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We constrain the coupling between axionlike particles (ALPs) and photons, measured with the superconducting resonant detection circuit of a cryogenic Penning trap. By searching the noise spectrum of our fixed-frequency resonant circuit for…

We propose a novel telescope concept based on Earth's gravitational lensing effect, optimized for the detection of distant dark matter sources, particularly axion-like particles (ALPs). When a unidirectional flux of dark matter passes…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-03 Taiyo Nakamura , Kensuke Homma

A consistent treatment of the quantum field theory of an axion-like particle (ALP) interacting with Standard Model fields requires to account for renormalisation group running and matching to the low-energy theory. Quantum sensor…

High Energy Physics - Phenomenology · Physics 2025-05-15 Martin Bauer , Sreemanti Chakraborti , Guillaume Rostagni

The axion is a hypothetical particle considered to be the most economical solution to the strong CP problem. It can also be formulated as a compelling component of dark matter. The haloscope, a leading axion detection scheme, relies on the…

Instrumentation and Detectors · Physics 2016-08-17 Ben T. McAllister , Stephen R. Parker , Michael E. Tobar

One kind of particularly interesting pseudoscalar particles, called axion-like particles (ALPs), have rich physical phenomenology at high- and low-energy collider experiments. After discussing most of single production channels of ALP at…

High Energy Physics - Phenomenology · Physics 2022-01-25 Chong-Xing Yue , Hua-Ying Zhang , Han Wang

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

The mixing of photons with axion-like particles (ALPs) in the large-scale magnetic field $B$ changes the polarization angle of a linearly polarized photon beam from active galactic nuclei in radio galaxies as it propagates over cosmological…

High Energy Astrophysical Phenomena · Physics 2012-06-13 D. Horns , L. Maccione , A. Mirizzi , M. Roncadelli

We propose an experimental setup to search for Axion-like particles (ALPs) using two superconducting radio-frequency cavities. In this light-shining-through-wall setup the axion is sourced by two modes with large fields and nonzero $\vec…

High Energy Physics - Phenomenology · Physics 2022-03-09 Christina Gao , Roni Harnik

The Center for Axion and Precision Physics Research (CAPP) was founded in 2013, with the ambition of shedding light on the strong CP problem and the proposed existence of axions. Much of CAPP's effort focuses on the direct detection of dark…

Instrumentation and Detectors · Physics 2018-02-14 Eleni Petrakou

Axion-like particles (ALPs) are pseudo Nambu-Goldstone bosons of spontaneously broken global symmetries in high-energy extensions of the Standard Model (SM). This makes them a prime target for future experiments aiming to discover new…

High Energy Physics - Phenomenology · Physics 2020-08-19 Martin Bauer , Mathias Heiles , Matthias Neubert , Andrea Thamm

Axion-like particles (ALPs) are pseudo Nambu-Goldstone bosons associated with spontaneously broken global symmetries emerging in many extensions of the Standard Model. Assuming the most general effective Lagrangian up to dimension-5…

High Energy Physics - Phenomenology · Physics 2020-12-08 Gholamhossein Haghighat , Daruosh Haji Raissi , Mojtaba Mohammadi Najafabadi

We present a search for the direct production of a light pseudoscalar $a$ decaying into two photons with the Belle II detector at the SuperKEKB collider. We search for the process ${e^+e^-\to\gamma a, a \to\gamma\gamma}$ in the mass range…

