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Related papers: Naturally astrophobic QCD axion

200 papers

Axion models generically suffer from a severe quality problem when coupled to gravity. In this article we provide a very simple model with a high quality axion. The axion is a pseudo-Nambu-Goldstone boson of the baryon number symmetry,…

High Energy Physics - Phenomenology · Physics 2025-10-10 Prateek Agrawal , Anson Hook , Vazha Loladze , Mario Reig

We consider an axion cloud around a black hole with background magnetic fields. We calculate the decay rate of the axion cloud due to the axion-photon conversion associated with the axion-photon coupling. For simplicity, we consider the…

High Energy Physics - Phenomenology · Physics 2021-12-15 Chul-Moon Yoo , Atsushi Naruko , Yusuke Sakurai , Keitaro Takahashi , Yohsuke Takamori , Daisuke Yamauchi

We propose a minimal model in which the flavour anomaly in the $b \to s \mu^+ \mu^-$ transition is connected to the breaking of Peccei-Quinn (PQ) symmetry. The flavour anomaly is explained from new physics contribution by introducing one…

High Energy Physics - Phenomenology · Physics 2020-12-02 Seungwon Baek

We compute the QCD axion contribution to the energy density of dark radiation, parameterized by $\Delta N_{\rm eff}$, by solving Boltzmann equations for the momentum distribution functions including the effects of quantum statistics for all…

High Energy Physics - Phenomenology · Physics 2025-02-26 Marcin Badziak , Maxim Laletin

Banks and Dine have recently shown that the M theory naturally accommodates the Peccei-Quinn axion. Since the decay constant $F_a$ of the axion is large as $F_a \simeq 10^{15}-10^{16}$GeV, the halo axion is hardly detected in coming…

High Energy Physics - Phenomenology · Physics 2009-10-30 M. Kawasaki , T. Yanagida

We consider a Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axion model extended with two right-handed neutrino fields to realize the minimal type-I seesaw. In this $\nu$DFSZ scheme we systematically determine the simplest quark and lepton…

High Energy Physics - Phenomenology · Physics 2025-12-03 J. R. Rocha , H. B. Câmara , F. R. Joaquim

Axions and other light particles appear ubiquitously in physics beyond the Standard Model, with a variety of possible couplings to ordinary matter. Cosmology offers a unique probe of these particles as they can thermalize in the hot…

Cosmology and Nongalactic Astrophysics · Physics 2022-04-04 Daniel Green , Yi Guo , Benjamin Wallisch

Scalar field dark matter likely is able to solve all small-scale cosmology problems facing the cold dark matter (CDM), and has become an emerging contender to challenge the CDM. It however requires a particle mass $\sim 1 - 2…

Cosmology and Nongalactic Astrophysics · Physics 2014-09-26 Tzihong Chiueh

The properties of axions that constitute 100% of cold dark matter (CDM) depend on the tensor-to-scalar ratio $r$ at the end of inflation. If $r=0.20^{+0.07}_{-0.05}$ as reported by the BICEP2 collaboration, then "half" of the CDM axion…

High Energy Physics - Phenomenology · Physics 2014-07-09 L. Visinelli , P. Gondolo

We propose a minimal realization of the Peccei Quinn mechanism in a realistic SU(5) model, where the axion mass is directly connected to the grand-unification scale. By taking into account constraints from proton decay, collider searches…

High Energy Physics - Phenomenology · Physics 2018-11-21 Luca Di Luzio , Andreas Ringwald , Carlos Tamarit

In an attempt to uncover any underlying physics in the standard model (SM), we suggest a $\mu$--$\tau$ power law in the lepton sector, such that relatively large 13 mixing angle with bi-large ones can be derived. On the basis of this, we…

High Energy Physics - Phenomenology · Physics 2015-03-18 Y. H. Ahn

In order to accommodate the QCD axion as the dark matter (DM) in a model in which the Peccei-Quinn (PQ) symmetry is broken before the end of inflation, a relatively low scale of inflation has to be invoked in order to avoid bounds from DM…

Cosmology and Nongalactic Astrophysics · Physics 2019-09-16 Tommi Tenkanen , Luca Visinelli

In axion gauge field inflation an axion-like particle driving cosmic inflation is coupled to the Chern-Simons density of an Abelian or non-Abelian gauge group. In the case of a non-Abelian gauge group, this can lead to the formation of a…

Cosmology and Nongalactic Astrophysics · Physics 2019-09-24 Valerie Domcke , Stefan Sandner

The recently proposed dark dimension scenario reveals that axions can be localized on the Standard Model brane, thereby predicting the quantum chromodynamics (QCD) axion decay constant from the Weak Gravity Conjecture: $f_a\lesssim M_5 \sim…

High Energy Physics - Theory · Physics 2025-04-15 Hai-Jun Li

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

The presence of a topological susceptibility in the electroweak sector of the Standard Model motivates the existence of a good quality weak axion $a_W$, associated with the spontaneous breaking of $B\!+\!L$. Its anomalous couplings and tiny…

High Energy Physics - Phenomenology · Physics 2025-10-17 Giacomo Cacciapaglia , Francesco Sannino , Jessica Turner

We present a comprehensive study of axion condensed neutron stars that arise in models of an exceptionally light axion that couples to quantum chromodynamics (QCD). These axions solve the strong-charge-parity (CP) problem, but have a…

High Energy Physics - Phenomenology · Physics 2025-08-15 Mia Kumamoto , Junwu Huang , Christian Drischler , Masha Baryakhtar , Sanjay Reddy

We present the first results of searches for axions and axion-like-particles with the XENON100 experiment. The axion-electron coupling constant, $g_{Ae}$, has been probed by exploiting the axio-electric effect in liquid xenon. A profile…

We revisit the domain wall problem for QCD axion models with more than one quark charged under the Peccei-Quinn symmetry. Symmetry breaking during or after inflation results in the formation of a domain wall network which would cause cosmic…

High Energy Physics - Phenomenology · Physics 2023-07-11 Konstantin A. Beyer , Subir Sarkar

We propose simple scenarios where lepton flavor-violating couplings generate the observed dark matter abundance through freeze-in of an axion-like particle with mass in the few keV range. Compared to flavor-diagonal freeze-in, this…

High Energy Physics - Phenomenology · Physics 2023-05-03 Paolo Panci , Diego Redigolo , Thomas Schwetz , Robert Ziegler