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Dark matter Axion search with riNg Cavity Experiment (DANCE) was proposed. To search for axion-like particles, we aim to detect the rotation and oscillation of optical linear polarization caused by axion-photon coupling with a bow-tie…

High Energy Physics - Phenomenology · Physics 2021-05-18 Yuka Oshima , Hiroki Fujimoto , Masaki Ando , Tomohiro Fujita , Yuta Michimura , Koji Nagano , Ippei Obata , Taihei Watanabe

The scan rate of an axion haloscope is proportional to the square of the cavity volume. In this paper, a new class of thin-shell cavities are proposed to search for axionic dark matter. These cavities feature active volume much larger…

Instrumentation and Detectors · Physics 2020-06-17 Chao-Lin Kuo

We report on the present progress in development of the dark matter axion search experiment with Rydberg-atom-cavity detectors in Kyoto, CARRACK I and CARRACK II. The axion search has been performed with CARRACK I in the 8 % mass range…

High Energy Physics - Phenomenology · Physics 2007-05-23 K. Yamamoto , M. Tada , Y. Kishimoto , M. Shibata , K. Kominato , T. Ooishi , S. Yamada , T. Saida , H. Funahashi , A. Masaike , S. Matsuki

The existence of a secluded gauge sector could explain several puzzling astrophysical observations. This hypothesis can be tested at low energy e+e- colliders such as DAPHNE. Preliminary results obtained with KLOE data and perpectives for…

We review searches for closed string axions and axion-like particles (ALPs) in IIB string flux compactifications. For natural values of the background fluxes and TeV scale gravitino mass, the moduli stabilisation mechanism of the LARGE…

High Energy Physics - Phenomenology · Physics 2017-04-26 Andreas Ringwald

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 $a\to\gamma\gamma$…

High Energy Physics - Experiment · Physics 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

Dark matter is a major constituent of our universe and the axion is a prime candidate. In this article, it is shown that by exploiting the axion induced magnetization in a magnetic rod and the Faraday effect, axions in the mass range $500$…

Cosmology and Nongalactic Astrophysics · Physics 2022-12-06 A. T. M. Anishur Rahman

We propose a search at Mu3e for lepton flavor violating axion(-like) particles in $\mu\to 3e + a$ decays. By requiring an additional $e^+e^-$ pair from internal conversion, one can circumvent the calibration challenges which plague the $\mu…

High Energy Physics - Phenomenology · Physics 2023-11-30 Simon Knapen , Kevin Langhoff , Toby Opferkuch , Diego Redigolo

The proposed LUXE experiment (Laser und XFEL Experiment) at DESY Hamburg, using the electron beam from the European XFEL, aims to probe QED in the non-perturbative regime created in collisions between high-intensity laser pulses and…

High Energy Physics - Experiment · Physics 2022-11-23 Shan Huang

Recently, the laser experiments BMV and GammeV, searching for light shining through walls, have published data and calculated new limits on the allowed masses and couplings for axion-like particles. In this note we point out that these…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Ahlers , H. Gies , J. Jaeckel , J. Redondo , A. Ringwald

The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interactions and also happens to be an excellent dark matter candidate. Axions constituting the dark matter halo of our galaxy may be detected by…

The LUXE experiment aims at studying strong-field QED in electron-laser and photon-laser interactions, with the $16.5$ GeV electron beam of the European XFEL and a laser beam with power of up to $350$ TW. The strong-field QED processes are…

Instrumentation and Detectors · Physics 2022-09-07 K. Fleck

The axion emerges in extensions of the Standard Model that explain the absence of CP violation in the strong interactions. Simultaneously, it can provide naturally the cold dark matter in our universe. Several searches for axions and…

We present a strong lensing system in which a double source is imaged 5 times by 2 early-type galaxies. We take advantage in this target of the multi-band photometry obtained as part of the CLASH program, complemented by the spectroscopic…

We introduce a new experimental method for solar hadronic axions search. It is suggested that these axions are created in the Sun during M1 transition between the first thermally excited level at 9.4 keV and the ground state in $^{83}Kr$.…

Nuclear Experiment · Physics 2009-12-08 K. Jakovcic , Z. Krecak , M. Krcmar , A. Ljubicic

Galaxy clusters contain large magnetic fields that make them excellent targets to search for ultralight Axion-Like Particles (ALPs). ALP-photon interconversion imprints quasi-sinusoidal oscillations on the X-ray spectra of point sources in…

High Energy Astrophysical Phenomena · Physics 2017-11-08 Nicholas Jennings

SLIM is a large area experiment (440 m2) installed at the Chacaltaya cosmic ray laboratory since 2001, and about 100 m2 at Koksil, Himalaya, since 2003. It is devoted to the search for intermediate mass magnetic monopoles (107-1013 GeV/c2)…