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相关论文: Orthopositronium: Annihilation of positron in gase…

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Positronium annihilation amplitudes that are computed by assuming a factorization approximation with on-shell intermediate leptons, do not exhibit good analytical behavior. We propose an ansatz which allows to include binding energy…

高能物理 - 唯象学 · 物理学 2007-05-23 G. Lopez Castro , J. Pestieau , C. Smith

Order alpha^2 contribution to the orthopositronium decay rate due to one-photon virtual annihilation is found to be delta Gamma = (alpha/pi)^2 (pi^2 ln(alpha) - 0.8622(9))Gamma_LO.

高能物理 - 唯象学 · 物理学 2009-10-31 Gregory Adkins , Kirill Melnikov , Alexander Yelkhovsky

We have obtained spectra of the Galactic center at energies 400-600 keV from high-resolution data acquired by the TGRS Ge spectrometer on board the WIND mission during 1995-1997. The data were obtained using an on-board occulter, and are…

天体物理学 · 物理学 2009-10-30 M. J. Harris , B. J. Teegarden , T. L. Cline , N. Gehrels , D. M. Palmer , R. Ramaty , H. Seifert

Positron lifetime spectra were measured in liquid water at temperatures between 0c and 50c. The long lifetime of ortho-positronium atoms (o-Ps) determined by electron pick-off in molecular substances decreases smoothly by 10% as the…

其他凝聚态物理 · 物理学 2009-11-10 Katsushige Kotera , Tadashi Saito , Taku Yamanaka

Historical Type Ia supernovae are a leading candidate for the source of positrons observed through their diffuse annihilation emission in the Galaxy. However, search for annihilation emission from individual Type Ia supernovae has not been…

天体物理学 · 物理学 2009-11-11 E. Kalemci , S. E. Boggs , P. A. Milne , S. P. Reynolds

Even 50 years after the discovery of a positron annihilation line from the inner Galaxy, no class of astrophysical sources has emerged as a definitive explanation for both the emission morphology and flux. Positrons produced by dark matter…

高能天体物理现象 · 物理学 2025-06-03 Souradeep Das , Mark R. Krumholz , Roland M. Crocker , Thomas Siegert , Laura Eisenberger

The life-time of the four-body atomic system MuPs ($\mu^{+} e^{-}_2 e^{+}$ or muonium-positronium) against positron annihilation has been evaluated as $\tau = \frac{1}{\Gamma} \approx 4.076453 \cdot 10^{-10}$ $sec$. Various annihilation…

高能物理 - 唯象学 · 物理学 2015-05-28 Alexei M. Frolov

The possibility of channeling the low-energy relativistic positrons around separate crystallographic axes with coaxial symmetry of negative ions in some types of crystals is shown. The process of annihilation of positrons with electrons of…

加速器物理 · 物理学 2017-01-23 Karen Badikyan

A method is proposed for detecting positron-atom bound states by observing enhanced positron annihilation due to electronic Feshbach resonances at electron-volt energies. The method is applicable to a range of open-shell transition metal…

原子物理 · 物理学 2010-12-10 V. A. Dzuba , V. V. Flambaum , G. F. Gribakin

Annihilation momentum densities and correlation enhancement factors for low-energy positron annihilation on valence and core electrons of noble-gas atoms are calculated using many-body theory. s, p and d-wave positrons of momenta up to the…

原子物理 · 物理学 2017-03-22 D. G. Green , G. F. Gribakin

In models of Randall-Sundrum type orthopositronium (o-Ps) can disappear due to tunnelling into additional dimension(s). The experimental signature of this effect is the invisible decay of orthopositronium. We point out that this process may…

高能物理 - 唯象学 · 物理学 2007-05-23 S. N. Gninenko , N. V. Krasnikov , A. Rubbia

Although the annihilation of positrons towards the Galactic centre was established more than 50 years ago through the detection of a 511 keV $\gamma$-ray line, the origin of the positrons remains unknown. The $\gamma$-ray line should be…

高能天体物理现象 · 物理学 2025-08-27 Jürgen Knödlseder , Karim Sabri , Pierre Jean , Peter von Ballmoos , Gerry Skinner , Werner Collmar

Currently, the experimental uncertainty for the determination of the ortho-positronium (o-Ps) decay rate is at 150 ppm precision; this is two orders of magnitude lower than the theoretical one, at 1 ppm level. Here we propose a new proof of…

原子物理 · 物理学 2022-01-26 C. Vigo , M. Raajimakers , L. Gerchow , B. Radics , A. Rubbia , P. Crivelli

The origin of the diffuse gamma-ray background in the range from hundreds keV to several MeV is not known conclusively. From current models and observations it is believed that, at least partially, this background is formed by blazars and…

高能天体物理现象 · 物理学 2024-03-14 B. A. Nizamov , M. S. Pshirkov

Supersymmetric neutralinos are one of the most promising candidates for the dark matter in the Universe. If they exist, they should make up some fraction of the Milky Way halo. We investigate the fluxes of positrons expected at the Earth…

天体物理学 · 物理学 2009-05-12 Edward A. Baltz , Joakim Edsjo

We report the first observation of the annihilation of positronium from the 2S state. Positronium (Ps) is excited with a two-photon transition from the 1S to the 2S state where its lifetime is increased by a factor of eight compared to the…

Enhanced positron annihilation on polyatomic molecules is a long-standing and complex problem. We report the results of calculations of resonant positron annihilation on methyl halides. A free parameter of our theory is the positron binding…

原子物理 · 物理学 2010-02-16 G. F. Gribakin , C. M. R. Lee

Electron antineutrinos are detected in organic liquid scintillator based neutrino experiments by means of the inverse beta decay, producing both a positron and a neutron. The positron may form a bound state together with an electron, called…

$\gamma$ spectra for positron annihilation in noble-gas atoms are calculated using many-body theory for positron momenta up to the positronium-formation threshold. This data is used, together with time-evolving positron-momentum…

原子物理 · 物理学 2017-11-22 D. G. Green

Annihilation spectra are presented for aromatic and heterocyclic ring molecules resolved as a function of incident positron energy using a trap-based positron beam. Comparisons with the vibrational mode spectra yield positron-molecule…