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Related papers: Stellar cooling anomalies and variant axion models

200 papers

X-ray spectroscopy of cooling-flow clusters reveal an unexpected deficit of soft X-ray emission lines from gas at ~1/3 of the ambient plasma temperature, across a wide range of X-ray luminosities and virial temperatures. We propose excess…

Astrophysics · Physics 2009-11-10 S. Peng Oh

The extreme conditions within the supernova core, a high-temperature and high-density environment, create an ideal laboratory for the search for new physics beyond the Standard Model. Of particular interest are low-energy supernovae,…

High Energy Physics - Phenomenology · Physics 2025-12-11 Zi-Miao Huang , Zuowei Liu

Strong evidence for cooling flows has been found in low resolution X-ray imaging and spectra of many clusters of galaxies. However high resolution X-ray spectra of several clusters from the Reflection Grating Spectrometer (RGS) on…

Astrophysics · Physics 2009-10-31 A. C. Fabian , R. F. Mushotzky , P. E. J. Nulsen , J. R. Peterson

We show that the hybrid inflation is naturally realized in the framework of a supersymmetric axion model, which is consistent with the WMAP observation if the Peccei-Quinn symmetry breaking scale is around 10^{15}GeV. By solving the post…

High Energy Physics - Phenomenology · Physics 2015-03-19 Masahiro Kawasaki , Naoya Kitajima , Kazunori Nakayama

We show that supersymmetric axion models breaking the PQ symmetry by the interplay of non-renormalizable supersymmetric terms and soft supersymmetry breaking terms provide a natural framework not only for generating the axion scale from…

High Energy Physics - Phenomenology · Physics 2015-06-19 Eung Jin Chun

Axion-like particles are predicted in many physics scenarios beyond the Standard Model (SM). Their interactions with SM particles may arise from the triangle anomaly of the associated global symmetry, along with other SM global and gauge…

High Energy Physics - Phenomenology · Physics 2024-05-03 Yang Bai , Carlos Henrique de Lima

The basic mechanisms responsible for producing winds from cool, late-type stars are still largely unknown. We take inspiration from recent progress in understanding solar wind acceleration to develop a physically motivated model of the…

Solar and Stellar Astrophysics · Physics 2015-05-30 Steven R. Cranmer , Steven H. Saar

The axion kinetic misalignment mechanism (KMM) opens the possibility of explaining dark matter for almost any axion mass and decay constant that are not accessible by the standard misalignment mechanism, in particular at low values of the…

High Energy Physics - Phenomenology · Physics 2024-08-19 Cem Eröncel , Ryosuke Sato , Géraldine Servant , Philip Sørensen

At finite temperature, the coupling of an axion to non-Abelian gauge fields causes dissipation due to sphaleron heating. This mechanism has been considered as ideal for realizing warm inflation since it can lead to large thermal friction…

High Energy Physics - Phenomenology · Physics 2025-10-21 Sebastian Zell

Recent work has shown that axions can be efficiently produced via non-stationary pair plasma discharges in the polar cap region of pulsars. Here, we point out that for axion masses $10^{-9} \, {\rm eV} \lesssim m_a \lesssim 10^{-4} \, \rm…

High Energy Physics - Phenomenology · Physics 2024-10-08 Dion Noordhuis , Anirudh Prabhu , Christoph Weniger , Samuel J. Witte

Solutions to the $\mu$ problem in supersymmetry based on the Kim-Nilles mechanism naturally feature a Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axion with decay constant of order the geometric mean of the Planck and TeV scales, consistent…

High Energy Physics - Phenomenology · Physics 2021-09-22 Prudhvi N. Bhattiprolu , Stephen P. Martin

If axions exist they are efficiently produced in the hot and dense interior of stars, providing a novel energy-loss mechanism. In order to avoid a conflict with the observed properties of stars, one can derive a lower limit on the…

High Energy Physics - Phenomenology · Physics 2008-02-03 Georg Raffelt

Axions are the natural consequence of the introduction of the Peccei-Quinn symmetry to solve the strong CP problem. All the efforts to detect such elusive particles have failed up to now. Nevertheless, it has been recently shown that the…

Solar and Stellar Astrophysics · Physics 2015-05-18 J. Isern , E. García-Berro , L. G. Althaus , A. H. Córsico

We propose a Standard Model extension, coined VISH$\nu$ (Variant-axIon Seesaw Higgs $\nu$-trino), that is an $N_{\text{DW}} = 1$ variation of its predecessor, the $\nu$DFSZ model. In accounting for the origin of neutrino masses, dark matter…

High Energy Physics - Phenomenology · Physics 2022-12-06 Alexei H. Sopov , Raymond R. Volkas

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 QCD axion is a well-motivated hypothetical particle beyond the Standard Model (SM) and a compelling dark matter candidate. Its relic abundance is highly sensitive to the thermal history of the universe when the temperature is around the…

High Energy Physics - Phenomenology · Physics 2025-06-26 Kun-Feng Lyu , Yue Zhao

We analyze the most salient cosmological features of axions in extensions of the Standard Model with a gauged anomalous extra U(1) symmetry. The model is built by imposing the constraint of gauge invariance in the anomalous effective…

High Energy Physics - Phenomenology · Physics 2015-03-17 Claudio Coriano , Marco Guzzi , George Lazarides , Antonio Mariano

We consider a type I or type X two Higgs doublets model with a modified lepton sector. The generalized lepton sector is also flavor conserving but with the new Yukawa couplings completely decoupled from lepton mass proportionality. The…

High Energy Physics - Phenomenology · Physics 2023-02-08 Francisco J. Botella , Fernando Cornet-Gomez , Carlos Miró , Miguel Nebot

We study collider implications of variant axion models which naturally avoid the cosmological domain wall problem. We find that in such models the branching ratio of $h \to \gamma\gamma$ can be enhanced by a factor of 5 up to 30 as compared…

High Energy Physics - Phenomenology · Physics 2014-11-21 Chuan-Ren Chen , Paul H. Frampton , Fuminobu Takahashi , Tsutomu T. Yanagida

The CERN Axion Solar Telescope (CAST) experiment searches for solar axions by the "helioscope" method. First results imply an upper limit on the axion-photon coupling of g_a-gamma < 1.16 x 10^-10 GeV^-1 (95% CL) for m_a < 0.02 eV, in this…

High Energy Physics - Phenomenology · Physics 2007-05-23 Georg G. Raffelt