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000297014 0881_ $$aarXiv:0809.0596; RESCEU-53-08
000297014 088__ $$2arXiv$$aarXiv:0809.0596
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000297014 1001_ $$0P:(DE-HGF)0$$aMinowa, M.$$b0
000297014 1112_ $$a4th Patras Workshop on Axions, WIMPs and WISPs$$cHamburg$$d2008-06-18 - 2008-06-21$$gAXION-WIMP 2008$$wGermany
000297014 245__ $$aTokyo Axion Helioscope
000297014 260__ $$aHamburg$$bDeutsches Elektronen-Synchrotron, DESY$$c2009
000297014 300__ $$a39-42
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000297014 520__ $$aA new search result of the Tokyo axion helioscope is presented. The axion helioscope consists of a dedicated cryogen-free 4T superconducting magnet with an effective length of 2.3 m and PIN photodiodes as x-ray detectors. Solar axions, if exist, would be converted into X-ray photons through the inverse Primakoff process in the magnetic field. Conversion is coherently enhanced even for massive axions by filling the conversion region with helium gas. The present third phase measurement sets a new limit of g_{a\gamma\gamma}<(5.6--13.4)\times10^{-10} GeV^{-1} for the axion mass of 0.84<m_a<1.0 eV at 95% confidence level.
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000297014 7001_ $$0P:(DE-HGF)0$$aInoue, Y.$$b1
000297014 7001_ $$0P:(DE-HGF)0$$aAkimoto, Y.$$b2
000297014 7001_ $$0P:(DE-HGF)0$$aOhta, R.$$b3
000297014 7001_ $$0P:(DE-HGF)0$$aMizumoto, T.$$b4
000297014 7001_ $$0P:(DE-HGF)0$$aYamamoto, A.$$b5
000297014 773__ $$a10.3204/DESY-PROC-2008-02/minowa_makoto
000297014 7870_ $$0PUBDB-2016-01759$$aLindner, Axel et.al.$$dVerlag Deutsches Elektronen-Synchrotron, 2008$$iIsPartOf$$rDESY-PROC-2008-02$$tProceedings, 4th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2008)
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