High Energy Physics - Experiment · Physics 2020-10-21 Belle II collaboration , F. Abudinen , I. Adachi , H. Aihara , N. Akopov , A. Aloisio , F. Ameli , N. Anh Ky , D. M. Asner , T. Aushev , V. Aushev , V. Babu , S. Baehr , S. Bahinipati , P. Bambade , Sw. Banerjee , S. Bansal , J. Baudot , J. Becker , P. K. Behera , J. V. Bennett , E. Bernieri , F. U. Bernlochner , M. Bertemes , M. Bessner , S. Bettarini , V. Bhardwaj , F. Bianchi , T. Bilka , S. Bilokin , D. Biswas , M. Bračko , P. Branchini , N. Braun , T. E. Browder , A. Budano , S. Bussino , M. Campajola , G. Casarosa , C. Cecchi , D. Červenkov , M. -C. Chang , P. Chang , R. Cheaib , V. Chekelian , B. G. Cheon , K. Chilikin , K. Chirapatpimol , H. -E. Cho , K. Cho , S. -J. Cho , S. -K. Choi , D. Cinabro , L. Corona , L. M. Cremaldi , S. Cunliffe , N. Dash , F. Dattola , E. De La Cruz-Burelo , G. De Nardo , M. De Nuccio , G. De Pietro , R. de Sangro , M. Destefanis , A. De Yta-Hernandez , F. Di Capua , Z. Doležal , T. V. Dong , K. Dort , D. Dossett , G. Dujany , S. Eidelman , T. Ferber , D. Ferlewicz , S. Fiore , A. Fodor , F. Forti , B. G. Fulsom , E. Ganiev , R. Garg , A. Garmash , V. Gaur , A. Gaz , U. Gebauer , A. Gellrich , T. Geßler , R. Giordano , A. Giri , B. Gobbo , R. Godang , P. Goldenzweig , B. Golob , P. Gomis , W. Gradl , E. Graziani , D. Greenwald , C. Hadjivasiliou , S. Halder , O. Hartbrich , K. Hayasaka , H. Hayashii , C. Hearty , M. T. Hedges , I. Heredia de la Cruz , M. Hernández Villanueva , A. Hershenhorn , T. Higuchi , E. C. Hill , H. Hirata , M. Hoek , M. Hohmann , C. -L. Hsu , Y. Hu , K. Inami , G. Inguglia , J. Irakkathil Jabbar , A. Ishikawa , R. Itoh , P. Jackson , W. W. Jacobs , D. E. Jaffe , E. -J. Jang , S. Jia , Y. Jin , C. Joo , A. B. Kaliyar , J. Kandra , G. Karyan , Y. Kato , H. Kichimi , C. Kiesling , C. -H. Kim , D. Y. Kim , H. J. Kim , S. -H. Kim , Y. -K. Kim , T. D. Kimmel , K. Kinoshita , C. Kleinwort , P. Kodyš , T. Koga , S. Kohani , I. Komarov , S. Korpar , T. M. G. Kraetzschmar , P. Križan , P. Krokovny , T. Kuhr , M. Kumar , R. Kumar , K. Kumara , S. Kurz , Y. -J. Kwon , S. Lacaprara , C. La Licata , L. Lanceri , J. S. Lange , I. -S. Lee , S. C. Lee , P. Leitl , D. Levit , P. M. Lewis , C. Li , L. K. Li , Y. B. Li , J. Libby , K. Lieret , L. Li Gioi , Z. Liptak , Q. Y. Liu , D. Liventsev , S. Longo , T. Luo , C. MacQueen , Y. Maeda , R. Manfredi , E. Manoni , S. Marcello , C. Marinas , A. Martini , M. Masuda , K. Matsuoka , D. Matvienko , F. Meggendorfer , F. Meier , M. Merola , F. Metzner , M. Milesi , C. Miller , K. Miyabayashi , R. Mizuk , K. Azmi , G. B. Mohanty , H. -G. Moser , M. Mrvar , F. J. Müller , R. Mussa , I. Nakamura , M. Nakao , H. Nakazawa , A. Natochii , C. Niebuhr , N. K. Nisar , S. Nishida , M. H. A. Nouxman , K. Ogawa , S. Ogawa , H. Ono , P. Oskin , H. Ozaki , P. Pakhlov , A. Paladino , A. Panta , E. Paoloni , S. Pardi , H. Park , S. -H. Park , B. Paschen , A. Passeri , A. Pathak , S. Patra , S. Paul , T. K. Pedlar , I. Peruzzi , R. Peschke , M. Piccolo , L. E. Piilonen , G. Polat , V. Popov , C. Praz , E. Prencipe , M. T. Prim , M. V. Purohit , N. Rad , P. Rados , R. Rasheed , M. Reif , S. Reiter , M. Remnev , I. Ripp-Baudot , M. Ritter , M. Ritzert , G. Rizzo , S. H. Robertson , D. Rodríguez Pérez , J. M. Roney , C. Rosenfeld , A. Rostomyan , N. Rout , D. Sahoo , Y. Sakai , D. A. Sanders , S. Sandilya , A. Sangal , L. Santelj , Y. Sato , V. Savinov , B. Scavino , C. Schwanda , A. J. Schwartz , R. M. Seddon , Y. Seino , A. Selce , K. Senyo , J. Serrano , M. E. Sevior , C. Sfienti , J. -G. Shiu , A. Sibidanov , F. Simon , R. J. Sobie , A. Soffer , E. Solovieva , S. Spataro , B. Spruck , M. Starič , S. Stefkova , Z. S. Stottler , R. Stroili , J. Strube , M. Sumihama , T. Sumiyoshi , D. J. Summers , W. Sutcliffe , H. Svidras , M. Tabata , M. Takizawa , U. Tamponi , S. Tanaka , K. Tanida , H. Tanigawa , P. Taras , F. Tenchini , D. Tonelli , E. Torassa , K. Trabelsi , M. Uchida , T. Uglov , K. Unger , Y. Unno , S. Uno , P. Urquijo , Y. Ushiroda , S. E. Vahsen , R. van Tonder , G. S. Varner , K. E. Varvell , A. Vinokurova , L. Vitale , E. Waheed , M. Wakai , H. M. Wakeling , C. H. Wang , M. -Z. Wang , X. L. Wang , A. Warburton , M. Watanabe , S. Watanuki , J. Webb , S. Wehle , M. Welsch , C. Wessel , J. Wiechczynski , H. Windel , E. Won , L. J. Wu , X. P. Xu , B. Yabsley , W. Yan , S. B. Yang , H. Ye , M. Yonenaga , C. Z. Yuan , Y. Yusa , L. Zani , Q. D. Zhou , V. I. Zhukova

