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    <channel>
      <title> Discover Magazine | Subatomic Particles</title>
      <link>http://discovermagazine.com</link>
      
      <description>
          Science, Technology, and The Future
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      <item>
        <title>Big Idea: Physicists Carve a Niche in Time</title>
        <link>http://discovermagazine.com/2012/apr/08-big-idea-physicists-carve-a-niche-in-time</link>
        <guid>http://discovermagazine.com/2012/apr/08-big-idea-physicists-carve-a-niche-in-time</guid>
        <description>&lt;img class="inline" src="http://discovermagazine.com/2012/apr/08-big-idea-physicists-carve-a-niche-in-time/time.jpg" alt="light &amp; time" align="left"&gt;
&lt;p&gt;Physicists routinely baffle reporters, but for once things went the other way. &lt;a href="http://focus.aep.cornell.edu/people.html" class="external-link"&gt;Alexander Gaeta&lt;/a&gt; was sitting in his Cornell University office in the fall of 2010 when a reporter called to ask his opinion of a &lt;a href="http://iopscience.iop.org/2040-8986/13/2/024003" class="external-link"&gt;strange new paper&lt;/a&gt; in the &lt;i&gt;Journal of Optics&lt;/i&gt;: What did he think about the claim that it might be possible to create a time cloak, a device that would render events undetectable?&lt;/p&gt;
&lt;p&gt;Gaeta was caught off guard. He was still grappling with the invisibility cloak, a wild idea that turned into reality in 2006, when physicists demonstrated that a &lt;a href="http://www.sciencemag.org/content/314/5801/977" class="external-link"&gt;class of synthetic materials could bend light completely around an object&lt;/a&gt;. (Think of water in a stream flowing around a rock.) Without light bouncing off the object, it would essentially disappear.&lt;/p&gt;
&lt;p&gt;But creating a time cloak–something that could hide not just an object but an event–is even more ambitious. Rather than just rerouting the rays of light striking an object, a time cloak would have to deflect all the light beams influenced by the object as it moves through space. The time cloak would, in essence, create an interval during which all information about what an object is doing disappears.&lt;/p&gt;
&lt;p&gt;Although Gaeta had not heard of the time-cloak study until that phone call, he dove into it as soon as the reporter sent it over. The author, theoretical physicist &lt;a href="http://www3.imperial.ac.uk/people/m.mccall" class="external-link"&gt;Martin McCall&lt;/a&gt;&amp;nbsp;of Imperial College London, proposed splitting a light beam into two segments moving at different speeds. As one fragment built a lead on the other, a gap of complete darkness would open up between them. Anything happening within that gap, McCall reasoned, would be impossible to detect, since there would be no light to scatter. Then, to complete the trick, McCall proposed bringing those two segments back together so that by the time the beam of light reached an observer, there would be no way to detect that the gap ever existed...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Adam Piore
          
        </creator> 

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            <url>http://discovermagazine.com/2012/apr/08-big-idea-physicists-carve-a-niche-in-time/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 07 May 2012 10:30:00 -0400</pubDate>
        <lastBuildDate>Mon, 07 May 2012 10:30:00 -0400</lastBuildDate>
        <type>Print Article</type>    
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      <item>
        <title>Is Einstein's Greatest Work All Wrong—Because He Didn't Go Far Enough? </title>
        <link>http://discovermagazine.com/2012/mar/09-is-einsteins-greatest-work-wrong-didnt-go-far</link>
        <guid>http://discovermagazine.com/2012/mar/09-is-einsteins-greatest-work-wrong-didnt-go-far</guid>
        <description>&lt;img src="http://discovermagazine.com/2012/mar/09-is-einsteins-greatest-work-wrong-didnt-go-far/abell1689.jpg" alt="Galaxy cluster Abell 1689"&gt;
&lt;p&gt;Julian Barbour cuts an unlikely figure for a radical. We sip afternoon tea at his farmhouse in the sleepy English village of South Newington, and he playfully quotes Faust: &lt;i&gt;That I may understand whatever binds the world’s innermost core together, see all its workings, and its seeds.&lt;/i&gt; His love of Goethe’s classic poem, about a scholar who sells his soul to the devil in exchange for unlimited knowledge, is apropos. Forty years ago, Barbour’s desire to uncover the innermost workings of the universe led him to make a seemingly reckless gamble. He sacrificed a secure and potentially prestigious career as an academic to strike out on independent research of his own. His starry-eyed quest: upending Albert Einstein’s theory of relativity, and with it our understanding of gravity, space, and time.&lt;/p&gt;
&lt;p&gt;It was less than a century ago that Einstein was the most radical physics thinker around. With his general theory of relativity, he discarded the traditional notion of space and time as fixed and redefined them as flexible dimensions woven together to create a four-dimensional fabric that pervades the universe. In Einstein’s vision, this stretchy version of space-time is the source of gravity. The fabric bends and warps severely around massive objects such as the sun, drawing smaller objects such as planets toward them. The force that we perceive as gravity is the result.&lt;/p&gt;
&lt;p&gt;Yet Einstein’s fabric left a few loose threads that cosmologists have struggled to tie up ever since. For one, general relativity alone cannot explain the observed motions of galaxies or the way the universe seems to expand. If Einstein’s model of gravity is correct, around 96 percent of the cosmos appears to be missing. To make up the difference, cosmologists have posited two mysterious, invisible, and as yet unidentified ingredients: dark matter and dark energy, a double budget deficit that makes many scientists uncomfortable. Einstein also failed to deliver an all-encompassing theory of “quantum gravity”—one that reconciled the laws of gravity observed on the scale of stars and galaxies with the laws of quantum mechanics, the branch of physics that explains the behavior of particles in the subatomic realm.&lt;/p&gt;
&lt;p&gt;While other scientists tread softly around the edges of Einstein’s theory, hoping to tweak it into compliance, Barbour and a growing cadre of collaborators see a need for a bold march forward. They aim to demolish the space-time fabric that stands as Einstein’s legacy and remap the universe without it. This new cosmic code could eliminate the need to invoke dark matter and dark energy. Even more exciting, it could also open the door to the theory of quantum gravity that Einstein was never able to derive. If Barbour is right, some of the most fundamental things cosmologists think they know about the origin and evolution of the universe would have to be revised...&lt;/p&gt;
&lt;p&gt;&lt;i&gt;Image: Galaxy cluster Abell 1689 seems to be held together by swaths of unseen dark matter; blue shows its theoretically inferred location. But could dark matter be an illusion? Courtesy of NASA&lt;/i&gt;&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Zeeya Merali
          
