Universal Journal of Physics and Application Vol. 10(2), pp. 58 - 59
DOI: 10.13189/ujpa.2016.100205
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Search for Low Mass WIMP and Axions, Emitted from the Sun

B. M. Ovchinnikov ^*, V. V. Parusov
Institute for Nuclear Research, Russian Academy of Sciences, Russia

ABSTRACT

The chamber for direct detection of WIMP with mass < 10 Gev/c² and axions, emitted from the Sun was developed. The chamber is filled with gas mixture H₂ +3ppm TMAE (1,5,10 bar), or D₂ + 3ppm TMAE. These gas fillings allow to suppress the electron background. For detecting of events is used the system GEM+pin-anode with coefficient multiplication about 10⁵. In experiment it is necessary to search the early or daily modulation effects.

KEYWORDS
Low Mass WIMP, Metallic GEM+Pin-Anode, H₂ + 3ppm TMAE Filling, Axion

Cite This Paper in IEEE or APA Citation Styles
(a). IEEE Format:
[1] B. M. Ovchinnikov , V. V. Parusov , "Search for Low Mass WIMP and Axions, Emitted from the Sun," Universal Journal of Physics and Application, Vol. 10, No. 2, pp. 58 - 59, 2016. DOI: 10.13189/ujpa.2016.100205.

(b). APA Format:
B. M. Ovchinnikov , V. V. Parusov (2016). Search for Low Mass WIMP and Axions, Emitted from the Sun. Universal Journal of Physics and Application, 10(2), 58 - 59. DOI: 10.13189/ujpa.2016.100205.