kottke.org posts about physics
Normally when someone says they’ve thought up a theoretically possible perpetual motion scheme, you roll your eyes and pass the dutchie to the left hand side. But when that someone is a Nobel laureate in physics, is not generally off his rocker, and has published his idea in a prestigious peer-reviewed journal, people pay attention. Frank Wilczek believes he’s invented something called time crystals.
In February 2012, the Nobel Prize-winning physicist Frank Wilczek decided to go public with a strange and, he worried, somewhat embarrassing idea. Impossible as it seemed, Wilczek had developed an apparent proof of “time crystals” — physical structures that move in a repeating pattern, like minute hands rounding clocks, without expending energy or ever winding down. Unlike clocks or any other known objects, time crystals derive their movement not from stored energy but from a break in the symmetry of time, enabling a special form of perpetual motion.
“Most research in physics is continuations of things that have gone before,” said Wilczek, a professor at the Massachusetts Institute of Technology. This, he said, was “kind of outside the box.”
An effort to prove or disprove Wilczek’s theory is underway…let’s hope it holds up to scientific scrutiny better than Time Cube. (via digg)
This video footage of metallic putty eating magnets is super freaky.
From Phil Plait at Bad Astronomy, a list of ten things you might not know about black holes. Some of this I knew, but this one is incredible:
If you were to rope off the solar system out past Neptune, enclose it in a giant sphere, and fill it with air, it would be a black hole!
See also this recent tweet from physicist Brian Greene:
Remove all the space within the atoms making up the human body, and every person that’s ever lived would fit inside a baseball.
(via @daveg & @rosecrans)
The other day I posted a video about how differential gears work to help cars go smoothly around curves. Trains don’t have differential gears, so how do they manage to go around curves without slipping or skidding? Richard Feynman explains:
Ha, it looks like I’ve posted this one before as well. Can never get enough Feynman. (thx, kerry)
Well, this is interesting. Graphene is a substance discovered relatively recently that has a number of unusual properties. In 2004, physicists at the University of Manchester and the Institute for Microelectronics Technology in Russia used ordinary scotch tape to isolate single-layer sheets of graphene. Once isolated, the sheets could be tested for the unusual properties I mentioned. The 2010 Nobel Prize in Physics was awarded for this work.
In 2012, a group of researchers at UCLA discovered they could make single-layer sheets of graphene by coating a DVD with graphite oxide and then “playing” the disc in a plain old DVD drive. And then in a happy accident, they found that graphene has unusually high supercapacitance properties, which could mean that graphene could be used, for example, as a mobile phone battery that lasts all day, charges in a few seconds, and can be thrown into a compost bin after use.
(via io9)
Paul Frampton is a 69-year-old theoretical particle physicist who has co-authored papers with Nobel laureates. In late 2011, the absentminded professor met a Czech bikini model online. Over email and Yahoo chat, they became romantically involved and she sent him a plane ticket to come meet her at a photo shoot in Bolivia. Then she asked him to bring a bag of hers with him on his flight.
While in Bolivia, Frampton corresponded with an old friend, John Dixon, a physicist and lawyer who lives in Ontario. When Frampton explained what he was up to, Dixon became alarmed. His warnings to Frampton were unequivocal, Dixon told me not long ago, still clearly upset: “I said: ‘Well, inside that suitcase sewn into the lining will be cocaine. You’re in big trouble.’ Paul said, ‘I’ll be careful, I’ll make sure there isn’t cocaine in there and if there is, I’ll ask them to remove it.’ I thought they were probably going to kidnap him and torture him to get his money. I didn’t know he didn’t have money. I said, ‘Well, you’re going to be killed, Paul, so whom should I contact when you disappear?’ And he said, ‘You can contact my brother and my former wife.’ ” Frampton later told me that he shrugged off Dixon’s warnings about drugs as melodramatic, adding that he rarely pays attention to the opinions of others.
On the evening of Jan. 20, nine days after he arrived in Bolivia, a man Frampton describes as Hispanic but whom he didn’t get a good look at handed him a bag out on the dark street in front of his hotel. Frampton was expecting to be given an Hermès or a Louis Vuitton, but the bag was an utterly commonplace black cloth suitcase with wheels. Once he was back in his room, he opened it. It was empty. He wrote to Milani, asking why this particular suitcase was so important. She told him it had “sentimental value.” The next morning, he filled it with his dirty laundry and headed to the airport.
