We found these successful collisions had a lower than
expected electron energy, which is clear evidence of radiation reaction.»
Not exact matches
Over the past few years, balloon and satellite cosmic - ray experiments have found high -
energy electrons and their positively charged counterparts, positrons, in concentrations much higher than they would
expect to see from the sun and other known sources of cosmic rays within our galaxy.
And, as Wefel notes, the Fermi spectrum seems to include more high -
energy electrons than
expected, which could also be evidence of the mysterious substance.
On 3 April, AMS designer Samuel Ting of the Massachusetts Institute of Technology reported an
expected rise in the ratio of positrons to
electrons at
energies between 10 and 350 gigaelectronvolts.