Scientists detected a chemical produced from reaction between ozone and alkenes that could help in ending Global Warming. Criegee Biradicals are chemical compounds that are mostly released by plants. Biradicals could oxidize sulfur dioxide, which eventually turns into sulphuric acid. Sulphuric acid acts as a cooling effect in the atmosphere.Since plants help in making Biradicals, the ecosystem can act as negative effect on global warming. For more information on this newly detected particle, check out!
Monthly Archives: January 2012
Dancers (apparently) defying the laws of physics @jordanmatter
Photos by Jordan Matter from the project “Dancers Among Us” are made with no digital manipulation.
Star system with three rocky planets found by @Kepler #exoplanets
The known population of exoplanets is getting smaller, rockier, and more numerous. See the full release. The largest system of small planets known to date is still the first discovered, but they were a bit different. In 1992, Alex Wolczan and Dail Frail found the first pulsar planets.
Notes from the observatory: the sound of astronomy
I once met a guy who worked in radio on a plane, and he said that when they interview people with interesting jobs (he thought astronomer qualified), he always asked them what sound should be played to set up the piece. Astronomy is historically a very visual science, and so it took me a minute to identify a characteristic sound. I think it has to be the noise of a dome turning to keep the shutter aligned with the telescope.
Because of the rotation of the Earth, a telescope has to move to follow objects while you’re taking data. When you’re observing from the ground at many observatories, the control room is in the same building as the telescope. So, while the instrument is taking data, you occasionally hear the deep rumble as the dome turns. It’s one of my favourite sounds.
I was once observing at the Shane Telescope at Lick Observatory (see image below) with a graduate student who only had experience at Keck – the 10m-class telescopes on Mauna Kea. Because observing at 14,000 ft is difficult if you’re not used to the altitude, the control room is at a lower altitude. When the Shane turned, he looked at me and said, “What is that?” He’d never heard the dome rumble before.
Most distant type 1a supernova yet discovered with Hubble
The Hubble Space Telescope imaged the most distant type 1a supernova (exploding stellar remnant) found to date. As astronomers push these detections to larger distances (and therefore further back in time), the size and expansion history of the Universe gets constrained more and more.
The lower panels in the image above (zooms of the top image) show the appearance of the supernova between the time the first one was taken (left) and the second. Here is the full press release.
Researchers now able to stop, restart light
Gazette Staff
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| Lene Hau and her colleagues created a new form of matter to bring a light beam to a complete stop, then restart it again. (Staff photo by Kris Snibbe) |
“Two years ago we slowed it down to 38 miles an hour; now we’ve been able to park it then bring it back up to full speed.” Lene Hau isn’t talking about a used motorbike, but about light – that ethereal, life-sustaining stuff that normally travels 93 million miles from the sun in about eight minutes.
Less than five years ago, the speed of light was considered one of the universe’s great constants. Albert Einstein theorized that light cannot travel faster than 186,282 miles per second. No one has proved him wrong, but he never said that it couldn’t go slower.
Hau, 41, a professor of physics at Harvard, admits that the famous genius would “probably be stunned” at the results of her experiments. Working at the Rowland Institute for Science, overlooking the Charles River and the gold dome of the state Capitol in Boston, she and her colleagues slowed light 20 million-fold in 1999, to an incredible 38 miles an hour. They did it by passing a beam of light through a small cloud of atoms cooled to temperatures a billion times colder than those in the spaces between stars. The atom cloud was suspended magnetically in a chamber pumped down to a vacuum 100 trillion times lower than the pressure of air in the room where you are reading this.
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“It’s nifty to look into the chamber and see a clump of ultracold atoms floating there,” Hau says. “In this odd state, light takes on a more human dimension; you can almost touch it.”
She and her team continued to tweak their system until they finally brought light to a complete stop. The light dims as it slows down, so you think that it’s being turned out. Then Hau shoots a yellow-orange laser beam into the cloud of atoms, and the light emerges at full speed and intensity.
Inspired by Hau’s success at slowing light, researchers working on a wooded hill a few miles away at the Harvard-Smithsonian Center for Astrophysics (CfA) used a similar technique to stop, then restart, a light beam. That team was headed by Ronald Walsworth and Mikhail Lukin, both associates of Harvard College. Their success was independent of Hau’s effort.
“We didn’t have much contact,” she notes, “just a few e-mails.”
Stopping cold
Besides stirring a research rush to explore exotic forms of matter, such experiments open the door to some practical applications. These include vastly more powerful computers as well as the possibility of communications that are much more secure from hackers and people trying to steal your credit and bank card numbers.
“We hope for wonderful things,” says David Phillips, who worked on the CfA “stop light” project. “Our imagination hasn’t figured out what the possibilities are yet.”
Hau, a tall, slender scientist educated as a theoretical physicist in Denmark, had a hunch several years ago that intensely cold atoms would become a hot area in physics. In the mid-1990s, she and her colleagues became excited about experiments aimed at crowding atoms so close together that unusual things happen. The key is to cool them to within a billionth of a degree of minus 459.7 degrees F. Called “absolute zero,” this is the temperature at which atoms have the least possible energy, and they all but cease to move around.
