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Related papers: Exploring 0.1-10$\,$eV axions with a new helioscop…

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Dark matter lighter than 10 GeV/c$^2$ encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a…

Instrumentation and Detectors · Physics 2023-06-21 P. Agnes , I. Ahmad , S. Albergo , I. F. M. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Atzori Corona , D. J. Auty , M. Ave , I. Ch. Avetisov , R. I. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , V. Barbarian , A. Barrado Olmedo , P. Barrillon , A. Basco , G. Batignani , E. Berzin , A. Bondar , W. M. Bonivento , E. Borisova , B. Bottino , M. G. Boulay , G. Buccino , S. Bussino , J. Busto , A. Buzulutskov , M. Cadeddu , M. Cadoni , A. Caminata , N. Canci , A. Capra , S. Caprioli , M. Caravati , M. Cárdenas-Montes , N. Cargioli , M. Carlini , P. Castello , V. Cataudella , P. Cavalcante , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , S. Chashin , A. Chepurnov , E Chyhyrynets , C. Cicalò , L. Cifarelli , D. Cintas , V. Cocco , E. Conde Vilda , L. Consiglio , S. Copello , G. Covone , S. Cross , P. Czudak , M. D'Aniello , S. D'Auria , M. D. Da Rocha Rolo , O. Dadoun , M. Daniel , S. Davini , A. De Candia , S. De Cecco , A. De Falco , G. De Filippis , D. De Gruttola , S. De Pasquale , G. De Rosa , G. Dellacasa , A. V. Derbin , A. Devoto , F. Di Capua , L. Di Noto , P. Di Stefano , C. Dionisi , G. Dolganov , F. Dordei , L. Doria , T. Erjavec , M. Fernandez Diaz , G. Fiorillo , A. Franceschi , P. Franchini , D. Franco , E. Frolov , N. Funicello , F. Gabriele , D. Gahan , C. Galbiati , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gendotti , C. Ghiano , R. A. Giampaolo , C. Giganti , M. A. Giorgi , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , D. Gorman , R. Graciani Diaz , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guan , M. Guerzoni , M. Gulino , C. Guo , B. R. Hackett , J. B. Hall , A. L. Hallin , A. Hamer , H. Helton , M. Haranczyk , T. Hessel , S. Hill , S. Horikawa , F. Hubaut , T. Hugues , E. V. Hungerford , An. Ianni , V. Ippolito , C. Jillings , P. Kachru , A. A. Kemp , C. L. Kendziora , G. Keppel , A. V. Khomyakov , M. Kimura , I. Kochanek , K. Kondo , G. Korga , S. Koulosousas , A. Kubankin , M. Kuss , M. Kuźniak , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , X. Li , L. Lidey , J. Lipp , M. Lissia , G. Longo , L. Luzzi , O. Macfadyen , I. N. Machulin , I. Manthos , L. Mapelli , A. Margotti , S. M. Mari , C. Mariani , J. Maricic , A. Marini , M. Martínez , C. J. Martoff , A. Masoni , K. Mavrokoridis , A. Mazzi , A. B. McDonald , A. Messina , R. Milincic , A. Moggi , A. Moharana , J. Monroe , M. Morrocchi , E. N. Mozhevitina , T. Mróz , V. N. Muratova , C. Muscas , P. Musico , R. Nania , T. Napolitano , M. Nessi , G. Nieradka , K. Nikolopoulos , I. Nikulin , J. Nowak , K. Olchansky , A. Oleinik , V. Oleynikov , P. Organtini , A. Ortiz de Solórzano , L. Pagani , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , G. Paternoster , P. A. Pegoraro , K. Pelczar , C. Pellegrino , F. Perotti , V. Pesudo , S. Piacentini , F. Pietropaolo , N. Pino , C. Pira , A. Pocar , D. M. Poehlmann , S. Pordes , P. Pralavorio , D. Price , F. Raffaelli , F. Ragusa , Y. Ramachers , A. Ramirez , M. Razeti , A. Razeto , A. L. Renshaw , M. Rescigno , F. Resnati , F. Retiere , L. P. Rignanese , C. Ripoli , A. Rivetti , A. Roberts , C. Roberts , J. Rode , G. Rogers , L. Romero , M. Rossi , A. Rubbia , S. Sadashivajois , T. R. Saffold , O. Samoylov , E. Sandford , S. Sanfilippo , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , G. Scioli , D. A. Semenov , A. Shchagin , A. Sheshukov , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , A. Sokolov , M. Spangenberg , R. Stefanizzi , A. Steri , S. Stracka , V. Strickland , M. Stringer , S. Sulis , A. Sung , Y. Suvorov , A. M. Szelc , C. Türkoğ , R. Tartaglia , A. Taylor , J. Taylor , S. Tedesco , G. Testera , K. Thieme , T. N. Thorpe , A. Tonazzo , S. Torres-Lara , A. Tricomi , E. V. Unzhakov , T. Vallivilayil John , M. Van Uffelen , T. Viant , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , M. Wada , M. B. Walczak , Y. Wang , S. Westerdale , R. J. Wheadon , L. Williams , I. Wingerter-Seez , R. Wojaczyński , Ma. M. Wojcik , Ma. Wojcik , T. Wright , Y. Xie , C. Yang , A. Zabihi , P. Zakhary , A. Zani , A. Zichichi , G. Zuzel , M. P. Zykova

