Posts tagged science
Ten things you probably did’nt know about dark energy
Dark energy is the biggest mystery in the cosmos, pervading the vast emptiness of space for billions of light-years. But if you thought you knew everything there was to know about this strange force, think again.
Discovery Space sat down with Michael Turner, a cosmologist at the University of Chicago, to pin down the 10 biggest things you didn’t know about dark energy.
10. Dark Energy’s Discoverer Didn’t Coin the Term
Who came up with the term? “I did,” Turner said. “That’s because when you find something new and weird, you have to name it. It can’t just be ‘the funny stuff that helps the universe speed up.’”
The term is also used to say that it’s different than dark matter, which is yet another weird constituent of the cosmos, and behaves more like energy than anything else that we know of.
9. Albert Einstein First Stumbled on Dark Energy’s Path
Thing is, Einstein didn’t even know it.
The German-born scientist derived an historic ”cosmological constant” to make the universe static — or in other words, prevent gravity from steering the cosmos into a “big crunch” billions of years in the future.
“Instead of counteracting gravity, however, Einstein’s cosmological constant overpowers it and causes the universe to expand at an accelerating pace,” Turner told Discovery Space. “People like to say that even when Einstein thought he made a mistake he was right, but that’s a bit of a stretch.”
If Einstein’s cosmological constant does exist, it’s about four times stronger than he first anticipated.
“We don’t think the universe is static,” he said. “It’s inconsistent with what we see out there.”
8. Dark Energy Could Be Nothing
The “gravity” of dark energy is repulsive, making it a large-scale anti-gravity that acts like an overzealous traffic cop between clusters of galaxies. What’s between those galaxies? Empty space.
“The simplest explanation for dark energy is that it’s associated with something called the ‘quantum vacuum,’” Turner said.
According to quantum mechanics — which explains how the universe works on a small scale — empty space is full of particles living on borrowed time and energy, Turner explained. So it’s not too unreasonable to suggest dark energy might also occupy that “empty” space.
7. Dark Energy Can’t Be Broken into Particles
About 2,500 years ago, Democritus suggested there were four elements in the universe: air, fire, earth and water, later adding “ether.”
“He started on this path that everything is made of indivisible particles called atoms, and that path eventually led us to subatomic particles called quarks today,” Turner said. “But dark energy isn’t made of quarks, or any other particle.”
6. Dark Energy Is Everywhere
According to Einstein’s famous equation E=MC^2, matter can be converted completely into energy, and the universe can be divided into a “pie” of energy.
“One of the most important things about dark energy is that it makes up most of the stuff in the universe,” Turner told Discovery Space. ” however, locally, we don’t notice it.”
The breakdown of the pie is roughly like this:
- 74 percent is dark energy
- 22 percent is dark matter
- 3.6 percent is nearly invisible gas between stars
- 0.4 percent is stars, planets, moons and everything else. Including you.
5. Dark Energy Is the Most Elastic Substance Ever
“It’d be safe to say it’s more than a zillion times more elastic than anything we know of,” Turner said. “Even NASA’s most stretchy material, whatever it may be.”
If one were to “weigh” the energy of dark energy in a large coffee cup, it would be about 1 x 10^-27 grams (0.000000000000000000000000001 grams) or, in other words, not a whole lot.
If you do the math, Turner explained, contracting a volume of dark energy between here and the sun would create enough juice to power the Earth for about nearly 100,000 years.
4. Dark Energy Shaped the Universe
The Big Bang is thought to have kick-started the universe we live in, but after the event, dark energy began to seize its grip on matter and overcome gravity.
“Our universe was shaped by battle between dark energy and matter,” Turner said. “For the first 8 billion years or so of the universe’s existence, the gravity of matter held sway and clusters of galaxies formed.”
Roughly five billion years after that — or about one billion years ago — dark energy took over, and “put its foot on accelerator,” Turner said. “The expansion of the universe began speeding up and no larger structures were built.”
3. Dark Energy May Not be Energy at All
If it’s not made of particles, and may be nothing, is it really safe to call it energy?
“Not in the least bit,” Turner told Discovery Space. “There may very well be no dark energy at all.”
Instead, Turner suggested that Einstein’s ideas about gravity might need to be replaced.
“Few people think Einstein got the last word on gravity. His story didn’t incorporate the details of the universe at the atomic level,” he said, which is what might hold the key to gravity.”
2. Dark Energy Holds the Destiny of the Cosmos
Until we understand what dark energy is, Turner thinks we won’t really know what the fate of the universe is.
“It could continue to accelerate as it is,” he said. “If it does, then in about 100 billion years the galaxies around us will be speeding away from us too quickly to see.”
Another scenario is that the acceleration of the universe’s expansion may be doubled. And that’s bad news for everyone that might be out there — the cosmos will rip itself to shreds.
“We don’t know if the acceleration we see today is accelerating,” Turner said. “If it is, the ‘big rip’ will occur in roughly 20 billion years.”
One last option is equally as frightening.
“Maybe dark energy’s next trick is to decelerate expansion and lead to the collapse of the universe,” Turner said. “We’ve trapped ourselves time and time again believing in the simplest case, only to correct ourselves. If you want to be squeaky-clean correct, we can’t confidently guess the future of the universe yet.”