Crazy story. (via @stevenstrogatz)
Another fine installment of XKCD’s What If? series: What would happen if you tried to fly a normal Earth airplane above different Solar System bodies?
Unfortunately, [the X-Plane simulator] is not capable of simulating the hellish environment near the surface of Venus. But physics calculations give us an idea of what flight there would be like. The upshot is: Your plane would fly pretty well, except it would be on fire the whole time, and then it would stop flying, and then stop being a plane.
(via stellar)
The timeline of the far future artice is far from the longest page on Wikipedia, but it might take you several hours to get through because it contains so many enticing detours. What’s Pangaea Ultima? Oooh, Roche limit! The Degenerate Era, Poincaré recurrence time, the Big Rip scenario, the cosmic light horizon, the list goes on and on. And the article itself is a trove of fascinating facts and eye-popping phrases. Here are a few of my favorites. (Keep in mind that the universe is only 13.75 billion years old. Unless we’re living in a computer simulation.)
50,000 years: “Niagara Falls erodes away the remaining 32 km to Lake Erie and ceases to exist.”
1 million years: “Highest estimated time until the red supergiant star Betelgeuse explodes in a supernova. The explosion is expected to be easily visible in daylight.”
1.4 million years: “The star Gliese 710 passes as close as 1.1 light years to the Sun before moving away. This may gravitationally perturb members of the Oort cloud; a halo of icy bodies orbiting at the edge of the Solar System. As a consequence, the likelihood of a cometary impact in the inner Solar System will increase.”
230 million years: “Beyond this time, the orbits of the planets become impossible to predict.”
800 million years: “Carbon dioxide levels fall to the point at which C4 photosynthesis is no longer possible. Multicellular life dies out.”
4 billion years: “Median point by which the Andromeda Galaxy will have collided with the Milky Way, which will thereafter merge to form a galaxy dubbed ‘Milkomeda’.”
7.9 billion years: “The Sun reaches the tip of the red giant branch, achieving its maximum radius of 256 times the present day value. In the process, Mercury, Venus and possibly Earth are destroyed. During these times, it is possible that Saturn’s moon Titan could achieve surface temperatures necessary to support life.”
100 billion years: “The Universe’s expansion causes all galaxies beyond the Milky Way’s Local Group to disappear beyond the cosmic light horizon, removing them from the observable universe.”
1 trillion years: “The universe’s expansion, assuming a constant dark energy density, multiplies the wavelength of the cosmic microwave background by 10^29, exceeding the scale of the cosmic light horizon and rendering its evidence of the Big Bang undetectable.”
1 quadrillion years: “Estimated time until stellar close encounters detach all planets in the Solar System from their orbits. By this point, the Sun will have cooled to five degrees above absolute zero.”
10^65 years: “Assuming that protons do not decay, estimated time for rigid objects like rocks to rearrange their atoms and molecules via quantum tunneling. On this timescale all matter is liquid.”
10^10^56 years: “Estimated time for random quantum fluctuations to generate a new Big Bang, according to Caroll and Chen.”
Read the whole thing, it’s worth the effort. (via @daveg)
Note: Illustration by Chris Piascik…prints & more are available.
In 2003, British philosopher Nick Bostrom suggested that we might live in a computer simulation. From the abstract of Bostrom’s paper:
This paper argues that at least one of the following propositions is true: (1) the human species is very likely to go extinct before reaching a “posthuman” stage; (2) any posthuman civilization is extremely unlikely to run a significant number of simulations of their evolutionary history (or variations thereof); (3) we are almost certainly living in a computer simulation. It follows that the belief that there is a significant chance that we will one day become posthumans who run ancestor-simulations is false, unless we are currently living in a simulation. A number of other consequences of this result are also discussed.
The gist appears to be that if The Matrix is possible, someone has probably already invented it and we’re in it. Which, you know, whoa.
But researchers believe they have devised a test to check if we’re living in a computer simulation.
However, Savage said, there are signatures of resource constraints in present-day simulations that are likely to exist as well in simulations in the distant future, including the imprint of an underlying lattice if one is used to model the space-time continuum.