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…

High Energy Physics - Experiment · Physics 2007-05-23 Donghwa Kang

The axion is a hypothetical particle proposed to solve the strong $CP$ problem, and also a candidate for dark matter. This non-relativistic particle in the galactic halo can be converted into a photon under a strong magnetic field and…

High Energy Physics - Experiment · Physics 2019-10-15 Soohyung Lee , Saebyeok Ahn , Jihoon Choi , Byeong Rok Ko , Yannis K. Semertzidis

Discovering the microscopic composition of dark matter is one of the most important open problems in physics today. Axions are a leading candidate to be dark matter; however, a search of the full range of all likely axion masses is hampered…

The mass of axion dark matter is only weakly bounded by cosmological observations, necessitating a variety of detection techniques over several orders of magnitude of mass ranges. Axions haloscopes based on resonant cavities have become the…

Instrumentation and Detectors · Physics 2018-10-29 Ben T. McAllister , Maxim Goryachev , Jeremy Bourhill , Eugene N. Ivanov , Michael E. Tobar

Axions, originally proposed to solve the strong CP problem of quantum chromodynamics, emerge now as leading candidates of WISP dark matter. The rich phenomenology associated to the light and stable QCD axion can be described as an effective…

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…

We report on an interesting realization of the QCD axion, with mass in the range $\mathcal{O}(10)$ MeV. It has previously been shown that although this scenario is stringently constrained from multiple sources, the model remains viable for…

High Energy Physics - Phenomenology · Physics 2021-05-18 Jia Liu , Navin McGinnis , Carlos E. M. Wagner , Xiao-Ping Wang

We present the prospects for detection of KK-axions using a large volume spherical TPC through natural decay to two gammas. The higher excited mass states of this axion model allows to reach densities which could be detectable by this…

Instrumentation and Methods for Astrophysics · Physics 2013-10-16 Javier Galan , Gilles Gerbier , Ioannis Giomataris , Thomas Papaevangelou , Ilias Savvidis

The axion is a compelling hypothetical particle that could account for the dark matter in our universe, while simultaneously explaining why quark interactions within the neutron do not appear to give rise to an electric dipole moment. The…

High Energy Physics - Experiment · Physics 2025-12-11 Andrew Engel , Thomas Braine , Christian Boutan

This paper reports on a cavity haloscope search for dark matter axions in the galactic halo in the mass range $2.81$-$3.31$ ${\mu}eV$. This search excludes the full range of axion-photon coupling values predicted in benchmark models of the…

We show that Earth's natural environment can serve as a powerful probe for ultralight axion dark matter. In the presence of global geomagnetic fields, the axions with masses ranging from $10^{-15}\,{\rm eV}-10^{-13}\,{\rm eV}$ induce…

High Energy Physics - Phenomenology · Physics 2025-09-19 Atsushi Taruya , Atsushi Nishizawa , Yoshiaki Himemoto

The axion was first introduced as a consequence of the Peccei-Quinn mechanism to solve the CP problem in strong interactions of particle physics and is a well motivated cold dark matter candidate. This particle is expected to interact…

Instrumentation and Detectors · Physics 2020-12-08 S. W. Youn , E. Sala , J. Jeong , J. Kim , Y. K. Semertzidis

Axions are a popular dark matter candidate which are often searched for in experiments known as ``haloscopes" which exploit a putative axion-photon coupling. These experiments typically rely on Transverse Magnetic (TM) modes in resonant…

Instrumentation and Detectors · Physics 2020-11-10 Aaron P. Quiskamp , Ben T. McAllister , Gray Rybka , Michael E. Tobar

A chamber for direct detection of WIMPs with masses < 10 GeV/c2 and solar axions is developed. The chamber is filled with a gas mixture of H2 +3ppm TMAE (1,5,10 bar), or D2 + 3ppm TMAE. These gas fillings make it possible to suppress an…

Instrumentation and Detectors · Physics 2016-03-21 B. M. Ovchinnikov , V. V. Parusov

The natural environment of the Earth can act as a sensitive detector for dark matter in ultralight axions. When axions with masses between $1\times10^{-15}\,{\rm eV}$ and $1\times10^{-13}\,{\rm eV}$ pass through the Earth, they interact…

High Energy Physics - Phenomenology · Physics 2025-04-23 Atsushi Nishizawa , Atsushi Taruya , Yoshiaki Himemoto

Axions and axion-like particles are well-motivated dark matter candidates. We propose an experiment that uses single photon detection interferometry to search for axions and axion-like particles in the galactic halo. We show that photon…

Instrumentation and Detectors · Physics 2025-09-23 Haocun Yu , Ohkyung Kwon , Hartmut Grote , Denis Martynov

Detection of axion dark matter heavier than a meV is hindered by its small wavelength, which limits the useful volume of traditional experiments. This problem can be avoided by directly detecting in-medium excitations, whose $\sim…

High Energy Physics - Phenomenology · Physics 2025-04-18 Asher Berlin , Tanner Trickle
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