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Related papers: Resolution Studies for Axion Searches with CUPID-0

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The Peccei-Quinn mechanism presents a neat solution to the strong CP problem. As a by-product, it provides an ideal dark matter candidate, "the axion", albeit with a tiny mass. Axions therefore can act as dark radiation if excited with…

High Energy Physics - Phenomenology · Physics 2016-09-28 Anupam Mazumdar , Saleh Qutub , Ken'ichi Saikawa

The absence of definitive results for WIMP dark matter has sparked growing interest in alternative dark matter candidates, such as axions and Axion-Like Particles (ALPs), which also provide insight into the strong CP problem. The Mitchell…

The Cryogenic Dark Matter Search experiment uses low-temperature solid-state detectors to seek Weakly Interacting Massive Particles (WIMPs) and has the world's best exclusion limit on the spin-independent WIMP-nucleon cross section. The…

High Energy Physics - Experiment · Physics 2019-08-13 Oleg Kamaev

A new method for searching for Dark Matter axions is proposed. It is shown that a two-contact SQUID can detect oscillating magnetic perturbations induced by the axions in a strong inhomogeneous magnetic field. A resonant signal is a…

High Energy Physics - Phenomenology · Physics 2016-05-30 Vladimir Popov

Two of the most pressing questions in physics are the microscopic nature of the dark matter that comprises 84% of the mass in the universe and the absence of a neutron electric dipole moment. These questions would be resolved by the…

An appealing candidate of the galactic dark matter is the axion, which was postulated to solve the strong CP (Charge-conjugation Parity) violation problem in the standard particle theory. A new experimental method is proposed to determine…

High Energy Physics - Phenomenology · Physics 2018-06-18 M. Yoshimura , N. Sasao

IAXO, the new International AXion Observatory, will feature the most ambitious detector for solar axions to date. Axions are hypothetical particles which were postulated to solve one of the puzzles arising in the standard model of particle…

Instrumentation and Detectors · Physics 2016-11-18 I. Shilon , A. Dudarev , H. Silva , U. Wagner , H. H. J. ten Kate

We have performed a high resolution search for galactic halo axions in cold flows using a microwave cavity detector. The analysis procedure and other details of this search are described. No axion signal was found in the mass range…

The Cryogenic Underground Observatory for Rare Events (CUORE) is a detector array comprised by 988 5$\;$cm$\times$5$\;$cm$\times$5$\;$cm TeO$_2$ crystals held below 20 mK, primarily searching for neutrinoless double-beta decay in…

High Energy Physics - Experiment · Physics 2024-06-19 CUORE Collaboration , D. Q. Adams , C. Alduino , K. Alfonso , F. T. Avignone , O. Azzolini , G. Bari , F. Bellini , G. Benato , M. Beretta , M. Biassoni , A. Branca , C. Brofferio , C. Bucci , J. Camilleri , A. Caminata , A. Campani , J. Cao , S. Capelli , C. Capelli , L. Cappelli , L. Cardani , P. Carniti , N. Casali , E. Celi , D. Chiesa , M. Clemenza , S. Copello , O. Cremonesi , R. J. Creswick , A. D'Addabbo , I. Dafinei , F. Del Corso , S. Dell'Oro , S. Di Domizio , S. Di Lorenzo , T. Dixon , V. Dompè , D. Q. Fang , G. Fantini , M. Faverzani , E. Ferri , F. Ferroni , E. Fiorini , M. A. Franceschi , S. J. Freedman , S. H. Fu , B. K. Fujikawa , S. Ghislandi , A. Giachero , M. Girola , L. Gironi , A. Giuliani , P. Gorla , C. Gotti , P. V. Guillaumon , T. D. Gutierrez , K. Han , E. V. Hansen , K. M. Heeger , D. L. Helis , H. Z. Huang , G. Keppel , Yu. G. Kolomensky , R. Kowalski , R. Liu , L. Ma , Y. G. Ma , L. Marini , R. H. Maruyama , D. Mayer , Y. Mei , M. N. Moore , T. Napolitano , M. Nastasi , C. Nones , E. B. Norman , A. Nucciotti , I. Nutini , T. O'Donnell , M. Olmi , B. T. Oregui , J. L. Ouellet , S. Pagan , C. E. Pagliarone , L. Pagnanini , M. Pallavicini , L. Pattavina , M. Pavan , G. Pessina , V. Pettinacci , C. Pira , S. Pirro , E. G. Pottebaum , S. Pozzi , E. Previtali , A. Puiu , S. Quitadamo , A. Ressa , C. Rosenfeld , B. Schmidt , V. Sharma , V. Singh , M. Sisti , D. Speller , P. Stark , P. T. Surukuchi , L. Taffarello , C. Tomei , A. Torres , J. A. Torres , K. J. Vetter , M. Vignati , S. L. Wagaarachchi , B. Welliver , J. Wilson , K. Wilson , L. A. Winslow , S. Zimmermann , S. Zucchelli