        </creator> 

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            <url>http://discovermagazine.com/2012/mar/09-is-einsteins-greatest-work-wrong-didnt-go-far/key_image</url>
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        <rights></rights>        
        <pubDate>Tue, 01 May 2012 12:35:00 -0400</pubDate>
        <lastBuildDate>Tue, 01 May 2012 12:35:00 -0400</lastBuildDate>
        <type>Print Article</type>    
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      <item>
        <title>20 Things You Didn't Know About... Math</title>
        <link>http://discovermagazine.com/2012/mar/09-things-you-didnt-know-about-math</link>
        <guid>http://discovermagazine.com/2012/mar/09-things-you-didnt-know-about-math</guid>
        <description>&lt;img src="http://discovermagazine.com/2012/mar/09-things-you-didnt-know-about-math/math.jpg" alt="chalkboard math"&gt;
&lt;p&gt;&lt;b&gt;5&amp;nbsp;&lt;/b&gt;&amp;nbsp;Sometimes the oddest bits of math often turn out to be useful. &lt;a class="external-link" href="http://en.wikipedia.org/wiki/Quaternion"&gt;Quaternions&lt;/a&gt;, which can describe the rotation of 3-D objects, were discovered in 1843. They were considered beautiful but useless until 1985, when computer scientists applied them to rendering digital animation.&lt;/p&gt;

&lt;p&gt;&lt;b&gt;8&amp;nbsp;&lt;/b&gt;&amp;nbsp;Kurt Gödel, the renowned Austrian logician, made math a lot more confusing in 1931 with his &lt;a class="external-link" href="http://en.wikipedia.org/wiki/G%C3%B6del's_incompleteness_theorems"&gt;first incompleteness theorem,&lt;/a&gt; which said that any sufficiently powerful math system must contain statements that are true but unprovable. Gödel starved himself to death in 1978.&lt;/p&gt;


&lt;p&gt;&lt;b&gt;19&amp;nbsp;&lt;/b&gt;&amp;nbsp;Graduate student George Dantzig arrived late to statistics class at Berkeley one day in 1939 and copied two problems off the blackboard. He handed in the answers a few days later, apologizing that they were harder than usual.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;20&amp;nbsp;&lt;/b&gt;&amp;nbsp;The “homework” was actually two well-known unproven theorems. Dantzig’s story became famous and inspired a scene from&lt;i&gt; Good Will Hunting&lt;/i&gt;...&lt;/p&gt;
</description>
        <publisher></publisher>        
        <creator>
          
