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    <title>Qualla: Sudbury Neutrino Observatory</title>
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    <description><![CDATA[Two kilometers underground in a Sudbury nickel mine, physicists built a cathedral-sized detector filled with heavy water and solved one of the great puzzles of particle physics, earning a Nobel Prize for proving that neutrinos change identity as they travel from the sun.]]></description>
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    <itunes:summary><![CDATA[Two kilometers underground in a Sudbury nickel mine, physicists built a cathedral-sized detector filled with heavy water and solved one of the great puzzles of particle physics, earning a Nobel Prize for proving that neutrinos change identity as they travel from the sun.]]></itunes:summary>
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      <title>Qualla: Sudbury Neutrino Observatory</title>
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      <title>Sudbury Neutrino Observatory: Introduction</title>
      <link>https://qualla.com/sudbury-neutrino-observatory/</link>
      <description><![CDATA[Photo credit User:Boardhead, CC0. Somewhere beneath your feet, if you are flying over Greater Sudbury, Ontario, a Nobel Prize was won in darkness. Two thousand one hundred meters below the surface, inside Vale's Creighton Mine, physicists constructed the Sudbury Neutrino Observatory -- a spherical detector lined with 9,600 photomultiplier tubes, watching a thousand tonnes of heavy water for the faintest flashes of blue light. The light came from neutrinos, ghost particles streaming from the core of the sun, passing through the Earth almost without a trace. Almost. Between May 1999 and November 2006, SNO caught enough of those traces to solve a mystery that had haunted physics for forty years. The sun was not broken. The neutrinos were changing.]]></description>
      <content:encoded><![CDATA[<p>Photo credit User:Boardhead, CC0. Somewhere beneath your feet, if you are flying over Greater Sudbury, Ontario, a Nobel Prize was won in darkness. Two thousand one hundred meters below the surface, inside Vale's Creighton Mine, physicists constructed the Sudbury Neutrino Observatory -- a spherical detector lined with 9,600 photomultiplier tubes, watching a thousand tonnes of heavy water for the faintest flashes of blue light. The light came from neutrinos, ghost particles streaming from the core of the sun, passing through the Earth almost without a trace. Almost. Between May 1999 and November 2006, SNO caught enough of those traces to solve a mystery that had haunted physics for forty years. The sun was not broken. The neutrinos were changing.</p>
<p><strong>Read more:</strong> <a href="https://qualla.com/sudbury-neutrino-observatory/">Sudbury Neutrino Observatory on Qualla</a></p><p><em>Image: User:Boardhead | CC0</em></p>]]></content:encoded>
      <pubDate>Mon, 23 Feb 2026 00:00:00 GMT</pubDate>
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      <itunes:duration>0:06</itunes:duration>
      <itunes:episode>1</itunes:episode>
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      <title>Sudbury Neutrino Observatory: The Missing Neutrinos</title>
      <link>https://qualla.com/sudbury-neutrino-observatory/</link>
      <description><![CDATA[Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. Since the 1960s, every detector on Earth had counted roughly a third to a half fewer neutrinos arriving from the sun than the Standard Solar Model predicted. The discrepancy became known as the solar neutrino problem, and it persisted for decades. Either the models of how the sun...]]></description>
      <content:encoded><![CDATA[<p>Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. Since the 1960s, every detector on Earth had counted roughly a third to a half fewer neutrinos arriving from the sun than the Standard Solar Model predicted. The discrepancy became known as the solar neutrino problem, and it persisted for decades. Either the models of how the sun...</p>
<p><strong>Read more:</strong> <a href="https://qualla.com/sudbury-neutrino-observatory/">Sudbury Neutrino Observatory on Qualla</a></p><p><em>Image: NASA, ESA, J. Hester and A. Loll (Arizona State University) | Public domain</em></p>]]></content:encoded>
      <pubDate>Mon, 23 Feb 2026 00:00:00 GMT</pubDate>
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      <itunes:episode>2</itunes:episode>
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      <title>Sudbury Neutrino Observatory: Heavy Water and Deep Rock</title>
      <link>https://qualla.com/sudbury-neutrino-observatory/</link>
      <description><![CDATA[Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. In 1984, physicist Herb Chen of the University of California at Irvine proposed a detector using heavy water, in which hydrogen atoms carry an extra neutron. Heavy water enabled two distinct detection reactions: one sensitive only to electron neutrinos, the other sensitive to all...]]></description>