We investigate the possibility of detecting 14.4 keV and 9.4 keV solar axions and axion-like particles that could be produced in the M1 nuclear transitions of $^{57}$Fe and $^{83}$Kr, respectively. To do so, we used data from soft X-ray…

High Energy Physics - Phenomenology · Physics 2026-05-26 Tanmoy Kumar , Newton Nath

The companion-axion model introduces a second QCD axion to rescue the Peccei-Quinn solution to the strong-CP problem from the effects of colored gravitational instantons. As in single-axion models, the two axions predicted by the…

High Energy Physics - Phenomenology · Physics 2025-06-18 Zhe Chen , Archil Kobakhidze , Ciaran A. J. O'Hare , Zachary S. C. Picker , Giovanni Pierobon

Existence of dark matter indicates the presence of unknown fundamental laws of nature. Ultralight axion-like particles are well-motivated dark matter candidates, emerging naturally from theories of physics at ultrahigh energies. We report…

High Energy Physics - Experiment · Physics 2021-01-11 Alexander V. Gramolin , Deniz Aybas , Dorian Johnson , Janos Adam , Alexander O. Sushkov

In dark matter axion searches, quantum uncertainty manifests as a fundamental noise source, limiting the measurement of the quadrature observables used for detection. We use vacuum squeezing to circumvent the quantum limit in a search for a…

We have searched for solar axions with a detector which consists of a 4T x 2.3m superconducting magnet, PIN-photodiode X-ray detectors, and an altazimuth mount to track the sun. The conversion region is filled with cold helium gas which…

Astrophysics · Physics 2011-04-11 Y. Inoue , M. Minowa , Y. Akimoto , R. Ota , T. Mizumoto , A. Yamamoto

There are a number of observational hints from astrophysics which point to the existence of stellar energy losses beyond the ones accounted for by neutrino emission. These excessive energy losses may be explained by the existence of a new…

High Energy Physics - Phenomenology · Physics 2017-10-18 Maurizio Giannotti , Igor G. Irastorza , Javier Redondo , Andreas Ringwald , Ken'ichi Saikawa

Although the standard {\Lambda}CDM model describes the cosmic microwave background radiation and the large scale structure of the Universe with great success, it has some tensions with observations in the effective number of neutrino…

High Energy Physics - Phenomenology · Physics 2012-11-26 Kiwoon Choi , Ki-Young Choi , Chang Sub Shin

A small, natural abundance, germanium detector (COSME) has been operating recently at the Canfranc Underground Laboratory (Spanish Pyrenees) in improved conditions of shielding and overburden with respect to a previous operation of the same…

CUPID, the CUORE Upgrade with Particle IDentification, is a next-generation experiment to search for neutrinoless double beta decay ($0\nu\beta\beta$) and other rare events using enriched Li$_2$$^{100}$MoO$_4$ scintillating bolometers. It…

