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Related papers: Structure Formation Limits on Axion-Like Dark Matt…

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The suppression of cosmological structure at small scales is a key signature of dark matter (DM) produced via freeze-in in the low-mass regime. We present a comprehensive analysis of its impact, incorporating recent constraints from Milky…

High Energy Physics - Phenomenology · Physics 2025-12-12 Francesco D'Eramo , Alessandro Lenoci , Ariane Dekker

Axion-like particles (ALP) are promising candidates to comprise all the dark matter in the universe. We investigate the ALP couplings to photons and electrons via astrophysical measurements through the search for very-high-energy gamma rays…

High Energy Astrophysical Phenomena · Physics 2025-01-23 Victor P. Goncalves , Emmanuel Moulin , Igor Reis , Aion Viana

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

Axion-like particles (ALPs) may undergo mixing with photons in the presence of astrophysical magnetic fields, leading to alterations in the observed high energy $\gamma$-ray spectra. In this study, we investigate the ALP-photon oscillation…

High Energy Astrophysical Phenomena · Physics 2024-03-06 Lin-Qing Gao , Xiao-Jun Bi , Jun-Guang Guo , Wenbin Lin , Peng-Fei Yin

There are several issues to do with dwarf galaxy predictions in the standard $\Lambda$CDM cosmology that have suscitated much recent debate about the possible modification of the nature of dark matter as providing a solution. We explore a…

Cosmology and Nongalactic Astrophysics · Physics 2017-07-07 David J. E. Marsh , Joe Silk

Dark matter energy injection in the early universe modifies both the ionization history and the temperature of the intergalactic medium. In this work, we improve the CMB bounds on sub-keV dark matter and extend previous bounds from…

Cosmology and Nongalactic Astrophysics · Physics 2023-06-30 Francesco Capozzi , Ricardo Z. Ferreira , Laura Lopez-Honorez , Olga Mena

We further explore a scenario in which the recently observed 3.55 keV photon line arises from dark matter decay to an axion-like particle (ALP) of energy 3.55 keV, which then converts to a photon in astrophysical magnetic fields. This ALP…

High Energy Physics - Phenomenology · Physics 2014-11-25 Joseph P. Conlon , Francesca V. Day

Axions and axion-like particles (ALPs) have gained immense attention in searches for beyond Standard Model (BSM) physics. Experiments searching for axions leverage their predicted couplings to Standard Model (SM) particles to look for…

High Energy Physics - Phenomenology · Physics 2026-03-24 Tanmoy Kumar , N. P. S. Mithun , Subhendra Mohanty , Sourov Roy , B. S. Bharath Saiguhan , Santosh Vadawale

We investigate the production of dark radiation (DR) from axions and axion-like particles (ALPs) as potential origins of dark matter. Focusing on the dark matter misalignment mechanism, we examine non-thermal, pre-inflationary scenarios…

Cosmology and Nongalactic Astrophysics · Physics 2024-11-12 José María Pérez-Poyatos , Veronica Sanz

Axion-Like Particles (ALPs) coupled with electrons would be produced in a Supernova (SN) via electron-proton bremsstrahlung and electron-positron fusion. We evaluate the ALP emissivity from these processes by taking into account the ALP…

High Energy Physics - Phenomenology · Physics 2021-11-16 Giuseppe Lucente , Pierluca Carenza

The production of very-high-energy (VHE, $E_{\gamma} \gtrsim 100$ GeV) gamma rays resulting from the scattering of high-energy cosmic-ray protons off axion-like particles (ALPs) populating the dark matter halo of the Milky Way is…

High Energy Physics - Phenomenology · Physics 2026-03-20 Victor P. Goncalves , Emmanuel Moulin , Igor Reis , Aion Viana

Axion-like particles (ALPs), a class of pseudoscalars common to many extensions of the Standard Model, have the capacity to drain energy from the interiors of stars. Consequently, stellar evolution can be used to derive many constraints on…

High Energy Physics - Phenomenology · Physics 2021-09-16 Matthew J. Dolan , Frederick J. Hiskens , Raymond R. Volkas

Axion-like particles (ALPs) arise from well-motivated extensions to the Standard Model and could account for dark matter. ALP dark matter would manifest as a field oscillating at an (as of yet) unknown frequency. The frequency depends…

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

Axion-like particles (ALPs) and photons inter-convert in the presence of a magnetic field. At keV energies in the environment of galaxy clusters, the conversion probability can become unsuppressed for light ALPs. Conversion of thermal X-ray…

High Energy Physics - Phenomenology · Physics 2016-07-06 Joseph P. Conlon , M. C. David Marsh , Andrew J. Powell

We set the strongest limits to-date on the velocity-independent dark matter (DM) - proton cross section $\sigma$ for DM masses $m = 10\,\mathrm{keV}$ to $100\,\mathrm{GeV}$, using large-scale structure traced by the Lyman-alpha forest:…

Cosmology and Nongalactic Astrophysics · Physics 2022-04-28 Keir K. Rogers , Cora Dvorkin , Hiranya V. Peiris

Axion-like particles (ALPs) are well-motivated extensions of the Standard Model (SM) that appear in many new physics scenarios, with masses spanning a broad range. In this work, we systematically study the production and detection prospects…

High Energy Physics - Phenomenology · Physics 2025-10-22 Shou-shan Bao , Yang Ma , Yongcheng Wu , Keping Xie , Hong Zhang

In the past few years, the search for axion-like particles (ALPs) has grown significantly due to their potential to account for the total abundance of the cold dark matter (CDM) in the universe. The coupling between ALPs and photons allows…

High Energy Astrophysical Phenomena · Physics 2022-03-09 Ahmed Ayad , Geoff Beck

We assume that dark matter is comprised of axion-like particles (ALPs) generated by the realignment mechanism in the post-inflationary scenario. This leads to isocurvature fluctuations with an amplitude of order one for scales comparable to…

Cosmology and Nongalactic Astrophysics · Physics 2019-05-16 Martin Feix , Johann Frank , Andreas Pargner , Robert Reischke , Bjoern Malte Schaefer , Thomas Schwetz

Ultralight axion like particles (ALPs) of mass $m_a\in (10^{-21}\rm{eV}-10^{-22}\rm{eV})$ with axion decay constant $f_a\sim 10^{17}\rm{GeV}$ can be candidates for fuzzy dark matter (FDM). If celestial bodies like Earth and Sun are immersed…

High Energy Physics - Phenomenology · Physics 2021-10-08 Tanmay Kumar Poddar