Many researchers find these ideas irresistible. Within the last few years, physicists in seemingly unrelated specialties have converged on this confluence of entanglement, space and wormholes. Scientists who once focused on building error-resistant quantum computers are now pondering whether the universe itself is a vast quantum computer that safely encodes spacetime in an elaborate web of entanglement. “It’s amazing how things have been progressing,” says Van Raamsdonk, of the University of British Columbia in Vancouver.
Physicists have high hopes for where this entanglement-spacetime connection will lead them. General relativity brilliantly describes how spacetime works; this new research may reveal where spacetime comes from and what it looks like at the small scales governed by quantum mechanics. Entanglement could be the secret ingredient that unifies these supposedly incompatible views into a theory of quantum gravity, enabling physicists to understand conditions inside black holes and in the very first moments after the Big Bang.
Catalyst: Virtual Universe — The Illustris supercomputer has modelled vast swathes of the universe, allowing us to visualise incredible scenarios in outer space.
Part of what makes astronomy so difficult is the inconceivability of space and its mind-boggling vastness. But an extraordinary new supercomputer called the Illustris has modelled a huge chunk of the universe: a cube 350 million light years across, an area the home to tens of thousands of galaxies. Illustris reveals how galaxies form and collide, shows what happens when unsuspecting matter falls into black holes, and lifts the lid on a host of other dramatic events that have unfolded since the Big Bang. Dr Graham Phillips takes us on a virtual tour of our wondrous universe.
ABC Australia — Ref 6510.
Journeyman Pictures brings you highlights from the cutting-edge science series, ‘Catalyst’, produced by our long-term content partners at ABC Australia. Every day we’ll upload a new episode that takes you to the heart of the most intriguing and relevant science-related stories of the day, transforming your perspective of the issues shaping our world.
The group has combined theoretical and computational physics techniques and used the Laboratory’s massively parallel 2-petaflop Vulcan supercomputer to devise a new model of dark matter. The model identifies today’s dark matter as naturally “stealthy.” But in the extremely high-temperature plasma conditions that pervaded the early universe, it would have been easy to see dark matter via interactions with ordinary matter, the model shows.
Next January Stephen Hawking will be 74 years old. He has lived much longer than most individuals with his debilitating condition. In addition to being an unquestionably gifted cosmologist, he has invited controversy by supporting the pro-Palestinian, Israel-BDS boycott and warning about the dangers of alien invaders who tap into our interstellar greetings
Antisemitism, notwithstanding, this man is a mental giant. He is Leonardo. He is Einstein. Like them, his discoveries and theories will echo for generations beyond his life on earth. He is that genius.
Forty years ago, when Stephen Hawking still had mobility, he delivered a paper on a mystery regarding information-loss for entities that cross the event boundary of a black hole.
In the mid 1970s, Astronomers were just discovering black holes and tossing about various theories about the event horizon and its effect on the surrounding space-time. Many individuals still considered black holes to be theoretical. Hawking’s analysis of the information paradox seemed extremely esoteric. Yet, last month (Aug 2015) , at Sweeden’s KTH Royal Institute of Technology, Hawking presented a possible solution to the paradox that he sparked.
I can barely understand the issue and cannot articulately rephrase the problem. But my interest in the black hole event horizon takes a back seat to my interest in the amazing tool created to compensate for the famous cosmologist’s handicap. Watch closely as Stephen Hawking offers a new theory that provides a possible explanation for the paradox.
Near the end of the video (beginning at 7:22), the camera begins a steady zoom up to Hawking’s face. Unlike a year ago, when he could still smile at a joke or move his eyes, he now appears completely motionless. Throughout his speech, there is no sense of animation—not even a twitch—with or without purpose. His eyebrow doesn’t move, his fingers are not restless, he doesn’t blink anymore.
So, how, then, does Hawking speak with normal cadence and just a short delay between sentences? (If we assume that his computer adds emphasis without additional effort, I estimate that his ASCII communications rate is roughly equivalent to a 1200-baud modem, circa 1980). Yet, clearly, there must be a muscular conduit between thought and speech. How is it that his thoughts are converted to speech at almost the same rate as someone who is not paralyzed?
That magic is enabled by a tiny camera that monitors a slowly deteriorating cheek muscle. It is Hawking’s last connection to the outside world. What began as index cards with words and then an Apple II computer, has evolved into a sophisticated upgrade process involving cutting edge analysis of the professor’s slightest tick combined with sophisticated computing algorithms. The camera and software that interprets this microscopic Morse code is tied to a process that optimizes options for successive words and phrases. He is actually communicating at far less than 1200 baud, because—like a court stenographer—he employs shorthand and Huffman encoding to compress words and phrases into his twitch pipeline. Drawing on a powerful processor and connected to the Web, his gear is constantly upgraded by a specialized Intel design team. They are engaged in a race to offer Hawking the potential for communication up until he has no capacity for interaction at all.
In a recent documentary by Hawking himself,* he laments the likely day when he will no longer have any capacity for output at all. No ability to discuss physics and cosmology; no way to say “I need help” or “I love you”; no way to show any sign of cognition. At that time, he reflects, the outside world will no longer be certain that there is anything going on behind his blank stare. They will never really know when or if he wants them to pull the plug. Even more mind boggling, humanity will never know what secrets his brilliant mind has unlocked to mysteries of the cosmos.
