The most energetic
parcels
of electromagnetic radiation -- Tera-electronvolt gamma rays -- ever determined to
have originated in the plane of our home galaxy were observed
recently by the Milagro detector, located at high mountain
elevations in New Mexico. The potent photons are believed to have
been part of the debris spawned when even more energetic cosmic rays
struck the matter-dense heart of the Milky
Way.
Photons in the TeV range arrive at the Earth very rarely, not
often enough to attempt observation from a space-based gamma
telescope: for a wristwatch-sized detector you'd have to wait about
10 years, on average. Therefore, terrestrial gamma observations are
usually carried out by large-area-arrays attached to the ground.
Milagro, operated by scientists from nine institutions, records the
arrival of energetic photons at Earth by observing the air shower of
secondary particles generated when the gamma rays hit the
atmosphere. These particles betray their presence by the light
(Cerenkov radiation) emitted when the particles pass through a
6-million-gallon pond instrumented with photo detectors. This method
of observation offers a rough ability to determine the direction of
arrival.
For the Milagro experiment so far, 70,000 TeV photon events
from within a region of the Milky Way plane were culled from an
inventory of about 240 million TeV-level events seen so far seen
from the same region. These numbers, says team member Roman
Fleysher of New York University (roman.fleysher@physics.nyu.edu), are consistent
with theoretical estimates for cosmic ray production.
And where do
the cosmic rays get their 100-TeV-and-more energies? Fleysher
recalled an analogy due to Enrico Fermi: imagine a pingpong ball
trapped between two hole-filled walls zooming toward each other.
The ball will ricochet many times, gaining energy, before eventually
escaping out one of the holes. Ions in the interstellar medium,
perhaps near a collapsed star or an active galactic nucleus (AGN),
can get caught up by shock waves and accelerated to high energies
like the pingpong ball.
Atkins et al., Physical Review Letters, 16
December 2005