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Related papers: Solar Axions from Nuclear Transitions

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A calculation of the expected signal due to Primakov coherent conversion of solar axions into photons via Bragg scattering in several solid-state detectors is presented and compared with present and future experimental sensitivities. The…

We estimate the production rate of axion-type particles in the core of the Earth, at a temperature T~5000K. We constrain thermal geo-axion emission by demanding a core-cooling rate less than 100K/Gyr, as suggested by geophysics. This yields…

High Energy Physics - Phenomenology · Physics 2010-04-15 Hooman Davoudiasl , Patrick Huber

We present an XMM-Newton spectrum of diffuse X-ray emission from within the solar system. The spectrum is dominated by probable C VI lines at 0.37 keV and 0.46 keV, an O VII line at 0.56 keV, O VIII lines at 0.65 keV and ~0.8 keV, Ne IX…

Astrophysics · Physics 2009-11-10 S. L. Snowden , M. R. Collier , K. D. Kuntz

Experimental and theoretical state-selective X-ray spectra resulting from single-electron capture in charge exchange (CX) collisions of Ne^10+ with He, Ne, and Ar are presented for a collision velocity of 933 km s^-1 (4.54 keV nucleon^-1),…

High Energy Astrophysical Phenomena · Physics 2015-05-19 R. Ali , P. A. Neill , P. Beiersdorfer , C. L. Harris , D. R. Schultz , P. C. Stancil

We report an extension of charged kaon transverse momentum ($p_T$) spectra at mid-rapidity ($\mid y\mid <$ 0.5) up to 15 GeV/$c$, neutral kaon $p_T$ spectra up to 12 GeV/$c$ using events triggered by the Barrel Electro-Magnetic Calorimeter…

High Energy Physics - Phenomenology · Physics 2009-11-18 Yichun Xu

The thermal evolution of a neutron star is studied by including the energy loss due to axion emission. Two axion models and three types of neutron-star matter equation of state are used with the effects of nucleon superfluidity properly…

Astrophysics · Physics 2007-05-23 Hideyuki Umeda , Naoki Iwamoto , Sachiko Tsuruta , Letao Qin , Ken'ichi Nomoto

Dark matter axions may cause transitions between atomic states that differ in energy by an amount equal to the axion mass. Such energy differences are conveniently tuned using the Zeeman effect. It is proposed to search for dark matter…

High Energy Physics - Phenomenology · Physics 2020-06-02 P. Sikivie

We constrain the coupling of thermally-produced axion-like particles (here axions) with photons and gluons, using data from the cosmic microwave background (CMB) spectra and baryon acoustic oscillations. The axion possesses an explicit soft…

Cosmology and Nongalactic Astrophysics · Physics 2022-09-12 Luca Caloni , Martina Gerbino , Massimiliano Lattanzi , Luca Visinelli

We derive constraints on the coupling constants of axion-like particles to nucleons and on the Yukawa-type corrections to Newton's gravitational law from the results of recent experiment on measuring the difference of Casimir forces between…

High Energy Physics - Phenomenology · Physics 2017-07-05 G. L. Klimchitskaya , V. M. Mostepanenko

Results are reported of an experimental search for the unique, rapidly varying temporal pattern of solar axions coherently converting into photons via the Primakoff effect in a single crystal germanium detector. This conversion is predicted…

The production of non-phi K+K- pairs by protons of 2.83 GeV kinetic energy on C, Cu, Ag, and Au targets has been investigated using the COSY-ANKE magnetic spectrometer. The K- momentum dependence of the differential cross section has been…

We investigate the effect of the axion cooling on the nucleosynthesis in a massive star with $16M_{\odot}$ by standard stellar evolution calculation. We find that the axion cooling suppresses the nuclear reactions in carbon, oxygen and…

Solar and Stellar Astrophysics · Physics 2015-10-07 Shohei Aoyama , Takeru K. Suzuki

Primordial decays of string theory moduli at z \sim 10^{12} naturally generate a dark radiation Cosmic Axion Background (CAB) with 0.1 - 1 keV energies. This CAB can be detected through axion-photon conversion in astrophysical magnetic…

Cosmology and Nongalactic Astrophysics · Physics 2014-05-26 Joseph P. Conlon , M. C. David Marsh

We present a novel approach to investigating axions and axion-like particles (ALPs) by studying their potential conversion into X-rays within the Sun's atmospheric magnetic field. Utilizing high-sensitivity data from the Nuclear…

When axion stars fly through an astrophysical magnetic background, the axion-to-photon conversion may generate a large electromagnetic radiation power. After including the interference effects of the spacially-extended axion-star source and…

High Energy Astrophysical Phenomena · Physics 2018-04-11 Yang Bai , Yuta Hamada

We present systematic case studies to investigate the sensitivity of axion searches by liquid xenon detectors, using the axio-electric effect (analogue of the photoelectric effect) on xenon atoms. Liquid xenon is widely considered to be one…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 K. Arisaka , P. Beltrame , C. Ghag , J. Kaidi , K. Lung , A. Lyashenko , R. D. Peccei , P. Smith , K. Ye

Azimuthal correlations of charged particles in xenon-xenon collisions at a center-of-mass energy per nucleon pair of $ \sqrt{s_{_\mathrm{NN}}} =$ 5.44 TeV are studied. The data were collected by the CMS experiment at the LHC with a total…

High Energy Physics - Experiment · Physics 2019-10-16 CMS Collaboration

Axions provide a natural and well-motivated dark matter candidate, with the capability to convert directly to photons in the presence of an electromagnetic field. A particularly compelling observational target is the conversion of dark…

We investigate the prospect of an alternative laboratory-based search for the coupling of axions and axion-like particles to photons. Here, the collision of two laser beams resonantly produces axions, and a signal photon is detected after…

High Energy Physics - Phenomenology · Physics 2020-05-18 K. A. Beyer , G. Marocco , R. Bingham , G. Gregori

Neutrino and axion production in neutron stars occurs mainly as bremsstrahlung from nucleon-nucleon (NN) scattering. The energy radiated via neutrinos or axions is typically very small compared to other scales in the two-nucleon system. The…

Astrophysics · Physics 2009-10-31 Christoph Hanhart , Daniel R. Phillips , Sanjay Reddy