Posts Tagged ‘gravity’
“The bigger, the better”*…
Thea Applebaum Licht with a reminder that, when it comes to size, Texas has got nothing on California…
Between about 1905 and 1915, the United States entered a golden age of postcards. Cheaper and faster mail service, the advent of “divided back” cards (freeing the entire front for images), and improved commercial printing all drove a new mass market for collectible communication. It was at this same moment that a craze for “tall-tale” or “exaggeration” postcards reached its peak. By cutting, collaging, and re-photographing images, artists created out-of-proportion illusions. One of the most popular genres was agricultural goods of fantastic dimensions.
Nowhere were such postcards more popular than in the western states. There, in the heart of the tough business of agriculture, illustrations of folkloric American abundance were understandable favorites. Pride and place were tied up with the prodigious crops. Supersized fruits and vegetables were often accompanied by brief captions: “How We Do Things at Attica, Wis.”, “The Kind We Raise in Our State”, or “The Kind We Grow in Texas”. Photographers like William “Dad” H. Martin and Alfred Stanley Johnson Jr. captured farmers harvesting furniture-sized onions and stacking corn cobs like timber, fisherman reeling in leviathans, and children sharing canoe-like slices of watermelon.
In the series of exaggeration postcards [produced in the run-up to the postcard boom, then published during it] collected [here], it is California that takes center stage. Produced by the prolific San Francisco–based publisher Edward H. Mitchell, each card features a single rail car rolling through lush farmland. Aboard are gargantuan, luminous fruits and vegetables: dimpled navel oranges, a dusky bunch of grapes, and mottled walnuts. Placed end-to-end, the cards would make a colorful train crossing California’s fertile valleys. Unlike other, more action-packed “tall-tale” cards — filled with farmers, fisherman, and children for scale — Mitchell’s series is restrained. Sharply illuminated, the colossal cargo lean toward artwork rather than gag. “A Carload of Mammoth Apples”[here], green-yellow and gleaming, could have been plucked from Rene Magritte’s The Son of Man [here].
Fabulous fruit and vegetables: “Calicornication: Postcards of Giant Produce (1909),” from @publicdomainrev.bsky.social.
In other art-related news: (very) long-term readers might recall that, back in 2008, (R)D reported that London’s Daily Mail believed that it had tracked him down, and that he is Robin Gunningham. Now as Boing Boing reports:
Anyone reading Banksy’s Wikipedia article at any point since a famous Mail on Sunday exposé in 2008 would likely get the impression the secretive stenciler is probably Robin Gunningham or Robert Del Naja, artists who came from the Bristol Underground. Reuters, having conducted extensive research into their movements, finds both men present at critical moments, but only one at all of them: an arrest report from New York City puts Gunningham firmly in the frame, and recent public records from Ukraine put it beyond doubt.
We later unearthed previously undisclosed U.S. court records and police reports. These included a hand-written confession by the artist to a long-ago misdemeanor charge of disorderly conduct – a document that revealed, beyond dispute, Banksy’s true identity. … Reuters presented that man with its findings about his identity and detailed questions about his work and career. He didn’t reply. Banksy’s company, Pest Control, said the artist “has decided to say nothing.”
His long-time lawyer, Mark Stephens, wrote to Reuters that Banksy “does not accept that many of the details contained within your enquiry are correct.” He didn’t elaborate. Without confirming or denying Banksy’s identity, Stephens urged us not to publish this report, saying doing so would violate the artist’s privacy, interfere with his art and put him in danger.
Del Naja (better known for other work) evidently participates in painting the murals and is perhaps the stencil draftsman (Banksy: “he can actually draw”). Banksy’s former manager, Steve Lazarides, organized a legal name change for Gunningham after the Mail on Sunday item, which successfully ended records for Banksy’s movements under his birth name and stymied researchers—until Reuters figured out the new one by poring through Ukrainian public records on days Del Naja was there. Gunningham used the name David Jones, among the most common in the U.K. If it rings a bell, you might be thinking of another famous British artist was who obliged by his record company to find something more unique.
* common idiom
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As we live large, we might spare a thought for Isaac Newton; he died on this date (O.S.) in 1727. A polymath who was a key figure in the Scientific Revolution and the Enlightenment that followed, Newton was a mathematician, physicist, astronomer, alchemist, theologian, author, and inventor. He contributed to and refined the scientific method, and his work is considered the most influential in bringing forth modern science. His book Philosophiæ Naturalis Principia Mathematica (Mathematical Principles of Natural Philosophy), first published in 1687, achieved the first great unification in physics and established classical mechanics. He also made seminal contributions to optics, and shares credit with the German mathematician Gottfried Wilhelm Leibniz for formulating infinitesimal calculus. (Newton developed calculus a couple of years before Leibniz, but published a couple of years after.) Newton spent the last three decades of his life in London, serving as Warden (1696–1699) and Master (1699–1727) of the Royal Mint, a role in which he increased the trustworthiness/accuracy and security of British coinage in a way crucial to the rise of Great Britain as a commercial and colonial power.