Hau was one of several researchers who succeeded in creating this novel state of matter. She corresponded with a colleague, Stepen Harris at Stanford University, and they came up with the idea that it might be possible to use a small ball of cold atoms to slow down light.
Hau and her group then figured out a way to make it work. Using sodium atoms and two laser beams, they made a new kind of medium that entangles light and slows it down. The laser beams glow yellow-orange like sodium streetlights, and the cigar-shaped cloud of atoms is about eight-thousandths of an inch long and about a third as wide.
Working with Chien Liu, a postdoctoral fellow at Rowland, and Harvard graduate students Zachary Dutton and Cyrus Behroozi, Hau kept tweaking the atoms until they completely stopped laser light. This happens when a second laser beam directed at right angles to the cloud of atoms is cut off. When that laser is switched on again, it abruptly frees the light from the trap and it goes on its way.
Hau explains that light entering the atomic entanglement transfers its energy to the atoms. Light energy raises the atoms to higher energy levels in ways that depend on the frequency and intensity of the light. The laser illuminating the cloud at right angles to the incoming beam acts like a parking brake, stopping the beam inside the cloud when it is shut off. When it is turned on again, the brake is released, the atoms transfer their energy back to the light, and it leaves the end of the cloud at full speed and intensity.
Hau’s team stopped light for one-thousandth of a second. Atomically speaking, “this is an amazingly long time,” Hau notes. “But we think it can be stopped for much longer.”
The CfA researchers used an easier method. They shot laser beams through a dense cloud of rubidium and helium gas. (Rubidium, in its solid or natural form, is a soft, silver-white metal.) The light bounced from atom to atom, gradually slowing down until it stopped. No supervacuum or ultra-cold was needed. In fact, the chamber where the light stopped was at a temperature of 176 degrees F.
This convenience comes at a cost, however. Only half of the incoming light was stored, then recovered, and the storage time was much shorter.
Think of both contraptions as sophisticated light switches that control not just light but information. Incoming light can carry information expressed by changes or modulations of its frequency, amplitude, and phase. When the light stops, that information is stored just like information is stored in the electronic memory of a computer. To access the information, you turn on a control laser, and out it comes.
Shrinking computers
Computers operating by these so-called quantum effects are much more efficient that those available today, or even on the drawing board. (“Quantum” refers to changes in the energy levels of the atoms.) Today’s machines represent information in bits, electronic combinations of zeros and ones. Bits represented by quantum states of atoms could carry much, much more information. Cubic inch for cubic inch, quantum computers could tackle problems that would stymie the most super of conventional computers. For example, they could perform many calculations simultaneously.
Another thing they could do would be to encrypt information in complex codes impossible to crack without extremely expensive and time-consuming methods. Financial and other information would be prodigiously safer with a quantum computer.
As marvelous as they are, however, both the Rowland and CfA systems take up more space and power than would be practical. Hau’s experiment requires a small room, CfA’s needs a large tabletop.
CfA researchers need to solve this problem and to make sure all the light is stored – not just half. That will take many years.
Hau has already started ordering and installing equipment with which she plans to construct a quantum light stopper no bigger than a fingernail. She envisions ultracold and supervacuums being achieved with devices less than one-thousandth of an inch in size. These would be built on chips no bigger than the Pentium IV that runs many of today’s small laptop and palm-sized computers.
“Wouldn’t that be nifty!” Hau says. She and her colleagues describe their experiment in detail in today’s issue of the journal Nature.
Team build world’s smallest hard drive
Team build world’s smallest hard drive
Related Stories
- Diamonds are a supercomputer’s best friend, Science Online, 27 Aug 2010
- Atoms bring quantum computing closer, Science Online, 24 May 2010
- Atom transistor to speed up computers, Science Online, 11 Dec 2009
Hard drives could one day be the size of rice grains, powering music players so small they would fit inside your ear.
Scientists at IBM and the German Center for Free-Electron Laser Science have built the world’s smallest unit of magnetic storage, using just 96 atoms to create one byte of data. Conventional drives require a half a billion atoms for each byte.
The advance could lead to tiny hard drives able to store 200 to 300 times more information than they can today. Just imagine an iPod Touch that held 12.8 terabytes of music.
“An effect that is common in nature can produce this information storage idea,” says Sebastian Loth of CFEL, lead author of the research, which is being published today in the journal Science.
The natural phenomenon Loth is referring to has to do with the way electrons spin inside an atom. Modern hard drives rely on magnetic materials such as iron, where electrons all spin in the same direction perfectly aligned with each other. The drives work by reading the magnetic states of small regions on a disk and using an external field to write to them.
But these so-called ferromagnetic materials can only be shrunk down so far. If the magnetic regions get too close to each other, their magnetic fields interfere with each other and make it difficult to accurately store data.
“This is a big problem if you want to pack in the magnetic density,” says Loth.
But with materials that are not magnetic, known as antiferromagnetic materials, the electrons spin in opposite directions from one another and are magnetically neutral.
