Extra Electrons in Cosmic Rays ✎ express

Original: "Possible structure in the cosmic ray electron spectrum measured by the ATIC-2 and ATIC-4 experiments"
arXiv:1104.3452 · 2011-04-18 · arXiv non-exclusive · independent analysis · 1 min
A balloon caught more particles than expected.

High above Antarctica, a balloon carried an instrument that caught electrons from space. These particles come from distant stellar explosions and other powerful events. The instrument measured their energy, like the force of an impact. And in one energy range, there were more impacts than calculations predicted.

The first analysis of the data showed a broad bump on the graph: as if an extra stream had appeared in the particle flux. Now the same data have been reprocessed using different methods. It turned out that the bump is not smooth but consists of several narrow peaks. As if individual drops were discerned in the noise of rain.

Energy of 300–800 GeV is like a single electron accelerated to a speed at which its mass becomes hundreds of thousands of times its rest mass.

Comparison with data from another experiment, a telescope on a satellite, showed that the peaks are not seen by everyone. Possibly this is a trace of some unknown source or an artifact of the measurements. But the mystery remains: where do so many fast electrons in space come from?

Electrons with energies of hundreds of GeV pass through the atmosphere and generate entire showers of secondary particles that can be detected on the ground.

Scientists
Enrico FermiMichael FaradayHendrik LorentzErnest RutherfordJocelyn Bell Burnell
Concepts
classical electron radius cosmic ray spectrum peak erg spectrum gigaelectronvolt electronvolt electron energy teraelectronvolt mass range kiloelectronvolt kink band gap band structure lyman alpha line knee katrin photoelectron fermi level Stark effect