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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

Orbiting $\gamma$-detectors combined with the magnetic field of the Earth or the Sun can work parasitically as cosmic axion telescopes. The relatively short field lengths allow the axion-to-photon conversion to be coherent for $m_{axion}…

天体物理学 · 物理学 2009-10-30 K. Zioutas , D. J. Thompson , E. A. Paschos

We have searched for axions which could be produced in the solar core by exploiting their conversion to X rays in a strong laboratory magnetic field. The signature of the solar axion is an increase in the rate of the X rays detected in a…

高能物理 - 实验 · 物理学 2008-11-26 Shigetaka Moriyama , Makoto Minowa , Toshio Namba , Yoshizumi Inoue , Yuko Takasu , Akira Yamamoto

A search for solar axions and axion-like particles produced in the $p+d\rightarrow\rm{^3He}+A~(5.5\rm{ ~MeV})$ reaction was performed using the complete dataset of the Borexino detector (3995 days of measurement live-time). The following…

高能物理 - 实验 · 物理学 2025-10-23 Borexino Collaboration

A search for 5.5-MeV solar axions produced in the $p+d\rightarrow\rm{^3He}+A (5.5 \rm{MeV})$ reaction was performed using the Borexino detector. The Compton conversion of axions to photons, ${\rm A}+e\rightarrow e+\gamma$; the axio-electric…

高能物理 - 实验 · 物理学 2012-08-27 The Borexino Collaboration

Axion-like particles (ALPs) are hypothetical bosons which may couple with photons. Since many ALPs can be emitted from hot and dense astrophysical plasma, nearby supernovae (SNe) are a possible probe into their properties including the ALP…

高能物理 - 唯象学 · 物理学 2021-08-18 Kanji Mori

We show that solar axion conversion to photons in the Earth's magnetosphere can produce an x-ray flux, with average energy \sim 4 keV, which is measurable on the dark side of the Earth. The smallness of the Earth's magnetic field is…

高能物理 - 唯象学 · 物理学 2009-11-11 Hooman Davoudiasl , Patrick Huber

The hot interiors of massive stars in the later stages of their evolution provide an ideal place for the production of heavy axion-like particles (ALPs) with mass up to O(100 keV) range. We show that a fraction of these ALPs could stream…

高能物理 - 唯象学 · 物理学 2024-12-31 James H. Buckley , P. S. Bhupal Dev , Francesc Ferrer , Takuya Okawa

We present a search for the direct production of a light pseudoscalar $a$ decaying into two photons with the Belle II detector at the SuperKEKB collider. We search for the process ${e^+e^-\to\gamma a, a \to\gamma\gamma}$ in the mass range…

