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Related papers: Status and Perspectives on Axion Searches

200 papers

We demonstrate that the scatter in the luminosity relations of astrophysical objects can be used to search for axion-like-particles (ALPs). This analysis is applied to observations of active galactic nuclei, where we find evidence strongly…

Cosmology and Nongalactic Astrophysics · Physics 2009-06-30 Clare Burrage , Anne-Christine Davis , Douglas J. Shaw

We establish strong gravitational lens systems as robust probes of axion-like particles (ALPs) -- a candidate for dark matter. A tiny interaction of photons with ALPs induces birefringence. Multiple images of gravitationally lensed…

Cosmology and Nongalactic Astrophysics · Physics 2021-05-19 Aritra Basu , Jishnu Goswami , Dominik J. Schwarz , Yuko Urakawa

The high-energy Universe is potentially a great laboratory for searching new light bosons such as axion-like particles (ALPs). Cosmic sources are indeed the scene of violent phenomena that involve strong magnetic field and/or very long…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Pierre Brun

One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-04 Laura Baudis

Axion-like particles (ALPs) are interesting dark matter candidates both from the theoretical as well as from the experimental perspective. Usually they are motivated as pseudo-Nambu-Goldstone bosons. In this case one of their most important…

High Energy Physics - Phenomenology · Physics 2018-08-01 Gonzalo Alonso-Álvarez , Joerg Jaeckel

Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This…

High Energy Physics - Experiment · Physics 2023-03-31 C. B. Adams , N. Aggarwal , A. Agrawal , R. Balafendiev , C. Bartram , M. Baryakhtar , H. Bekker , P. Belov , K. K. Berggren , A. Berlin , C. Boutan , D. Bowring , D. Budker , A. Caldwell , P. Carenza , G. Carosi , R. Cervantes , S. S. Chakrabarty , S. Chaudhuri , T. Y. Chen , S. Cheong , A. Chou , R. T. Co , J. Conrad , D. Croon , R. T. D'Agnolo , M. Demarteau , N. DePorzio , M. Descalle , K. Desch , L. Di Luzio , A. Diaz-Morcillo , K. Dona , I. S. Drachnev , A. Droster , N. Du , K. Dunne , B. Döbrich , S. A. R. Ellis , R. Essig , J. Fan , J. W. Foster , J. T. Fry , A. Gallo Rosso , J. M. García Barceló , I. G. Irastorza , S. Gardner , A. A. Geraci , S. Ghosh , B. Giaccone , M. Giannotti , B. Gimeno , D. Grin , H. Grote , M. Guzzetti , M. H. Awida , R. Henning , S. Hoof , G. Hoshino , V. Irsic , K. D. Irwin , H. Jackson , D. F. Jackson Kimball , J. Jaeckel , K. Jakovcic , M. J. Jewell , M. Kagan , Y. Kahn , R. Khatiwada , S. Knirck , T. Kovachy , P. Krueger , S. E. Kuenstner , N. A. Kurinsky , R. K. Leane , A. F. Leder , C. Lee , K. W. Lehnert , E. W. Lentz , S. M. Lewis , J. Liu , M. Lynn , B. Majorovits , D. J. E. Marsh , R. H. Maruyama , B. T. McAllister , A. J. Millar , D. W. Miller , J. Mitchell , S. Morampudi , G. Mueller , S. Nagaitsev , E. Nardi , O. Noroozian , C. A. J. O'Hare , N. S. Oblath , J. L. Ouellet , K. M. W. Pappas , H. V. Peiris , K. Perez , A. Phipps , M. J. Pivovaroff , P. Quílez , N. M. Rapidis , V. H. Robles , K. K. Rogers , J. Rudolph , J. Ruz , G. Rybka , M. Safdari , B. R. Safdi , M. S. Safronova , C. P. Salemi , P. Schuster , A. Schwartzman , J. Shu , M. Simanovskaia , J. Singh , S. Singh , K. Sinha , J. T. Sinnis , M. Siodlaczek , M. S. Smith , W. M. Snow , A. V. Sokolov , A. Sonnenschein , D. H. Speller , Y. V. Stadnik , C. Sun , A. O. Sushkov , T. M. P. Tait , V. Takhistov , D. B. Tanner , F. Tavecchio , D. J. Temples , J. H. Thomas , M. E. Tobar , N. Toro , Y. -D. Tsai , E. C. van Assendelft , K. van Bibber , M. Vandegar , L. Visinelli , E. Vitagliano , J. K. Vogel , Z. Wang , A. Wickenbrock , L. Winslow , S. Withington , M. Wooten , J. Yang , B. A. Young , F. Yu , K. Zhou , T. Zhou

The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interactions and also happens to be an excellent dark matter candidate. Axions constituting the dark matter halo of our galaxy may be detected by…

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…

Revealing the essence of dark matter (DM) and dark energy is essential for understanding our universe. Ultralight (rest energy $<$10 eV) bosonic particles, including pseudoscalar axions and axion-like particles (ALPs) have emerged among…

High Energy Physics - Experiment · Physics 2024-07-10 Xiaofei Huang , Xiaolin Ma , Lei Cong , Wei Ji , Jia Liu , Wei Quan , Kai Wei

Axion-like particles (ALPs) can provide a portal to new states of a dark sector. We study the phenomenology of this portal when the ALP mainly decays invisibly, while its interaction with the standard model sector proceeds essentially via…

High Energy Physics - Phenomenology · Physics 2021-06-16 Luc Darmé , Federica Giacchino , Enrico Nardi , Mauro Raggi