            Peter Coy
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/mar/09-things-you-didnt-know-about-math/key_image</url>
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        <rights></rights>        
        <pubDate>Fri, 23 Mar 2012 11:20:00 -0400</pubDate>
        <lastBuildDate>Fri, 23 Mar 2012 11:20:00 -0400</lastBuildDate>
        <type>Print Article</type>    
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      <item>
        <title>How to Survive the End of the Universe</title>
        <link>http://discovermagazine.com/2011/dec/16-how-to-survive-the-end-of-the-universe</link>
        <guid>http://discovermagazine.com/2011/dec/16-how-to-survive-the-end-of-the-universe</guid>
        <description>&lt;img src="http://discovermagazine.com/2011/dec/16-how-to-survive-the-end-of-the-universe/opener.jpg" align="right" alt=""&gt;
&lt;p&gt;Next year will be a doozy for doomsayers. depending on the prophecy, the world is predestined to expire by means of a solar storm, asteroid strike, rogue-planet collision, plague, falling stars, earthquake, debt crisis, or some combination thereof. Of course, nobody seems to be preparing for any of these impending 2012 apocalypses, with the exception of a porn studio reportedly building a clothing-optional underground bunker.&lt;/p&gt;
&lt;p&gt;And why should we? Scientifically speaking, the prophecies are strictly ballyhoo. Physicists can do a lot better. When it comes to end-times scenarios, cosmological data-crunchers have at their disposal far more meaningful prognostication tools that can tell us how it’s really going to end—not just Earth, but the whole universe. Best of all, they can tell us how to survive it.&lt;/p&gt;
&lt;p&gt;Science, oddly, is a lot better at predicting things like the death of stars than next week’s weather. The same laws of physics that enable scientists to study the Big Bang that occurred 13.7 billion years ago also allow them to gaze into the future with great precision. And few people have peered farther than University of California, Santa Cruz, astronomer Greg Laughlin, science’s leading soothsayer. As a graduate student in 1992, he was plugging away at a simple computer simulation of star formation when he broke for lunch and accidentally left the simulation running. When he returned an hour later, the simulation had advanced 100 million billion years, much further into the future than most scientists ever think (or dare) to explore.&lt;/p&gt;
&lt;p&gt;The program itself didn’t reveal anything terribly startling—the simulated star had long since gone cold and died—but Laughlin was intrigued by the concept of using physical simulations to traverse enormous gulfs of time. “It opened my eyes to the fact that things are going to evolve and are still going to be there in timescales that dwarf the current age of the universe,” he says.&lt;/p&gt;
&lt;p&gt;Four years later, still fascinated, Laughlin teamed up with Fred Adams, a physics professor at the University of Michigan, to investigate the future of the universe more rigorously. Working in their spare time, the two researchers coauthored a 57-page paper in the journal&lt;i&gt; Reviews of Modern Physics&lt;/i&gt; that detailed a succession of future apocalypses: the death of the sun, the end of the stars, and multiple scenarios for the fate of the universe as a whole...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Andrew Grant; illustration by Chris Gall
          
        </creator> 

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            <url>http://discovermagazine.com/2011/dec/16-how-to-survive-the-end-of-the-universe/key_image</url>
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        <rights></rights>        
        <pubDate>Tue, 28 Feb 2012 10:25:00 -0500</pubDate>
        <lastBuildDate>Tue, 28 Feb 2012 10:25:00 -0500</lastBuildDate>
        <type>Print Article</type>    
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        <title>How to See the Invisible: 3 Approaches to Finding Dark Matter</title>
        <link>http://discovermagazine.com/2011/nov/18-how-see-invisible-3-approaches-dark-matter</link>
        <guid>http://discovermagazine.com/2011/nov/18-how-see-invisible-3-approaches-dark-matter</guid>
        <description>&lt;img src="http://discovermagazine.com/2011/nov/18-how-see-invisible-3-approaches-dark-matter/spiralgalaxy.jpg" align="right" alt=""&gt;Spiral galaxy M74 holds 100 billion stars. Oddly, stars at its outer edges rotate with the same velocity as those closer in, suggesting the influence of a substantial mass of unseen dark matter. &lt;br&gt;&lt;br&gt;Credit: NASA&lt;/p&gt;
&lt;p&gt; Although we live in a renaissance era of cosmology, in which theories and observations have advanced to the stage where ideas can be precisely tested, we also live in the dark ages. About 23 percent of the universe consists of dark matter, mysterious stuff that exerts gravitational forces but doesn’t interact with light. Ordinary matter makes up just 4 percent. (Another 73 percent is dark energy, an even more mysterious component that permeates the universe.)&lt;/p&gt;
&lt;p&gt;The last time something was called “dark” in physics was in the mid-1800s, when Urbain-Jean-Joseph Leverrier of France proposed an unseen dark planet, which he named Vulcan. Leverrier’s goal was to explain the peculiar trajectory of the planet Mercury. Leverrier, along with John C. Adams of England, had previously deduced the existence of Neptune based on its effects on the planet Uranus. Yet he was wrong about Mercury. It turned out that the reason for Mercury’s strange orbit was much more dramatic than the existence of another planet. The explanation could be found only with Einstein’s theory of relativity. The first confirmation that the theory of general relativity was correct came when Einstein proved it could be used it to accurately predict Mercury’s orbit.&lt;/p&gt;
&lt;p&gt;It could turn out that dark matter presages a similar paradigm change. Even so, I’d say that it is very likely to have a more conventional explanation, consistent with the type of physical laws we now know. After all, even if novel matter acts in accordance with force laws similar to those we know, why should all matter behave exactly like familiar matter? To put it more succinctly, why should all matter interact with light? If the history of science has taught us anything, it should be the shortsightedness of believing that what we see is all there is...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Lisa Randall
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2011/nov/18-how-see-invisible-3-approaches-dark-matter/key_image</url>
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        <rights></rights>        
        <pubDate>Wed, 22 Feb 2012 10:30:00 -0500</pubDate>
        <lastBuildDate>Wed, 22 Feb 2012 10:30:00 -0500</lastBuildDate>
        <type>Print Article</type>    
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        <title>How I Dismantled the World’s Deadliest Weapon</title>
        <link>http://discovermagazine.com/2012/mar/01-how-i-dismantled-the-worlds-deadliest-weapon</link>
        <guid>http://discovermagazine.com/2012/mar/01-how-i-dismantled-the-worlds-deadliest-weapon</guid>
        <description>&lt;p&gt;&lt;b&gt;&lt;i&gt;In October Sandia National Laboratories engineer Phil Hoover dismantled the U.S. arsenal’s last B53, a 9-megaton bomb 600 times as powerful as the one dropped on Hiroshima. Hoover talked to DISCOVER about taking apart America’s most powerful weapon.&lt;/i&gt;&lt;/b&gt;&lt;/p&gt;
&lt;p&gt;&lt;img alt="Phil Hoover dissembling B53 bomb" src="http://discovermagazine.com/2012/mar/01-how-i-dismantled-the-worlds-deadliest-weapon/atomic.jpg"&gt;&lt;/p&gt;
&lt;p&gt;The B53 was big and heavy, about the size of a minivan and 10,000 pounds. We needed 130 engineers and scientists from across the nuclear weapons enterprise to take it apart. Even though &lt;a href="http://en.wikipedia.org/wiki/B53_nuclear_bomb" class="external-link"&gt;the B53&lt;/a&gt; was designed to be rather easily disassembled, it still took us about two weeks per bomb.&lt;/p&gt;
&lt;p&gt;All of the nuclear explosive disassembly was done in one well-lit, clean, and orderly room large enough to hold a Volkswagen van. We wore cover­alls, safety glasses, gloves, safety shoes, and dosimeters to track radiation exposure. Typically three or four people at a time actually did the work. There wasn’t much small talk—the operation required focus...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Phil Hoover, as told to Michael Rosenwald;  illustration by Zina Saunders
          
