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Detecting solar axions using Earth's magnetic field.
Hooman Davoudiasl1, Patrick Huber
1Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA.
Physical Review Letters
|December 13, 2006
Summary
Solar axion conversion to photons in Earth's magnetosphere can create a detectable X-ray flux. This study proposes a new method to probe axion properties, exceeding current laboratory sensitivities.
Area of Science:
- Astrophysics
- Particle Physics
Background:
- Axions are hypothetical particles proposed as dark matter candidates.
- Solar axions can convert to photons within planetary magnetospheres.
Purpose of the Study:
- To investigate the potential for detecting solar axions via photon conversion in Earth's magnetosphere.
- To establish a new experimental approach for probing axion-photon coupling.
Main Methods:
- Simulating solar axion to photon conversion within the Earth's magnetosphere.
- Proposing the use of a low-Earth-orbit X-ray detector with a large effective area.
- Targeting the detector towards the solar core for optimal signal detection.
Main Results:
- Solar axion-photon conversion can generate a measurable X-ray flux (approx. 4 keV) on Earth's night side.
- The large magnetized volume of the magnetosphere compensates for the weak magnetic field.
- Sensitivity to photon-axion coupling down to 10(-11) GeV-1 is achievable for axion masses < 10(-4) eV within one year.
Conclusions:
- This method offers a novel way to detect solar axions.
- The proposed X-ray detection strategy provides an order of magnitude improvement over current laboratory limits.
- The study opens new avenues for exploring fundamental physics with astrophysical observations.
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