Javascript must be enabled to continue!
NuSTAR as an Axion Helioscope
View through CrossRef
We present a novel approach to investigating axions and axionlike particles by studying their potential conversion into x-rays within the Sun’s atmospheric magnetic field. Utilizing high-sensitivity data from the nuclear spectroscopic telescope array (NuSTAR) collected during the 2020 solar minimum, along with advanced solar atmospheric magnetic field models, we establish a new limit on the axion-photon coupling strength gaγ≲7.3×10−12 GeV−1 at 95% CL for axion masses ma≲4×10−7 eV. This constraint surpasses current ground-based experimental limits, studying previously unexplored regions of the axion-photon coupling parameter space up to masses of ma≲3.4×10−4 eV. These findings mark a significant advancement in our ability to probe axion properties and strengthen indirect searches for dark matter candidates.
American Physical Society (APS)
Title: NuSTAR as an Axion Helioscope
Description:
We present a novel approach to investigating axions and axionlike particles by studying their potential conversion into x-rays within the Sun’s atmospheric magnetic field.
Utilizing high-sensitivity data from the nuclear spectroscopic telescope array (NuSTAR) collected during the 2020 solar minimum, along with advanced solar atmospheric magnetic field models, we establish a new limit on the axion-photon coupling strength gaγ≲7.
3×10−12 GeV−1 at 95% CL for axion masses ma≲4×10−7 eV.
This constraint surpasses current ground-based experimental limits, studying previously unexplored regions of the axion-photon coupling parameter space up to masses of ma≲3.
4×10−4 eV.
These findings mark a significant advancement in our ability to probe axion properties and strengthen indirect searches for dark matter candidates.
Related Results
Source number counts at high energies: Swift versus NuSTAR
Source number counts at high energies: Swift versus NuSTAR
The hard X-ray sky at energies above 10 keV has been extensively explored by the Swift/Gehrels and the NuSTAR missions in the 14−195 keV and the 3−24 keV bands. respectively. The m...
The QCD axion sum rule
The QCD axion sum rule
Abstract
We demonstrate that the true QCD axion that solves the strong CP problem can be found in all generality outside the customary standard QCD band, with ...
Digging into Axion Physics with (Baby)IAXO
Digging into Axion Physics with (Baby)IAXO
Dark matter searches have been ongoing for three decades; the lack of a positive discovery of the main candidate, the WIMP, after dedicated efforts, has put axions and axion-like p...
NuSTAR as an Axion Helioscope
NuSTAR as an Axion Helioscope
Abstract
The nature of dark matter in the Universe is still an open question in astrophysics and cosmology. Axions and axionlike particles (ALPs) offer a compelling solutio...
Novel strategies for new low-mass particles searches at Colliders and from Stellar Objects
Novel strategies for new low-mass particles searches at Colliders and from Stellar Objects
Nouvelles stratégies pour la recherche de nouvelles particules légères dans les collisionneurs et des objets stellaires
Le Modèle Standard (SM) de la physique des p...
Axion Bose--Einstein Condensates and Astrophysical Implications
Axion Bose--Einstein Condensates and Astrophysical Implications
The prospect that dark matter axions may form Bose–Einstein condensates (BECs) establishes a profound connection between particle physics, condensed matter theory, and astrophysics...
Axion assisted Schwinger effect
Axion assisted Schwinger effect
Abstract
We point out an enhancement of the pair production rate of charged fermions in a strong electric field in the presence of time dependent classical axi...
Structured-light control of axion electrodynamics in topological insulator scattering
Structured-light control of axion electrodynamics in topological insulator scattering
Abstract
Topological insulators exhibit an axion-mediated magnetoelectric response that generates cross-polarised scattering channels strictl...

