In science fiction, finding antimatter on board your spaceship is not
good news. Usually, it means you're moments away from an explosion.
In real life, though, finding antimatter could lead to a Nobel Prize.
On April 3rd, researchers led by Nobel Laureate Samuel Ting of MIT
announced that the Alpha Magnetic Spectrometer, a particle detector
operating onboard the International Space Station since 2011, has
counted more than 400,000 positrons, the antimatter equivalent of
electrons. There’s no danger of an explosion, but the discovery is
sending shock waves through the scientific community.
A new ScienceCast video explores the possibility that signs of
dark matter have been detected onboard the International Space Station. Play it
"These data show the existence of a new physical phenomenon," wrote Ting and colleagues in an article published in the Physical Review Letters. "It could be a sign of dark matter."
The Alpha Magnetic Spectrometer (“AMS” for short) was delivered to
the ISS by the space shuttle Endeavour on its final flight in May 2011.
In its first 18 months of operations, from May 19, 2011 to December 10,
2012, the AMS analyzed 25 billion cosmic ray events. Of these, an
unprecedented number were unambiguously identified as positrons.
Cosmic rays are subatomic particles such as protons and helium
nuclei accelerated to near-light speed by supernova explosions and other
violent events in the cosmos. Researchers have long known that cosmic
rays contain a sprinkling of antimatter. Italy's PAMELA satellite
detected high-energy positrons in 2009, and NASA's Fermi gamma-ray
observatory confirmed the find two years later.
But where do the positrons come from? The Universe is almost
completely devoid of antimatter, so the positron fraction of cosmic ray
electrons--as much as 10%--is a little surprising.
One idea is dark matter. Astronomers know that the vast majority
of the material Universe is actually made of dark matter rather than
ordinary matter. They just don't know what dark matter is. It exerts
gravity, but emits no light, which makes it devilishly difficult to
study.
A leading theory holds that dark matter is made of a particle
called the neutralino. Collisions between neutralinos should produce a
large number of high-energy positrons, which the AMS should be able to
detect with unprecedented sensitivity.
"The accuracy of our measurements is 1%, which is excellent, and
we have statistics unmatched by any other spacecraft," says Ting.
"So far the evidence supports the hypothesis of dark matter. But,"
he cautions," it does not rule out another possibility--pulsars."
Pulsars are strongly-magnetized neutron stars formed in the
aftermath of supernova explosions. They can spin on their axes
thousands of times a second, flinging particles into space with
fantastic energies that accelerators on Earth can't match. Among these
particles are pairs of electrons and positrons.
AMS can distinguish between pulsars and dark matter--but not yet.
"We need more data at higher energies to decide which is the correct
explanation," says Ting. "It is only a matter of time, perhaps months
or a few years."
Built by scientists from 16 countries with support from the US
Dept. of Energy, the Alpha Magnetic Spectrometer will continue operating
for the rest of the life of the space station at least until 2020.
Between now and then, the mystery of dark matter could be solved, once
and for all.
Credits:
Author: Dr. Tony Phillips | Production editor: Dr. Tony Phillips
Credit: Science@NASA
More information:
Alpha Magnetic Spectrometer -- home page