We search for dark matter in the form of axionlike particles (ALPs) in the mass range $5.576741 \,\mathrm{neV/c^2}$ - $5.577733\,\mathrm{neV/c^2}$ by probing their possible coupling to fermion spins through the ALP field gradient. This is…

We presented a complete calculation of the one-loop fermionic correction to the effective coupling between axion-like particles (ALPs) and photons within a constant, homogeneous magnetic field of arbitrary strength. This interaction,…

High Energy Physics - Phenomenology · Physics 2026-02-04 Ozan Semin

Axion-like particles (ALPs), predicted in theories beyond the Standard Model, can have observational effects on the transparency of the Universe to $\gamma$ rays in the presence of magnetic fields. In this work, we search for effects…

High Energy Astrophysical Phenomena · Physics 2020-10-30 Rolf Buehler , Galo Gallardo , Gernot Maier , Alberto Domínguez , Marcos López , Manuel Meyer

We update the globular cluster bound on massive ($m_a$ up to a few 100 keV) axion-like particles (ALP) interacting with photons. The production of such particles in the stellar core is dominated by the Primakoff $\gamma + Ze\to Ze +a$ and…

High Energy Physics - Phenomenology · Physics 2020-09-04 Pierluca Carenza , Oscar Straniero , Babette Döbrich , Maurizio Giannotti , Giuseppe Lucente , Alessandro Mirizzi

Axion-like particles (ALPs) and Higgs bosons can interact in scalar sectors beyond the Standard Model, leading the Higgs boson to decay into pairs of gluons and photons through the ALP interaction and giving rise to resonances in the decay…

High Energy Physics - Phenomenology · Physics 2021-05-05 Alexandre Alves , A. G. Dias , D. D. Lopes

Machine learning (ML) techniques have been applied with tremendous success in many areas of physics. In this work, we use ML to place bounds on the coupling between photons and axion-like particles (ALPs). This coupling causes ALPs and…

High Energy Astrophysical Phenomena · Physics 2020-03-24 Francesca Day , Sven Krippendorf

Axions or more generally axion-like particles (ALPs) are pseudo-scalar particles predicted by many extensions of the Standard Model of particle physics (SM) and considered as viable candidates for dark matter (DM) in the universe. If they…

High Energy Astrophysical Phenomena · Physics 2020-05-20 Ahmed Ayad , Geoff Beck
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