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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…

High Energy Physics - Experiment · Physics 2025-10-23 Borexino Collaboration

We consider the dimming of photons from high redshift type 1a supernovae by mixing with a pseudoscalar axion field in the intergalactic medium. We model the electron density using a lognormal probability distribution and assume frozen in…

Astrophysics · Physics 2009-11-07 Mattias Christensson , Malcolm Fairbairn

Excited conduction electrons, conduction holes, and valence holes in monolayer electron-doped graphene exhibit unusual Coulomb decay rates. The deexcitation processes are studied using the screened exchange energy. They might utilize the…

Mesoscale and Nanoscale Physics · Physics 2019-02-26 Chih-Wei Chiu , Chiun-Yan Lin , Rong-Bin Chen

Several mechanisms have been proposed to generate primordial magnetic fields and it is often assumed that magnetic fields are not affected by a sharp drop in ionization rate due to the cosmic recombination. We investigate the validity of…

Astrophysics · Physics 2008-04-23 Keitaro Takahashi

Once formed in a supernova explosion, a neutron star cools rapidly via neutrino emission during the first 10^4-10^5 yr of its life-time. Here we compute the axion emission rate from baryonic components of a star at temperatures below their…

Cosmology and Nongalactic Astrophysics · Physics 2012-11-27 Jochen Keller , Armen Sedrakian

The impact of strong magnetic fields B>10e13 G on the thermal evolution of neutron stars is investigated, including crustal heating by magnetic field decay. For this purpose, we perform 2D cooling simulations with anisotropic thermal…

Astrophysics · Physics 2010-11-11 Deborah N. Aguilera , José A. Pons , Juan A. Miralles

We study the evolution of axions interacting with primordial magnetic fields (PMFs) starting just from the QCD phase transition in the expanding universe. This interaction is owing to the Primakoff effect. Adopting the zero mode…

High Energy Physics - Phenomenology · Physics 2020-12-17 Maxim Dvornikov , V. B. Semikoz

Influence of permanent magnetic field up to 7.5 T on plasma emission and laser-assisted Au nanoparticles fragmentation in water is experimentally studied. It is found that presence of magnetic field causes the breakdown plasma emission to…

The motional electric field experienced by an H2+ ion moving in a magnetic field induces an electric dipole, so that one-photon dipole transitions between rovibrational states become allowed. Field induced spontaneous decay rates are…

Atomic Physics · Physics 2018-12-12 Jean-Philippe Karr

We use a modified pulsar current analysis to study magnetic field decay in radio pulsars. In our approach we analyse the flow, not along the spin period axis as has been performed in previous studies, but study the flow along the direction…

High Energy Astrophysical Phenomena · Physics 2014-09-30 A. P. Igoshev , S. B. Popov

Axion-photon oscillation refers to the process of mutual conversion between photons and axions when they propagate in a magnetic field. This process depends on the strength of the background magnetic field, and magnetic white dwarfs provide…

High Energy Physics - Phenomenology · Physics 2026-05-29 Hao-Chen Tian , Zhao-Yang Wang , Yun-Feng Liang , Zhao-Wei Du

The width of the neutrino decay into the electron and $W$ boson in a strong external magnetic field is obtained from the imaginary part of the neutrino self-energy. This result corrects the formulae existing in the literature. The mean free…

High Energy Physics - Phenomenology · Physics 2010-10-05 A. V. Kuznetsov , N. V. Mikheev , A. V. Serghienko

Muons decay in vacuum mainly via the leptonic channel to an electron, a muon neutrino and an electron antineutrino. Previous investigations have concluded that muon decay can only be significantly altered in a strong electromagnetic field…

High Energy Physics - Phenomenology · Physics 2026-01-09 B. King , D. Liu

We present a new mechanism to deplete the energy density of the QCD axion, making decay constants as high as $f_a \simeq 10^{17}\,\rm{GeV}$ viable for generic initial conditions. In our setup, the axion couples to a massless dark photon…

High Energy Physics - Phenomenology · Physics 2018-04-04 Prateek Agrawal , Gustavo Marques-Tavares , Wei Xue

Optical orientation of localized/bound excitons is shown to be effectively enhanced by the application of magnetic fields as low as 20 mT in monolayer WS$_2$. At low temperatures, the evolution of the polarization degree of different…

We study the exciton magnetic polaron (EMP) formation in (Cd,Mn)Se/(Cd,Mg)Se diluted-magnetic-semiconductor quantum wells using time-resolved photoluminescence (PL). The magnetic field and temperature dependencies of this dynamics allow us…

The dynamics of an argon plasma in the gap of a thermionic diode is investigated using particle-in-cell (PIC) simulations. The time-averaged diode current, as a function of the relative electrical potential between the electrodes, is…

Plasma Physics · Physics 2021-02-24 R. E. Groenewald , S. Clark , A. Kannan , P. Scherpelz

In the presence of a background magnetic field, axion dark matter induces an electric field and can thus excite phonon-polaritons in suitable materials. We revisit the calculation of the axion-photon conversion power output from such…

High Energy Physics - Phenomenology · Physics 2023-04-18 David J. E. Marsh , Jamie I. McDonald , Alexander J. Millar , Jan Schütte-Engel

The lifetime of two dimensional electrons in GaAs quantum wells, placed in weak quantizing magnetic fields, is measured using a simple transport method in broad range of temperatures from 0.3 K to 20 K. The temperature variations of the…

Mesoscale and Nanoscale Physics · Physics 2015-05-30 Scott Dietrich , S. A. Vitkalov , D. V. Dmitriev , A. A. Bykov

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…

Earth and Planetary Astrophysics · Physics 2010-08-17 V. D. Rusov , E. P. Linnik , K. Kudela , S. Cht. Mavrodiev , T. N. Zelentsova , V. P. Smolyar , K. K. Merkotan