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相关论文: Constraining Axions with ZTF J1901+1458

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Axion dark matter can be converted into photons in the magnetospheres of neutron stars leading to a spectral line centred on the Compton wavelength of the axion. Due to the rotation of the star and the plasma effects in the magnetosphere…

宇宙学与河外天体物理 · 物理学 2023-11-29 R. A. Battye , M. J. Keith , J. I. McDonald , S. Srinivasan , B. W. Stappers , P. Weltevrede

Axions that couple to nuclear spins via the axial current interaction can be both produced and detected using nuclear magnetic resonance (NMR) techniques. In this scheme, nuclei driven by a real oscillating magnetic field in one device act…

高能物理 - 唯象学 · 物理学 2025-10-23 Jeff A. Dror , Qiushi Wei , Fengwei Yang

The Tokyo Axion Helioscope experiment aims to detect axions which are produced in the solar core. The helioscope uses a strong magnetic field in order to convert axions into X-ray photons and has a mounting to follow the sun very…

天体物理仪器与方法 · 物理学 2012-01-24 R. Ohta , Y. Akimoto , Y. Inoue , M. Minowa , T. Mizumoto , S. Moriyama , T. Namba , Y. Takasu , A. Yamamoto

Low mass axion-like particles could be produced in abundance within the cores of hot, compact magnetic white dwarf (MWD) stars from electron bremsstrahlung and converted to detectable X-rays in the strong magnetic fields surrounding these…

高能天体物理现象 · 物理学 2024-11-11 Orion Ning , Christopher Dessert , Vi Hong , Benjamin R. Safdi

Axions produced copiously in core-collapse supernovae can convert into photons as they propagate through various astrophysical magnetic fields. The cumulative emission from the cosmic population of supernovae can therefore generate a…

高能物理 - 唯象学 · 物理学 2026-04-21 Brijesh Kanodia , Debajit Bose , Subhadip Bouri , Ranjan Laha

Searches for pseudoscalar axion-like-particles (ALPs) typically rely on their decay in beam dumps or their conversion into photons in haloscopes and helioscopes. We point out a new experimental direction for ALP probes through their…

高能物理 - 唯象学 · 物理学 2020-06-24 James B. Dent , Bhaskar Dutta , Doojin Kim , Shu Liao , Rupak Mahapatra , Kuver Sinha , Adrian Thompson

The search for solar axions produced by Compton ($\gamma+e^-\rightarrow e^-+A$) and bremsstrahlung-like ($e^-+Z \rightarrow Z+e^-+A$) processes has been performed. The axion flux in the both cases depends on the axion-electron coupling…

高能物理 - 实验 · 物理学 2011-02-25 A. V. Derbin , A. S. Kayunov , V. N. Muratova , D. A. Semenov , E. V. Unzhakov

A search for solar axions and axion-like particles produced in the $p+d\rightarrow\rm{^3He}+A~(5.5\rm{ ~MeV})$ reaction was performed using the complete dataset of the Borexino detector (3995 days of measurement live-time). The following…

高能物理 - 实验 · 物理学 2025-10-23 Borexino Collaboration

We present a theoretical model for detecting axions from neutron stars in a QCD phase of quark matter. The axions would be produced from a quark-antiquark pair $u\bar{u}$ or $d\bar{d}$, in loop(s) involving gluons. The chiral anomaly of QCD…

高能天体物理现象 · 物理学 2025-08-11 Bijan Berenji

We present a systematic study of QCD axion production in environments with finite baryon density and temperature, implying significant changes to axion phenomenology. Within heavy baryon chiral perturbation theory, we derive the effective…

高能物理 - 唯象学 · 物理学 2025-03-03 Konstantin Springmann , Michael Stadlbauer , Stefan Stelzl , Andreas Weiler

We show that the magnetic component of the photon field produced by dark matter axions via the two-photon coupling mechanism in a Sikivie Haloscope is an important parameter passed over in previous analysis and experiments. The interaction…

高能物理 - 唯象学 · 物理学 2016-06-13 Ben T. McAllister , Stephen R. Parker , Michael E. Tobar

Axion-like particles (ALPs) can couple to photons in strong magnetic fields, producing characteristic fluctuations in X-ray spectra. Using data from NASA's Neutron Star Interior Composition Explorer (NICER), we analyzed three pulsars: PSR…

高能天体物理现象 · 物理学 2026-02-10 Yen-Jhen Liu , Yi Yang

Axions, if realized in nature, can be copiously produced in the early universe via thermal processes, contributing to the mass-energy density of thermal hot relics. In light of the most recent cosmological observations, we analyze two…

宇宙学与河外天体物理 · 物理学 2021-05-27 William Giarè , Eleonora Di Valentino , Alessandro Melchiorri , Olga Mena

We propose a novel method to detect axions which uniquely depends on the dimensionless axion-photon coupling $g_{\gamma}$, independent of the suppressive axion decay constant $f_a$. Using neutron star PSR B1919+21 data from the…

高能物理 - 唯象学 · 物理学 2025-06-10 Jun-Chen Wang , Shunshun Cao , Jinchen Jiang , Yandong Liu , Qing-Hong Cao , Lijing Shao

The soft X-ray flux produced by solar axions in the Earth's magnetic field is evaluated in the context of ESA's XMM-Newton observatory. Recent calculations of the scattering of axion-conversion X-rays suggest that the sunward magnetosphere…

高能天体物理现象 · 物理学 2014-09-16 G. W. Fraser , A. M. Read , S. Sembay , J. A. Carter , E. Schyns

We show that solar axion conversion to photons in the Earth's magnetosphere can produce an x-ray flux, with average energy \sim 4 keV, which is measurable on the dark side of the Earth. The smallness of the Earth's magnetic field is…

高能物理 - 唯象学 · 物理学 2009-11-11 Hooman Davoudiasl , Patrick Huber

In non-hadronic axion models, which have a tree-level axion-electron interaction, the Sun produces a strong axion flux by bremsstrahlung, Compton scattering, and axio-recombination, the "BCA processes." Based on a new calculation of this…

One of the promising new proposals to search for axions in astrophysical environments is to look for narrow radio lines produced from the resonant conversion of axion dark matter falling through the magnetospheres of neutron stars. For…

高能物理 - 唯象学 · 物理学 2024-01-05 Jonas Tjemsland , Jamie McDonald , Samuel J. Witte

The search for resonant absorption of Compton and bremsstrahlung solar axions by $^{169}$Tm nuclei have been performed. Such an absorption should lead to the excitation of low-lying nuclear energy level: $A+^{169}$Tm $\rightarrow…

高能物理 - 实验 · 物理学 2013-12-03 A. V. Derbin , I. S. Dratchnev , A. S. Kayunov , V. N. Muratova , D. A. Semenov , E. V. Unzhakov