle called axion. Thu...
We propose, design and construct a variant of the conventional axion haloscope concept that could be...
Abstract We propose an experimental setup to search for Axion-like particles (ALPs) using two superc...
Joint ILIAS-CAST-CERN Axion Training - Cavity Microwave Searches for Cosmological Axione - The topic...
The CASCADE experiment is a "light shining through a wall" (LSW) experiment consisting of microwave ...
An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic ...
Experimental methods to search for the ``invisible axion`` (f{sub a} {much_gt} 250 GeV) are reviewed...