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001     297014
005     20211110133939.0
024 7 _ |a 10.3204/DESY-PROC-2008-02/minowa_makoto
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024 7 _ |a arXiv:0809.0596
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037 _ _ |a PUBDB-2016-01767
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088 1 _ |a arXiv:0809.0596; RESCEU-53-08
088 _ _ |a arXiv:0809.0596
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088 _ _ |a RESCEU-53-08
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100 1 _ |a Minowa, M.
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111 2 _ |a 4th Patras Workshop on Axions, WIMPs and WISPs
|g AXION-WIMP 2008
|c Hamburg
|d 2008-06-18 - 2008-06-21
|w Germany
245 _ _ |a Tokyo Axion Helioscope
260 _ _ |c 2009
|b Deutsches Elektronen-Synchrotron, DESY
|a Hamburg
300 _ _ |a 39-42
336 7 _ |a Conference Paper
|0 33
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336 7 _ |a Internal Report
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336 7 _ |a INPROCEEDINGS
|2 BibTeX
520 _ _ |a A new search result of the Tokyo axion helioscope is presented. The axion helioscope consists of a dedicated cryogen-free 4T superconducting magnet with an effective length of 2.3 m and PIN photodiodes as x-ray detectors. Solar axions, if exist, would be converted into X-ray photons through the inverse Primakoff process in the magnetic field. Conversion is coherently enhanced even for massive axions by filling the conversion region with helium gas. The present third phase measurement sets a new limit of g_{a\gamma\gamma}<(5.6--13.4)\times10^{-10} GeV^{-1} for the axion mass of 0.84
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700 1 _ |a Inoue, Y.
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700 1 _ |a Akimoto, Y.
|0 P:(DE-HGF)0
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700 1 _ |a Ohta, R.
|0 P:(DE-HGF)0
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700 1 _ |a Mizumoto, T.
|0 P:(DE-HGF)0
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700 1 _ |a Yamamoto, A.
|0 P:(DE-HGF)0
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773 _ _ |a 10.3204/DESY-PROC-2008-02/minowa_makoto
787 0 _ |a Lindner, Axel et.al.
|d Verlag Deutsches Elektronen-Synchrotron, 2008
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|0 PUBDB-2016-01759
|r DESY-PROC-2008-02
|t Proceedings, 4th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2008)
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