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Although axion-like particles (ALPs) are popular dark matter candidates, their mass generation mechanisms as well as cosmic thermal evolutions are still unclear. In this letter, we propose a new mass generation mechanism of ALP during the…

High Energy Physics - Phenomenology · Physics 2022-10-25 Wei Chao , Mingjie Jin , Hai-Jun Li , Ying-Quan Peng

In the beyond Standard Model (BSM) scenarios, the possibility of neutrinos decaying into a lighter state is one of the prime quests for the new-generation neutrino experiments. The observation of high-energy astrophysical neutrinos by…

High Energy Astrophysical Phenomena · Physics 2024-03-08 Bhanu Prakash Pant

Axion-Like Particles (ALPs) are pseudo Nambu-Goldstone bosons associated with spontaneously broken global $U(1)$ symmetries. Such particles can have lepton-flavor-violating (LFV) couplings to the SM charged leptons. LFV ALPs provide the…

High Energy Physics - Phenomenology · Physics 2022-05-24 Gholamhossein Haghighat , Mojtaba Mohammadi Najafabadi

Axion-like particles (ALPs) are very light, neutral, spin zero bosons predicted by many theories which try to complete the standard model of elementary particles. ALPs interact primarily with two photons and can generate photon-ALP…

High Energy Astrophysical Phenomena · Physics 2023-02-09 Giorgio Galanti

Axion-like particles (ALPs) are known to be produced through axion-photon conversion in the presence of a stationary external magnetic field. Devices such as undulators and wigglers, which are used widely for photon production, e.g., in…

High Energy Physics - Phenomenology · Physics 2024-09-24 Wen Yin , Junya Yoshida

We investigate the non-perturbatively generated axion-like particle (ALP) potential, involving fermions in the dark sector that couple to the ALP, in an early cosmological inflationary stage with the ALP being a spectator field. The…

High Energy Physics - Phenomenology · Physics 2023-02-02 Anish Ghoshal , Abhishek Naskar

Light pseudoscalars, or axion like particles (ALPs), are much studied due to their potential relevance to the fields of particle physics, astrophysics and cosmology. The most relevant coupling of ALPs from the viewpoint of current…

High Energy Physics - Theory · Physics 2014-02-19 L. H. C. Borges , A. G. Dias , A. F. Ferrari , J. R. Nascimento , A. Yu. Petrov

Dark sector may exist and interact with Standard Model (SM) through the $U(1)$ kinetic mixing. Through this portal-type interaction, dark photon from dark sector couples to SM fermions, and may explain the discrepancy between experimental…

High Energy Physics - Phenomenology · Physics 2026-02-04 Chuan-Ren Chen , Yuan-Feng Hsieh , Chrisna Setyo Nugroho

Axion-like particles (ALPs) rotate the linear polarization of photons through the ALP-photon coupling and convert the cosmic microwave background (CMB) $E$-mode to the $B$-mode. We derive the relation between the ALP dynamics and the…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-12 Tomohiro Fujita , Yuto Minami , Kai Murai , Hiromasa Nakatsuka

Axion-Like Particles (ALPs) are well-motivated extensions of the Standard Model of Particle Physics and a generic prediction of some string theories. X-ray observations of bright Active Galactic Nuclei (AGN) hosted by rich clusters of…

High Energy Astrophysical Phenomena · Physics 2023-07-05 Júlia Sisk-Reynés , Christopher S. Reynolds , Michael L. Parker , James H. Matthews , M. C. David Marsh

We consider the search for axion-like particles (ALPs) by using time series data of the polarization angle of the light. If the condensation of an ALP plays the role of dark matter, the polarization plane of the light oscillates as a…

Cosmology and Nongalactic Astrophysics · Physics 2020-02-19 So Chigusa , Takeo Moroi , Kazunori Nakayama

We examine the resonant conversion of axion-like particle (ALP) or dark photon to the electromagnetic photon in the early Universe, which takes place due to the ALP-photon-dark photon oscillations in background dark photon gauge fields. It…

High Energy Physics - Phenomenology · Physics 2020-10-28 Kiwoon Choi , Hyeonseok Seong , Seokhoon Yun

The low-energy effective field theory (LEFT) provides the appropriate framework to describe particle interactions below the scale of electroweak symmetry breaking, $\mu_w\sim v$. By matching the Standard Model onto the LEFT, non-zero Wilson…

High Energy Physics - Phenomenology · Physics 2023-08-04 Anne Mareike Galda , Matthias Neubert

Axion like particles (ALPs) are fundamental pseudo scalar particles with properties similar to Axions which are a well-known extension of the standard model to solve the strong CP problem in Quantum Chromodynamics. ALPs can oscillate into…

High Energy Astrophysical Phenomena · Physics 2017-10-30 Jhilik Majumdar , Francesca Calore , Dieter Horns

We revisit the ALP miracle scenario where the inflaton and dark matter are unified by a single axion-like particle (ALP). We first extend our previous analysis on the inflaton dynamics to identify the whole viable parameter space consistent…

High Energy Physics - Phenomenology · Physics 2020-06-24 Ryuji Daido , Fuminobu Takahashi , Wen Yin

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

In the Standard Model (SM), the rare transitions where a bottom quark decays into a strange quark and a pair of light leptons exhibit a potential sensitivity to physics beyond the SM. In addition, the SM embeds Lepton Flavour Universality…

High Energy Physics - Phenomenology · Physics 2018-02-14 Bernat Capdevila , Andreas Crivellin , Sébastien Descotes-Genon , Joaquim Matias , Javier Virto

We argue that a large region of so far unconstrained parameter space for axion-like particles (ALPs), where their couplings to the Standard Model are of order $(0.01\!-\!1)\,\mbox{TeV}^{-1}$, can be explored by searches for the exotic Higgs…

High Energy Physics - Phenomenology · Physics 2017-07-26 Martin Bauer , Matthias Neubert , Andrea Thamm

The decay of Axion-Like Particles (ALPs) trapped in the solar gravitational field would contribute to the observed solar X-ray flux, hence constraining ALP models. We improve by one order of magnitude the existing limits in the parameter…

High Energy Physics - Phenomenology · Physics 2023-06-21 Cyprien Beaufort , Mar Bastero-Gil , Tiffany Luce , Daniel Santos

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
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