        </creator> 

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            <url>http://discovermagazine.com/2012/mar/01-how-i-dismantled-the-worlds-deadliest-weapon/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 20 Feb 2012 07:05:00 -0500</pubDate>
        <lastBuildDate>Mon, 20 Feb 2012 07:05:00 -0500</lastBuildDate>
        <type>Print Article</type>    
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        <title>20 Things You Didn't Know About... Clouds</title>
        <link>http://discovermagazine.com/2012/jan-feb/20-things-you-didnt-know-about-clouds</link>
        <guid>http://discovermagazine.com/2012/jan-feb/20-things-you-didnt-know-about-clouds</guid>
        <description>&lt;p class="imgcapright"&gt;&lt;img class="inline" src="clouds.jpg" alt="" kupu-src="http://72.32.204.61/2012/jan-feb/14-things-you-didn2019t-know-about-clouds/clouds.jpg"&gt;&lt;/p&gt;

&lt;p&gt;&lt;b&gt;4 &amp;nbsp;&lt;/b&gt;So much for People Power. After reviewing 40 years of cloud-seeding efforts in an area north of Israel, researchers at Tel Aviv University have concluded that &lt;a class="external-link" href="http://www.tau.ac.il/~pinhas/papers/2010/Levin_et_al_AR_2010.pdf"&gt;seeding doesn’t actually produce additional precipitation&lt;/a&gt;&amp;nbsp;(pdf).&lt;/p&gt;


&lt;p&gt;&lt;b&gt;12&amp;nbsp;&lt;/b&gt;&amp;nbsp;Highest of them all: 50 miles up,  &lt;a class="external-link" href="http://science.nasa.gov/science-news/science-at-nasa/2003/19feb_nlc/"&gt;noctilucent, or “night shining,” clouds&lt;/a&gt; glow an eerie bluish white. They are invisible by day, but after sunset they catch solar rays shining from far below the horizon.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;13 &amp;nbsp;&lt;/b&gt;Noctilucent clouds seemed to first appear after the 1883 eruption of Krakatoa and are now a common sight.&lt;/p&gt;


&lt;p&gt;&lt;b&gt;18&amp;nbsp;&lt;/b&gt;&amp;nbsp;In 1959 Lt. Col. William Rankin was flying his F-8 fighter jet over a cumulonimbus when the engine failed. He parachuted out and spent the next 30 minutes bounced around inside the storm. Amazingly, he survived.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;19&amp;nbsp;&lt;/b&gt;&amp;nbsp;In 2007 German paragliding champion Ewa Wisnierska experienced “&lt;a class="external-link" href="http://en.wikipedia.org/wiki/Cloud_suck"&gt;cloud suck&lt;/a&gt;.” While gliding under a cumulonimbus, she was pulled upward to 32,000 feet. She blacked out due to lack of oxygen but regained consciousness at roughly 23,000 feet.&lt;/p&gt;

&lt;p&gt;&lt;i&gt;Image: A lenticular cloud over the Tararua Mountains in the North Island of New Zealand. Courtesy: NASA&lt;/p&gt;&lt;/i&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Rebecca Coffey
          
        </creator> 

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            <url>http://discovermagazine.com/2012/jan-feb/20-things-you-didnt-know-about-clouds/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 30 Jan 2012 12:35:00 -0500</pubDate>
        <lastBuildDate>Mon, 30 Jan 2012 12:35:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #1: Faster than the Speed of Light</title>
        <link>http://discovermagazine.com/2012/jan-feb/01</link>
        <guid>http://discovermagazine.com/2012/jan-feb/01</guid>
        <description>&lt;p&gt;Einstein, relativity, and much of 20th-century physics have come under assault from an esoteric but far-reaching experiment. A collaboration of 174 physicists fired bursts of neutrinos from the headquarters of CERN, the European Organization for Nuclear Research, in Geneva, Switzerland, to a detector in Gran Sasso, Italy. They tracked 16,111 of the ghostlike particles and measured how long they took to complete the trip. After three years of experiments and intense analysis, the team reported in September that the neutrinos were arriving one 17-millionth of a second early.&lt;/p&gt;
The minuscule discrepancy revealed by the experiment, dubbed OPERA (Oscillation Project with Emulsion-tRacking Apparatus), has staggering implications. It seems to indicate that the neutrinos were traveling faster than light, violating what has long been regarded as an ironclad cosmic law. If neutrinos really can do that, then Einstein’s theory of relativity, the backbone of modern physics, could break down. Time could flow in reverse. Neutrino-based messages could reach recipients before they were sent. An effect could precede its cause, which would explode our entire way of thinking about the universe...&lt;/p&gt;
&lt;p&gt;&lt;b&gt;&lt;i&gt;The full text of this article is available only to DISCOVER subscribers. Click through to the article to subscribe, log in, or buy a digital version of this issue.&lt;/i&gt;&lt;/b&gt;&lt;/p&gt;
</description>
        <publisher></publisher>        
        <creator>
          
