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It is difficult to construct a post-inflation QCD axion model that solves the axion quality problem (and hence the Strong CP problem) without introducing a cosmological disaster. In a post-inflation axion model, the axion field value is…

High Energy Physics - Phenomenology · Physics 2024-08-27 Qianshu Lu , Matthew Reece , Zhiquan Sun

We explore the phenomenology of QCD axion and axion-like particle (ALP) dark matter production via misalignment during inflationary reheating. We investigate scenarios involving inflaton oscillating in a generic potential $\sim \phi^n$,…

High Energy Physics - Phenomenology · Physics 2023-10-13 Yong Xu

The Axion is a particle arising from the Peccei-Quinn solution to the strong CP problem. Peccei-Quinn symmetry breaking in the early universe could produce a large number of axions which would still be present today, making the axion a…

Cosmology and Nongalactic Astrophysics · Physics 2011-12-07 Dmitry Lyapustin

The physical origin of the strong CP problem in QCD, rooted in the structures of the vacuum of the standard model, is reviewed. The chiral solution to this problem, with its accompanying axion, is explained and various characteristics of…

High Energy Physics - Phenomenology · Physics 2011-04-11 R. D. Peccei

The QCD axion in the pre-inflation scenario faces a stringent isocurvature constraint, which requires a relatively low Hubble scale during inflation. If the axion was heavier than the Hubble scale during inflation, its isocurvature is…

High Energy Physics - Phenomenology · Physics 2026-01-19 Priyesh Chakraborty , Junyi Cheng , Matthew Reece , Zekai Wang

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

We propose a solution to the strong CP problem that specifically relies on massless quarks and has no light axion. The QCD color group $SU(3)_c$ is embedded into a larger, simple gauge group (grand-color) where one of the massless, colored…

High Energy Physics - Phenomenology · Physics 2024-08-22 Ravneet Bedi , Tony Gherghetta , Keisuke Harigaya

We construct a theory in which the solution to the strong CP problem is an emergent property of the background of the dark matter in the Universe. The role of the axion degree of freedom is played by multi-body collective excitations…

High Energy Physics - Phenomenology · Physics 2021-08-05 Jason Arakawa , Arvind Rajaraman , Tim M. P. Tait

We present a connection between two known solutions to the strong-CP problem: the standard introduction of axions and the extra-dimensional one, relying on topological arguments. Using an equivalent lower-dimensional set-up with a warped…

High Energy Physics - Theory · Physics 2011-06-13 Yannis Burnier , Florian Kuhnel

We propose a new solution to the strong-CP problem. It involves the existence of an unbroken gauged $U(1)_X$ symmetry whose gauge boson gets a Stuckelberg mass term by combining with a pseudoscalar field $\eta (x)$. The latter has…

High Energy Physics - Phenomenology · Physics 2009-11-07 G. Aldazabal , L. E. Ibanez , A. M. Uranga

The QCD axion was originally predicted as a dynamical solution to the strong CP problem. Axion like particles (ALPs) are also a generic prediction of many high energy physics models including string theory. Theoretical models for axions are…

High Energy Physics - Phenomenology · Physics 2017-12-11 David J. E. Marsh

We study the mirror world with dark matter arising from the thermal freeze-out of the lightest, stable mirror particle -- the mirror electron. The dark matter abundance is achieved for mirror electrons of mass 225 GeV, fixing the mirror…

High Energy Physics - Phenomenology · Physics 2023-02-10 David I. Dunsky , Lawrence J. Hall , Keisuke Harigaya

The axion mass receives a large correction from small instantons if the QCD gets strongly coupled at high energies. We discuss the size of the new CP violating phases caused by the fact that the small instantons are sensitive to the UV…

High Energy Physics - Phenomenology · Physics 2021-07-28 Ryuichiro Kitano , Wen Yin

We point out that the hypothesis of a SU(5)-like supersymmetric Grand Unified Theory (GUT) implies a generic relation within the flavour structure of up-type squarks. Contrary to other well-known SU(5) relations between the down-quark and…

High Energy Physics - Phenomenology · Physics 2015-06-19 Sylvain Fichet , Björn Herrmann , Yannick Stoll

For all the success of the Standard Model (SM), it is on the verge of being surpassed. In this regard we argue, by showing a minimal flavor-structured model based on the non-Abelian discrete $SL_2(F_3)$ symmetry, that $U(1)$…

High Energy Physics - Phenomenology · Physics 2019-02-20 Y. H. Ahn

We construct semi-local and global realizations of SU(5) GUTs in F-theory that utilize a U(1)_PQ symmetry to protect against dimension four proton decay. Symmetries of this type, which assign charges to H_u and H_d that forbid a tree level…

High Energy Physics - Theory · Physics 2010-05-12 Joseph Marsano , Natalia Saulina , Sakura Schafer-Nameki

We construct a flavor model in an anti-SU(5) GUT with a tetrahedral symmetry $A_4$. We choose a basis where $Q_{text{em}}=-\frac13$ quarks and charged leptons are already mass eigenstates. This choice is possible from the $A_4$ symmetry.…

High Energy Physics - Phenomenology · Physics 2020-03-25 Paul H. Frampton , Jihn E. Kim , Se-Jin Kim , Soonkeon Nam

A four-dimensional effective model with $G_{\rm SM}\times SL(2,\mathbb{Z}) \times U(1)_X$ is proposed in string-derived supergravity framework, where $G_{\rm SM}$ is the Standard Model (SM) gauge group and $U(1)_X$ is gauged. We show…

High Energy Physics - Phenomenology · Physics 2026-03-10 Yang Hwan Ahn

The axion is the most attractive candidate to solve the strong CP problem in QCD. If it exists, the inflationary universe produces axion fluctuations which are mixtures of isocurvature and adiabatic fluctuations in general. We investigate…

Astrophysics · Physics 2009-10-30 Toshiyuki Kanazawa , M. Kawasaki , Naoshi Sugiyama , T. Yanagida

The string axion may provide the most attractive solution to the strong CP problem in QCD. However, the axion energy density easily exceeds the dark matter density in the present universe due to a large decay constant around $10^{16}$ GeV,…

High Energy Physics - Phenomenology · Physics 2015-12-24 Masahiro Kawasaki , Tsutomu T. Yanagida , Norimi Yokozaki
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