高能物理 - 实验 · 物理学 2020-10-21 Belle II collaboration , F. Abudinen , I. Adachi , H. Aihara , N. Akopov , A. Aloisio , F. Ameli , N. Anh Ky , D. M. Asner , T. Aushev , V. Aushev , V. Babu , S. Baehr , S. Bahinipati , P. Bambade , Sw. Banerjee , S. Bansal , J. Baudot , J. Becker , P. K. Behera , J. V. Bennett , E. Bernieri , F. U. Bernlochner , M. Bertemes , M. Bessner , S. Bettarini , V. Bhardwaj , F. Bianchi , T. Bilka , S. Bilokin , D. Biswas , M. Bračko , P. Branchini , N. Braun , T. E. Browder , A. Budano , S. Bussino , M. Campajola , G. Casarosa , C. Cecchi , D. Červenkov , M. -C. Chang , P. Chang , R. Cheaib , V. Chekelian , B. G. Cheon , K. Chilikin , K. Chirapatpimol , H. -E. Cho , K. Cho , S. -J. Cho , S. -K. Choi , D. Cinabro , L. Corona , L. M. Cremaldi , S. Cunliffe , N. Dash , F. Dattola , E. De La Cruz-Burelo , G. De Nardo , M. De Nuccio , G. De Pietro , R. de Sangro , M. Destefanis , A. De Yta-Hernandez , F. Di Capua , Z. Doležal , T. V. Dong , K. Dort , D. Dossett , G. Dujany , S. Eidelman , T. Ferber , D. Ferlewicz , S. Fiore , A. Fodor , F. Forti , B. G. Fulsom , E. Ganiev , R. Garg , A. Garmash , V. Gaur , A. Gaz , U. Gebauer , A. Gellrich , T. Geßler , R. Giordano , A. Giri , B. Gobbo , R. Godang , P. Goldenzweig , B. Golob , P. Gomis , W. Gradl , E. Graziani , D. Greenwald , C. Hadjivasiliou , S. Halder , O. Hartbrich , K. Hayasaka , H. Hayashii , C. Hearty , M. T. Hedges , I. Heredia de la Cruz , M. Hernández Villanueva , A. Hershenhorn , T. Higuchi , E. C. Hill , H. Hirata , M. Hoek , M. Hohmann , C. -L. Hsu , Y. Hu , K. Inami , G. Inguglia , J. Irakkathil Jabbar , A. Ishikawa , R. Itoh , P. Jackson , W. W. Jacobs , D. E. Jaffe , E. -J. Jang , S. Jia , Y. Jin , C. Joo , A. B. Kaliyar , J. Kandra , G. Karyan , Y. Kato , H. Kichimi , C. Kiesling , C. -H. Kim , D. Y. Kim , H. J. Kim , S. -H. Kim , Y. -K. Kim , T. D. Kimmel , K. Kinoshita , C. Kleinwort , P. Kodyš , T. Koga , S. Kohani , I. Komarov , S. Korpar , T. M. G. Kraetzschmar , P. Križan , P. Krokovny , T. Kuhr , M. Kumar , R. Kumar , K. Kumara , S. Kurz , Y. -J. Kwon , S. Lacaprara , C. La Licata , L. Lanceri , J. S. Lange , I. -S. Lee , S. C. Lee , P. Leitl , D. Levit , P. M. Lewis , C. Li , L. K. Li , Y. B. Li , J. Libby , K. Lieret , L. Li Gioi , Z. Liptak , Q. Y. Liu , D. Liventsev , S. Longo , T. Luo , C. MacQueen , Y. Maeda , R. Manfredi , E. Manoni , S. Marcello , C. Marinas , A. Martini , M. Masuda , K. Matsuoka , D. Matvienko , F. Meggendorfer , F. Meier , M. Merola , F. Metzner , M. Milesi , C. Miller , K. Miyabayashi , R. Mizuk , K. Azmi , G. B. Mohanty , H. -G. Moser , M. Mrvar , F. J. Müller , R. Mussa , I. Nakamura , M. Nakao , H. Nakazawa , A. Natochii , C. Niebuhr , N. K. Nisar , S. Nishida , M. H. A. Nouxman , K. Ogawa , S. Ogawa , H. Ono , P. Oskin , H. Ozaki , P. Pakhlov , A. Paladino , A. Panta , E. Paoloni , S. Pardi , H. Park , S. -H. Park , B. Paschen , A. Passeri , A. Pathak , S. Patra , S. Paul , T. K. Pedlar , I. Peruzzi , R. Peschke , M. Piccolo , L. E. Piilonen , G. Polat , V. Popov , C. Praz , E. Prencipe , M. T. Prim , M. V. Purohit , N. Rad , P. Rados , R. Rasheed , M. Reif , S. Reiter , M. Remnev , I. Ripp-Baudot , M. Ritter , M. Ritzert , G. Rizzo , S. H. Robertson , D. Rodríguez Pérez , J. M. Roney , C. Rosenfeld , A. Rostomyan , N. Rout , D. Sahoo , Y. Sakai , D. A. Sanders , S. Sandilya , A. Sangal , L. Santelj , Y. Sato , V. Savinov , B. Scavino , C. Schwanda , A. J. Schwartz , R. M. Seddon , Y. Seino , A. Selce , K. Senyo , J. Serrano , M. E. Sevior , C. Sfienti , J. -G. Shiu , A. Sibidanov , F. Simon , R. J. Sobie , A. Soffer , E. Solovieva , S. Spataro , B. Spruck , M. Starič , S. Stefkova , Z. S. Stottler , R. Stroili , J. Strube , M. Sumihama , T. Sumiyoshi , D. J. Summers , W. Sutcliffe , H. Svidras , M. Tabata , M. Takizawa , U. Tamponi , S. Tanaka , K. Tanida , H. Tanigawa , P. Taras , F. Tenchini , D. Tonelli , E. Torassa , K. Trabelsi , M. Uchida , T. Uglov , K. Unger , Y. Unno , S. Uno , P. Urquijo , Y. Ushiroda , S. E. Vahsen , R. van Tonder , G. S. Varner , K. E. Varvell , A. Vinokurova , L. Vitale , E. Waheed , M. Wakai , H. M. Wakeling , C. H. Wang , M. -Z. Wang , X. L. Wang , A. Warburton , M. Watanabe , S. Watanuki , J. Webb , S. Wehle , M. Welsch , C. Wessel , J. Wiechczynski , H. Windel , E. Won , L. J. Wu , X. P. Xu , B. Yabsley , W. Yan , S. B. Yang , H. Ye , M. Yonenaga , C. Z. Yuan , Y. Yusa , L. Zani , Q. D. Zhou , V. I. Zhukova

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

Axions are expected to be produced in the sun via the Primakoff process. They may be detected through the inverse process in the laboratory, under the influence of a strong magnetic field, giving rise to X-rays of energies in the range of a…