Two black holes, circling one another on their way to merging together, can create ripples in spacetime, but the waves are weaker than previously thought.
The dimensionless aspect, since it has no dimensions, is outside of space and time. This is the key aspect to existence: an aspect outside of space and time perpetually interacting dialectically with an aspect inside space and time. All of the weird and wonderful phenomena of the universe are the products of this ultimate dichotomy.
Does this sound crazy? Then consider the evidence provided by black holes.
The R = 0 Universe.
Black holes are objects where gravity is so strong that light itself cannot escape the gravitational pull. They are the most mysterious objects in the universe and hold the key to the nature of reality. They open the door to understanding the fundamental composition of the universe.
Their hypothetical existence was first predicted in Einstein’s famous theory of General Relativity, but Einstein himself believed it was impossible for them to become real objects in the universe. The reason for that is that they exhibit a feature that physics cannot cope with or comprehend.
Einstein’s equations contain a term that involves dividing the mass of the black hole by the distance “r” from the black hole. The question is what happens when r=0? Division by zero gives a result of infinity. To physicists, it is impossible for infinity to appear in the real world, so they consider r = 0 to be the point at which physics breaks down. At r = 0, the centre of a black hole, gravity is infinite and time itself stops: all of the mass of the black hole is contained within an infinitely small point where the concept of space no longer makes any sense. The point takes up precisely no space at all. Since this point is outside space and time, it is dimensionless. The physical universe collapses into an ineffable twilight state at this point. This apparently impossible object of infinite density and infinite gravity is known as the singularity. No predictions can be made about it, or about what might emerge from it. At the singularity, physicists’ understanding of nature fails completely. Therefore, they believe that there is a fatal flaw in the formulation of Einstein’s theory of general relativity, despite its immense success.
The one thing no physicist has ever contemplated is this: there is no flaw whatsoever. The reason why physics seems to disintegrate at r = 0 is for the extremely simple reason that r = 0 is not in the physical universe. It is in the mental universe, the universe of mind, as we have described in the previous section.
When scientists spotted this pair of black holes, it was a rare chance to observe black holes in the process of colliding. Soon, however, as they looked closer, scientists were consumed with a brand new question: Uh, hey, what’s that blinking light?
The light isn’t coming from the pair of colliding black holes (named PG 1302-102) 3.5 billion light years away from us, it’s coming from the turbulence around them. What that doesn’t explain, though, is why the light “flashes” rhythmically—regularly brightening, then dimming. So researchers Daniel D’Orazio, Zoltan Haiman, and David Schiminovich at Columbia University built a simulation of the pair and have now come up with an explanation for just what we’re seeing.
As a follow-up to Shailesh Prasad’s thought provoking video (just below this article), I offer two equally impressive visualizations of the scope and magnificence of our universe. These videos are the epitome of a teachable moment. And it’s fun, too!
Check out this simple, one-button interactive Scale of the Universe by Cary Huang. Simply pull a slider left or right to zoom in or out. It covers the Universe from 1027 meters down to 10-35 meters (from the entire universe to the Plank length and quantum foam).
Charles and Ray Eames
Unlike the classic film by Charles & Ray Eames (more about that later), the zoom doesn’t really take viewers closer or further away. Rather, it compares relative size by allowing users navigate by magnitudes (a circle indicates each power-of-ten).
Nikon, the camera and optics maker, created an alternate spin on this idea with more user control (identify and study objects used to illustrate size–and jump directly to any magnitude along the size continuum). Instead of panning in and out, the Nikon presentation crawls familiar objects along the horizontal axis. Interestingly, they end at modest lower limit of 10-15 meters, rather than attempting to illustrate quarks, charm and quantum foam.
In 1968, Charles & Ray Eames were already famous as sculptors, architects and designers of modern furniture. That’s when they created Powers of 10, one of the most popular educational films of all time. Just 9 minutes long, it was intended as a “rough sketch” in an effort to attract an animation partner to add visual punch. 9 years after the original film was released, IBM collaborated with the designers and the film was re-released with improved special effects. Both versions are included on the commercial DVD. I prefer the original rough sketch.
Eames Lounge Chair
In the original film, two clocks sit outside the main frame. As we » accelerate away from earth (covering 10X as much distance every ten seconds), the clocks track relative time from a traveler’s frame of reference –vs– a person on earth.
You can view the 1977 re-release (Be sure to raise quality to 480p). Interestingly, IBM has also posted a user-controlled, Zoomable version.
I can’t find the original film on the web. But I own it. Write to me if you want me to “loan” it to you via a web link.
By all counts, Earth is on a one way trip to oblivion. Our aging Sun will see to that. Within 500 to 900 million years from now, photosynthesis and plant life on Earth will reach a death-spiral tipping point as the Sun continues its normal expansion and increases in luminosity over time.
Trouble is, researchers are still unsure about all the grisly endgame details, and their models of such slow motion horrors are hard to test. But a team of researchers now say that finding and observing nearby aging Earth-analogues, undergoing the ravages of their own expanding sun-like stars, will help Earth scientists understand how the stellar evolution of our own sun will affect life here on Earth.
“[Within] 500 million years figure most plants become extinct, although some could potentially last up to 900 million years from now by employing more carbon-efficient photosynthetic pathways,” Jack O’Malley-James, an astrobiologist at the University of St. Andrews in the U.K. told Forbes. “At this point the biosphere as we know it on Earth will be dramatically different, but not necessarily completely dead.”.