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Related papers: New Limits on Ultralight Axionlike Dark Matter fro…

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We report new constraints on axion-like particles (ALPs) using data from the NEON experiment, which features a 16.7 kg of NaI(Tl) target located 23.7 meters from a 2.8 GW thermal power nuclear reactor. Analyzing a total exposure of 3063…

The observed properties of stars and especially the neutrino signal of the supernova 1987A provide an upper limit to the axion mass, while the age and expansion rate of the universe provide a lower limit. There remains a "window of…

Astrophysics · Physics 2008-02-03 Georg G. Raffelt

We use our recent electric dipole moment (EDM) measurement data to constrain the possibility that the HfF$^+$ EDM oscillates in time due to interactions with candidate dark matter axion-like particles (ALPs). We employ a Bayesian analysis…

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…

High Energy Physics - Phenomenology · Physics 2007-05-23 Georg G. Raffelt

New light particles produced in supernovae can lead to additional energy loss and a consequent deficit in neutrino production in conflict with the neutrinos observed from Supernova 1987A (SN1987A). Contrary to the majority of previous…

High Energy Physics - Phenomenology · Physics 2021-02-03 Djuna Croon , Gilly Elor , Rebecca K. Leane , Samuel D. McDermott

We revise the bound from the supernova SN1987A on the coupling of ultralight axion-like particles (ALPs) to photons. In a core-collapse supernova, ALPs would be emitted via the Primakoff process, and eventually convert into gamma rays in…

High Energy Astrophysical Phenomena · Physics 2015-02-09 Alexandre Payez , Carmelo Evoli , Tobias Fischer , Maurizio Giannotti , Alessandro Mirizzi , Andreas Ringwald

We use cosmological observations in the post-Planck era to derive limits on thermally produced cosmological axions. In the early universe such axions contribute to the radiation density and later to the hot dark matter fraction. We find an…

Cosmology and Nongalactic Astrophysics · Physics 2015-02-02 Maria Archidiacono , Steen Hannestad , Alessandro Mirizzi , Georg Raffelt , Yvonne Y. Y. Wong

Several laboratory experiments have published limits on axionlike particles (ALPs) with feeble couplings to electrons and masses in the keV-MeV range, under the assumption that such ALPs comprise the dark matter. We note that ALPs decay…

High Energy Physics - Phenomenology · Physics 2022-06-15 Ricardo Z. Ferreira , M. C. David Marsh , Eike Müller

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

We present a novel approach to investigating axions and axion-like particles (ALPs) by studying their potential conversion into X-rays within the Sun's atmospheric magnetic field. Utilizing high-sensitivity data from the Nuclear…

The axion-like particles (ALPs) are very good candidates of the cosmological dark matter, which can exist in many extensions of the standard model (SM). The mass range of the ALPs as the dark matter can extend from a sub-eV scale to almost…

High Energy Physics - Phenomenology · Physics 2018-12-05 Guo-yuan Huang , Newton Nath

We present new constraints on the couplings of axions and more generic axion-like particles using data from the EDELWEISS-II experiment. The EDELWEISS experiment, located at the Underground Laboratory of Modane, primarily aims at the direct…

Experiments aimed at detecting ultralight dark matter typically rely on resonant effects, which are sensitive to the dark matter mass that matches the resonance frequency. In this study, we investigate the nucleon couplings of ultralight…

High Energy Physics - Phenomenology · Physics 2024-07-12 Zitong Xu , Xiaolin Ma , Kai Wei , Yuxuan He , Xing Heng , Xiaofei Huang , Tengyu Ai , Jian Liao , Wei Ji , Jia Liu , Xiao-Ping Wang , Dmitry Budker

We consider the constraints from Supernova 1987A on particles with small couplings to the Standard Model. We discuss a model with a fermion coupled to a dark photon, with various mass relations in the dark sector; millicharged particles;…

High Energy Physics - Phenomenology · Physics 2018-09-18 Jae Hyeok Chang , Rouven Essig , Samuel D. McDermott

A finite axion-nucleon coupling enables the production of axions in stellar environments via the thermal excitation and subsequent de-excitation of the $^{57}$Fe isotope. Given its low-lying excited state at 14.4 keV, $^{57}$Fe can be…

High Energy Physics - Phenomenology · Physics 2026-01-09 Francisco R. Candón , Pablo Casaseca , Maurizio Giannotti , Mathieu Kaltschmidt , Jaime Ruz , Julia K. Vogel

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

We investigate the possible parametric growth of photon amplitudes in a background of axion-like particle (ALP) dark matter. The observed extragalactic background radiation limits the allowed enhancement effect. We derive the resulting…

Cosmology and Nongalactic Astrophysics · Physics 2019-07-11 Günter Sigl , Pranjal Trivedi