            Gregory Mone
          
        </creator> 

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            <url>http://discovermagazine.com/2012/jan-feb/01/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 14:20:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 14:20:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #14: Astronomers Watch Black Hole Devour Star </title>
        <link>http://discovermagazine.com/2012/jan-feb/14</link>
        <guid>http://discovermagazine.com/2012/jan-feb/14</guid>
        <description>&lt;p&gt; Black holes have a reputation for destruction but it was only in 2011 that scientists caught one in the act, watching it  devour an errant star. In March NASA’s Swift satellite detected a gamma-ray burst, an eruption of high-energy radiation that usually indicates a stellar explosion. But whereas most bursts last only seconds, this one kept on going. Josh Bloom, an astronomer at the University of California, Berkeley, traced the burst to the center of a galaxy that hosts a black hole millions of times as massive as the sun, and concluded that the hole had just eaten a star-size meal (illustrated below). “It’s a pretty fantastic way for a star to die,” he says...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Gillian Conahan
          
        </creator> 

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            <url>http://discovermagazine.com/2012/jan-feb/14/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 13:15:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 13:15:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #17: Quantum Weirdness Enters the Larger World </title>
        <link>http://discovermagazine.com/2012/jan-feb/17</link>
        <guid>http://discovermagazine.com/2012/jan-feb/17</guid>
        <description>&lt;p&gt;An octopus-shaped molecule is giving Schrödinger’s cat competition as the mascot of the bizarre world of quantum physics, where matter can simultaneously exist in different states. Physicist Erwin Schrödinger’s famous thought experiment posited that a cat behaving according to quantum principles could be dead and alive at the same time. We are spared such paradoxes because the rules of quantum physics seem confined to subatomic objects— in the human-scale world, a cat is either alive or dead...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Katie Palmer
          
        </creator> 

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            <url>http://discovermagazine.com/2012/jan-feb/17/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 13:10:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 13:10:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #20: Helium’s Antimatter Twin Created  </title>
        <link>http://discovermagazine.com/2012/jan-feb/20</link>
        <guid>http://discovermagazine.com/2012/jan-feb/20</guid>
        <description>&lt;p&gt;In an atom smasher on long island, gold nuclei smash headlong into each other at nearly the speed of light, unleashing a fountain of matter and antimatter, which possess identical mass but reverse properties. Within that maelstrom, physicists have now found 18 particles of anti-helium-4: the antimatter twin of helium, and the heaviest piece of antimatter ever made...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Gillian Conahan 
          
        </creator> 

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            <url>http://discovermagazine.com/2012/jan-feb/20/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 13:05:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 13:05:00 -0500</lastBuildDate>
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      <item>
        <title>Top 100 Stories of 2011: #26: The New Physics of Bicycles</title>
        <link>http://discovermagazine.com/2012/jan-feb/26</link>
        <guid>http://discovermagazine.com/2012/jan-feb/26</guid>
        <description>&lt;p&gt;Some of the great mysteries of science hide in plain sight—and, in this case, roll on two wheels. As hands-free cyclists know, a bicycle in motion can recover from wobbles with no steering input, or even with no rider at all. But physicists have never agreed on how this self-balancing act works. Some argue the rotating wheels act like a gyroscope to help the bicycle correct itself; others believe the “trail” (the angle between a bike’s steering axis and its point of contact with the ground) forces the bike into a stabilizing turn. Now American and Dutch engineers have built a bicycle that defies both theories...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Gillian Conahan
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/26/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 13:00:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 13:00:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #32: Where’s the Higgs?</title>
        <link>http://discovermagazine.com/2012/jan-feb/32</link>
        <guid>http://discovermagazine.com/2012/jan-feb/32</guid>
        <description>&lt;p&gt;Particle physicists entered 2011 with high hopes. The Large Hadron Collider (LHC), a 17-mile tunnel straddling the border of France and Switzerland, was smashing protons together at unprecedented energies. By June the LHC had exceeded its full-year target of 70 million million collisions. But by the end of the year, many physicists were starting to sweat. The LHC delivered a flood of data, but none of it seemed to yield the discoveries everyone was hoping for. There were no signs of dark matter, no hints of extra dimensions, and not a whisper from the Higgs boson, the long-sought particle that is an essential component of the leading model of quantum physics...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Andrew Grant; photograph by Saverio Truglia
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/32/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 12:55:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 12:55:00 -0500</lastBuildDate>
        <type>Print Article</type>    
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        <title>Top 100 Stories of 2011: #62: Star Birth Seen in Action </title>
        <link>http://discovermagazine.com/2012/jan-feb/62</link>
        <guid>http://discovermagazine.com/2012/jan-feb/62</guid>
        <description>&lt;p&gt;As a star forms, it attracts a swirling disk of gas and dust. Most of that material collapses into the star. Some remains in orbit, where it clumps to form planets. And some shoots like a jet from the disk’s center at velocities up to 30 times the speed of sound, triggering supersonic shock waves. Last year, Patrick Hartigan of Rice University selected images from 14 years of Hubble Space Telescope observations to produce a flip-book animation of the rippling wakes and collisions in those shock waves...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Paul Raeburn
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/62/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 12:50:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 12:50:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #65: America’s Atom Smasher, 1983–2011</title>
        <link>http://discovermagazine.com/2012/jan-feb/65</link>
        <guid>http://discovermagazine.com/2012/jan-feb/65</guid>
        <description>&lt;p&gt;The Tevatron, a particle accelerator based at the Fermi National Accelerator Laboratory in Batavia, Illinois, shut down on September 30. The machine was 28. The cause of death was the bigger, more powerful Large Hadron Collider (LHC) in Geneva, Switzerland...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Gregory Mone
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/65/key_image</url>
        </image>

