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Related papers: Misalignment vs Topology in Axion-Like Models

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We consider cosmological consequences of the spontaneous breaking of a global symmetry that is anomalous under technicolor interactions, leading to the emergence of a light axion-like particle. Avoiding overclosure of the universe by such…

High Energy Physics - Phenomenology · Physics 2008-11-26 Hooman Davoudiasl

The axion is arguably one of the best motivated candidates for dark matter. For a decay constant greater than about 10^9 GeV, axions are dominantly produced non-thermally in the early universe and hence are "cold", their velocity dispersion…

High Energy Physics - Phenomenology · Physics 2016-12-30 Andreas Ringwald

Although the standard {\Lambda}CDM model describes the cosmic microwave background radiation and the large scale structure of the Universe with great success, it has some tensions with observations in the effective number of neutrino…

High Energy Physics - Phenomenology · Physics 2012-11-26 Kiwoon Choi , Ki-Young Choi , Chang Sub Shin

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 generic expectation in string/supergravity models is that there are multiple moduli fields with masses of the order of the supersymmetry breaking scale. We study the cosmology that arises as a result of vacuum misalignment of these…

High Energy Physics - Theory · Physics 2020-01-23 Bobby S. Acharya , Mansi Dhuria , Diptimoy Ghosh , Anshuman Maharana , Francesco Muia

We argue that coherent oscillations of the axion field excited by the misalignment mechanism and non-thermal leptogenesis by the saxion decay can naturally explain the observed abundance of dark matter and baryon asymmetry, thus providing a…

High Energy Physics - Phenomenology · Physics 2015-06-12 Kwang Sik Jeong , Fuminobu Takahashi

I present an introduction and topical review on axions as a dark matter candidate. Emphasis is placed on issues surrounding the cosmology of axion dark matter that are relevant for present-day searches, including: early-Universe production…

High Energy Physics - Phenomenology · Physics 2024-05-28 Ciaran A. J. O'Hare

Generating axion dark matter through the kinetic misalignment mechanism implies the generation of large asymmetries for Standard Model fermions in the early universe. Even if these asymmetries are washed out at later times, they can trigger…

High Energy Physics - Phenomenology · Physics 2023-08-09 Raymond T. Co , Valerie Domcke , Keisuke Harigaya

The axion has emerged in recent years as a leading particle candidate to provide the mysterious dark matter in the cosmos, as we review here for a general scientific audience. We describe first the historical roots of the axion in the…

High Energy Physics - Phenomenology · Physics 2022-10-18 Francesca Chadha-Day , John Ellis , David J. E. Marsh

Dark matter axions form a rethermalizing Bose-Einstein condensate. This provides an opportunity to distinguish axions from other forms of dark matter on observational grounds. I show that if the dark matter is axions, tidal torque theory…

Astrophysics of Galaxies · Physics 2015-05-18 Pierre Sikivie

Axion-like fields are naturally generated by a mechanism of anomaly cancellation of one or more anomalous gauge abelian symmetries at the Planck scale, emerging as duals of a two-form from the massless bosonic sector of string theory. This…

High Energy Physics - Phenomenology · Physics 2018-07-04 Claudio Coriano , Paul H. Frampton

The companion-axion model introduces a second QCD axion to rescue the Peccei-Quinn solution to the strong-CP problem from the effects of colored gravitational instantons. As in single-axion models, the two axions predicted by the…

High Energy Physics - Phenomenology · Physics 2025-06-18 Zhe Chen , Archil Kobakhidze , Ciaran A. J. O'Hare , Zachary S. C. Picker , Giovanni Pierobon

Axions and axion-like particles (ALPs) are among the most popular candidates that explain the origin of the mysterious dark matter. The most popular ALP production mechanism studied in the literature is the misalignment mechanism, where an…

High Energy Physics - Phenomenology · Physics 2025-01-22 Cem Eröncel

Here we generally prove that the axion as a coherently oscillating scalar field acts as a cold dark matter in nearly all cosmologically relevant scales. The proof is made in the linear perturbation order. Compared with our previous proof…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-28 Jai-chan Hwang , Hyerim Noh

In addition to spectacular signatures such as black hole superradiance and the rotation of CMB polarization, the plenitude of axions appearing in the string axiverse may have potentially dangerous implications. An example is the…

High Energy Physics - Phenomenology · Physics 2021-10-05 Mario Reig

We show that very compact axion mini-clusters can form in models where axion-like-particle (ALP) dark matter is produced via the kinetic misalignment mechanism, which is well-motivated in pre-inflationary $U(1)$ symmetry breaking scenarios.…

High Energy Physics - Phenomenology · Physics 2024-05-06 Cem Eröncel , Géraldine Servant

An axion rotating in field space can produce dark photons in the early universe via tachyonic instability. This explosive particle production creates a background of stochastic gravitational waves that may be visible at pulsar timing arrays…

High Energy Physics - Phenomenology · Physics 2022-01-05 Raymond T. Co , Keisuke Harigaya , Aaron Pierce

The current cosmological constraints on a dark matter axion are reviewed. We describe the basic mechanisms by which axions are created in the early universe, both in the standard thermal scenario in which axion strings form and in…

Astrophysics · Physics 2016-10-26 E. P. S. Shellard , R. A. Battye

The QCD axion is a good dark matter candidate. The observed dark matter abundance can arise from misalignment or defect mechanisms, which generically require an axion decay constant $f_a \sim \mathcal{O}(10^{11})$ GeV (or higher). We…

High Energy Physics - Phenomenology · Physics 2018-07-27 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

We study axion dark matter production from a misalignment mechanism in scenarios featuring a general nonstandard cosmology. Before the onset of Big Bang nucleosynthesis, the energy density of the universe is dominated by a particle field…

High Energy Physics - Phenomenology · Physics 2021-12-13 Paola Arias , Nicolás Bernal , Dimitrios Karamitros , Carlos Maldonado , Leszek Roszkowski , Moira Venegas