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The most energetic light recorded thus far hits Tibetan plateau

Gamma-ray particles trillions of times more energetic than regular light hit the Tibetan plateau.

Tibi PuiubyTibi Puiu
June 27, 2019
in News, Space
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An experiment involving over 600 particle detectors stretched over 36,900 square meters has measured the most energetic light ever witnessed on this planet. The photons were part of gamma rays emanating from the famous Crab Nebula, the remains of a supernova that was first observed in 1054 AD, which is located approximately 6,500 light years away. These photons measured tremendously high values exceeding 100 trillion electron volts (TeV), with one measurement clocking in 450TeV — the highest ever recorded. Previously, photons measuring no more than tens of trillions of electronvolts had been recorded.

Physicists started the Tibet Air Shower Gamma Collaboration, an observatory in the Tibetan Plateau some 4,300 meters above sea level because rarified air at this altitude allows more secondary particles to reach detectors. Secondary subatomic particles are created when cosmic rays and gamma rays interact with particles in the upper atmosphere.

By measuring and excluding muon particles — an elementary subatomic particle similar to the electron but 207 times heavier — physicists were able to backtrack the energy and origin of the incoming gamma rays that caused the showers. A total of 24 events caused by intense photons with energies higher than 100 trillion electronvolts were reported. To get a sense of the scale involved, regular photons that emanate from the sun — particles of visible light — have an energy of only a few electronvolts.

Now that scientists have experimental confirmation that high-energy photons reach Earth, they can elaborate a more precise model for how such particles are created and whether or not there’s a limit to how much energy they can carry.

In this particular case, researchers think that the gamma rays were accelerated by a process known as Inverse Compton scattering — a process during which super high-energy electrons bounce off lower energy photons. Inside the Crab Nebula, electrons may have scattered off low-energy photons from the cosmic microwave radiation (photons created soon after the Big Bang).

The findings appeared in the journal Physical Review Letters.

Tags: Crab Nebulagamma raylightnebula

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Tibi Puiu

Tibi Puiu

Tibi is a science journalist and co-founder of ZME Science. He writes mainly about emerging tech, physics, climate, and space. In his spare time, Tibi likes to make weird music on his computer and groom felines. He has a B.Sc in mechanical engineering and an M.Sc in renewable energy systems.

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This Picture of the Week shows a stunning spiral galaxy known as NGC 4945. This little corner of space, near the constellation of Centaurus and over 12 million light-years away, may seem peaceful at first — but NGC 4945 is locked in a violent struggle. At the very centre of nearly every galaxy is a supermassive black hole. Some, like the one at the centre of our own Milky Way, aren’t particularly hungry. But NGC 4945’s supermassive black hole is ravenous, consuming huge amounts of matter — and the MUSE instrument at ESO’s Very Large Telescope (VLT) has caught it playing with its food. This messy eater, contrary to a black hole’s typical all-consuming reputation, is blowing out powerful winds of material. This cone-shaped wind is shown in red in the inset, overlaid on a wider image captured with the MPG/ESO telescope at La Silla. In fact, this wind is moving so fast that it will end up escaping the galaxy altogether, lost to the void of intergalactic space. This is part of a new study that measured how winds move in several nearby galaxies. The MUSE observations show that these incredibly fast winds demonstrate a strange behaviour: they actually speed up far away from the central black hole, accelerating even more on their journey to the galactic outskirts. This process ejects potential star-forming material from a galaxy, suggesting that black holes control the fates of their host galaxies by dampening the stellar birth rate. It also shows that the more powerful black holes impede their own growth by removing the gas and dust they feed on, driving the whole system closer towards a sort of galactic equilibrium. Now, with these new results, we are one step closer to understanding the acceleration mechanism of the winds responsible for shaping the evolution of galaxies, and the history of the universe. Links  Research paper in Nature Astronomy by Marconcini et al. Close-up view of NGC 4945’s nucleus
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