        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 12:45:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 12:45:00 -0500</lastBuildDate>
        <type>Print Article</type>    
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        <title>Top 100 Stories of 2011: #82: Could Random Airplane Boarding Speed Your Trip? </title>
        <link>http://discovermagazine.com/2012/jan-feb/82</link>
        <guid>http://discovermagazine.com/2012/jan-feb/82</guid>
        <description>&lt;p&gt;Slow boarding annoyed Jason Steffen. but rather than complain about it, like most of us would, the Fermilab astrophysicist took to his computer and began writing algorithms to model potential solutions. In 2008 he announced a method that he claimed would cut boarding times in half, but it wasn’t until last year that he finally had the opportunity to test his technique in a realistic setting...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Stephen Ornes
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/82/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 12:40:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 12:40:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #83: Gravity Probe B Gives Einstein an A </title>
        <link>http://discovermagazine.com/2012/jan-feb/83</link>
        <guid>http://discovermagazine.com/2012/jan-feb/83</guid>
        <description>&lt;p&gt;Faster-than-light neutrinos may eventually sully Einstein’s legacy (see story #1), but in the meantime another experiment has confirmed two predictions of his general theory of relativity. The $700 million Gravity Probe B satellite, launched in 2004, contained four nearly perfectly spherical gyroscopes isolated from all outside influences—magnetic fields, friction, gravity—leaving them exposed only to relativistic effects. Einstein’s theory predicted that the orientation of the gyroscopes should slowly drift due to two phenomena: the geodetic effect, or Earth’s warping of space-time due to its mass, and frame-dragging, the tug on space-time that occurs as Earth rotates on its axis...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Andrew Grant
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/83/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 12:35:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 12:35:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #93: Super- Rocket Tested </title>
        <link>http://discovermagazine.com/2012/jan-feb/93</link>
        <guid>http://discovermagazine.com/2012/jan-feb/93</guid>
        <description>&lt;p&gt;While private space companies were making their move (see below), NASA began testing the J-2X rocket engine, one of the powerhouses behind the agency’s Space Launch System that could drive the next stage of manned space exploration...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Sarah Stanley
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/93/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 12:30:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 12:30:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #95: Computer Builds  A Perfect Galaxy </title>
        <link>http://discovermagazine.com/2012/jan-feb/95</link>
        <guid>http://discovermagazine.com/2012/jan-feb/95</guid>
        <description>&lt;p&gt;It took nature 13 billion years to create our galaxy, the Milky Way. Last August a group of scientists reported that they had replicated the feat in just nine months. To be fair, they created only a digital simulation, nicknamed Eris, but it is the first one to accurately reproduce the details of a galaxy like our own...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Adam Hadhazy
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/95/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 09 Jan 2012 12:25:00 -0500</pubDate>
        <lastBuildDate>Mon, 09 Jan 2012 12:25:00 -0500</lastBuildDate>
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        <title>Top 100 Stories of 2011: #11: Scientist of the  Arab Spring</title>
        <link>http://discovermagazine.com/2012/jan-feb/11</link>
        <guid>http://discovermagazine.com/2012/jan-feb/11</guid>
        <description>&lt;p&gt;When Ahmed Zewail first heard of the popular revolt against Egyptian president Hosni Mubarak on January 25, 2011, he immediately left for Cairo. “It was a very emotional time. I have family in Egypt, and I owe the country my early education,” says Zewail, who is a professor of chemistry at Caltech. “I knew I had to take action.”&lt;/p&gt;
&lt;p&gt;Zewail was in a unique position to help: He won the Nobel Prize in Chemistry in 1999 for his groundbreaking work using lasers to observe chemical reactions, becoming Egypt’s first and only Nobel laureate in science. He also became a national celebrity and a sympathetic ear for the growing frustrations over Egypt’s failing educational system. Under Mubarak, scientists were underpaid; public universities were run by party favorites and crammed with more than 1,000 students per class...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Amy Barth; photograph by Shawn Baldwin
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2012/jan-feb/11/key_image</url>
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        <rights></rights>        
        <pubDate>Tue, 03 Jan 2012 12:35:00 -0500</pubDate>
        <lastBuildDate>Tue, 03 Jan 2012 12:35:00 -0500</lastBuildDate>
        <type>Print Article</type>    
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      <item>
        <title>Selling Cheap: Abandoned, Half-Finished, Would-Be Collider Facility</title>
        <link>http://discovermagazine.com/2011/nov/10-selling-cheap-abandoned-half-finished-collider</link>
        <guid>http://discovermagazine.com/2011/nov/10-selling-cheap-abandoned-half-finished-collider</guid>
        <description>&lt;img src="http://discovermagazine.com/2011/nov/10-selling-cheap-abandoned-half-finished-collider/ssc.jpg" align="right" alt=""&gt;Image: Wikimedia Commons&lt;/p&gt;
&lt;p&gt;&lt;b&gt;$6.5 million&lt;/b&gt;: The initial asking price for the 135-acre property in Texas that two decades ago was supposed to be the site of the world’s most powerful particle accelerator, the Superconducting Super Collider. Congress canceled the project in 1993 after spending $2 billion (300 times the site’s current price) to construct eight buildings and 14 miles of underground tunnels. At press time the property was under contract. Bryan Loewen, a real estate agent at Newmark Knight Frank who is handling the sale, says potential buyers expressed interest in using the tunnels  for alternative energy generation, secure storage, and mushroom farming. Nobody has accessed the tunnels since the government closed them off in the mid-90s...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Andrew Grant
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2011/nov/10-selling-cheap-abandoned-half-finished-collider/key_image</url>
        </image>

