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Related papers: Stellar Evolution Bounds on the ALP-Photon Couplin…

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Almost all stars in the 1-8 Msun range evolve through the Asymptotic Giant Branch (AGB), preplanetary nebula (PPN) and planetary nebula (PN) evolutionary phases. Most stars that leave the main sequence in a Hubble time will end their lives…

Understanding the galaxy in which we live is one of the great intellectual challenges facing modern science. With the advent of high quality observational data, the chemical evolution modeling of our galaxy has been the subject of numerous…

Astrophysics · Physics 2009-11-11 Dany Vanbeveren , Erwin De Donder

We extend previous searches for X-ray spectral modulations induced by ALP-photon conversion to a variety of new sources, all consisting of quasars or AGNs located in or behind galaxy clusters. We consider a total of seven new sources, with…

High Energy Astrophysical Phenomena · Physics 2017-07-19 Joseph P. Conlon , Francesca Day , Nicholas Jennings , Sven Krippendorf , Markus Rummel

Low-mass stars play a key role in many different areas of astrophysics. In this article, I provide a brief overview of the evolution of low-mass stars, and discuss some of the uncertainties and problems currently affecting low-mass stellar…

Solar and Stellar Astrophysics · Physics 2015-06-12 M. Catelan

Markarian 421 is a well-known nearby BL Lac blazar at the redshift $z=0.031$. Many previous works were investigated to constrain the axion-photon coupling from its TeV gamma-ray observations, showing the upper limit on the coupling constant…

High Energy Physics - Phenomenology · Physics 2024-10-15 Hai-Jun Li , Wei Chao , Yu-Feng Zhou

We provide a fresh look at the cosmological constraints on axion-like particles (ALPs) that couple predominantly to photons, focusing on lifetimes $\tau_{a} \lesssim 10^{4}\, {\rm s}$ and masses $m_a\lesssim 10\,{\rm GeV}$. We consider Big…

High Energy Physics - Phenomenology · Physics 2026-05-12 Miguel Escudero , Clara Garcia-Perez , Maksym Ovchynnikov

Axion-like particles (ALPs) appear in various new physics models with spontaneous global symmetry breaking. When the ALP mass is in the range of MeV to GeV, the cosmology and astrophysics bounds are so far quite weak. In this work, we…

High Energy Physics - Phenomenology · Physics 2021-12-08 Jie Ren , Daohan Wang , Lei Wu , Jin Min Yang , Mengchao Zhang

The connection between AGB evolution of stellar populations and infrared vs. ultraviolet properties of the parent galaxies is reviewed relying on the updated lookout provided by population-synthesis theory. In particular, planetary-nebula…

Astrophysics · Physics 2007-05-23 Alberto Buzzoni

We reexamine the theoretical limit on the axion coupling to two photons, $g_{a\gamma \gamma}$, in the light of a new solar model (seismic solar model) and the latest solar neutrino observations, the Super-Kamiokande and the Sudbury Neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 Satoru Watanabe , Hiromoto Shibahashi

In this review, we present a self-contained introduction to axion-like particles (ALPs) with a particular focus on their effects on photon polarization: both theoretical and phenomenological aspects are discussed. We derive the photon…

High Energy Physics - Phenomenology · Physics 2024-08-01 Giorgio Galanti

We discuss constraints on soft CP-violating couplings of axion-like particles with photon and fermions by using data on electric dipole moments of Standard Model particles. In particular, for the ALP leptophilic scenario we derive bounds on…

High Energy Physics - Phenomenology · Physics 2020-12-29 D. V. Kirpichnikov , Valery E. Lyubovitskij , Alexey S. Zhevlakov

The thermal evolution of a neutron star is studied by including the energy loss due to axion emission. Two axion models and three types of neutron-star matter equation of state are used with the effects of nucleon superfluidity properly…

Astrophysics · Physics 2007-05-23 Hideyuki Umeda , Naoki Iwamoto , Sachiko Tsuruta , Letao Qin , Ken'ichi Nomoto

By adopting empirical estimates of the Helium enhancement (Delta Y) between consecutive stellar generations for a sample of Galactic globular clusters (GGC), we uniquely constraint the star formation efficiency of each stellar generation in…

Astrophysics of Galaxies · Physics 2019-07-10 Guillermo Tenorio-Tagle , Sergiy Silich , Jan Palous , Casiana Muñoz-Tuñón , Richard Wunsch

Asteroseismology is a very useful tool for exploring the stellar interiors and evolutionary status and for determining stellar fundamental parameters, such as stellar mass, radius, surface gravity, and the stellar mean density. In the…

Solar and Stellar Astrophysics · Physics 2018-05-29 Tao Wu , Yan Li

Neutron stars provide ideal astrophysical laboratories for probing new physics beyond the Standard Model. If axions exist, photons can develop linear polarization during photon-axion conversion in the magnetic field of a neutron star. We…

High Energy Physics - Phenomenology · Physics 2025-02-12 Ningqiang Song , Liangliang Su , Lei Wu

Axionlike particles (ALPs), hypothetical particles beyond the Standard Model, are considered as promising dark matter candidates. ALPs can convert into photons and vice versa in a magnetic field via the Primakoff effect, potentially…

High Energy Physics - Phenomenology · Physics 2025-10-21 Zhi-Qi Guo , Yue-Lin Sming Tsai , Lei Wu , Zi-Qing Xia

In young dense clusters repeated collisions between massive stars may lead to the formation of a very massive star (above 100 Msun). In the past the study of the long-term evolution of merger remnants has mostly focussed on collisions…

Solar and Stellar Astrophysics · Physics 2015-06-16 Evert Glebbeek , Evghenii Gaburov , Simon Portegies Zwart , Onno R. Pols

Many extensions of the Standard Model predict the existence of ALPs, which are very light spin-zero bosons with a two-photon coupling. Photon-ALP oscillations occur in the presence of an external magnetic field, and ALPs can lead to…

High Energy Astrophysical Phenomena · Physics 2015-03-19 Alessandro De Angelis , Giorgio Galanti , Marco Roncadelli

Neutrino experiments lie at the edge of the intensity frontier and therefore can be exploited to search for new light particles weakly coupled to the visible sector. In this work we derive new constraints on axion-like particles (ALPs)…

High Energy Physics - Phenomenology · Physics 2023-10-17 Pilar Coloma , Pilar Hernández , Salvador Urrea

The most massive Galactic globular cluster, Omega centauri, appears to have multiple populations. Its bluest main sequence and extended horizontal branch stars are suggested to have the common origin, that is, an extremely high helium…

Astrophysics · Physics 2009-11-13 Ena Choi , Sukyoung K. Yi
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