高能物理 - 实验 · 物理学 2009-01-06 Christos Eleftheriadis

Dark matter may be charged under dark electromagnetism with a dark photon that kinetically mixes with the Standard Model photon. In this framework, dark matter will collect at the center of the Earth and annihilate into dark photons, which…

高能物理 - 唯象学 · 物理学 2017-10-05 Jonathan L. Feng , Jordan Smolinsky , Philip Tanedo

Dark matter may interact with the Standard Model through the kinetic mixing of dark photons, $A'$, with Standard Model photons. Such dark matter will accumulate in the Sun and annihilate into dark photons. The dark photons may then leave…

高能物理 - 唯象学 · 物理学 2017-10-05 Jonathan L. Feng , Jordan Smolinsky , Philip Tanedo

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 a search for axion-like particles, $a$, produced in photon-proton collisions at a center-of-mass energy of approximately 4 GeV, focusing on the scenario where the $a$-gluon coupling is dominant. The search uses $a\to\gamma\gamma$…

高能物理 - 实验 · 物理学 2022-03-28 GlueX Collaboration , S. Adhikari , C. S. Akondi , M. Albrecht , A. Ali , M. Amaryan , A. Asaturyan , A. Austregesilo , Z. Baldwin , F. Barbosa , J. Barlow , E. Barriga , R. Barsotti , T. D. Beattie , V. V. Berdnikov , T. Black , W. Boeglin , W. J. Briscoe , T. Britton , W. K. Brooks , E. Chudakov , S. Cole , P. L. Cole , O. Cortes , V. Crede , M. M. Dalton , A. Deur , S. Dobbs , A. Dolgolenko , R. Dotel , M. Dugger , R. Dzhygadlo , D. Ebersole , H. Egiyan , T. Erbora , A. Ernst , P. Eugenio , C. Fanelli , S. Fegan , J. Fitches , A. M. Foda , S. Furletov , L. Gan , H. Gao , A. Gasparian , C. Gleason , K. Goetzen , V. S. Goryachev , L. Guo , M. Hagen , H. Hakobyan , A. Hamdi , J. Hernandez , N. D. Hoffman , G. Hou , G. M. Huber , A. Hurley , D. G. Ireland , M. M. Ito , I. Jaegle , N. S. Jarvis , R. T. Jones , V. Kakoyan , G. Kalicy , M. Kamel , V. Khachatryan , M. Khatchatryan , C. Kourkoumelis , S. Kuleshov , A. LaDuke , I. Larin , D. Lawrence , D. I. Lersch , H. Li , W. B. Li , B. Liu , K. Livingston , G. J. Lolos , L. Lorenti , K. Luckas , V. Lyubovitskij , D. Mack , A. Mahmood , H. Marukyan , V. Matveev , M. McCaughan , M. McCracken , C. A. Meyer , R. Miskimen , R. E. Mitchell , K. Mizutani , V. Neelamana , F. Nerling , L. Ng , A. I. Ostrovidov , Z. Papandreou , C. Paudel , P. Pauli , R. Pedroni , L. Pentchev , K. J. Peters , J. Reinhold , B. G. Ritchie , J. Ritman , G. Rodriguez , D. Romanov , C. Romero , K. Saldana , C. Salgado , S. Schadmand , A. M. Schertz , A. Schick , A. Schmidt , R. A. Schumacher , J. Schwiening , P. Sharp , X. Shen , M. R. Shepherd , A. Smith , E. S. Smith , D. I. Sober , A. Somov , S. Somov , O. Soto , J. R. Stevens , I. I. Strakovsky , B. Sumner , K. Suresh , V. V. Tarasov , S. Taylor , A. Teymurazyan , A. Thiel , G. Vasileiadis , T. Viducic , T. Whitlatch , N. Wickramaarachchi , M. Williams , Y. Yang , S. Yoon , J. Zarling , Z. Zhang , Z. Zhao , J. Zhou , X. Zhou , B. Zihlmann

The purpose of this paper is to assess the feasibility of axion detection by X-ray spectroscopy of the sun. We review the theory of axion-photon mode conversion with special attention to axions emitted in the 14.4 keV M1 decay of 57Fe at…

太阳与恒星天体物理 · 物理学 2015-06-15 J. Martin Laming

New feebly interacting particles would emerge from a supernova core with 100-MeV-range energies and produce $\gamma$-rays by subsequent decays. These would contribute to the diffuse cosmic $\gamma$-ray background or would have shown up in…

高能物理 - 唯象学 · 物理学 2023-07-17 Melissa Diamond , Damiano F. G. Fiorillo , Gustavo Marques-Tavares , Edoardo Vitagliano

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

The CAST (CERN Axion Solar Telescope) experiment at CERN searches for solar axions with energies in the keV range. It is possible that axions are produced in the core of the sun by the interaction of thermal photons with virtual photons of…

高能物理 - 实验 · 物理学 2007-05-23 Donghwa Kang

Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with…

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