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The EDELWEISS experiment primarily aims at the direct detection of WIMPs using germanium bolometers. It is also sensitive to the low-energy electron recoils that would be induced by axions. We present new constraints on the couplings of…

High Energy Physics - Phenomenology · Physics 2019-08-14 Thibault de Boissière

The cores of dense stars are a powerful laboratory for studying feebly coupled particles such as axions. Some of the strongest constraints on axionlike particles and their couplings to ordinary matter derive from considerations of stellar…

High Energy Physics - Phenomenology · Physics 2024-04-30 Hong-Yi Zhang , Ray Hagimoto , Andrew J. Long

The metastable hypermassive neutron star produced in the coalescence of two neutron stars can copiously produce axions that radiatively decay into $\mathcal{O}(100)$~MeV photons. These photons can form a fireball with characteristic…

High Energy Physics - Phenomenology · Physics 2024-03-11 Melissa Diamond , Damiano F. G. Fiorillo , Gustavo Marques-Tavares , Irene Tamborra , Edoardo Vitagliano

Axions or axion-like particles (ALPs) are one of the promising dark matter (DM) candidates. A prevalent method to detect axion-like DM is to seek periodic oscillation in the polarization angles (PAs) of linearly polarized light emitted from…

High Energy Astrophysical Phenomena · Physics 2025-04-03 Bao Wang , Xuan Yang , Jun-Jie Wei , Song-Bo Zhang , Xue-Feng Wu

Axions provide a natural and well-motivated dark matter candidate, with the capability to convert directly to photons in the presence of an electromagnetic field. A particularly compelling observational target is the conversion of dark…

Cosmic Microwave Background (CMB) photons can undergo resonant conversion into axions in the presence of magnetized plasma distributed inside non-linear large-scale structure (LSS). This process leads to axion-induced patchy screening:…

High Energy Physics - Phenomenology · Physics 2024-11-12 Cristina Mondino , Dalila Pîrvu , Junwu Huang , Matthew C. Johnson

We report new searches for the solar axions and galactic axion-like dark matter particles, using the first low-background data from PandaX-II experiment at China Jinping Underground Laboratory, corresponding to a total exposure of about…

We constrain the coupling of thermally-produced axion-like particles (here axions) with photons and gluons, using data from the cosmic microwave background (CMB) spectra and baryon acoustic oscillations. The axion possesses an explicit soft…

Cosmology and Nongalactic Astrophysics · Physics 2022-09-12 Luca Caloni , Martina Gerbino , Massimiliano Lattanzi , Luca Visinelli

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…

High Energy Physics - Phenomenology · Physics 2025-05-30 Elisa Todarello , Marco Regis

We report on the first axion search results from the Cryogenic Dark Matter Search (CDMS) experiment at the Soudan Underground Laboratory. An energy threshold of 2 keV for electron-recoil events allows a search for possible solar axion…

High Energy Physics - Experiment · Physics 2012-08-27 CDMS Collaboration

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…

Astrophysics · Physics 2011-06-07 Y. Inoue , Y. Akimoto , R. Ohta , T. Mizumoto , A. Yamamoto , M. Minowa

Axion-photon mixing has been proposed as an alternative to acceleration as the explanation for supernovae dimming. We point out that the loss of photons due to this mixing will induce a strong asymmetry between the luminosity, d_L(z), and…

Astrophysics · Physics 2009-11-10 Bruce A. Bassett , Martin Kunz

We present a new constraint for the axion monopole-dipole coupling in the range of 1 micrometer to a few millimeters, previously unavailable for experimental study. The constraint was obtained using our recent results on the observation of…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. Baessler , V. V. Nesvizhevsky , K. V. Protasov , A. Yu. Voronin

We present an analysis of electron recoils in cryogenic germanium detectors operated during the SuperCDMS Soudan experiment. The data are used to set new constraints on the axioelectric coupling of axion-like particles and the kinetic…

High Energy Physics - Experiment · Physics 2021-01-20 SuperCDMS Collaboration , T. Aralis , T. Aramaki , I. J. Arnquist , E. Azadbakht , W. Baker , S. Banik , D. Barker , C. Bathurst , D. A. Bauer , L. V. S Bezerra , R. Bhattacharyya , T. Binder , M. A. Bowles , P. L. Brink , R. Bunker , B. Cabrera , R. Calkins , R. A. Cameron , C. Cartaro , D. G. Cerdeño , Y. -Y. Chang , J. Cooley , H. Coombes , J. Corbett , B. Cornell , P. Cushman , F. De Brienne , M. L. di Vacri , M. D. Diamond , E. Fascione , E. Figueroa-Feliciano , C. W. Fink , K. Fouts , M. Fritts , G. Gerbier , R. Germond , M. Ghaith , S. R. Golwala , H. R. Harris , N. Herbert , B. A. Hines , M. I. Hollister , Z. Hong , E. W. Hoppe , L. Hsu , M. E. Huber , V. Iyer , D. Jardin , A. Jastram , M. H. Kelsey , A. Kennedy , A. Kubik , N. A. Kurinsky , R. E. Lawrence , A. Li , B. Loer , E. Lopez Asamar , P. Lukens , D. MacDonell , D. B. MacFarlane , R. Mahapatra , V. Mandic , N. Mast , É. M. Michaud , E. Michielin , N. Mirabolfathi , B. Mohanty , J. D. Morales Mendoza , S. Nagorny , J. Nelson , H. Neog , J. L. Orrell , S. M. Oser , W. A. Page , P. Pakarha , R. Partridge , R. Podviianiuk , F. Ponce , S. Poudel , M. Pyle , W. Rau , R. Ren , T. Reynolds , A. Roberts , A. E. Robinson , H. E. Rogers , T. Saab , B. Sadoulet , J. Sander , D. Toback , R. Underwood , S. Verma , A. N. Villano , B. von Krosigk , S. L. Watkins , L. Wills , J. S. Wilson , M. J. Wilson , J. Winchell , D. H. Wright , S. Yellin , B. A. Young , T. C. Yu , E. Zhang , X. Zhao , L. Zheng

Cosmological structure formation simulations of ultralight axion-like dark matter have shown that an axion star forms at the center of every dark matter halo in the Universe. These axion stars would then form in large numbers during the…

High Energy Physics - Phenomenology · Physics 2024-02-12 Miguel Escudero

Axions are possible candidates of dark matter in the present Universe. They have been argued to form axionic boson stars with small masses $\sim 10^{-12}M_{\odot}$. Since they possess oscillating electric fields in a magnetic field, they…

High Energy Physics - Phenomenology · Physics 2014-11-17 Aiichi Iwazaki

We report on new results of a search for two-photon interaction with axionlike particles (ALPs). The experiment was carried out at a synchrotron radiation facility using a "light shining through a wall (LSW)" technique. For this purpose, we…

High Energy Physics - Experiment · Physics 2017-02-21 T. Inada , T. Yamazaki , T. Namba , S. Asai , T. Kobayashi , K. Tamasaku , Y. Tanaka , Y. Inubushi , K. Sawada , M. Yabashi , T. Ishikawa , A. Matsuo , K. Kawaguchi , K. Kindo , H. Nojiri

Ultralight dark photons and axions are well-motivated hypothetical dark matter candidates. Both dark photon dark matter and axion dark matter can resonantly convert into electromagnetic waves in the solar corona when their mass is equal to…

High Energy Physics - Phenomenology · Physics 2024-02-02 Haipeng An , Xingyao Chen , Shuailiang Ge , Jia Liu , Yan Luo
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