The supercomputers performing lattice quantum chromodynamics calculations essentially divide space-time into a four-dimensional grid. That allows researchers to examine what is called the strong force, one of the four fundamental forces of nature and the one that binds subatomic particles called quarks and gluons together into neutrons and protons at the core of atoms.
“If you make the simulations big enough, something like our universe should emerge,” Savage said. Then it would be a matter of looking for a “signature” in our universe that has an analog in the current small-scale simulations.
If it turns out we’re all really living in an episode of St. Elsewhere, I’m going to be really bummed. (via @CharlesCMann)
Aired as The Quest For Tannu Tuva in the UK and The Last Journey Of A Genius in the US, this hour-long program is the last extended interview that physicist Richard Feynman gave; he died a few days after the recording.
Richard Feynman was not only an iconoclastic and influential theoretical physicist and Nobel laureate but also an explorer at heart. Feynman through video recordings and comments from his friend and drumming partner Ralph Leighton tell the extraordinary story of their enchantment with Tuva, a strange and distant land in the centre of Asia.
While few Westerners knew about Tuva, Feynman discovered its existence from the unique postage stamps issued there in the early 20th century. He was intrigued by the unusual name of its capital, Kyzyl, and resolved to travel to the remote, mountainous land. However, the Soviets, who controlled access, were mistrustful, unconvinced that he was interested only in the scenery. They obstructed his plans throughout 13 years.
I could watch this guy talk all day long. Feynman is a national treasure; we should give Andrew Jackson the boot and put Feynman on the $20.
A European team of exoplanet hunters has discovered a planet about the size of Earth orbiting Alpha Centauri B, which is in a group of stars closest to the solar system, a mere 4.3 light years away. Lee Billings explains the significance.
At a distance of just over 4.3 light years, the stars of Alpha Centauri are only a cosmic stone’s throw away. To reach Alpha Centauri B b, as this new world is called, would require a journey of some 25 trillion miles. For comparison, the next-nearest known exoplanet is a gas giant orbiting the orange star Epsilon Eridani, more than twice as far away. But don’t pack your bags quite yet. With a probable surface temperature well above a thousand degrees Fahrenheit, Alpha Centauri B b is no Goldilocks world. Still, its presence is promising: Planets tend to come in packs, and some theorists had believed no planets at all could form in multi-star systems like Alpha Centauri, which are more common than singleton suns throughout our galaxy. It seems increasingly likely that small planets exist around most if not all stars, near and far alike, and that Alpha Centauri B may possess additional worlds further out in clement, habitable orbits, tantalizingly within reach.
Hey, if Randall keeps writing them, I’m gonna keep posting links to them…today’s XKCD What If is “If every person on Earth aimed a laser pointer at the Moon at the same time, would it change color?”
Unfortunately, the laser energy flow would turn the atmosphere to plasma, instantly igniting the Earth’s surface and killing us all.
Gorilla Glass is the thin strong glass used for the screens of most smartphones. It was invented in the 1960s by Corning but was shelved in the early 1970s due to a lack of demand. The iPhone brought it out of retirement in a big way.
Chemical strengthening, the method of fortifying glass developed in the ’60s, creates a compressive layer too, through something called ion exchange. Aluminosilicate compositions like Gorilla Glass contain silicon dioxide, aluminum, magnesium, and sodium. When the glass is dipped in a hot bath of molten potassium salt, it heats up and expands. Both sodium and potassium are in the same column on the periodic table of elements, which means they behave similarly. The heat from the bath increases the migration of the sodium ions out of the glass, and the similar potassium ions easily float in and take their place. But because potassium ions are larger than sodium, they get packed into the space more tightly. (Imagine taking a garage full of Fiat 500s and replacing most of them with Chevy Suburbans.) As the glass cools, they get squeezed together in this now-cramped space, and a layer of compressive stress on the surface of the glass is formed. (Corning ensures an even ion exchange by regulating factors like heat and time.) Compared with thermally strengthened glass, the “stuffing” or “crowding” effect in chemically strengthened glass results in higher surface compression (making it up to four times as strong), and it can be done to glass of any thickness or shape.
