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Related papers: Orthopositronium: Annihilation of positron in gase…

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The positron-neutrino correlation in the $0^+ \to 0^+ \beta$ decay of $^{32}$Ar was measured at ISOLDE by analyzing the effect of lepton recoil on the shape of the narrow proton group following the superallowed decay. Our result is…

The annihilation channel is implemented into the front form calculations of the positronium spectrum presented in a previous publication. The effective Hamiltonian is calculated analytically. Its eigensolutions are obtained numerically. A…

High Energy Physics - Theory · Physics 2007-05-23 Uwe Trittmann

We present the energy spectra of the fluxes of positrons, anti-protons and photons generated by Dark Matter annihilations in our galaxy, as univocally predicted by the model of Minimal Dark Matter. Due to multi-TeV masses and to the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Marco Cirelli , Roberto Franceschini , Alessandro Strumia

The atmospheric neutrino anomaly is the apparent reduction of the $\nu_{\mu}/\nu_{e}$ ratio observed in underground detectors. It represents either a reduction in the muon neutrino interaction rate or an excess of the electron neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. M. LoSecco

A method for measuring the tensor polarization in a positronium (Ps) beam is proposed, which is based on the determination of the Ps lifetime as a function of the orientation of a homogeneous magnetic field. The dependence of the…

Materials Science · Physics 2008-11-26 Alexander J. Silenko

The positron-electron pair annihilation in two photons is known for its numerous applications using PET scanners. The decay of Positronium (Ps) from a standard sealed source in more than two photons is less likely but can be observed with a…

Physics Education · Physics 2011-09-20 M. E. A. Elbasher , W. Erasmus , E. A. M. Khaleel , J. Ndayishimye , P. Papka

The Galaxy hosts a widespread population of low-energy positrons revealed by successive generations of gamma-ray telescopes through a bright annihilation emission from the bulge region, with a fainter contribution from the inner disk. The…

High Energy Astrophysical Phenomena · Physics 2015-06-05 P. Martin , A. W. Strong , P. Jean , A. Alexis , R. Diehl

The $\gamma$ ray emission originating from in-flight annihilation (IA) of positrons is a powerful observable for constraining high-energy positron production from exotic sources. By comparing diffuse $\gamma$ ray observations of INTEGRAL,…

High Energy Physics - Phenomenology · Physics 2024-05-15 Pedro De la Torre Luque , Shyam Balaji , Pierluca Carenza , Leonardo Mastrototaro

A model-potential approach to calculating positron-molecule binding energies and annihilation rates is developed. Unlike existing ab initio calculations, which have mostly been applied to strongly polar molecules, the present methodology…

Atomic Physics · Physics 2018-12-31 A. R. Swann , G. F. Gribakin

Recent preliminary results from the PAMELA experiment indicate the presence of an excess of cosmic ray positrons above 10 GeV. In this letter, we consider possibility that this signal is the result of dark matter annihilations taking place…

High Energy Physics - Phenomenology · Physics 2009-12-30 Ilias Cholis , Lisa Goodenough , Dan Hooper , Melanie Simet , Neal Weiner

A model-potential approach has been developed to study positron interactions with molecules. Binding energies and annihilation rates are calculated for positron bound states with a range of alkane molecules, including rings and isomers. The…

Atomic Physics · Physics 2019-09-17 A. R. Swann , G. F. Gribakin

All results of the neutron lifetime measurements performed in the last 20 years with the UCN storage method are in a good agreement. These results are consistent with the latest most accurate measurements of the neutron decay asymmetry…

Nuclear Experiment · Physics 2021-04-21 A. P. Serebrov , M. E. Chaikovskii , G. N. Klyushnikov , O. M. Zherebtsov , A. V. Chechkin

The main properties of the interaction of ultra low-energy antiprotons ($% E\le10^{-6}$ a.u.) with atomic hydrogen are established. They include the elastic and inelastic cross sections and Protonium (Pn) formation spectrum. The inverse…

Atomic Physics · Physics 2009-10-31 A. Yu. Voronin , J. Carbonell

Corrections $\sim \alpha^2 $ to the positronium decay rate, induced by one--loop vacuum polarization diagram, are calculated. Their relative values are $0.4468(3)(\alpha/\pi)^2$ for para- and $0.960(3)(\alpha/\pi)^2$ for orthopositronium.

High Energy Physics - Phenomenology · Physics 2007-05-23 A. P. Burichenko , D. Yu. Ivanov

We report on the abundance of interstellar neutral nitrogen (NI) for 30 sightlines, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE) and the Hubble Space Telescope (HST). NI column densities are derived by measuring the…

Astrophysics · Physics 2008-11-26 Adam G. Jensen , Brian L. Rachford , Theodore P. Snow

The recent experimental data obtained by the OBELIX group on $\bar{p}$D and $\bar{p}^4$He total annihilation cross sections are analyzed. The combined analysis of these data with existing antiprotonic atom data allows, for the first time,…

Nuclear Theory · Physics 2009-10-31 K. V. Protasov , G. Bonomi , E. Lodi Rizzini , A. Zenoni

The effect of confinement on the self-annihilation rate of positronium is studied in three levels of approximation. Artificial restriction of the electron-positron separation leads to an increase in the annihilation rate over its vacuum…

Atomic Physics · Physics 2021-08-05 A. R. Swann , D. G. Green , G. F. Gribakin

These proceedings summarize the first MiniBooNE electron antineutrino appearance search results, corresponding to a data sample collected for 3.39$\times10^{20}$ protons on target (POT). The search serves as a direct test of the LSND…

High Energy Physics - Experiment · Physics 2019-08-13 G. Karagiorgi

The X-ray spectra of Anomalous X-ray Pulsars have long been fit by smooth, empirical models such as the sum of a black-body plus a power law. These reproduce the ~0.5 to 10 keV range well, but fail at lower and higher energies, grossly…

Astrophysics · Physics 2008-11-26 Martin Durant , Marten H. van Kerkwijk

Assuming Galactic positrons do not go far before annhilating, a difference between the observed 511 keV annihilation flux distribution and that of positron production, expected from beta-plus decay in Galactic iron nucleosynthesis, was…

High Energy Astrophysical Phenomena · Physics 2009-09-02 R. E. Lingenfelter , J. C. Higdon , R. E. Rothschild