Contribution to a conference proceedings/Internal Report

PUBDB-2016-01767

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Tokyo Axion Helioscope

Minowa, M. ; Inoue, Y. ; Akimoto, Y. ; Ohta, R. ; Mizumoto, T. ; Yamamoto, A.

2009
Deutsches Elektronen-Synchrotron, DESY Hamburg

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2008-02/minowa_makoto

Report No.: RESCEU-53-08; arXiv:0809.0596

Abstract: 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<m_a<1.0 eV at 95% confidence level.

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Contributing Institute(s):

1. Bibliothek und Dokumentation (L)

Research Program(s):

1. 899 - ohne Topic (POF3-899) (POF3-899)

Experiment(s):

1. Facility (machine) HERA

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Proceedings/Internal Report Lindner, A. (Editor)DESY* ; Redondo, J. (Editor)DESY* ; Ringwald, A. (Editor)DESY*
Proceedings, 4th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2008)
20084th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2008, HamburgHamburg, Germany, 18 Jun 2008 - 21 Jun 20082008-06-182008-06-21 Verlag Deutsches Elektronen-Synchrotron (2008)2008     Files BibTeX | EndNote: XML, Text | RIS

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