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We introduce a mechanism by which a misaligned ALP can be dynamically converted into a dark photon in the presence of a background magnetic field. An abundance of non-relativistic ALPs will convert to dark photons with momentum of order the…

High Energy Physics - Phenomenology · Physics 2025-06-18 Edward Broadberry , Saurav Das , Anson Hook , Gustavo Marques-Tavares

Cosmological moduli generically come to dominate the energy density of the early universe, and thereby trigger an early matter dominated era. Such non-standard cosmological histories are expected to have profound effects on the evolution…

High Energy Physics - Phenomenology · Physics 2025-06-13 Robert Wiley Deal , Leia Barrowes , John T. Giblin, , Kuver Sinha , Scott Watson , Fred C. Adams

Pulsar magnetospheres admit non-stationary vacuum gaps that are characterized by non-vanishing ${\bf{E}} \cdot {\bf{B}}$. The vacuum gaps play an important role in plasma production and electromagnetic wave emission. We show that these gaps…

High Energy Physics - Phenomenology · Physics 2021-10-04 Anirudh Prabhu

Cosmology and particle physics are closer today than ever before, with several searches underway at the interface between cosmology, particle physics, and field theory. The mystery of dark matter (DM) is one of the greatest common unsolved…

High Energy Physics - Phenomenology · Physics 2022-03-14 Ahmed Ayad

The relic density of dark matter in the $\Lambda$CDM model restricts the parameter space for a cosmological axion field, constraining the axion decay constant, the initial amplitude of the axion field and the axion mass. It is shown via…

High Energy Physics - Phenomenology · Physics 2024-01-23 Filippo Anzuini , Angelo Maggi

We study the stochastic axion dark matter scenario in the axion landscape, where one of the axions is light and stable and therefore explains dark matter. If the axion mass at the potential is a typical value of the curvature along the…

High Energy Physics - Phenomenology · Physics 2020-05-20 Shota Nakagawa , Fuminobu Takahashi , Wen Yin

A number of proposed and ongoing experiments search for axion dark matter with a mass nearing the limit set by small scale structure (${\cal O} ( 10 ^{ - 21 } {\rm eV} ) $). We consider the late universe cosmology of these models, showing…

High Energy Physics - Phenomenology · Physics 2021-01-11 Jeff A. Dror , Jacob M. Leedom

Axion-like particles are promising candidates to make up the dark matter of the universe, but it is challenging to design experiments that can detect them over their entire allowed mass range. Dark matter in general, and in particular…

High Energy Physics - Phenomenology · Physics 2018-04-30 Peter W. Graham , David E. Kaplan , Jeremy Mardon , Surjeet Rajendran , William A. Terrano , Lutz Trahms , Thomas Wilkason

Dark matter (DM) refers to a new type of matter that may explain observed rotation curves of galaxies and the composite structure of the Universe. It may couple to the Standard Model particles via portals, which include the possibility of…

High Energy Physics - Experiment · Physics 2023-11-30 Vindhyawasini Prasad

We investigate the production of QCD axion dark matter in a nonstandard cosmological era triggered by primordial black holes (PBHs) that fully evaporate before the onset of BBN. Even if PBHs cannot emit the whole axion cold dark matter…

High Energy Physics - Phenomenology · Physics 2021-10-13 Nicolás Bernal , Fazlollah Hajkarim , Yong Xu

Recently, Csaki, Kaloper and Terning (CKT) suggested that axion-photon oscillation in the intergalactic medium can explain the observed dimming of distant type Ia supernovae. This mechanism works only if the initial axion flux is much…

High Energy Physics - Phenomenology · Physics 2014-11-17 Yuval Grossman , Sourov Roy , Jure Zupan

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

Cosmological structure formation simulations of ultralight axion-like dark matter have shown that an axion star forms at the center of every dark matter halo in the Universe. These axion stars would then form in large numbers during the…

High Energy Physics - Phenomenology · Physics 2024-02-12 Miguel Escudero

Axion-photon conversion at dielectric interfaces, immersed in a near-homogeneous magnetic field, is the basis for the dielectric haloscope method to search for axion dark matter. In analogy to transition radiation, this process is possible…

High Energy Physics - Phenomenology · Physics 2017-09-07 Ara N. Ioannisian , Narine Kazarian , Alexander J. Millar , Georg G. Raffelt

Axions are some of the best motivated particles beyond the Standard Model. We show how the attractive self-interactions of dark matter (DM) axions over a broad range of masses, from $10^{-22}$ eV to $10^7$ GeV, can lead to nongravitational…

Cosmology and Nongalactic Astrophysics · Physics 2020-04-15 Asimina Arvanitaki , Savas Dimopoulos , Marios Galanis , Luis Lehner , Jedidiah O. Thompson , Ken Van Tilburg

If the dark matter in the Universe is made of $\mu$eV axion-like particles (ALPs), then a rich phenomenology can emerge in connection to their stimulated decay into two photons. We discuss the ALP stimulated decay induced by electromagnetic…

High Energy Physics - Phenomenology · Physics 2024-04-09 Elisa Todarello , Francesca Calore , Marco Regis

In the strong magnetic field of a neutron star's magnetosphere, axions coupled to electromagnetism develop a nonzero probability to convert into photons. Past studies have revealed that the axion-photon conversion can be resonantly…

High Energy Physics - Phenomenology · Physics 2024-08-16 Andrew J. Long , Enrico D. Schiappacasse

For the minimal QCD axion model it is generally believed that overproduction of dark matter constrains the axion mass to be above a certain threshold, or at least that the initial misalignment angle must be tuned if the mass is below that…

High Energy Physics - Phenomenology · Physics 2018-08-17 Peter W. Graham , Adam Scherlis

The axion particle, a consequence of an elegant hypothesis that resolves the strong-CP problem of quantum chromodynamics, is a plausible origin for cosmological dark matter. In searches for axionic dark matter that detect the conversion of…

High Energy Physics - Phenomenology · Physics 2016-07-20 Huaixiu Zheng , Matti Silveri , R. T. Brierley , S. M. Girvin , K. W. Lehnert

We study a scenario in which the baryon asymmetry is created through Hawking radiation from primordial black holes via a dynamically-generated chemical potential. This mechanism can also be used to generate the observed dark matter…

High Energy Physics - Phenomenology · Physics 2022-03-14 Nolan Smyth , Lillian Santos-Olmsted , Stefano Profumo