I did glass research in college so I’m a sucker for this sort of thing. (via @joeljohnson)
XKCD’s What If? science feature continues to delight. This week’s question is “What if a rainstorm dropped all of its water in a single giant drop?”
The drop is now falling at 90 meters per second (200 mph). The roaring wind whips up the surface of the water into spray. The leading edge of the droplet turns to foam as air is forced into the liquid. If it kept falling for long enough, these forces would gradually disperse the entire droplet into rain.
Before that can happen, about 20 seconds after formation, the edge of the droplet hits the ground. The water is now moving at over 200 m/s (450 mph). Right under the point of impact, the air is unable to rush out of the way fast enough, and the compression heats it so quickly that the grass would catch fire if it had time.
Fortunately for the grass, this heat lasts only a few milliseconds because it’s doused by the arrival of a lot of cold water. Unfortunately for the grass, the cold water is moving at over half the speed of sound.
It turns out that yo-yos work pretty well in space. Astronaut Don Pettit demontrates from the International Space Station.
(via explore)
Researchers in Germany have found evidence of room temperature superconductivity in graphite powder that has been soaking in water and then dried. Not surprisingly, the results come with a few caveats:
First, this is not a conventional bulk material. The claim from Germany is that the superconductivity occurs at the interface between grains of graphite after they have dried out.
So that’s a surface effect which involves only a tiny fraction of the total mass of carbon in the powder—just 0.0001 per cent of the mass, according to Esquinazi and co.
What’s more the effect is clearly fragile. Esquinazi and co say the superconductivity disappears if the treated powder is pressed into pellets.
So whatever allows the superconductivity to occur at the grain interfaces is destroyed when the grains are pressed together.
I’m pretty sure this is the technology used by the aliens who designed The Machine in Contact.
Opening on September 15 at Edward Tufte’s gallery in Chelsea is All Possible Photons, an exhibit of sculptures by Tufte of Richard Feynman’s subatomic particle diagrams.
Made from stainless steel and air, the artworks grow out of Richard Feynman’s famous diagrams describing Nature’s subatomic behavior. Feynman diagrams depict the space-time patterns of particles and waves of quantum electrodynamics. These mathematically derived and empirically verified visualizations represent the space-time paths taken by all subatomic particles in the universe.
The resulting conceptual and cognitive art is both beautiful and true. Along with their art, the stainless steel elements of All Possible Photons actually represent something: the precise activities of Nature at her highest resolution.
In this slow-motion video, you can see how cats rotate themselves in the air while conserving angular momentum.
This is an interesting companion to yesterday’s owl rotation video. (via @stevenstrogatz)
Ignoring the prequels (of course), how much power does Yoda put out when he’s using the Force? It’s perhaps less than you’d realize.
Yoda’s greatest display of raw power in the original trilogy came when he lifted Luke’s X-Wing from the swamp. As far as physically moving objects around goes, this was easily the biggest expenditure of energy through the Force we saw from anyone in the trilogy.
The energy it takes to lift an object to height h is equal to the object’s mass times the force of gravity times the height it’s lifted. The X-Wing scene lets us use this to put a lower limit on Yoda’s peak power output.
First we need to know how heavy the ship was. The X-Wing’s mass has never been canonically established, but its length has-16 meters. An F-22 is 19 meters long and weighs 19,700 lbs, so scaling down from this gives an estimate for the X-Wing of about 12,000 lbs (5 metric tons).
XKCD is answering “hypothetical questions with physics” once a week and the first installment is just flat-out delightful: What would happen if you tried to hit a baseball pitched at 90% the speed of light?
The ideas of aerodynamics don’t apply here. Normally, air would flow around anything moving through it. But the air molecules in front of this ball don’t have time to be jostled out of the way. The ball smacks into them hard that the atoms in the air molecules actually fuse with the atoms in the ball’s surface. Each collision releases a burst of gamma rays and scattered particles.
These gamma rays and debris expand outward in a bubble centered on the pitcher’s mound. They start to tear apart the molecules in the air, ripping the electrons from the nuclei and turning the air in the stadium into an expanding bubble of incandescent plasma. The wall of this bubble approaches the batter at about the speed of light-only slightly ahead of the ball itself.
All science writing should (and probably could!) be this entertaining. (via @delfuego)
Motherboard journeyed out onto the streets of Williamsburg to see if the hipster on the street knew what the Higgs boson was. And he/she did not.
