Antimatter research in space

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Antimatter Research in Space

Two of the most compelling issues facing astrophysics and cosmology today are to understand the nature of the dark matter that pervades the universe and to understand the apparent absence of cosmological antimatter. For both issues, sensitive measurements of cosmic-ray antiprotons and positrons, in a wide energy range, are crucial. Many different mechanisms can contribute to antiprotons and pos...

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Search for Antimatter in Space with the Alpha Magnetic Spectrometer

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Cosmological Matter-antimatter Asymmetry and Antimatter in the Universe

Prediction of antimatter by Dirac (1928) and quick subsequent discovery of the first antimatter particle, positron, by Anderson 2 (1933) are among greatest scientific achievements of XX century. Discovery of antiproton 22 years later 3 was the next step which had opened a whole new world of antiparticles. Now for (almost) every elementary particle a corresponding antiparticle has also been obse...

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Antimatter in the Universe

The world in our neighbourhood, as we observe it, is 100% charge asymmetric. We see only matter and any considerable amount of antimatter nearby is excluded [1,2]. A small number of antiprotons and positrons in the cosmic rays (to say nothing of those produced in accelerators) can be prescribed to the secondary origin. Charge asymmetry in terms of visible massive matter defined as/3B = (riB -nf...

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Antimatter transport processes

A comparison of the 1S-2S transitions of hydrogen and antihydrogen will yield a stringent test of CPT conservation. Necessarily, the antihydrogen atoms need to be trapped to perform high precision spectroscopy measurements. Therefore, an approximately 0.75 T deep neutral atom trap, equivalent to about 0.5 K for ground state (anti)hydrogen atoms, has been superimposed on a Penning-Malmberg trap ...

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ژورنال

عنوان ژورنال: Journal of Physics G: Nuclear and Particle Physics

سال: 2003

ISSN: 0954-3899,1361-6471

DOI: 10.1088/0954-3899/29/5/311