Instrumentation and Detectors · Physics 2025-07-14 The CUPID Collaboration , K. Alfonso , A. Armatol , C. Augier , F. T. Avignone , O. Azzolini , A. S. Barabash , G. Bari , A. Barresi , D. Baudin , F. Bellini , G. Benato , L. Benussi , V. Berest , M. Beretta , L. Bergé , M. Bettelli , M. Biassoni , J. Billard , F. Boffelli , V. Boldrini , E. D. Brandani , C. Brofferio , C. Bucci , M. Buchynska , J. Camilleri , A. Campani , J. Cao , C. Capelli , S. Capelli , V. Caracciolo , L. Cardani , P. Carniti , N. Casali , E. Celi , C. Chang , M. Chapellier , H. Chen , D. Chiesa , D. Cintas , M. Clemenza , I. Colantoni , S. Copello , O. Cremonesi , R. J. Creswick , A. D'Addabbo , I. Dafinei , F. A. Danevich , F. De Dominicis , M. De Jesus , P. de Marcillac , S. Dell'Oro , S. Di Domizio , S. Di Lorenzo , T. Dixon , A. Drobizhev , L. Dumoulin , M. El Idrissi , M. Faverzani , E. Ferri , F. Ferri , F. Ferroni , E. Figueroa-Feliciano , J. Formaggio , A. Franceschi , S. Fu , B. K. Fujikawa , J. Gascon , S. Ghislandi , A. Giachero , M. Girola , L. Gironi , A. Giuliani , P. Gorla , C. Gotti , C. Grant , P. Gras , P. V. Guillaumon , T. D. Gutierrez , K. Han , E. V. Hansen , K. M. Heeger , D. L. Helis , H. Z. Huang , M. T. Hurst , L. Imbert , A. Juillard , G. Karapetrov , G. Keppel , H. Khalife , V. V. Kobychev , Yu. G. Kolomensky , R. Kowalski , H. Lattaud , M. Lefevre , M. Lisovenko , R. Liu , Y. Liu , P. Loaiza , L. Ma , F. Mancarella , N. Manenti , A. Mariani , L. Marini , S. Marnieros , M. Martinez , R. H. Maruyama , Ph. Mas , D. Mayer , G. Mazzitelli , E. Mazzola , Y. Mei , M. N. Moore , S. Morganti , T. Napolitano , M. Nastasi , J. Nikkel , C. Nones , E. B. Norman , V. Novosad , I. Nutini , T. O'Donnell , E. Olivieri , M. Olmi , B. T. Oregui , S. Pagan , M. Pageot , L. Pagnanini , D. Pasciuto , L. Pattavina , M. Pavan , Ö. Penek , H. Peng , G. Pessina , V. Pettinacci , C. Pira , S. Pirro , O. Pochon , D. V. Poda , T. Polakovic , O. G. Polischuk , E. G. Pottebaum , S. Pozzi , E. Previtali , A. Puiu , S. Puranam , S. Quitadamo , A. Rappoldi , G. L. Raselli , A. Ressa , R. Rizzoli , C. Rosenfeld , P. Rosier , M. Rossella , J. A. Scarpaci , B. Schmidt , R. Serino , A. Shaikina , K. Shang , V. Sharma , V. N. Shlegel , V. Singh , M. Sisti , P. Slocum , D. Speller , P. T. Surukuchi , L. Taffarello , S. Tomassini , C. Tomei , A. Torres , J. A. Torres , D. Tozzi , V. I. Tretyak , D. Trotta , M. Velazquez , K. J. Vetter , S. L. Wagaarachchi , G. Wang , L. Wang , R. Wang , B. Welliver , J. Wilson , K. Wilson , L. A. Winslow , F. Xie , M. Xue , J. Yang , V. Yefremenko , V. I. Umatov , M. M. Zarytskyy , T. Zhu , A. Zolotarova , S. Zucchelli

The QCD axion stands as one of the most promising candidates for resolving the strong CP problem. However, the value of the axion's decay constant $f_a$ and, by extension, its mass $m_a$, remain uncertain within the framework of effective…

High Energy Physics - Phenomenology · Physics 2024-11-01 Qiaoli Yang , Runchao Huang

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