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相关论文: A Telescope Search for Decaying Relic Axions

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The axion is a hypothetical elementary particle and a cold dark matter candidate. It could dominate potential wells of most astrophysical objects. Axions spontaneously decay into nearly monochromatic microwave photons. We present results…

天体物理学 · 物理学 2009-10-31 B. D. Blout , E. J. Daw , M. P. Decowski , Paul T. P. Ho , L. J Rosenberg , D. B. Yu

We study cross correlations between line intensity and weak lensing maps to search for axion-like particles (ALPs). Radiative decay of eV-mass ALPs can contribute to cosmic background emissions at optical and infrared wavelengths. Line…

宇宙学与河外天体物理 · 物理学 2021-05-26 Masato Shirasaki

Axion-like particles (ALPs) can decay into two photons with a rest-frame frequency given by half of the ALP mass. This implies that ultra-violet searches can be used to investigate ALPs in the multi-eV mass range. We use archival data from…

高能物理 - 唯象学 · 物理学 2025-05-30 Elisa Todarello , Marco Regis

A search for solar axions has been performed using an axion helioscope which is equipped with a 2.3m-long 4T superconducting magnet, PIN-photodiode X-ray detectors, and a telescope mount mechanism to track the sun. In addition, a gas…

天体物理学 · 物理学 2008-11-26 Y. Inoue , T. Namba , S. Moriyama , M. Minowa , Y. Takasu , T. Horiuchi , A. Yamamoto

Axion-like particles (ALPs) can account for the observed dark matter (DM) of the Universe and if their masses are at the eV scale, they can decay into infrared, optical and ultraviolet photons with a decay lifetime larger than the age of…

高能物理 - 唯象学 · 物理学 2025-06-03 Arpan Kar , Sourov Roy , Pratick Sarkar

Bounds are derived on the axion-like particle (ALP) to two-photon coupling in the mass range $2.65-5.27$ eV. The bounds are obtained by searching for the signal from ALP decay in the Multi Unit Spectroscopic Explorer (MUSE) observations of…

宇宙学与河外天体物理 · 物理学 2023-10-04 Elisa Todarello

Decaying axion-like particles (ALP) with masses in the eV range which might occupy dark matter halos of the Milky Way and other galaxies produce a characteristic "bump" feature in the spectrum of extragalactic background light (EBL). This…

高能物理 - 唯象学 · 物理学 2020-04-20 A. Korochkin , A. Neronov , D. Semikoz

We have searched for solar axions or similar particles that couple to two photons by using the CERN Axion Solar Telescope (CAST) setup with improved conditions in all detectors. From the absence of excess X-rays when the magnet was pointing…

高能物理 - 实验 · 物理学 2012-08-27 CAST Collaboration

(abridged) We present extensive multi-color imaging and low resolution VIMOS Integral Field Unit spectroscopic observations of the X-ray luminous cluster Abell 2667 (z=0.233). An extremely bright giant gravitational arc (z=1.0334) is easily…

天体物理学 · 物理学 2009-11-11 G. Covone , J. -P. Kneib , G. Soucail , J. Richard , E. Jullo , H. Ebeling

We study prospects to detect axion-like particles (ALPs) with the upcoming near-infrared telescope SPHEREx. The signal under investigation is the ALP decay into two photons. Assuming dark matter (DM) to be in the form of ALPs, we analyze…

宇宙学与河外天体物理 · 物理学 2025-05-09 Marco Regis , Marco Taoso , Jorge Terol Calvo

The CERN Axion Solar Telescope (CAST) experiment searches for solar axions by the "helioscope" method. First results imply an upper limit on the axion-photon coupling of g_a-gamma < 1.16 x 10^-10 GeV^-1 (95% CL) for m_a < 0.02 eV, in this…

高能物理 - 唯象学 · 物理学 2007-05-23 Georg G. Raffelt

We present the first results of a search for invisible axion dark matter using a multiple-cell cavity haloscope. This cavity concept was proposed to provide a highly efficient approach to high mass regions compared to the conventional…

高能物理 - 实验 · 物理学 2020-12-09 Junu Jeong , SungWoo Youn , Sungjae Bae , Jihngeun Kim , Taehyeon Seong , Jihn E Kim , Yannis K. Semertzidis

This Letter reports results from a haloscope search for dark matter axions with masses between 2.66 and 2.81 $\mu$eV. The search excludes the range of axion-photon couplings predicted by plausible models of the invisible axion. This…

We investigate the use of next generation radio telescopes such as the Square Kilometre Array (SKA) to detect axion two-photon coupling in the astrophysical environment. The uncertainty surrounding astrophysical magnetic fields presents new…

宇宙学与河外天体物理 · 物理学 2017-10-31 Katharine Kelley , P. J. Quinn

A search for solar axions has been performed using an axion helioscope which is equipped with a 2.3m-long 4T superconducting magnet, a gas container to hold dispersion-matching gas, PIN-photodiode X-ray detectors, and a telescope mount…

天体物理学 · 物理学 2011-06-07 Y. Inoue , Y. Akimoto , R. Ohta , T. Mizumoto , A. Yamamoto , M. Minowa

We have searched for axions which could have been produced in the solar core using an axion helioscope with a 2.3m-long 4T superconducting magnet. Axion mass region up to m_a=0.26eV was newly explored by introducing dispersion-matching gas.…

天体物理学 · 物理学 2016-11-03 Y. Inoue , T. Namba , S. Moriyama , M. Minowa , Y. Takasu , T. Horiuchi , A. Yamamoto

We use MUSE spectroscopic observations of the dwarf spheroidal galaxy Leo T between 470 and 935 nm to search for radiative decays of axion like particles (ALPs). Under the assumption that ALPs constitute the dark matter component of the Leo…

宇宙学与河外天体物理 · 物理学 2021-01-21 Marco Regis , Marco Taoso , Daniel Vaz , Jarle Brinchmann , Sebastiaan L. Zoutendijk , Nicolas F. Bouché , Matthias Steinmetz

A radiative decaying Big Bang relic with a mass $m_a\simeq 5-25 \,\rm eV$, which we dub "blue axion", can be probed with direct and indirect observations of the cosmic optical background (COB). The strongest bounds on blue-axion cold dark…

高能物理 - 唯象学 · 物理学 2024-07-25 Pierluca Carenza , Giuseppe Lucente , Edoardo Vitagliano

We present a brief overview of the ongoing searches for the axion particle via its coupling to photons. Both the classical QCD axions and more recently proposed Axion-Like-Particles are considered. Astrophysical bounds on the axion-photon…

高能物理 - 唯象学 · 物理学 2013-09-27 G. Carosi , A. Friedland , M. Giannotti , M. J. Pivovaroff , J. Ruz , J. K. Vogel
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