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  • richardmitnick 10:32 am on December 4, 2018 Permalink | Reply
    Tags: , , , , , EDGES collaboration, First stars may have been in massive dark matter halos, Institute for Advanced Study in Princeton New Jersey US, New observations challenge universe model   

    From COSMOS Magazine: “New observations challenge universe model” 

    Cosmos Magazine bloc

    From COSMOS Magazine

    04 December 2018
    Lauren Fuge

    First stars may have been in massive dark matter halos.

    1
    The cosmic microwave background, captured by NASA’s Wilkinson Microwave Anistropy Probe. NASA

    Observations of the very first stars to form might change accepted models of the dawn of the universe.

    A team of astronomers led by Alexander Kaurov of the Institute for Advanced Study in New Jersey, US, says these observations may indicate that the majority of the first stellar generation were located in rare and massive dark matter halos.

    First, though, a quick cosmology refresher.

    Current models tell us that for almost 400,000 years after the Big Bang, the universe was so hot that atoms couldn’t form yet. All that existed was a searing soup of plasma, with photons trapped within it like a fog. But when the universe finally cooled enough for protons and electrons to combine into hydrogen atoms, those photons escaped.

    Today, this jailbreak radiation is known as the cosmic microwave background (CMB). It’s like the universe’s baby photo, and by studying it and the tiny fluctuations within it, we can learn about the system’s infancy and how stars and galaxies began to form.

    The first generation of stars appear so faint and distant that they’re difficult to detect directly. However, astronomers theorised that these stars emitted ultraviolet radiation that heated up the gas around them, which in turn absorbed some of CMB – at radio wavelengths of 21 centimetres, to be specific.

    In March 2018, the Experiment to Detect the Global Epoch of Reionization Signature (EDGES) detected this signal as a small distortion in the CMB, like a fingerprint of the first stars.

    EDGES telescope in a radio quiet zone at the Murchison Radio-astronomy Observatory in Western Australia.

    But upon analysis, the EDGES team realised that the signal’s shape was much deeper than predicted, with sharper boundaries.

    Any number of studies have since attempted to explain the unexpected depth, using new physics or astrophysics. Now, Kaurov’s team at the US Institute for Advanced Study has tackled the signal’s sharp boundaries.

    In a study published in The Astrophysical Journal Letters, he and co-authors argue that this feature indicates that as the first stars lit up, ultraviolet photons flooded the universe much more quickly than expected. The team’s computer simulations showed that this suddenness would occur naturally if the first stars were concentrated in the most massive and rarest dark matter halos – rather than distributed evenly throughout the universe as previously thought.

    These halos, weighing over a billion times more than our Sun, exploded in number in the universe’s infancy and could have easily produced the huge influx of ultraviolet photons necessary to explain the EDGES signal.

    If this scenario is correct, then these rare halos might be bright enough to be observed by the James Webb Space Telescope, which will launch in 2021.

    Time, thus, in more ways than one, will tell.

    See the full article here .


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    Please help promote STEM in your local schools.

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  • richardmitnick 2:34 pm on May 30, 2018 Permalink | Reply
    Tags: , , , , , , Does Some Dark Matter Carry an Electric Charge?, EDGES collaboration   

    From Harvard-Smithsonian Center for Astrophysics: “Does Some Dark Matter Carry an Electric Charge?” 

    Harvard Smithsonian Center for Astrophysics


    From Harvard-Smithsonian Center for Astrophysics

    May 30, 2018

    Megan Watzke
    Harvard-Smithsonian Center for Astrophysics
    +1 617-496-7998
    mwatzke@cfa.harvard.edu

    Peter Edmonds
    Harvard-Smithsonian Center for Astrophysics
    +1 617-571-7279
    pedmonds@cfa.harvard.edu

    1

    Astronomers have proposed a new model for the invisible material that makes up most of the matter in the Universe. They have studied whether a fraction of dark matter particles may have a tiny electrical charge.

    “You’ve heard of electric cars and e-books, but now we are talking about electric dark matter,” said Julian Munoz of Harvard University in Cambridge, Mass., who led the study that has been published in the journal Nature. “However, this electric charge is on the very smallest of scales.”

