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    Home»Space»Mysterious “Empty Sky” Gamma-Ray Puzzle Solved – May Lead Astrophysicists To Unravel Dark Matter
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    Mysterious “Empty Sky” Gamma-Ray Puzzle Solved – May Lead Astrophysicists To Unravel Dark Matter

    By Australian National UniversitySeptember 20, 20214 Comments3 Mins Read
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    Fermi's Five-year View of the Gamma-ray Sky
    A detailed look at the gamma-ray sky. Credit: NASA/DOE/Fermi LAT Collaboration

    Star-forming galaxies are responsible for creating gamma-rays that until now had not been associated with a known origin.

    Star-forming galaxies are responsible for creating gamma-rays that until now had not been associated with a known origin, researchers from The Australian National University (ANU) have confirmed.

    Lead author Dr. Matt Roth, from the ANU Research School of Astronomy and Astrophysics, said until now it has been unclear what created gamma-rays — one of the most energetic forms of light in the Universe — that appear in patches of seemingly ’empty sky’.

    The discovery could offer clues to help astronomers solve other mysteries of the Universe, such as what kind of particles make up Dark Matter — one of the holy grails of astrophysics.

    “It’s a significant milestone to finally discover the origins of this gamma-ray emission, solving a mystery of the Universe astronomers have been trying to decipher since the 1960s,” Dr. Roth said.

    Sources of Gamma-Ray Emission

    “There are two obvious sources that produce large amounts of gamma-rays seen in the Universe. One is when gas falls into the supermassive black holes which are found at the centers of all galaxies — called an active galactic nucleus (AGN) — and the other is associated with star formation in the disks of galaxies.

    “We modeled the gamma-ray emission from all the galaxies in the Universe and compared our results with the predictions for other sources and found that it is star-forming galaxies that produce the majority of this diffuse gamma-ray radiation and not the AGN process.”

    ANU researchers were able to pinpoint what created these mysterious gamma-rays after obtaining a better understanding of how cosmic rays — particles that travel at speeds very close to the speed of light — move through the gas between the stars. Cosmic rays are important because they create large amounts of gamma-ray emission in star-forming galaxies when they collide with the interstellar gas.

    “It’s a significant milestone to finally discover the origins of this gamma-ray emission.” Dr. Matt Roth

    Data from NASA’s Hubble Space Telescope and Fermi Gamma-Ray Space Telescope was a key resource used to uncover the unknown origins of the gamma-rays. Researchers analyzed information about many galaxies such as their star-formation rates, total masses, physical size and distances from Earth.

    Predicting Galaxy Radio Emissions

    “Our model can also be used to make predictions for radio emission — the electromagnetic radiation that has a frequency similar to a car radio — from star-forming galaxies, which could help researchers understand more about the internal structure of galaxies,” Dr. Roth said.

    “We are currently looking at producing maps of the gamma-ray sky that can be used to inform upcoming gamma-ray observations from next-generation telescopes. This includes the Cherenkov Telescope Array, which Australia is involved in.

    “This new technology will hopefully allow us to observe many more star-forming galaxies in gamma-rays than we can detect with current gamma-ray telescopes.”

    Reference: “The diffuse γ-ray background is dominated by star-forming galaxies” by Matt A. Roth, Mark R. Krumholz, Roland M. Crocker and Silvia Celli, 15 September 2021, Nature.
    DOI: 10.1038/s41586-021-03802-x

    This research, published in Nature, features authors from Australia and Italy. The ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) was also involved.

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    4 Comments

    1. Howard Jeffrey Bender, Ph.D. on September 20, 2021 7:37 am

      Gamma rays are one thing, but Dark Matter is something else entirely. One possibility, from a view of String Theory, is that Dark Matter appears to us as an effect of string/anti-string annihilations. As you may know, quantum mechanics requires that strings must be formed as pairs in the quantum foam – a string and an anti-string – that immediately annihilate each other. Quantum mechanics also requires both the string and anti-string to be surrounded by “jitters” that reduce their monstrous vibrating energies. What if this jitter remains for a fraction of an instant after their string/anti-string annihilations? This temporary jitter would be seen by us as matter, via E=mc2, for that instant before it too returns to the foam. That’s why we never see it – the “mass” lasts only for that instant but is repeated over and over and over, all over. Specifics on this can be found in my YouTube at https://www.youtube.com/watch?v=N84yISQvGCk

      Reply
      • Torbjörn Larsson on September 20, 2021 12:16 pm

        Pseudoscience link.

        And an aside on dark matter do not warrant another on string theory.

        Reply
      • Runesmith on September 21, 2021 4:54 am

        That wouldn’t explain the apparent concentration of dark matter around visible matter (galaxies and clusters).

        Reply
        • Howard Jeffrey Bender, Ph.D. on September 23, 2021 7:58 am

          Actually, there is no “concentration” of Dark Matter around galaxies and clusters, just the understanding that some form of extra gravitational attraction has to be there for those structures to exist. There could be Dark Matter all around, but we wouldn’t see it without galaxies etc. to be there, too.

          Reply
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