In this review, we present a self-contained introduction to axion-like particles (ALPs) with a particular focus on their effects on photon polarization: both theoretical and phenomenological aspects are discussed. We derive the photon…

High Energy Physics - Phenomenology · Physics 2024-08-01 Giorgio Galanti

We propose the use of FASER as a light-shining-through-walls experiment to search for axions and axion-like particles (ALPs). LHC collisions generate a high intensity and high energy photon flux in the forward direction which can oscillate…

High Energy Physics - Phenomenology · Physics 2023-02-16 Felix Kling , Pablo Quílez

The axion is a light pseudoscalar particle postulated to solve issues with the Standard Model, including the strong CP problem and the origin of dark matter. In recent years, there has been remarkable progress in the physics of axions in…

High Energy Physics - Phenomenology · Physics 2021-11-03 Kiwoon Choi , Sang Hui Im , Chang Sub Shin

We propose new signals for the direct detection of ultralight dark matter such as the axion. Axion or axion like particle (ALP) dark matter may be thought of as a background, classical field. We consider couplings for this field which give…

High Energy Physics - Phenomenology · Physics 2013-09-11 Peter W. Graham , Surjeet Rajendran

The first FASER search for a light, long-lived particle decaying into a pair of photons is reported. The search uses LHC proton-proton collision data at $\sqrt{s}=13.6~\text{TeV}$ collected in 2022 and 2023, corresponding to an integrated…

High Energy Physics - Experiment · Physics 2024-12-18 FASER collaboration , Roshan Mammen Abraham , Xiaocong Ai , John Anders , Claire Antel , Akitaka Ariga , Tomoko Ariga , Jeremy Atkinson , Florian U. Bernlochner , Emma Bianchi , Tobias Boeckh , Jamie Boyd , Lydia Brenner , Angela Burger , Franck Cadoux , Roberto Cardella , David W. Casper , Charlotte Cavanagh , Xin Chen , Eunhyung Cho , Dhruv Chouhan , Andrea Coccaro , Stephane Débieux , Monica D'Onofrio , Ansh Desai , Sergey Dmitrievsky , Radu Dobre , Sinead Eley , Yannick Favre , Deion Fellers , Jonathan L. Feng , Carlo Alberto Fenoglio , Didier Ferrere , Max Fieg , Wissal Filali , Elena Firu , Edward Galantay , Ali Garabaglu , Stephen Gibson , Sergio Gonzalez-Sevilla , Yuri Gornushkin , Carl Gwilliam , Daiki Hayakawa , Michael Holzbock , Shih-Chieh Hsu , Zhen Hu , Giuseppe Iacobucci , Tomohiro Inada , Luca Iodice , Sune Jakobsen , Hans Joos , Enrique Kajomovitz , Hiroaki Kawahara , Alex Keyken , Felix Kling , Daniela Köck , Pantelis Kontaxakis , Umut Kose , Rafaella Kotitsa , Susanne Kuehn , Thanushan Kugathasan , Lorne Levinson , Ke Li , Jinfeng Liu , Yi Liu , Margaret S. Lutz , Jack MacDonald , Chiara Magliocca , Toni Mäkelä , Lawson McCoy , Josh McFayden , Andrea Pizarro Medina , Matteo Milanesio , Théo Moretti , Mitsuhiro Nakamura , Toshiyuki Nakano , Laurie Nevay , Ken Ohashi , Hidetoshi Otono , Lorenzo Paolozzi , Brian Petersen , Titi Preda , Markus Prim , Michaela Queitsch-Maitland , Hiroki Rokujo , André Rubbia , Jorge Sabater-Iglesias , Osamu Sato , Paola Scampoli , Kristof Schmieden , Matthias Schott , Anna Sfyrla , Davide Sgalaberna , Mansoora Shamim , Savannah Shively , Yosuke Takubo , Noshin Tarannum , Ondrej Theiner , Eric Torrence , Oscar Ivan Valdes Martinez , Svetlana Vasina , Benedikt Vormwald , Di Wang , Yuxiao Wang , Eli Welch , Yue Xu , Samuel Zahorec , Stefano Zambito , Shunliang Zhang

We review topics in searches for axion-like-particles (ALPs), covering material that is complementary to other recent reviews. The first half of our review covers ALPs in the extreme environments of neutron star cores, the magnetospheres of…

High Energy Physics - Phenomenology · Physics 2021-06-16 Jean-François Fortin , Huai-Ke Guo , Steven P. Harris , Doojin Kim , Kuver Sinha , Chen Sun

Several extensions of the Standard Model predict the existence of Axion-Like Particles (ALPs), very light spin-zero bosons with a two-photon coupling. ALPs can give rise to observable effects in very-high-energy astrophysics. Above roughly…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Marco Roncadelli , Alessandro De Angelis , Giorgio Galanti

Axion-like particles (ALPs) are light, neutral, pseudo-scalar bosons predicted by several extensions of the Standard Model of particle physics -- such as the String Theory -- and are supposed to interact primarily only with two photons. In…

High Energy Astrophysical Phenomena · Physics 2019-11-22 Giorgio Galanti

Axions and other very weakly interacting slim particles (WISPs) may be non-thermally produced in the early universe and survive as constituents of the dark universe. We describe their theoretical motivation and their phenomenology. A huge…

High Energy Physics - Phenomenology · Physics 2012-11-01 Andreas Ringwald

In the late 1970's, the axion was proposed as a solution to the Strong CP Problem, i.e. the puzzle why the strong interactions conserve parity P and the product CP of charge conjugation and parity in spite of the fact that the Standard…

High Energy Physics - Phenomenology · Physics 2021-02-24 Pierre Sikivie