antimatter at the beginning of the Universe antimatter index antimatter at the University of Bologna

Antimatter today in the Universe

Are 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.
This is confirmed by negative results from observatories on satellites, which could detect high energy photons, called gamma rays, with energies which would correspond to those expected.

Fig. 1: Collision between two spiral galaxies.
(
Credit: NASA and Hubble Heritage Team (STScI))

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.
The AMS detector (Alpha Magnetic Spectrometer), to be installed in the International Space Station, will search for antinuclei of medium and high energy.

Fig. 2: Diagram of the method used to detect nuclei (matter) and antinuclei (antimatter) with the PAMELA spectrometer. Nuclei and antinuclei coming from above will be curved by a magnet in opposite directions. An antinucleus would then annihilate with matter (bottom left) yielding an "event" with many tracks.
(
Credit: PAMELA experiment)
Fig. 3: The International Space Station where the AMS experiment will be installed.
(
Credit: NASA)

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.