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In this work, we investigate the impact of uncertainties due to convective boundary mixing (CBM), commonly called `overshoot', namely the boundary location and the amount of mixing at the convective boundary, on stellar structure and…

Solar and Stellar Astrophysics · Physics 2020-07-20 Etienne A. Kaiser , Raphael Hirschi , W. David Arnett , Cyril Georgy , Laura J. A. Scott , Andrea Cristini

We search for the existence of ultralight axions coupling to electrons and photons using data from the NuSTAR telescope directed toward the galaxies M82, M87, and M31. We focus on electron bremsstrahlung and Compton scattering for axion…

High Energy Physics - Phenomenology · Physics 2025-03-14 Orion Ning , Benjamin R. Safdi

Convective boundary mixing (CBM) in the advanced evolutionary stages of massive stars is not well understood. Structural changes caused by convection have an impact on the evolution as well as the subsequent supernova, or lack thereof. The…

Solar and Stellar Astrophysics · Physics 2018-12-26 Austin Davis , Sam Jones , Falk Herwig

Astrophysical gamma-ray sources come in a variety of sizes and magnetizations. We deduce general conditions under which gamma-ray spectra from such sources would be significantly affected by axion-photon mixing. We show that, depending on…

Astrophysics · Physics 2008-11-26 Kathrin A. Hochmuth , Guenter Sigl

The discovery of an axion-like particle above the QCD line would rule out Grand Unified Theories, including the perturbative heterotic string with the Standard Model embedded in a single $E_8$ factor or $SO(32)$. In this work we study a…

High Energy Physics - Theory · Physics 2025-11-19 Mario Reig , Timo Weigand

The treatment of convective boundaries remains an important source of uncertainty within stellar evolution, with drastic implications for the thermally-pulsing stars on the Asymptotic Giant Branch (AGB). Various sources are taken as…

Solar and Stellar Astrophysics · Physics 2020-02-19 Graham Wagstaff , Marcelo M. Miller Bertolami , Achim Weiß

The Humphreys-Davidson (HD) limit empirically defines a region of high luminosities (log L > 5.5) and low effective temperatures (T < 20kK) on the Hertzsprung-Russell Diagram in which hardly any supergiant stars are observed. Attempts to…

Solar and Stellar Astrophysics · Physics 2021-02-17 Avishai Gilkis , Tomer Shenar , Varsha Ramachandran , Adam S. Jermyn , Laurent Mahy , Lidia M. Oskinova , Iair Arcavi , Hugues Sana

We apply novel, recently developed plasma ray-tracing techniques to model the propagation of radio photons produced by axion dark matter in neutron star magnetospheres and combine this with both archival and new data for the galactic centre…

Cosmology and Nongalactic Astrophysics · Physics 2022-01-13 R. A. Battye , J. Darling , J. McDonald , S. Srinivasan

Context: Internal chemical mixing in intermediate- and high-mass stars represents an immense uncertainty in stellar evolution models.In addition to extending the main-sequence lifetime, chemical mixing also appreciably increases the mass of…

Solar and Stellar Astrophysics · Physics 2021-11-10 Cole Johnston

We revise the bound from the supernova SN1987A on the coupling of ultralight axion-like particles (ALPs) to photons. In a core-collapse supernova, ALPs would be emitted via the Primakoff process, and eventually convert into gamma rays in…

High Energy Astrophysical Phenomena · Physics 2015-02-09 Alexandre Payez , Carmelo Evoli , Tobias Fischer , Maurizio Giannotti , Alessandro Mirizzi , Andreas Ringwald

The QCD axion has important connections to early universe cosmology. For example, it is often said that isocurvature limits rule out a combination of high axion decay constant, $f_a$, and high inflationary Hubble scale, $H_I$. High scales…

High Energy Physics - Phenomenology · Physics 2025-12-23 Peter W. Graham , Davide Racco

Axion-like particles (ALPs) are hypothetical pseudoscalar bosons that arise in many extensions of the Standard Model and are well-motivated dark matter candidates. Nearby massive stars in the late stages of stellar evolution provide a…

Axion-like particles (ALPs) provide a compelling avenue for exploring physics beyond the Standard Model. In astrophysical magnetized plasmas an ALP-photon coupling $g_{a\gamma}$ induces energy-dependent oscillations in the photon survival…

High Energy Astrophysical Phenomena · Physics 2025-07-30 Yu Zhou , Jiejia Liu , Volodymyr Takhistov , Kazuhisa Mitsuda

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

We study the evolution of binary stars in globular clusters using a novel approach combining a state-of-the-art population synthesis code with a simple treatment of dynamical interactions in the dense cluster core. We find that the…

Astrophysics · Physics 2007-05-23 N. Ivanova , K. Belczynski , J. M. Fregeau , F. A. Rasio

We report new searches for the solar axions and galactic axion-like dark matter particles, using the first low-background data from PandaX-II experiment at China Jinping Underground Laboratory, corresponding to a total exposure of about…

We present a novel approach to investigating axions and axion-like particles (ALPs) by studying their potential conversion into X-rays within the Sun's atmospheric magnetic field. Utilizing high-sensitivity data from the Nuclear…

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

Context. Massive contact binaries are both stellar merger and gravitational wave progenitors, but their evolution is still uncertain. An open problem in the population synthesis of massive contact binaries is the predicted mass ratio…

Solar and Stellar Astrophysics · Physics 2025-02-26 Jelle Vandersnickt , Matthias Fabry
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