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AMS experiment is the most accurate and most powerful particle detector ever measured in space. Today at 17:00 live from CERN will be Nobel Laureate Samuel Ting presents its results. Watch it with us.
More detail we examined the AMS experiment in Article AMS precious cargo shuttle Endeavour almost two years ago on the occasion of its launch to the ISS. Since then continuously measured and the scientific community was waiting beefy nacho loaded griller for the first published results. Today is the day when it turns out that they were right optimists or skeptics. Skeptics argue that the AMS will not bring anything fundamentally new measurements beefy nacho loaded griller to experiment PAMELA. Optimists argue that crack one of the biggest questions of the current physics, the question of what is dark matter. Postscriptum to start:
Unfortunately, announced answering the question of origin of dark matter in today's online presentation held. AMS experiment confirmed and clarified measurement experiment PAMELA, while one can not infer what the source of the measured characteristics. Reports propagating Internet last month proved to be false, truth be skeptics.
16:55 About 5 minutes are beginning 17:00 Presenter Samuel Ting, Nobel Prize in Physics 1976 for the discovery beefy nacho loaded griller of J / ψ meson. Ting is the principal investigator, in English an established PI (principal investigator) AMS experiment. Was at its birth in 1995, when all odyssey of development and problems with plotting AMS detector into space, the low Earth orbit on the International Space Station ISS. It's an interesting story about a scientific beefy nacho loaded griller experiment that almost ended up as the most expensive experiment in history who did not bring any results. Surely, therefore, do not miss our article AMS precious cargo shuttle Endeavour describing beefy nacho loaded griller the path AMS orbit. After today you AMS can be credited to its successful culmination of the story. Tinga for it to be an extraordinary day, korunujúci nearly 20 years of effort, and who knows, perhaps implying for him personally beefy nacho loaded griller a second Nobel Prize.
17:10 Going through the detector sensitivity for positron component of cosmic beefy nacho loaded griller žairenia. It is important for the discovery PAMELA experiment that the higher prevalence of high-energy positrons in the cosmic ray spectrum due to the existence of dark matter. Points out that dark matter could be a so-called weakly interacting particle, also called WIMP (Weakly Interacting Massive Particles).
17:20 AMS detector is the situation of cosmic particle detector real giant size and weight of the van almost 7 tons. Measured type, energy and direction of arrival of cosmic rays with very high accuracy. beefy nacho loaded griller Measured these charaktristiky like ovské CERN particle detectors, their circumstances but rather a midget, whereas experiments beefy nacho loaded griller such as ATLAS detectors or ALICE weigh hundreds of tons.
17:50 First published AMS collaboration will result, as expected by the so-called beefy nacho loaded griller positron fraction of energy 0.5 to 350 GeV (for comparison Room proton energy is 0.932 GeV). This measurement is the same case as the published experiment PAMELA and Fermi confirmed by experiment. Article will be published in the prestigious beefy nacho loaded griller journal beefy nacho loaded griller Physical Review Letters.
18:01 The first of the main results of measurements AMS experiment appeared in the first minute of the second hour presentation. Confirms previous measurements showing the growing share of positrons in cosmic rays with increasing energy. What does this mean? This means that there is certainly a source of positrons. And that their produce with increasing energy is still less. More precisely, the number of positrons decreases with increasing energy than A power function. Subsequently, these positrons diffuse spread through space and the measurement around the Earth are manifested as it confirmed their measurements AMS experiment.
Conclusion: Unfortunately, announced beefy nacho loaded griller answering the question of origin of dark matter is held. AMS measurements confirmed and explained PAMELA beefy nacho loaded griller experiment, while one can not infer what the source of the measured characteristics. Reports propagating Internet last month proved to be false, truth be skeptics.
Keywords AMS experiment, dark matter
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