“Antiferromagnetic regions don’t have a magnetic field so you can pack them closer,” Loth says.
In fact, the scientists were able to squeeze bits into a space just one nanometre apart.
Built atom by atom
The team assembled the tiny hard drive from the atom up, using a special tool known as scanning tunnelling microscope, or STM. They carefully placed atoms into rows of six atoms each. Two rows were enough to store one bit of information. Eight pairs of rows amounted to one byte of data.
Each pair of rows has two possible magnetic states, representing the classical 0 and 1 of binary computer data. An electric pulse from the STM tip flips the magnetic configuration from one to the other. A weaker pulse was used to read it.
“What this shows is you have all the ingredients for storing information on an antiferromagnetic grain,” says Dr Matthias Bode, an experimental physics professor at the University of Würzburg, who was not involved in the research.
It will be some time before this technology is used in a hard drive for a computer, as there are a few problems that still have to be overcome. First, this hard drive was built atom-by-atom, using an STM – an impractical and slow method for manufacturing.
Secondly, the storage of the information, the magnetic state, is only stable at very cold temperatures, about 5 degrees above absolute zero. Warmer than that and the spins of the atoms get jostled.
Bode says that finding a material that works at room temperature isn’t impossible. What material will work, however, remains to be seen.
Loth notes there are lots of other materials to experiment with that are known to hold antiferromagnetic states at room temperature. “This isn’t like superconductors, where we are looking for ways to boost the critical temperature,” says Loth. “We know that antiferromagnetic materials are stable.”
This work is also important because it demonstrated for the scientists how few atoms they could use before the effects of quantum mechanics took over. It turns out that twelve atoms are the minimum number required. Fewer than that and quantum effects begin to mess around with the stored information.
Thunderstorms proven to create antimatter
Thunderstorms have been shown to create positrons and send them to space. As the late, great, Johnny Carson of the Tonight Show used to say, “That is some weird, wild, stuff“.
First Quantum Effects Seen in Visible Object
Does Schrödinger’s cat really exist? You bet. The first ever quantum superposition in an object visible to the naked eye has been observed.
Aaron O’Connell and colleagues at the University of California, Santa Barbara, did not actually produce a cat that was dead and alive at the same time, as Erwin Schrödinger proposed in a notorious thought experiment 75 years ago. But they did show that a tiny resonating strip of metal – only 60 micrometres long, but big enough to be seen without a microscope – can both oscillate and not oscillate at the same time. Alas, you couldn’t actually see the effect happening, because that very act of observation would take it out of superposition.
“We talk about quantum weirdness and things being in two places at once, but it all involves atoms and molecules, stuff we don’t normally interact with,” says O’Connell, who presented the results at the March meeting of the American Physical Society in Portland, Oregon.
Bridge between worlds?
Proving that all objects, whatever their size, obeys the same rules has long been a goal of physicists. But with quantum mechanics it is no trivial matter: the larger an object, the more easily its fragile quantum state is destroyed by the disruptive influence of the world around it. O’Connell’s experiments required delicate control and a temperature of just 25 millikelvin to measure the state in the few nanoseconds before it was broken down by disruptive influences from outside.
“It was a close call, but sufficient to see a first quantum signature,” says Markus Aspelmeyer of the University of Vienna, Austria, who was not involved in the research.
The key was to connect the resonating strip to a superconducting qubit – a tiny electric circuit that can easily be prepared in a quantum superposition of two energy states. “The qubit acts as a bridge between the microscopic and the macroscopic worlds,” says O’Connell. By tuning the frequency at which the qubit cycled between its two states to match the resonant frequency of the metallic strip, the qubit’s quantum state could be transferred to the resonator at will.
When measured afterwards, the resonator was sometimes in its non-oscillating ground state and sometimes in an oscillating “excited” state. The number of times it was measured to be in each state followed the probabilistic rules of quantum mechanics.
Next, the cat?
“It’s like you have a child’s swing that goes back and forth,” says O’Connell. “We pushed the swing and didn’t push the swing at the same time.”
“This is challenging and creative work,” says Khaled Karrai of Ludwig-Maximilian University Munich, Germany. “If correct, it is a breakthrough.”
Schrödinger’s cat would be unlikely to survive the frigid temperatures of such experiments, so it is perhaps not the next milestone to look out for. But now the spooky influence of quantum physics on visible objects has been proved, can we expect to be putting an object as large as a real child’s swing into an indeterminate quantum state any time soon? O’Connell thinks so. “I’d say in the near future – in the next 20 years.”
Journal reference: Nature, DOI: 10.1038/nature08967
This article by Richard Webb appeared originally on New Scientist.
Physics of Rock Climbing
To help teach my first year engineering physics students last term about forces, I used an example of someone climbing up a crevice with their feet on one side and their back on the other. This pair of physics teachers also feels that rock climbing, by example, is a great way of explaining forces. Though cheesy, this video may help to understand forces, and rock climbing: [youtube http://www.youtube.com/watch?v=VSHxa9WI7Qw?wmode=transparent]







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