Titanium in Cosmic Rays ✎ express

Original: "Energy dependence of Ti/Fe ratio in the Galactic cosmic rays measured by the ATIC-2 experiment"
arXiv:0905.0049 · 2009-05-01 · arXiv non-exclusive · independent analysis · 1 min
Rare titanium in cosmic rays has been separated from iron, and its fraction measured across a wide range of energies.

In the stream of cosmic rays, particles flying toward us from the depths of the Galaxy, titanium is rare. Its nuclei are almost indistinguishable from iron: both are heavy, and both leave similar tracks in detectors. But in the ATIC experiment, using a silicon matrix, researchers managed to separate titanium from iron and trace how their ratio changes with energy.

In everyday terms, it's like telling apart two similar twins in a crowd by a barely visible birthmark. The silicon matrix acts as a very attentive observer that notices the difference in how particles slow down in matter. Titanium is slightly lighter than iron, and at high energies this difference becomes more pronounced.

The measurements covered the range from 5 to 500 GeV per nucleon. It's as if we were watching runners on a course from a sprint to a marathon and seeing how their pace changes.

The result is a curve of the titanium-to-iron ratio as a function of energy. Such data are needed to test how cosmic rays are accelerated and how much matter they traverse on their way to Earth. Rare nuclei like titanium act as markers that allow us to reconstruct the particle's journey history.

Titanium in cosmic rays is about ten times rarer than iron, even though in ordinary Solar System matter their abundances are comparable.

Scientists
Enrico FermiErnest RutherfordJohannes RydbergMurray Gell-Mann
Concepts
titanium titan titanium oxide iron tritium chromium saturn teraelectronvolt sulfur active galactic nucleus galactic center glycine helium flash metallicity in stellar evolution cosmic rays argon gigaelectronvolt wolf rayet star barium titanate carbon fiber