        <rights></rights>        
        <pubDate>Fri, 02 Dec 2011 12:50:00 -0500</pubDate>
        <lastBuildDate>Fri, 02 Dec 2011 12:50:00 -0500</lastBuildDate>
        <type>Print Article</type>    
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      <item>
        <title>20 Things You Didn't Know About... The Periodic Table</title>
        <link>http://discovermagazine.com/2011/nov/20-things-you-didnt-know-about-periodic-table</link>
        <guid>http://discovermagazine.com/2011/nov/20-things-you-didnt-know-about-periodic-table</guid>
        <description>&lt;img src="http://discovermagazine.com/2011/nov/20-things-you-didnt-know-about-periodic-table/periodic-table.jpg" align="right" alt="periodic table"&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;1 &amp;nbsp; &lt;/b&gt;You may remember the Periodic Table of the Elements as a dreary chart on your classroom wall. If so, you never guessed its real purpose: It’s a giant cheat sheet.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;4 &amp;nbsp; &lt;/b&gt;To determine atomic weights, scientists had passed currents through various solutions to break them up into their constituent atoms. Responding to a battery’s polarity, the atoms of one element would go thisaway, the atoms of another thataway. The atoms were collected in separate containers and then weighed.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;6 &amp;nbsp; &lt;/b&gt;Fond of card games, Mendeleyev wrote the weight for each element on a separate index card and sorted them as in solitaire. Elements with similar properties formed a “suit” that he placed in columns ordered by ascending atomic weight. &lt;/p&gt;
&lt;p&gt; &lt;b&gt;9 &amp;nbsp; &lt;/b&gt;Ehen argon was discovered in 1894, it didn’t fit into any of Mendeleyev’s columns, so he denied its existence—as he did for helium, neon, krypton, xenon, and radon...&lt;/p&gt;
&lt;p&gt;&lt;i&gt;Image: Lawrence Berkeley National Lab&lt;/i&gt;&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Rebecca Coffey
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2011/nov/20-things-you-didnt-know-about-periodic-table/key_image</url>
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        <rights></rights>        
        <pubDate>Wed, 30 Nov 2011 12:40:00 -0500</pubDate>
        <lastBuildDate>Wed, 30 Nov 2011 12:40:00 -0500</lastBuildDate>
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        <title>Out There: Are There Mysterious Forces Lurking in Our Atoms and Galaxies?</title>
        <link>http://discovermagazine.com/2011/nov/12-out-there-mysterious-fifth-force-atoms-galaxies</link>
        <guid>http://discovermagazine.com/2011/nov/12-out-there-mysterious-fifth-force-atoms-galaxies</guid>
        <description>&lt;img src="http://discovermagazine.com/2011/nov/12-out-there-mysterious-fifth-force-atoms-galaxies/web.jpg" align="right" alt=""&gt;Caption: Far more delicate than the tug on a spider's web: If a fifth force is out there, its impact on our world must be nearly imperceptible. &lt;br&gt;&lt;br&gt;iStockphoto&lt;/p&gt;
&lt;p&gt; At the turn of the 20th century, finding a new form of radiation could put a physicist’s career on the fast track. Wilhelm Röntgen changed the world by discovering X-rays in 1895. Soon thereafter, Ernest Rutherford and Paul Villard identified three different kinds of radiation, dubbed alpha, beta, and gamma rays, emitted by radioactive compounds. In 1903 French scientist René Blondlot added to the frenzy with his announcement of N-rays, a strangely democratic form of radiation emitted by wood, iron, living organisms—just about anything at all.&lt;/p&gt;
&lt;p&gt;Some 300 scientific papers were written about N-rays. There was just one problem: They weren’t real. A skeptical physicist named Robert Wood visited Blondlot’s lab and secretly removed a key part of his apparatus; this had no effect on Blondlot’s perception of N-rays, showing that they were purely a product of the imagination.&lt;/p&gt;
&lt;p&gt;Blondlot’s reversal of fortune served as a reminder that the world isn’t really full of countless kinds of radiation waiting patiently to be discovered. Nature is more parsimonious than that. Even as forms of radiation seemed to proliferate, theory was driving physics the other way, toward consolidation. X-rays and gamma rays were soon recognized as different forms of electromagnetic radiation, like radio waves and visible light but more energetic. Beta rays are simply fast-moving electrons, and alpha rays are fast-moving helium nuclei. Beneath the dazzling array of new phenomena lurked just a few simple ingredients...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Sean Carroll
          
