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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…

太阳与恒星天体物理 · 物理学 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…

高能物理 - 唯象学 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

天体物理学 · 物理学 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…

高能物理 - 理论 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能物理 - 唯象学 · 物理学 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…

高能天体物理现象 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

天体物理学 · 物理学 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…

高能物理 - 唯象学 · 物理学 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…

太阳与恒星天体物理 · 物理学 2025-02-26 Jelle Vandersnickt , Matthias Fabry