    Munoz and his collaborator, Avi Loeb of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Mass., explore the possibility that these charged dark matter particles interact with normal matter by the electromagnetic force.

    Their new work dovetails with a recently announced result from the Experiment to Detect the Global EoR (Epoch of Reionization) Signature (EDGES) collaboration. In February, scientists from this project said they had detected the radio signature from the first generation of stars, and possible evidence for interaction between dark matter and normal matter. Some astronomers quickly challenged the EDGES claim. Meanwhile, Munoz and Loeb were already looking at the theoretical basis underlying it.

    “We’re able to tell a fundamental physics story with our research no matter how you interpret the EDGES result,” said Loeb, who is the chair of the Harvard astronomy department. “The nature of dark matter is one of the biggest mysteries in science and we need to use any related new data to tackle it.”

    The story begins with the first stars, which emitted ultraviolet (UV) light. According to the commonly accepted scenario, this UV light interacted with cold hydrogen atoms in gas lying between the stars and enabled them to absorb the cosmic microwave background (CMB) radiation, the leftover radiation from the Big Bang.

    CMB per ESA/Planck

    ESA/Planck 2009 to 2013

    This absorption should have led to a drop in intensity of the CMB during this period, which occurs less than 200 million years after the Big Bang. The EDGES team claimed to detect evidence for this absorption of CMB light, though this has yet to be independently verified by other scientists. However, the temperature of the hydrogen gas in the EDGES data is about half of the expected value.

    “If EDGES has detected cooler than expected hydrogen gas during this period, what could explain it?” said Munoz. “One possibility is that hydrogen was cooled by the dark matter.”

    At the time when CMB radiation is being absorbed, the any free electrons or protons associated with ordinary matter would have been moving at their slowest possible speeds (since later on they were heated by X-rays from the first black holes). Scattering of charged particles is most effective at low speeds. Therefore, any interactions between normal matter and dark matter during this time would have been the strongest if some of the dark matter particles are charged. This interaction would cause the hydrogen gas to cool because the dark matter is cold, potentially leaving an observational signature like that claimed by the EDGES project.

    “We are constraining the possibility that dark matter particles carry a tiny electrical charge – equal to one millionth that of an electron – through measurable signals from the cosmic dawn,” said Loeb. “Such tiny charges are impossible to observe even with the largest particle accelerators.”

    Only small amounts of dark matter with weak electrical charge can both explain the EDGES data and avoid disagreement with other observations. If most of the dark matter is charged, then these particles would have been deflected away from regions close to the disk of our own Galaxy, and prevented from reentering. This conflicts with observations showing that large amounts of dark matter are located close to the disk of the Milky Way.

    Scientists know from observations of the CMB that protons and electrons combined in the early Universe to form neutral atoms. Only a small fraction of these charged particles, about one in a few thousand, remained free. Munoz and Loeb are considering the possibility that dark matter may have acted in a similar way. The data from EDGES, and similar experiments, might be the only way to detect the few remaining charged particles, as most of the dark matter would be neutral.

    “The viable parameter space for this scenario is quite constrained, but if confirmed by future observations, of course we would be learning something fundamental about the nature of dark matter, one of the biggest puzzles that we have in physics today,” said Harvard’s Cora Dvorkin who was not involved with the new study.

    Lincoln Greenhill also from the CfA is currently testing the observational claim by the EDGES team. He leads the Large Aperture Experiment to Detect the Dark Ages (LEDA) project, which uses the Long Wavelength Array in Owen’s Valley California and Socorro, New Mexico.

    A paper describing these results appear in the May 31, 2018 issue of the journal Nature.

    See the full article here .


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    Stem Education Coalition

    The Center for Astrophysics combines the resources and research facilities of the Harvard College Observatory and the Smithsonian Astrophysical Observatory under a single director to pursue studies of those basic physical processes that determine the nature and evolution of the universe. The Smithsonian Astrophysical Observatory (SAO) is a bureau of the Smithsonian Institution, founded in 1890. The Harvard College Observatory (HCO), founded in 1839, is a research institution of the Faculty of Arts and Sciences, Harvard University, and provides facilities and substantial other support for teaching activities of the Department of Astronomy.

     
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