If you’re in that same boat, take a few minutes to learn about what the Higgs is. (via @alexismadrigal)
Or, to put it in the cautious words of science, researchers have observed a “particle consistent with long-sought Higgs boson”.
“We observe in our data clear signs of a new particle, at the level of 5 sigma, in the mass region around 126 GeV. The outstanding performance of the LHC and ATLAS and the huge efforts of many people have brought us to this exciting stage,” said ATLAS experiment spokesperson Fabiola Gianotti, “but a little more time is needed to prepare these results for publication.”
“The results are preliminary but the 5 sigma signal at around 125 GeV we’re seeing is dramatic. This is indeed a new particle. We know it must be a boson and it’s the heaviest boson ever found,” said CMS experiment spokesperson Joe Incandela. “The implications are very significant and it is precisely for this reason that we must be extremely diligent in all of our studies and cross-checks.”
How sure are they that they’ve found the Higgs? Brian Cox notes on Twitter:
5 sigma is the usual particle physics threshold for discovery. It roughly means that you’re 99.9999% sure
In this series of slow motion clips, you can see that if you hold a Slinky by one end and drop it, the bottom end doesn’t actually move until the top end catches up with it.
I’ve watched this like six times and it drops my jaw every time…the bottom of the Slinky JUST. DOES. NOT. MOVE. Here’s the scientific explanation:
The explanation that “it takes time for the bottom of the slinky to feel the change” might work ok, but it isn’t the best.
Then why doesn’t the bottom of the slinky fall as the top is let go? I think the best thing is to think of the slinky as a system. When it is let get, the center of mass certainly accelerates downward (like any falling object). However, at the same time, the slinky (spring) is compressing to its relaxed length. This means that top and bottom are accelerating towards the center of mass of the slinky at the same time the center of mass is accelerating downward.
(via @stevenstrogatz)
Update: See also The Physics of a Falling Slinky. (via @jeffhellman)
From The Royal Observatory, Greenwich, a short video explanation of how scientists measure the size of the Universe.
This is science for the layperson done right…PBS or the Discovery Channel would have inflated this into a 30-minute show. (via ★interesting)
The Tacoma Narrows Bridge was open for about four months in 1940 before a steady wind set it twisting and ultimately tore the bridge apart.
Damn Interesting has a detailed account of the bridge’s short history and demise.
After opening, the new bridge shortly came to be known as “Galloping Gertie,” so named by white-knuckled motorists who braved the writhing bridge on windy days. Even in a light breeze, Gertie’s undulations were known to produce waves up to ten feet tall. Sometimes these occurrences were brief, and other times they lasted for hours at a time. Numerous travelers shunned the route altogether to avoid becoming seasick, whereas many thrill-seeking souls paid the 75-cent toll to traverse Gertie during her more spirited episodes.
The 99% Invisible podcast devoted a show to the collapse of the bridge.
(via sarah pavis)
I missed this last July when the news came out, but since I’ve been following the Pioneer Anomaly for the past eight years, I wanted to mention it here for closure purposes. First, what the hell is the Pioneer Anomaly?
The Pioneer anomaly or Pioneer effect is the observed deviation from predicted accelerations of the Pioneer 10 and Pioneer 11 spacecraft after they passed about 20 astronomical units (3×10^9 km; 2×10^9 mi) on their trajectories out of the Solar System. Both Pioneer spacecraft are escaping the Solar System, but are slowing under the influence of the Sun’s gravity. Upon very close examination of navigational data, the spacecraft were found to be slowing slightly more than expected. The effect is an extremely small but unexplained acceleration towards the Sun, of 8.74±1.33x10^-10 m/s^2.
A team at JPL has tracked the problem to uneven heat emissions from the probes’ fuel source.
For their new analysis, Turyshev et. al. compiled a lot more data than had ever been analyzed before, spanning a much longer period of the Pioneers’ flight times. They studied 23 years of data from Pioneer 10 instead of just 11, and 11 years of data from Pioneer 11 instead of 3. As explained in their new paper, the more complete data sets reveal that the spacecraft’s anomalous acceleration did indeed seem to decrease with time. In short, the undying force had been dying after all, just like the decaying plutonium.
