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Orbiting $\gamma$-detectors combined with the magnetic field of the Earth or the Sun can work parasitically as cosmic axion telescopes. The relatively short field lengths allow the axion-to-photon conversion to be coherent for $m_{axion}…

天体物理学 · 物理学 2009-10-30 K. Zioutas , D. J. Thompson , E. A. Paschos

Axions generated thermally in the solar core can convert nearly directly to X-rays as they pass through the solar atmosphere via interaction with the magnetic field. The result of this conversion process would be a diffuse…

太阳与恒星天体物理 · 物理学 2012-01-24 Hugh S. Hudson , L. W. Acton , E. DeLuca , I. G. Hannah , K. Reardon , K. Van Bibber

Supernovae provide fascinating opportunities to study various particles and their interactions. Among these there are neutrinos, axions, and other light weakly interacting particles, which play a significant role in our understanding of…

高能物理 - 唯象学 · 物理学 2023-09-27 Pierluca Carenza

The axion solution of the strong CP problem provides a number of possible windows to physics beyond the standard model, notably in the form of searches for solar axions and for galactic axion dark matter, but in a broader context also…

高能物理 - 唯象学 · 物理学 2008-11-26 Georg G. Raffelt

The origin of various celestial phenomena have remained mysterious for conventional astrophysics. Therefore, alternative solutions should be considered, taking into account the involvement of unstable dark-matter particle candidates, such…

天体物理学 · 物理学 2007-05-23 K. Zioutas , Y. Semertzidis , Th. Papaevangelou

The possibility of detection of 5.5 MeV and 14.4 keV solar axions by observing axion-induced nuclear and atomic transitions is investigated. The presence of nuclear transitions between spin-orbit partners can be manifested by the subsequent…

高能物理 - 唯象学 · 物理学 2021-12-14 John D. Vergados , Paraskevi C. Divari , Hiroyasu Ejiri

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 CAST (CERN Axion Solar Telescope) experiment at CERN searches for solar axions with energies in the keV range. It is possible that axions are produced in the core of the sun by the interaction of thermal photons with virtual photons of…

高能物理 - 实验 · 物理学 2007-05-23 Donghwa Kang

The working principle of axion helioscopes can be behind unexpected solar X-ray emission, being associated with solar magnetic fields, which become the catalyst. Solar axion signals can be transient brightenings as well as continuous…

天体物理学 · 物理学 2016-11-09 K. Zioutas , M. Tsagri , Y. Semertzidis , Th. Papaevangelou , A. Nordt , V. Anastassopoulos

Hypothetical axion-like particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field they would be transformed into X-rays with energies of a few keV. The CAST experiment at…

高能物理 - 实验 · 物理学 2019-08-14 Berta Beltran

Relativistic axions can be readily produced in a broad variety of transient sources, such as axion star bosenova explosions, supernovae or even evaporating primordial black holes. We develop a general framework describing the resulting…

高能物理 - 唯象学 · 物理学 2024-03-13 Joshua Eby , Volodymyr Takhistov

If axions or axion-like particles exist and are detected, they will not only extend the standard model of particle physics but will also open a new way to probe their sources. Axion helioscopes aim to detect axions which are produced in the…

太阳与恒星天体物理 · 物理学 2020-01-28 Joerg Jaeckel , Lennert J. Thormaehlen

Axions are expected to be produced in the sun via the Primakoff process. They may be detected through the inverse process in the laboratory, under the influence of a strong magnetic field, giving rise to X-rays of energies in the range of a…

高能物理 - 实验 · 物理学 2009-01-06 Christos Eleftheriadis

Axions can be copiously produced in localized regions of neutron star magnetospheres where the ambient plasma is unable to efficiently screen the induced electric field. As these axions stream away from the neutron star they can resonantly…

高能物理 - 唯象学 · 物理学 2023-07-26 Dion Noordhuis , Anirudh Prabhu , Samuel J. Witte , Alexander Y. Chen , Fábio Cruz , Christoph Weniger

A brief review of particle physics motivations for axion existence is followed by a discussion of optical observables that can be used for axion detection. It is emphasised that the resonant photon - axion transition can occur in the…

高能物理 - 唯象学 · 物理学 2009-09-25 Ryszard Stroynowski , Ariel R. Zhitnitsky

Axion-like particles lead to a plethora of new phenomena relating to compact astrophysical objects including stellar and black hole superradiance, axion stars and axion clusters. In this work, we investigate a new scenario in which…

宇宙学与河外天体物理 · 物理学 2018-08-08 B Garbrecht , J I McDonald

Magnetic field dependent transient solar observations are suggestive for axion-photon oscillations with light axion(-like) particle involvement. Novel dark-moon measurements with the SMART X-ray detectors can be conclusive for radiatively…

Magnetic fields mix axions with photons, allowing for the cyclotron process e -> e + a by virtue of an intermediate plasmon even if axions do not couple to electrons at tree level. The axion and longitudinal-plasmon dispersion relations…

高能物理 - 唯象学 · 物理学 2009-10-31 N. V. Mikheev , G. Raffelt , L. A. Vassilevskaya

We present a novel method for the search of high energy extraterrestrial neutrinos in extended regions. The method is based on the study of the spatial correlations between the events recorded by neutrino telescopes. Extended regions…

高能天体物理现象 · 物理学 2015-06-12 Yolanda Sestayo , Elisa Resconi

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
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