      <content:encoded><![CDATA[<p>Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. In 1984, physicist Herb Chen of the University of California at Irvine proposed a detector using heavy water, in which hydrogen atoms carry an extra neutron. Heavy water enabled two distinct detection reactions: one sensitive only to electron neutrinos, the other sensitive to all...</p>
<p><strong>Read more:</strong> <a href="https://qualla.com/sudbury-neutrino-observatory/">Sudbury Neutrino Observatory on Qualla</a></p><p><em>Image: NASA, ESA, J. Hester and A. Loll (Arizona State University) | Public domain</em></p>]]></content:encoded>
      <pubDate>Mon, 23 Feb 2026 00:00:00 GMT</pubDate>
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      <title>Sudbury Neutrino Observatory: A Cathedral of Light</title>
      <link>https://qualla.com/sudbury-neutrino-observatory/</link>
      <description><![CDATA[Photo credit Boardhead at English Wikipedia, CC BY-SA 3.0. The finished detector was an engineering marvel. A 12-meter acrylic vessel held the heavy water, surrounded by a cavity filled with ordinary water for buoyancy and radiation shielding. Approximately 9,600 photomultiplier tubes, mounted on a geodesic sphere, watched for the tellta...]]></description>
      <content:encoded><![CDATA[<p>Photo credit Boardhead at English Wikipedia, CC BY-SA 3.0. The finished detector was an engineering marvel. A 12-meter acrylic vessel held the heavy water, surrounded by a cavity filled with ordinary water for buoyancy and radiation shielding. Approximately 9,600 photomultiplier tubes, mounted on a geodesic sphere, watched for the tellta...</p>
<p><strong>Read more:</strong> <a href="https://qualla.com/sudbury-neutrino-observatory/">Sudbury Neutrino Observatory on Qualla</a></p><p><em>Image: Boardhead at English Wikipedia | CC BY-SA 3.0</em></p>]]></content:encoded>
      <pubDate>Mon, 23 Feb 2026 00:00:00 GMT</pubDate>
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      <itunes:episode>4</itunes:episode>
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      <title>Sudbury Neutrino Observatory: Neutrinos Change Their Stripes</title>
      <link>https://qualla.com/sudbury-neutrino-observatory/</link>
      <description><![CDATA[Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. On June 18, 2001, SNO published its first results: clear evidence that solar neutrinos oscillate, transforming from one flavor to another during their journey from the sun. The total neutrino flux across all three flavors matched the Standard Solar Model's predictions. The sun wa...]]></description>
      <content:encoded><![CDATA[<p>Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. On June 18, 2001, SNO published its first results: clear evidence that solar neutrinos oscillate, transforming from one flavor to another during their journey from the sun. The total neutrino flux across all three flavors matched the Standard Solar Model's predictions. The sun wa...</p>
<p><strong>Read more:</strong> <a href="https://qualla.com/sudbury-neutrino-observatory/">Sudbury Neutrino Observatory on Qualla</a></p><p><em>Image: NASA, ESA, J. Hester and A. Loll (Arizona State University) | Public domain</em></p>]]></content:encoded>
      <pubDate>Mon, 23 Feb 2026 00:00:00 GMT</pubDate>
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      <itunes:episode>5</itunes:episode>
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      <title>Sudbury Neutrino Observatory: Nobel Recognition</title>
      <link>https://qualla.com/sudbury-neutrino-observatory/</link>
      <description><![CDATA[Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. In 2015, the Nobel Prize in Physics was awarded jointly to SNO's director, Arthur B. McDonald, and Takaaki Kajita of Super-Kamiokande for the discovery of neutrino oscillation. The SNO team had already received the inaugural John C. Polanyi Award in 2006 and the 2016 Fundamental ...]]></description>
      <content:encoded><![CDATA[<p>Photo credit NASA, ESA, J. Hester and A. Loll (Arizona State University), Public domain. In 2015, the Nobel Prize in Physics was awarded jointly to SNO's director, Arthur B. McDonald, and Takaaki Kajita of Super-Kamiokande for the discovery of neutrino oscillation. The SNO team had already received the inaugural John C. Polanyi Award in 2006 and the 2016 Fundamental ...</p>
<p><strong>Read more:</strong> <a href="https://qualla.com/sudbury-neutrino-observatory/">Sudbury Neutrino Observatory on Qualla</a></p><p><em>Image: NASA, ESA, J. Hester and A. Loll (Arizona State University) | Public domain</em></p>]]></content:encoded>
      <pubDate>Mon, 23 Feb 2026 00:00:00 GMT</pubDate>
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