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Related papers: QCD Axion Dark Matter with a Small Decay Constant

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A major fraction of the mass content of the universe is composed of dark matter (DM), i.e. particles not interacting significantly with electromagnetic radiation, with ordinary matter or self-interacting (cold dark matter). The axion is…

High Energy Physics - Experiment · Physics 2018-12-12 Woohyun Chung

We demonstrate that the observed cosmological excess of matter over antimatter may originate from a heavy QCD axion that solves the strong CP problem but has a mass much larger than that given by the Standard Model QCD strong dynamics. We…

High Energy Physics - Phenomenology · Physics 2022-11-09 Raymond T. Co , Tony Gherghetta , Keisuke Harigaya

The QCD axion may offer a unified origin for the baryon asymmetry and dark matter through axiogenesis. However, in the minimal QCD axion scenario, axiogenesis either underproduces baryons or overproduces dark matter, and the required…

High Energy Physics - Phenomenology · Physics 2025-11-21 Pouya Asadi , David Cyncynates , Stefania Gori

The QCD axion is one of the most appealing candidates for the dark matter in the Universe. In this article, we discuss the possibility to predict the axion mass in the context of a simple renormalizable grand unified theory where the…

High Energy Physics - Phenomenology · Physics 2019-11-21 Pavel Fileviez Perez , Clara Murgui , Alexis D. Plascencia

Invoking the Peccei-Quinn (PQ) solution to the strong CP problem substitutes the puzzle of why $\theta_{qcd}$ is so small with the puzzle of why the PQ symmetry is of such high quality. Cosmological and astrophysical considerations raise…

High Energy Physics - Theory · Physics 2009-12-30 Linda M. Carpenter , Michael Dine , Guido Festuccia

The axion is a promising dark matter candidate, which was originally proposed to solve the strong-CP problem in particle physics. To date, the available parameter space for axion and axion-like particle dark matter is relatively unexplored,…

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

The domain wall problem of the Peccei-Quinn mechanism can be solved if the Peccei-Quinn symmetry is explicitly broken by a small amount. Domain walls decay into axions, which may account for dark matter of the universe. This scheme is…

High Energy Physics - Phenomenology · Physics 2018-05-02 Keisuke Harigaya , Masahiro Kawasaki

The presence of dark matter provides some of the most tangible evidence for the existence of physics beyond the Standard Model. One compelling dark matter candidate is the axion, a light boson that was originally postulated as a solution to…

High Energy Physics - Experiment · Physics 2019-05-17 Chiara P. Salemi

Current upper bounds of the neutron electric dipole moment constrain the physically observable quantum chromodynamic (QCD) vacuum angle $|\bar\theta| \lesssim 10^{-11}$. Since QCD explains vast experimental data from the 100 MeV scale to…

High Energy Physics - Phenomenology · Physics 2020-01-08 Jihn E. Kim , Gianpaolo Carosi

The axion, which has yet to be discovered, is a promising candidate for dark matter that emerges from Peccei-Quinn theory. This article presents the search for axion dark matter with the "Student Project for an Axion Cavity Experiment"…

High Energy Physics - Experiment · Physics 2025-10-29 M. A. Akgümüs , N. Salama , J. Egge , E. Garutti , M. Maroudas , L. H. Nguyen , D. Leppla-Weber

The quantum chromodynamics axion with a decay constant near the Grand Unification (GUT) scale has an ultralight mass near a neV. We show, however, that axion-like particles with masses near the keV - PeV range with GUT-scale decay constants…

High Energy Physics - Phenomenology · Physics 2023-01-18 Joshua W. Foster , Soubhik Kumar , Benjamin R. Safdi , Yotam Soreq

Axions as dark matter is an increasingly important subject in astrophysics and cosmology. Experimental and observational searches are mounting across the mass spectrum of axion-like particles, many of which require detailed knowledge of…

Cosmology and Nongalactic Astrophysics · Physics 2019-03-13 Erik W. Lentz , Thomas R. Quinn , Leslie J Rosenberg

Relativistic axions are good candidates for the dark radiation for which there are mounting observational hints. The primordial decays of heavy fields produce axions which are ultra-energetic compared to thermalised matter and inelastic…

High Energy Physics - Phenomenology · Physics 2015-06-15 Joseph P. Conlon , M. C. David Marsh

Axions solve the Strong CP Problem and are a cold dark matter candidate. The combined constraints from accelerator searches, stellar evolution limits and cosmology suggest that the axion mass is in the range $3 \cdot 10^{-3} > m_a >…

High Energy Physics - Phenomenology · Physics 2007-05-23 Pierre Sikivie

Two of the most pressing questions in physics are the microscopic nature of the dark matter that comprises 84% of the mass in the universe and the absence of a neutron electric dipole moment. These questions would be resolved by the…

The existence of dark matter provides strong evidence for physics beyond the Standard Model. Extending the Standard Model with the Peccei-Quinn symmetry and/or supersymmetry, compelling dark matter candidates appear. For the axion, the…

High Energy Physics - Phenomenology · Physics 2009-02-18 Frank Daniel Steffen

The Peccei-Quinn mechanism presents a neat solution to the strong CP problem. As a by-product, it provides an ideal dark matter candidate, "the axion", albeit with a tiny mass. Axions therefore can act as dark radiation if excited with…

High Energy Physics - Phenomenology · Physics 2016-09-28 Anupam Mazumdar , Saleh Qutub , Ken'ichi Saikawa

Recently, indications for an emission line at 3.55 keV have been found in the combined spectra of a large number of galaxy clusters and also in Andromeda. This line could not be identified with any known spectral line. It is tempting to…

High Energy Physics - Phenomenology · Physics 2014-05-14 Joerg Jaeckel , Javier Redondo , Andreas Ringwald

The origin of dark matter in the universe may be weakly interacting scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We present two interesting cases, the case of small…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ram Brustein , Merav Hadad