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Related papers: The Cosmophenomenology of Axionic Dark Radiation

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Axions seem ubiquitous in string theories and some of them may be produced non-thermally by heavy scalar decays, contributing to dark radiation. We study various cosmological effects of photons produced from the axionic dark radiation…

High Energy Physics - Phenomenology · Physics 2015-06-16 Tetsutaro Higaki , Kazunori Nakayama , Fuminobu Takahashi

Recent studies of the cosmic microwave background, large scale structure, and big bang nucleosynthesis (BBN) show trends towards extra radiation. Within the framework of supersymmetric hadronic axion models, we explore two…

High Energy Physics - Phenomenology · Physics 2014-01-03 Peter Graf , Frank Daniel Steffen

Existing searches for cosmic axions relics have relied heavily on the axion being non-relativistic and making up dark matter. However, light axions can be copiously produced in the early Universe and remain relativistic today, thereby…

High Energy Physics - Phenomenology · Physics 2022-11-10 Jeff A. Dror , Hitoshi Murayama , Nicholas L. Rodd

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

The Cosmic Background (CB) is defined as the isotropic diffuse radiation field with extragalactic origin found across the electromagnetic spectrum. Different astrophysical sources dominate the CB emission at different energies, such as…

Cosmology and Nongalactic Astrophysics · Physics 2024-11-13 S. Porras-Bedmar , M. Meyer , D. Horns

Axions arise in many theoretical extensions of the Standard Model of particle physics, in particular the "string axiverse". If the axion masses, $m_a$, and (effective) decay constants, $f_a$, lie in specific ranges, then axions contribute…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-18 Matthew J. Stott , David J. E. Marsh , Chakrit Pongkitivanichkul , Layne C. Price , Bobby S. Acharya

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

Axions are a theoretically promising dark matter (DM) candidate. In the presence of radiation from bright astrophysical sources at radio frequencies, nonrelativistic DM axions can undergo stimulated decay to two nearly back-to-back photons,…

High Energy Physics - Phenomenology · Physics 2022-03-25 Yitian Sun , Katelin Schutz , Anjali Nambrath , Calvin Leung , Kiyoshi Masui

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

Hot axions are produced in the early Universe via their interactions with Standard Model particles, contributing to dark radiation commonly parameterized as $\Delta N_{\text{eff}}$. In standard QCD axion benchmark models, this contribution…

High Energy Physics - Phenomenology · Physics 2024-03-12 Marcin Badziak , Keisuke Harigaya , Michał Łukawski , Robert Ziegler

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

If there are a plethora of axions in nature, they may have a complicated potential and create an axion landscape. We study a possibility that one of the axions is so light that it is cosmologically stable, explaining the observed dark…

High Energy Physics - Phenomenology · Physics 2017-03-03 Ryuji Daido , Takeshi Kobayashi , Fuminobu Takahashi

In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too…

High Energy Physics - Phenomenology · Physics 2017-08-03 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall , Keisuke Harigaya

Axions and axion-like particles are ubiquitous in extensions of the Standard Model and offer a unifying framework for addressing open problems in cosmology. Depending on their mass and interactions, axions can act as dark matter, drive…

High Energy Physics - Phenomenology · Physics 2026-05-01 Luca Visinelli

By coupling to both the Higgs and electroweak gauge sectors, an axion can generate the matter-antimatter asymmetry in the universe via electroweak baryogenesis when the axion decay constant lies within the range of approximately $10^5$ and…

High Energy Physics - Phenomenology · Physics 2025-02-11 Kwang Sik Jeong , Ju Hyeong Kang , Shota Nakagawa

The recent observations imply that there is an extra relativistic degree of freedom coined dark radiation. We argue that the QCD axion is a plausible candidate for the dark radiation, not only because of its extremely small mass, but also…

High Energy Physics - Phenomenology · Physics 2015-06-03 Kwang Sik Jeong , Fuminobu Takahashi

Recently it has been suggested that dark radiation in the form of axions produced during the decay of string theory moduli fields could be responsible for the soft x-ray excess in galaxy clusters. These soft X-ray photons come about due to…

Cosmology and Nongalactic Astrophysics · Physics 2014-03-19 Malcolm Fairbairn

In this work, we investigate the dark sector of a supersymmetric axion model, consisting of the late-decaying gravitino/axino dark matter and axion dark radiation. In the early universe, the decay of the scalar superpartner of the axion…

High Energy Physics - Phenomenology · Physics 2022-05-25 Yuchao Gu , Lei Wu , Bin Zhu

Despite growing interest and extensive effort to search for ultralight dark matter in the form of a hypothetical dark photon, how it fits into a consistent cosmology is unclear. Several dark photon dark matter production mechanisms proposed…

High Energy Physics - Phenomenology · Physics 2019-05-03 Raymond T. Co , Aaron Pierce , Zhengkang Zhang , Yue Zhao

We propose simple scenarios where the observed dark matter abundance arises from decays and scatterings of heavy quarks through freeze-in of an axion-like particle with mass in the $10 {\rm \, keV} - 1 {\rm \, MeV}$ range. These models can…

High Energy Physics - Phenomenology · Physics 2024-04-19 Mohammad Aghaie , Giovanni Armando , Angela Conaci , Alessandro Dondarini , Peter Matak , Paolo Panci , Zuzana Sinska , Robert Ziegler
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