A more recent paper by the same researchers offers even more support for their theory. Case closed, I say.
Aisha Mustafa, a 19-year-old Egyptian physics student, has invented a promising new quantum propulsion system for spacecraft.
Mustafa invented a way of tapping this quantum effect via what’s known as the dynamic Casimir effect. This uses a “moving mirror” cavity, where two very reflective very flat plates are held close together, and then moved slightly to interact with the quantum particle sea. It’s horribly technical, but the end result is that Mustafa’s use of shaped silicon plates similar to those used in solar power cells results in a net force being delivered. A force, of course, means a push or a pull and in space this equates to a drive or engine.
Soon after the US dropped two nuclear bomb on Japan in 1945, a group of physicists at the University of Pennsylvania decided to investigate for themselves how nuclear fission and the bomb might work using non-classified materials. In doing so, they ventured into classified territory and raised questions about the nature of science and secrecy.
To what degree would nuclear research become shackled by the requirements of national security? Would the open circulation of new scientific knowledge cease if that knowledge was relevant to nuclear fission? Those questions were hardly idle speculation: From the fall of 1945 through the summer of 1946, the US Congress was crafting new, unprecedented legislation that would legally define the bounds of open scientific research and even free speech. The idea of restricting open scientific communication “may seem drastic and far-reaching,” President Harry S. Truman argued in an October 1945 statement exhorting Congress to rapid action. But, he said, the atomic bomb “involves forces of nature too dangerous to fit into any of our usual concepts.”
The former Manhattan Project scientists who founded what would eventually become the Federation of American Scientists were adamantly opposed to keeping nuclear technology a closed field. From early on they argued that there was, as they put it, “no secret to be kept.” Attempting to control the spread of nuclear weapons by controlling scientific information would be fruitless: Soviet scientists were just as capable as US scientists when it came to discovering the truths of the physical world. The best that secrecy could hope to do would be to slightly impede the work of another nuclear power. Whatever time was bought by such impediment, they argued, would come at a steep price in US scientific productivity, because science required open lines of communication to flourish.
At the University of Pennsylvania were nine scientists sympathetic to that message. All had been involved with wartime work, but in the area of radar, not the bomb. Because they had not been part of the Manhattan Project in any way, they were under no legal obligation to maintain secrecy; they were simply informed private citizens. In the fall of 1945, they tried to figure out the technical details behind the bomb.
Dr. Sergio Cittolin has worked at CERN for the past 30 years as a research physicist. He has also made several drawings of the Large Hadron Collider in the style of Leonardo da Vinci.
Symmetry magazine profiled Cittolin a few years ago.
As a naturalist, da Vinci probed, prodded, and tested his way to a deeper understanding of how organisms work and why, often dissecting his object of study with this aim. “I thought, why not present the idea of data analysis to the world within the naturalist world of Leonardo?” Cittolin says. In the drawing below, the CMS detector is the organism to be opened; the particles passing through it and the tracks they leave behind are organs exposed for further investigation.
Cittolin brings a sense of humor to his work. For example, after betting CMS colleague Ariella Cattai that he could produce a quality drawing for the cover of the CMS tracker technical proposal by a given deadline, he included in the drawing a secret message in mirror-image writing-which was also a favorite of da Vinci’s. The message jokingly demanded a particular reward for his hard work. The completed picture was delivered on time and within a few hours Cattai cleverly spotted and deciphered the message. She promptly presented him with the requested bottle of wine.
(via ★johnpavlus)
Up until 2007, Kodak operated a small nuclear reactor that contained 3.5 pounds of weapons-grade highly enriched uranium.
The Democrat and Chronicle learned of the facility when an employee happened to mention it to a reporter a few months ago.
The recent silence was by design. Detailed information about nuclear power plants and other entities with radioactive material has been restricted since the 2001 terrorist attacks.
Nuclear non-proliferation experts express surprise that an industrial manufacturer like Eastman Kodak had had weapons-grade uranium, especially in a post-9/11 world.
“I’ve never heard of it at Kodak,” said Miles Pomper, senior research associate at the Center for Nonproliferation Studies in Washington. “It’s such an odd situation because private companies just don’t have this material.”
(via @kdawson)
Newer posts
Older posts
Socials & More