Newton, of course, had a famous relationship with fruit:
Newton often told the story that he was inspired to formulate his theory of gravitation by watching the fall of an apple from a tree. The story is believed to have passed into popular knowledge after being related by Catherine Barton, Newton’s niece, to Voltaire. Voltaire then wrote in his Essay on Epic Poetry (1727), “Sir Isaac Newton walking in his gardens, had the first thought of his system of gravitation, upon seeing an apple falling from a tree.” – source
Newton’s apple is thought to have been the green skinned ‘Flower of Kent’ variety.

“Gravity. It’s not just a good idea; it’s the law!”*…
… But what is gravity? George Musser unpacks a new argument that explores how the growth of disorder could cause massive objects to move toward one another– one that has left some physicists interested, and some skeptical…
Isaac Newton was never entirely happy with his law of universal gravitation. For decades after publishing it in 1687, he sought to understand how, exactly, two objects were able to pull on each other from afar. He and others came up with several mechanical models, in which gravity was not a pull, but a push. For example, space might be filled with unseen particles that bombard the objects on all sides. The object on the left absorbs the particles coming from the left, the one on the right absorbs those coming from the right, and the net effect is to push them together.
Those theories never quite worked, and Albert Einstein eventually provided a deeper explanation of gravity as a distortion of space and time. But Einstein’s account, called general relativity, created its own puzzles, and he himself recognized that it could not be the final word. So the idea that gravity is a collective effect — not a fundamental force, but the outcome of swarm behavior on a finer scale — still compels physicists.
Earlier this year, a team of theoretical physicists put forward what might be considered a modern version of those 17th-century mechanical models. “There’s some kind of gas or some thermal system out there that we can’t see directly,” said Daniel Carney of Lawrence Berkeley National Laboratory, who led the effort. “But it’s randomly interacting with masses in some way, such that on average you see all the normal gravity things that you know about: The Earth orbits the sun, and so forth.”
This project is one of the many ways that physicists have sought to understand gravity, and perhaps the bendy space-time continuum itself, as emergent from deeper, more microscopic physics. Carney’s line of thinking, known as entropic gravity, pegs that deeper physics as essentially just the physics of heat. It says gravity results from the same random jiggling and mixing up of particles — and the attendant rise of entropy, loosely defined as disorder — that governs steam boilers, car engines and refrigerators.
Attempts at modeling gravity as a consequence of rising entropy have cropped up now and again for several decades. Entropic gravity is very much a minority view. But it’s one that won’t die, and even detractors are loath to dismiss it altogether. The new model has the virtue of being experimentally testable — a rarity when it comes to theories about the mysterious underpinnings of the universal attraction…
[Musser explains the hypothesis, traces is origin, and reviews other scientists’ reactions, and traces possible approaches to testing it…]
… if this long-shot theory does work out, physicists will need to update the artist Gerry Mooney’s famous gravity poster, which reads: “Gravity. It isn’t just a good idea. It’s the law.” Perhaps gravity is not, in fact, a law, just a statistical tendency…
“Is Gravity Just Entropy Rising? Long-Shot Idea Gets Another Look” from @georgemusser.com in @quantamagazine.bsky.social.
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As we fumble with forces, we might send insightful birthday greetings to a man who encourages us to see in different ways, M. C. Escher; he was born on this date in 1898. A graphic artist inspired by mathematics, he created woodcuts, lithographs, and mezzotints, that— while largely ignored by the art world in his lifetime, have become widely celebrated. He’s been recognized as an heir to Parmigianino, Hogarth, and Piranesi.
His work features mathematical objects and operations including impossible objects, explorations of infinity, reflection, symmetry, perspective, truncated and stellated polyhedra, hyperbolic geometry, and tessellations. And though Escher believed he had no mathematical ability, he interacted with the mathematicians George Pólya, Roger Penrose, and Donald Coxeter, and the crystallographer Friedrich Haag, and conducted his own research into tessellation.
For more on (and more examples of) Escher’s work, see here.


“What happens when you get to the end of things?”*…
Charlie Wood introduces a remarkable new collection in Quanta…
A couple of years ago, I was chatting about black holes with Dan Harlow of the Massachusetts Institute of Technology when he made a casual comment that left a deep impression on me. I asked if some new work he’d been doing strengthened the case that space-time was “emergent.” Without missing a beat he replied, “Sure, if it needed strengthening.”
