Astronaut Ron Garan took this image during the spacewalk conducted on Tues., July 12, 2011. It shows the International Space Station with Space Shuttle Atlantis docked on the right and a Russian Soyuz on the far left. In the foreground is the Alpha Magnetic Spectrometer (AMS) experiment installed during the STS-134 mission. AMS is a state-of-the-art particle physics detector designed to use the unique environment of space to advance knowledge of the universe and lead to the understanding of the universe’s origin by searching for antimatter and dark matter, and measuring cosmic rays. Credit: NASA
AMS announced the first results in its search for dark matter, reporting the observation of an excess of positrons in the cosmic ray flux.
Geneva 3 April 2013. The international team running the Alpha Magnetic Spectrometer (AMS) today announced the first results in its search for dark matter. The results, presented by AMS spokesperson Professor Samuel Ting in a seminar at CERN, are to be published in the journal Physical Review Letters. They report the observation of an excess of positrons in the cosmic ray flux.
The AMS results are based on some 25 billion recorded events, including 400,000 positrons with energies between 0.5 GeV and 350 GeV, recorded over a year and a half. This represents the largest collection of antimatter particles recorded in space. The positron fraction increases from 10 GeV to 250 GeV, with the data showing the slope of the increase reducing by an order of magnitude over the range 20-250 GeV. The data also show no significant variation over time, or any preferred incoming direction. These results are consistent with the positrons originating from the annihilation of dark matter particles in space, but not yet sufficiently conclusive to rule out other explanations.
“As the most precise measurement of the cosmic ray positron flux to date, these results show clearly the power and capabilities of the AMS detector,” said AMS spokesperson, Samuel Ting. “Over the coming months, AMS will be able to tell us conclusively whether these positrons are a signal for dark matter, or whether they have some other origin.”
Cosmic rays are charged high-energy particles that permeate space. The AMS experiment, installed on the International Space Station, is designed to study them before they have a chance to interact with the Earth’s atmosphere. An excess of antimatter within the cosmic ray flux was first observed around two decades ago. The origin of the excess, however, remains unexplained. One possibility, predicted by a theory known as supersymmetry, is that positrons could be produced when two particles of dark matter collide and annihilate. Assuming an isotropic distribution of dark matter particles, these theories predict the observations made by AMS. However, the AMS measurement can not yet rule out the alternative explanation that the positrons originate from pulsars distributed around the galactic plane. Supersymmetry theories also predict a cut-off at higher energies above the mass range of dark matter particles, and this has not yet been observed. Over the coming years, AMS will further refine the measurement’s precision, and clarify the behavior of the positron fraction at energies above 250 GeV.
“When you take a new precision instrument into a new regime, you tend to see many new results, and we hope this will be the first of many,” said Ting. “AMS is the first experiment to measure to 1% accuracy in space. It is this level of precision that will allow us to tell whether our current positron observation has a Dark Matter or pulsar origin.”
Dark matter is one of the most important mysteries of physics today. Accounting for over a quarter of the universe’s mass-energy balance, it can be observed indirectly through its interaction with visible matter but has yet to be directly detected. Searches for dark matter are carried out in space-borne experiments such as AMS, as well as on the Earth at the Large Hadron Collider and a range of experiments installed in deep underground laboratories.
“The AMS result is a great example of the complementarity of experiments on Earth and in space,” said CERN Director General Rolf Heuer. “Working in tandem, I think we can be confident of a resolution to the dark matter enigma sometime in the next few years.”
Electron – Positron pair emission from materialization of high power gamma rays were observed in cosmic rays. Generally these anti matter and matter particles are equal in number and annihilate each other. But Nobel Laurette recently suggested that excess of matter particles (very slight) over anti matter particles during Big Bang particularly in third generation of matter like Top, which takes two different routes of disintegration resulted in the matter Universe and not anti matter Universe. Now powerful anti matter positrons in AMS experiment with cosmic ray flux raises a doubt of source of production of this anti matter. Since we do not yet know the actual structure of this Dark Matter all possible explanations are possible. They could be from high power cosmic rays from billions of pulsars all around. Still, we grope in the dark in finding this elusive Dark Matter. Thank You.