Antimatter today in the UniverseAre we really sure that in some remote parts of the Universe there is no antimatter, including antistars and antigalaxies? In the last 20 years a lot of research has been carried out using
increasingly sophisticated instruments. Given that, when antimatter collides with ordinary matter,
there are
annihilations
producing electromagnetic
radiations,
scientists tried to detect antimatter via the produced electromagnetic radiations,
light in particular. Fig.1 shows the collision between two galaxies. They are not
one galaxy and one antigalaxy because, from the colliding region, we do not observe any extra light, annihilation of particles and antiparticles. A different line of research tries to find heavy antinuclei in primary cosmic rays. In order to avoid collisions of the antinuclei with the nuclei of the atmosphere the instruments are installed on satellites. Two experiments in particular are now searching for antimatter coming from outer space. PAMELA (Payload for Antimatter Matter Exploration and
Light-nuclei Astrophysics) will be installed on the Russian satellite Artica
and will search for medium energy antinuclei.
Protons and helium nuclei were produced in the first moments of the Universe. Instead heavier nuclei, like carbon, iron and all the others existing on Earth, were "cooked" inside some heavy stars, which later exploded and spread this matter in space. This matter was later included in the cosmic cloud from where our solar system was born. We therefore think that if we find even only few anti-carbon or anti-iron antinuclei this would prove that there are regions in space where antistars exist.
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