Harlow isn’t the only physicist with serious doubts about what reality is made of. For more than a decade now, Nima Arkani-Hamed of the Institute for Advanced Study has been delivering a polished lecture arguing that space-time is “doomed.” Time and again, I’ve heard theorists in high-energy physics make similar-sounding statements, and I’ve always been struck by their confidence. We don’t have the faintest idea what the next theory of physics will look like, whether it will involve strings, loops, triangles or something entirely new that no one has thought to propose. And yet so many theorists seem rather convinced that whatever it will be, it won’t involve space or time.
Why? What does that statement mean? What would it look like to do physics without referring to space or time? I’ve spent most of this year trying to find out. The results have just been published in “The Unraveling of Space-Time,” a massive package that includes articles, videos and interactive animations from me and my colleagues Mark Belan, Emily Buder, Amanda Gefter and Joseph Howlett.
Over the course of more than 40 interviews with nearly 30 physicists, I learned that there are many ways to define emergent space-time. But at the most basic level, “emergent space-time” means that space and time are the outputs of a theory instead of the inputs. A classic analogy is heat. To explain why a teacup cools, scientists of the 1700s put heat into their theory of the world as a substance that repels itself and naturally spreads out. But this “caloric theory” was ultimately replaced by thermodynamics, a theory where a primary input is molecules that buzz around with some energy. As molecules crash into each other, their energy spreads, and we now recognize this process as the origin of heat transfer. Heat is an output — a prediction — of thermodynamics. It is an emergent phenomenon.
Space-time is the ultimate input. If physics is largely about predicting what happens where and when, you need a stage upon which things can happen. Albert Einstein became a household name for revealing that this stage acts like a fabric that bends in ways we experience as gravity. He described in spectacular detail how space-time behaves, much as 19th-century scientists described how heat behaves with caloric theory. The idea that space-time is emergent is the idea that space-time will eventually go the way of heat, water, air and so many other substances before it; we will someday understand it to be the inevitable consequence of the behavior of simpler entities. Call them the “atoms” of space-time.This week’s series explores the mind-bending notion of emergent space-time from a number of angles. There is, of course, the why of it all. This mostly boils down to the strange things that happen when Einstein’s theory of space-time collides with quantum mechanics, the theory of the subatomic world. When we combine features from both theories, we see that any experiment that tries to probe reality a little too closely will get thwarted by the appearance of a black hole, an enigma that undermines the familiar picture of space-time in its own way.
For this and other reasons, physicists are pushing to escape our familiar space-time, often referred to as the “bulk,” in search of alien environments conducive to new ways of doing physics.
Where else might one do physics, if not in the bulk? A few ideas are being developed, including one that goes by the name of holography. This is roughly the idea that any gravitational system — even the entire universe — can have an alternative description as a collection of quantum particles moving around a flat surface. From these gravity-free surfaces, a bulk world with gravity somehow pops out. It’s a remarkable theoretical claim, and over the past few years, holographers have developed a suite of tools that have helped them decode the bulk from the behavior of these surface particles.Another research program, spearheaded by Arkani-Hamed, has even more ambitious aims — getting both space-time and quantum mechanics as outputs from even more alien inputs. His group has recently developed an entirely new language for making predictions, one that makes no reference to space-time. Instead, it uses only geometric shapes and primitive counting tasks.
Is space-time, at least in its current form, definitely doomed? The idea tortured one of the pioneers of gravitational theory, John Wheeler. And today, the end of space-time is even more widely accepted. Most of the theorists I spoke with struggled to think of colleagues in the quantum gravity community who would defend space-time as a fundamental ingredient of reality. However, some researchers are pursuing alternatives. I spoke at length with Latham Boyle about patterns in particle physics that have led him and his collaborators to the more conservative notion that space-time might come in two “sheets.”
The various proposals under development are unlikely to see experimental tests this century, so a conclusive answer doesn’t seem near. But if it were someday established that space-time does break down, what would that mean for us?
On a practical level, not much. Einstein’s fabric of space-time is so sturdy that little short of a black hole would put a noticeable dent in it. But at a conceptual level, it’s hard to imagine a more dramatic rethinking of reality. When Democritus suggested that matter emerges from tiny barbed “atoms” more than 2,000 years ago, he couldn’t possibly have foreseen that parts of his proposal would ultimately be realized in the form of quantum theory — a framework asserting that reality is an ocean of overlapping waves of possibility that resolve into fixed objects only in certain situations.
If the void itself emerges from something, that something will be at least as alien. Just as individual molecules don’t themselves have a well-defined notion of heat, the base level of reality could lack marquee features of our existence that we take for granted. Places. Times. The ability to influence only nearby objects. The requirement that causes precede effects. Physicists are already finding that these notions seem unlikely to be present in a more precise accounting of the world. They seem to be the approximate outputs of something stranger.“One of the most spectacular aspects of these new findings is the emergence of causality can only happen in the approximate description,” Elliott Gesteau, a quantum gravity researcher at the California Institute of Technology, told me over Zoom earlier this year. If there is gravity, he continued, “which is what we have in our world, then this causal structure is only approximate and must break down.”…
Are we on the verge of a new physics? “Why Space-Time Looks Doomed,” from @walkingthedot in @QuantaMagazine.
