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It has been pointed out in the literature that in the presence of an external magnetic field the axion mass receives an electromagnetic contribution. We show that if a magnetic field with energy density larger than ~10^{-8} times the energy…

天体物理学 · 物理学 2009-11-13 L. Campanelli , M. Giannotti

We discuss the decays X^* -> Xe^+e^- (``Dalitz decays'') of excited heavy mesons into their ground states and an electron-positron pair. We argue that the measurement of the invariant mass spectrum of the lepton pair gives clear indication…

高能物理 - 唯象学 · 物理学 2009-10-31 Gad Eilam , Frank Krauss

The decay of a massive pseudoscalar, scalar and U(1) boson into an electron-positron pair in the presence of strong electromagnetic backgrounds is calculated. Of particular interest is the constant-crossed-field limit, relevant for…

高能物理 - 唯象学 · 物理学 2020-01-07 B. King , B. M. Dillon , K. A. Beyer , G. Gregori

The energy loss rate of a magnetized electron gas emitting axions a due to the process $e^- \to e^- +a$ is derived for arbitrary magnetic field strength B. Requiring that for a strongly magnetized neutron star the axion luminosity is…

天体物理学 · 物理学 2008-11-26 M. Kachelriess , C. Wilke , G. Wunner

Electron-positron pairs have been observed in the 10.95-MeV $0^-\to0^+$ decay in $^{16}$O. The branching ratio of the e$^+$e$^-$ pairs compared to the 3.84-MeV $0^-\to2^+$ $\gamma$ decay of the level is deduced to be $20(5)\times10^{-5}$.…

We show existence of strong negative correlation between the temporal variations of magnetic field toroidal component of the solar tachocline (the bottom of convective zone) and the Earth magnetic field (Y-component). The possibility that…

地球与行星天体物理 · 物理学 2010-08-17 V. D. Rusov , E. P. Linnik , K. Kudela , S. Cht. Mavrodiev , T. N. Zelentsova , V. P. Smolyar , K. K. Merkotan

Damping of an electromagnetic wave in a strong magnetic field is analyzed in the kinematic region near the threshold of electron-positron pair production. Damping of the electromagnetic field is shown to be noticeably nonexponential in this…

高能物理 - 唯象学 · 物理学 2010-11-15 N. V. Mikheev , M. V. Chistyakov

The electromagnetic response of three-dimensional topological insulators can be described by an effective axion action with a quantized axion field. Once both time-reversal and inversion symmetries are broken, for example, in…

介观与纳米尺度物理 · 物理学 2025-02-20 Tongshuai Zhu , Huaiqiang Wang , Dingyu Xing , Haijun Zhang

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

We show the existence of the strong inverse correlation between the temporal variations of the toroidal component of the magnetic field in the solar tachocline (the bottom of the convective zone) and the Earth magnetic field (the…

We study the process of neutrino decay to electron and $W$-boson in the external magnetic field using the semiclassical "worldline instanton" approach. Being interested only in the leading exponential factor, we make calculations in a toy…

高能物理 - 唯象学 · 物理学 2015-09-02 Petr Satunin

We consider the vacuum decay by electron-positron pair production in spatially homogeneous, time dependent electric fields by means of quantum kinetic equations. Our focus is on the impact of various pulse shapes as envelopes of oscillating…

高能物理 - 唯象学 · 物理学 2018-04-04 Andreas Otto , Hans Oppitz , Burkhard Kämpfer

We show that Earth's natural environment can serve as a powerful probe for ultralight axion dark matter. In the presence of global geomagnetic fields, the axions with masses ranging from $10^{-15}\,{\rm eV}-10^{-13}\,{\rm eV}$ induce…

高能物理 - 唯象学 · 物理学 2025-09-19 Atsushi Taruya , Atsushi Nishizawa , Yoshiaki Himemoto

The process of the photon decay into the neutrino - antineutrino pair in a magnetic field is investigated. The amplitude and the probability are analysed in the limits of relatively small and strong fields. The probability is suppressed by…

高能物理 - 唯象学 · 物理学 2009-10-30 A. V. Kuznetsov , N. V. Mikheev , L. A. Vassilevskaya

Axion dark matter induces electromagnetic radiation in conductors through nearly perpetual oscillations of electrons, driven by axion-electron interactions through the so-called chiral magnetic effect. It therefore provides a complementary…

高能物理 - 唯象学 · 物理学 2025-07-29 Deog Ki Hong , Sang Hui Im , Jinsu Kim , TaeHun Kim , SungWoo Youn

In the presence of an external magnetic field the axion and the photon mix. In particular, the dispersion relation of a longitudinal plasmon always crosses the dispersion relation of the axion (for small axion masses), thus leading to a…

高能物理 - 唯象学 · 物理学 2020-07-01 Andrea Caputo , Alexander J. Millar , Edoardo Vitagliano

The process of electron-positron pair production by a photon with subsequent annihilation to a single photon in a strong magnetic field has been studied. The general amplitude has been calculated and the process rate have been found in the…

高能物理 - 唯象学 · 物理学 2017-02-14 M. M. Diachenko , O. P. Novak , R. I. Kholodov

We study the axion-photon conversion process in pulsar binary systems with high Shapiro time delay. In these binary systems, the orbital plane is nearly parallel to the line of sight. When the companion star is positioned between the pulsar…

高能天体物理现象 · 物理学 2026-05-29 Zhao-Yang Wang , Hao-Chen Tian , Yun-Feng Liang

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

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