If protons and neutrons are Dirac particles, as one usually assumes, the corresponding antiparticles should exist, but these have never been observed. The coupling of nucleons with the meson field offers processes by which these particles could be created in energetic collisions between nucleons and mesons or other nucleons. In this thesis the pseudoscalar meson theory is used to calculate cross-sections for the production of antiprotons in such collision processes. These are applied to estimate the numbers of antiprotons to be expected from the interaction of cosmic ray particles with the nucleons of the atmosphere. It is found that meson production is about 60 times more frequent than antinucleon production for th...
Journals published by the American Physical Society can be found at http://publish.aps.org
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
Cosmic ray antiprotons provide an important probe for the study of the galactic Dark Matter, as they...
One of the striking features of Dirac's theory of the electron was the appearance of solutions to hi...
We present antiproton invariant multiplicities from Experiment 941 using 12 and 19 GeV/c proton beam...
We present a RQMD calculation of antiproton yields and their momentum distribution in Ne + NaF colli...
Nuclear reactions in the hot accretion plasma surrounding a collapsed star are a source of neutrons,...
Antiproton beams of relatively low energies (below hundreds of MeV) have recently become available. ...
The production of antibaryons is calculated in a microscopic transport approach employing multiple m...
In the exposure to a 7 0 0-MeV/c negative particle beam, 35 antiproton stars have been found. Of the...
Journals published by the American Physical Society can be found at http://publish.aps.org/Antiproto...
Journals published by the American Physical Society can be found at http://publish.aps.org/Antiproto...
In the present work, the origin of antiprotons observed in cosmic rays (above the atmosphere) is ana...
In this thesis, the flux of light antinuclei induced near earth by Cosmic Ray interactions with the ...
Interactions of antiprotons on protons at 6 and 9 GeV/c are investigated from a 520K picture exposur...
Journals published by the American Physical Society can be found at http://publish.aps.org
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
Cosmic ray antiprotons provide an important probe for the study of the galactic Dark Matter, as they...
One of the striking features of Dirac's theory of the electron was the appearance of solutions to hi...
We present antiproton invariant multiplicities from Experiment 941 using 12 and 19 GeV/c proton beam...
We present a RQMD calculation of antiproton yields and their momentum distribution in Ne + NaF colli...
Nuclear reactions in the hot accretion plasma surrounding a collapsed star are a source of neutrons,...
Antiproton beams of relatively low energies (below hundreds of MeV) have recently become available. ...
The production of antibaryons is calculated in a microscopic transport approach employing multiple m...
In the exposure to a 7 0 0-MeV/c negative particle beam, 35 antiproton stars have been found. Of the...
Journals published by the American Physical Society can be found at http://publish.aps.org/Antiproto...
Journals published by the American Physical Society can be found at http://publish.aps.org/Antiproto...
In the present work, the origin of antiprotons observed in cosmic rays (above the atmosphere) is ana...
In this thesis, the flux of light antinuclei induced near earth by Cosmic Ray interactions with the ...
Interactions of antiprotons on protons at 6 and 9 GeV/c are investigated from a 520K picture exposur...
Journals published by the American Physical Society can be found at http://publish.aps.org
A balloon-borne instrument has measured the cosmic-ray antiproton flux between 130 and 320 MeV and s...
Cosmic ray antiprotons provide an important probe for the study of the galactic Dark Matter, as they...