The full interactive collection is here, and eminently worth reading in full.
* John Wheeler
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As we wrestle with reality, we might spare a thought for a physicist whose work helped move the questions we face forward– Max Karl Ernst Ludwig Planck; he died on this date in 1947. A theoretical physicist, he is best remembered as the originator of quantum theory. It was his discovery of energy quanta that won him the Nobel Prize in Physics in 1918.

“This is not your average, everyday darkness. This is… ADVANCED darkness.”*…
As Rob Beschizza explains, Pere Rosselló, an astrophysics student at Universidad de La Laguna in Tenerife, Spain, has created an animation depicting the gravitational collapse of Spongebob…
Beschizza muses…
Just imagine being part of a civilization on the cusp of attaining a decent model of the universe’s origins—somewhere between Halley and Lemaître, and you start plotting backwards from where we are and where the Big Bang should be you find Spongebob instead. Running the numbers again and again. Such a universe has no need of Lovecraft, cosmic horror would be right there in the maths.
Rosselló [also] solved a three-body problem: the one of animating three bodies to look really cool…
“N-body simulation of the gravitational collapse of Spongebob Squarepants,” by @PeRossello via @Beschizza in @BoingBoing.
* SpongeBob, “Rock Bottom“
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As we deconstruct deconstruction, we might recall that it was on this date (in an unspecified year) that SpongeBob met the green seahorse Mystery.
“‘Space-time’ – that hideous hybrid whose very hyphen looks phoney”*…

Space and time seem about as basic as anything could be, even after Einstein’s theory of General Relativity threw (in) a curve. But as Steven Strogatz discusses with Sean Carroll, the reconciliation of Einstein’s work with quantum theory is seeming to suggest that space and time might actually be emergent properties of quantum reality, not fundamental parts of it…
… we’re going to be discussing the mysteries of space and time, and gravity, too. What’s so mysterious about them?
Well, it turns out they get really weird when we look at them at their deepest levels, at a super subatomic scale, where the quantum nature of gravity starts to kick in and become crucial. Of course, none of us have any direct experience with space and time and gravity at this unbelievably small scale. Up here, at the scale of everyday life, space and time seem perfectly smooth and continuous. And gravity is very well described by Isaac Newton’s classic theory, a theory that’s been around for over 300 years now.
But then, about 100 years ago, things started to get strange. Albert Einstein taught us that space and time could warp and bend like a piece of fabric. This warping of the space-time continuum is what we experience as gravity. But Einstein’s theory is mainly concerned with the largest scales of nature, the scale of stars, galaxies and the whole universe. It doesn’t really have much to say about space and time at the very smallest scales.
And that’s where the trouble really starts. Down there, nature is governed by quantum mechanics. This amazingly powerful theory has been shown to account for all the forces of nature, except gravity. When physicists try to apply quantum theory to gravity, they find that space and time become almost unrecognizable. They seem to start fluctuating wildly. It’s almost like space and time fall apart. Their smoothness breaks down completely, and that’s totally incompatible with the picture in Einstein’s theory.
s physicists try to make sense of all of this, some of them are coming to the conclusion that space and time may not be as fundamental as we always imagined. They’re starting to seem more like byproducts of something even deeper, something unfamiliar and quantum mechanical. But what could that something be?….
Find out at: “Where Do Space, Time and Gravity Come From?, ” from @stevenstrogatz and @seanmcarroll in @QuantaMagazine.
* Vladimir Nabokov
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As we fumble with the fundamental, we might send far-sighted birthday greetings to Jocelyn Bell Burnell; she was born on this date in 1943. An astrophysicist, she discovered the first pulsar, while working as a post-doc, in 1957. She then discovered the next three detected pulsars.
The discovery eventually earned the Nobel Prize in Physics in 1974; however, she was not one of the prize’s recipients. The paper announcing the discovery of pulsars had five authors. Bell’s thesis supervisor Antony Hewish was listed first, Bell second. Hewish was awarded the Nobel Prize, along with the astronomer Martin Ryle.
A pulsar— or pulsating radio star– a highly magnetized, rotating neutron star that emits a beam of electromagnetic radiation. The precise periods of pulsars make them very useful tools. Observations of a pulsar in a binary neutron star system were used to confirm (indirectly) the existence of gravitational radiation. The first extrasolar planets were discovered around a pulsar, PSR B1257+12. And certain types of pulsars rival atomic clocks in their accuracy in keeping time.






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