Pith. sign in

REVIEW 20 cited by

Axion Astrophysics

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2411.02492 v2 pith:SDRAP3GK submitted 2024-11-04 hep-ph astro-ph.SRhep-exhep-th

classification hep-phastro-ph.SRhep-exhep-th
keywords starsaxionbeenstellaraccurateadvancesastrophysicsaxions
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Stars have been recognized as optimal laboratories to probe axion properties. In the last decades there have been significant advances in this field due to a better modelling of stellar systems and accurate observational data. In this work we review the current status of constraints on axions from stellar physics. We focus in particular on the Sun, globular cluster stars, white dwarfs and (proto)-neutron stars.

Discussion (0). Sign in to comment.

Forward citations

Cited by 20 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Lights, Camera, Axion: Tracing Axions from Supernovae in the Diffuse $\gamma$-ray Sky

    hep-ph 2026-04 unverdicted novelty 7.0 of 10

    Axions produced in supernovae generate a diffuse gamma-ray signal through conversion in magnetic fields, yielding competitive constraints on the axion-photon coupling from COMPTEL, EGRET, and Fermi-LAT data plus forec...

  2. Solar axion searches with RES-NOVA: projected sensitivity and first prototype limit

    hep-ex 2026-07 conditional novelty 6.0 of 10

    RES-NOVA's projected 1 ton-year sensitivity reaches within a factor of ~2 of XENONnT on the solar-axion electron coupling, and a 32.4 g-day archaeological-lead prototype excludes new parts of the (g_ae, g_aγ) plane.

  3. MeV Electrophilic Axion-like Particles from Sun

    hep-ph 2026-07 conditional novelty 6.0 of 10

    MeV axion-like particles could be made when 5.5 MeV solar fusion photons Compton-scatter off electrons; current LZ, PandaX-4T and Borexino data would then constrain g_ae to (1.7-3.7)e-6 in the 0.4-1 MeV window.

  4. Landau-Zener formula and resonant axion conversion in neutron star magnetospheres

    hep-ph 2026-06 unverdicted novelty 6.0 of 10

    The Landau-Zener approximation for axion-photon conversion in neutron star magnetospheres fails when resonance width exceeds conversion region size, leading to revised axion constraints from optical-band searches.

  5. Heavy Axion from a Confining Mirror GUT

    hep-ph 2026-05 unverdicted novelty 6.0 of 10

    A mirror GUT model confines dynamically to produce a heavy axion solving the strong CP problem while allowing observable EDMs and a rich hidden sector.

  6. Rotation-induced Relaxation of Supernova Constraints on Axionlike Particles

    astro-ph.HE 2026-04 unverdicted novelty 6.0 of 10

    Stellar rotation relaxes supernova energy-loss bounds on axion-like particles by reducing core temperatures but has negligible impact on gamma-ray constraints from SN 1987A.

  7. Axion-photon conversion in stochastic magnetic fields

    hep-ph 2025-12 accept novelty 6.0 of 10

    Axion-photon conversion in random Gaussian magnetic fields fixes the expectation values and variances of photon Stokes parameters, including a circular-polarization signal from helical fields.

  8. Stripped-Envelope Supernovae for QCD Axion Detection

    hep-ph 2025-11 unverdicted novelty 6.0 of 10

    Stripped-envelope supernovae enable QCD axion detection to masses around 10^{-4} eV via gamma-ray signals from conversion in progenitor magnetic fields.

  9. Gamma Rays from ALP-Photon Conversion and Inverse Compton Reprocessing in Neutron Star Magnetospheres

    astro-ph.HE 2026-08 conditional novelty 5.0 of 10

    ALP-to-photon conversion near four pulsars produces mostly sub-MeV emission: Fermi-LAT is insensitive to the channel, COMPTEL data already exclude new parameter space at high ALP mass, and COSI could probe much more.

  10. Reappraisal of the Constraints on Heavy Axion-like Particles from Gamma-Ray Bursts

    hep-ph 2026-07 conditional novelty 5.0 of 10

    Realistic GRB parameters weaken previous ALP cooling bounds, but ALP-induced secondary fireballs in GRBs could still be probed via isotropic X-ray emission from future telescopes.

  11. Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades

    hep-ph 2026-05 unverdicted novelty 5.0 of 10

    Non-thermal photon cascades via Compton reprocessing and positron annihilation in stars create a broad photon spectrum that substantially boosts photon-coupled WISP production, as shown for solar dark photons.

  12. Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities

    hep-ph 2025-09 unverdicted novelty 5.0 of 10

    Analytical expressions for ALP-photon conversion in transient compact stars yield an updated bound g_aγ < 5×10^{-12} GeV^{-1} for m_a ≲ 10^{-9} eV from SN 1987A, plus sensitivity forecasts for future Galactic SN and N...

  13. Spatial resolution studies with the BabyIAXO Micromegas prototype

    physics.ins-det 2025-09 conditional novelty 5.0 of 10

    The IAXO-D1 Micromegas prototype achieves 100 to 300 micrometer spatial resolution at 5 to 10 keV, below the 1 mm BabyIAXO requirement, with simulations matching the measurements.

  14. INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_{i}-L_{j}$ Vectors

    hep-ph 2025-07 unverdicted novelty 5.0 of 10

    This work sets new upper limits on decay lifetimes and couplings for axion-like particles, dark photons, scalars, and B-L or L_i-L_j vector bosons using 511 keV line, X-ray continuum, and cosmic-ray flux observations.

  15. Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling

    hep-ph 2026-06 unverdicted novelty 4.0 of 10

    Varying neutron star core composition with hyperons and Delta resonances mildly affects the QCD axion mass limit from cooling, potentially bringing the DFSZ limit into the IAXO sensitivity window.

  16. NuSTAR as an Axion Helioscope: probing axion-nucleon and axion-electron couplings

    astro-ph.CO 2026-05 unverdicted novelty 4.0 of 10

    NuSTAR solar minimum data sets g_ae · g_aγ ≲ 1.1×10^{-24} GeV^{-1} and g_aN^eff · g_aγ ≲ 2.3×10^{-19} GeV^{-1} at 95% CL for m_a ≲ 10^{-6} eV.

  17. Production of Leptophilic Bosons in Ultradegenerate Relativistic Matter

    hep-ph 2026-05 unverdicted novelty 4.0 of 10

    Derives bremsstrahlung production rates and T-dependent energy-loss scalings for leptophilic bosons in NS cores to enable coupling constraints from cooling data.

  18. Looking for Lights from the Darkness: Signals from MeV-scale Solar Axion-like Particles

    hep-ph 2026-04 unverdicted novelty 4.0 of 10

    Solar axion-like particles up to 5.5 MeV produce off-axis MeV photons via two-body decay, enabling new space and terrestrial searches that could probe g_aγ down to 10^{-12} GeV^{-1}.

  19. Flavor phenomenology of light dark particles

    hep-ph 2026-06 unverdicted novelty 2.0 of 10

    Review surveying limits and prospects for flavor-violating decays of light axion-like particles, highlighting complementarity of lab, astro, and cosmo probes up to 10^12 GeV scales.

  20. Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments

    hep-ph 2026-03 conditional novelty 2.0 of 10

    The meV axion window is presented as a coherent, cross-validated search program in which string theory, stellar cooling, dark matter, and new detector concepts converge on the same mass range.

Pith tools