Search for solar Kaluza–Klein axions by annual modulation with the XMASS-I detector
Search for solar Kaluza–Klein axions by annual modulation with the XMASS-I detector
复制标题
使用 XMASS-I 探测器通过年调制搜索太阳卡鲁扎-克莱因轴子
DOI:
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发表时间:
2017
期刊:
影响因子:
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通讯作者:
S. Nakamura
中科院分区:
文献类型:
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作者:
X. C. N. Oka;K. Abe;K. Hiraide;K. Ichimura;Y. Kishimoto;K. Kobayashi;M. Kobayashi;S. Moriyama;M. Nakahata;T. Norita;H. Ogawa;K. Sato;H. Sekiya;O. Takachio;A. Takeda;S. Tasaka;M. Yamashita;B. Yang;N. Y. Kim;Y. Kim;Y. Itow;K. Kanzawa;R. Kegasa;K. Masuda;H. Takiya;K. Fushimi;G. Kanzaki;K. Martens;Y. Suzuki;B. D. Xu;R. Fujita;K. Hosokawa;K. Miuchi;Y. Takeuchi;Y. H. Kim;K. Lee;M. K. Lee;Y. Fukuda;M. Miyasaka;K. Nishijima;S. Nakamura
In theories with the large extra dimensions beyond the standard 4-dimensional spacetime, axions could propagate in such extra dimensions, and acquire Kaluza-Klein (KK) excitations. These KK axions are produced in the Sun and could solve unexplained heating of the solar corona. While most of the solar KK axions escape from the solar system, a small fraction is gravitationally trapped in orbits around the Sun. They would decay into two photons inside a terrestrial detector. The event rate is expected to modulate annually depending on the distance from the Sun. We have searched for the annual modulation signature using $832 imes 359$ kg$cdot$days of XMASS-I data. No significant event rate modulation is found, and hence we set the first experimental constraint on the KK axion-photon coupling of $4.8 imes 10^{-12}, mathrm{GeV}^{-1}$ at 90% confidence level for a KK axion number density of $ar{n}_mathrm{a} = 4.07 imes 10^{13}, mathrm{m}^{-3}$, the total number of extra dimensions $n = 2$, and the number of extra dimensions $delta = 2$ that axions can propagate in.