        </creator> 

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            <url>http://discovermagazine.com/2011/nov/12-out-there-mysterious-fifth-force-atoms-galaxies/key_image</url>
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        <rights></rights>        
        <pubDate>Fri, 04 Nov 2011 14:40:00 -0400</pubDate>
        <lastBuildDate>Fri, 04 Nov 2011 14:40:00 -0400</lastBuildDate>
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        <title>Out There: Welcome to the Multiverse</title>
        <link>http://discovermagazine.com/2011/oct/18-out-there-welcome-to-the-multiverse</link>
        <guid>http://discovermagazine.com/2011/oct/18-out-there-welcome-to-the-multiverse</guid>
        <description>&lt;img src="http://discovermagazine.com/2011/oct/18-out-there-welcome-to-the-multiverse/wizardnebula.jpg" align="right" alt="wizard nebula"&gt;
&lt;p&gt;Theoretical cosmologist isn’t one of the more hazardous occupations of the modern world. The big risks include jet lag, caffeine overdose, and possibly carpal tunnel syndrome. It wasn’t always so. On February 17, 1600, Giordano Bruno, a mathematician and Dominican friar, was stripped naked and driven through the streets of Rome. Then he was tied to a stake in the Campo de’ Fiori and burned to death. The records of Bruno’s long prosecution by the Inquisition have been lost, but one of his major heresies was cosmological. He advocated that other stars were like our sun, and that they could each support planets teeming with life. Orthodox thought of the time preferred to think that Earth and humanity were unique.&lt;/p&gt;
&lt;p&gt;These days, cosmologists like me may be safer, but our ideas have grown only more radical. One of the most controversial but widely discussed concepts in the field resembles a hugely amplified version of Bruno’s cosmology: the idea that the thing we call “the universe” is just one of an infinite number of regions in a much larger universe of universes, or multiverse. A big focus of my own research asks whether a multiverse can help explain the arrow of time...&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Sean Carroll
          
        </creator> 

        <image>
            <url>http://discovermagazine.com/2011/oct/18-out-there-welcome-to-the-multiverse/key_image</url>
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        <rights></rights>        
        <pubDate>Tue, 18 Oct 2011 12:35:00 -0400</pubDate>
        <lastBuildDate>Tue, 18 Oct 2011 12:35:00 -0400</lastBuildDate>
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        <title>Twisting Radio Waves Could Give Us 100x More Wireless Bandwidth</title>
        <link>http://discovermagazine.com/2011/oct/13-twisting-radio-waves-100x-more-wireless-bandwidth</link>
        <guid>http://discovermagazine.com/2011/oct/13-twisting-radio-waves-100x-more-wireless-bandwidth</guid>
        <description>&lt;img src="http://discovermagazine.com/2011/oct/13-twisting-radio-waves-100x-more-wireless-bandwidth/wires.jpg" align="right" alt=""&gt;
&lt;p&gt;As more people stream video to their mobile devices, wireless bandwidth is becoming an increasingly precious commodity. Data traffic increased 8,000 percent in the past four years on AT&amp;amp;T’s network alone. In trying to avoid what the Federal Communications Commission calls a “looming spectrum crisis,” telecommunications companies are lobbying the government to assign them more spectrum space in the 300- to 3,000-megahertz range, the sweet spot for wireless communication. But Italian astrophysicist Fabrizio Tamburini says a solution may lie in making better use of the frequencies already in use. In a recent paper, he demonstrated a potential way to squeeze 100 times more bandwidth out of existing frequencies.&lt;/p&gt;
&lt;p&gt;The idea is to twist radio waves like corkscrews and create multiple subfrequencies, distinguished by their degree of twistedness. Each subchannel carries discrete data sets. “You can tune the wave with a given frequency as you normally do, but there is also a fingerprint left by the twist,” Tamburini says...&lt;/p&gt;
&lt;p&gt;&lt;i&gt;Image: Warped radio waves may satisfy the ballooning demand for spectrum space. Source: iStockphoto&lt;i&gt;&lt;/p&gt;</description>
        <publisher></publisher>        
        <creator>
          
            Edwin Cartlidge
          
        </creator> 

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            <url>http://discovermagazine.com/2011/oct/13-twisting-radio-waves-100x-more-wireless-bandwidth/key_image</url>
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        <rights></rights>        
        <pubDate>Mon, 10 Oct 2011 14:25:00 -0400</pubDate>
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