1. No One Knows What Dark Energy Is
If you thought you were clueless, even the experts don’t know.
“Welcome to the club,” Turner said. “It’s the most profound mystery in all of science. It ties together the destiny of the universe, mysteries about gravity and quantum nothingness. How’s that for a mystery?”
(via sagansense)
The Connection Between Memory and Sleep
Researchers found information can be better retained with reinforcing stimuli delivered during sleep
When you’re studying for an exam, is there something you can do while you sleep to retain the information better?
“The question is, ‘What determines which information is going to be kept and which information is lost?’” says neuroscientist Ken Paller.
With support from the National Science Foundation (NSF), Paller and his team at Northwestern University are studying the connection between memory and sleep, and the possibilities of boosting memory storage while you snooze.
“We think many stages of sleep are important for memory. However, a lot of the evidence has shown that slow-wave sleep is particularly important for some types of memory,” explains Paller.
Slow-wave sleep is often referred to as “deep sleep,” and consists of stages 3 and 4 of non-rapid-eye-movement sleep.
Paller’s lab group members demonstrated for Science Nation two of the tests they run on study participants. In the first experiment, the subjects learned two pieces of music in a format similar to the game Guitar Hero. During a short nap following learning, just one of the learned tunes was played softly several times, to selectively reinforce the memory for playing that tune without any reinforcement but not for the other tune. Paller wanted to know whether the test subjects could more accurately produce the tune played during sleep.
In the second exercise, the subjects were asked to memorize the location of 50 objects on a computer screen. The presentation of each object was coupled with a unique sound. During the post-learning nap, memory for the location of 25 objects was reinforced by the play-back of only 25 of the sounds. In this case, Paller wanted to know whether the subjects could remember object locations better if the associated sounds were played during sleep.
Researchers recorded electrical activity generated in the brain using EEG electrodes attached to the scalp. They thus determined whether the subjects entered “deep sleep,” and only those who did participated in the reinforcement experiments. In both experiments, participants did a better job remembering what was reinforced while they slept, compared to what was not reinforced.
“We think that memory processing happens during sleep every night,” says Paller. “We’re at the beginning of finding out what types of memory can be reinforced, how large reinforcement effects can be, and what sorts of stimuli can be used to reactivate memories so that they can be better consolidated.”
Paller’s goal is to better understand the fundamental brain mechanisms responsible for memory. And that, in turn, may help people with memory problems, including those who find themselves more forgetful as they age.
“We experience progressively less slow-wave sleep as we age. Of course, many brain mechanisms come into play to allow us to remember, including some processing that transpires during sleep. So, there’s a lot to figure out about how memory works, but I think it’s fair to say that the person you are when you’re awake is partly a function of what your brain does when you’re asleep,” explains Paller. He says these reactivation techniques could turn out to be valuable for enhancing what people have learned.
“What is beautiful about this set of experiments is that Dr. Paller identified ‘deep sleep’ as a critical time window during which memory for specific experiences can be selectively enhanced by the method of reactivation without conscious effort,” says Akaysha Tang, director of the cognitive neuroscience program in the NSF Directorate for Social, Behavioral and Economic Sciences.
“Normally, conscious rehearsal of memorized material is needed if one wants to remember something better or retain it for longer, and one has to find time to review or rehearse,” continues Tang. “Dr. Paller and the members of his lab group showed that such selective enhancement could be achieved without conscious effort and without demanding more of one’s waking hours. So, instead of pulling that all-nighter to memorize the material, in the future, it may be possible to consolidate the memory by sleeping with a scientifically programmed lullaby!”
There may be a hundred billion planetary systems in the galaxy awaiting exploration. Not one of those worlds will be identical to Earth. A few will be hospitable; most will appear hostile. Many will be achingly beautiful. In some worlds there will be many suns in the daytime sky, many moons in the heavens at night, or great particle ring systems soaring from horizon to horizon. Some moons will be so close that their planet will loom high in the heavens, covering half the sky. And some worlds will look out into a vast gaseous nebula, all those skies, rich in distant and exotic constellations, there will be a faint yellow star — perhaps barely seen by the naked eye, perhaps visible only through the telescope — the home star of the fleet of interstellar transports exploring this tiny region of the Milky Way Galaxy.
The themes of space and time are, we have seen, intertwined. Worlds and stars, like people, are born, live and die. The lifetime of a human being measured in decades; the lifetime of the Sun is a hundred million times longer. Compared to a star, we are like mayflies, fleeting ephemeral creatures who live out their whole lives in the course of a single day. From the point of view of a mayfly, human beings are stolid, boring, almost entirely immovable, offering hardly a hint that they ever do anything. From the point of view of a star, a human being is a tiny flash, one of the billions of brief lives flickering tenuously on the surface of a strangely cold, anomalously solid, exotically remote sphere of silicate and iron.
In all these other worlds in space there are events in progress, occurrences that will determine their futures. And on our small planet, this moment in history is a historical branch point as profound as the confrontation of the Ionian scientists with the mystics 2,500 years ago. What we do with our world in this time will propagate down though the centuries and powerfully determine the destiny of our descendants and their fate, if any, among the stars.
Carl Sagan — Travels in Space and Time — Cosmos (via ikenbot)(via pineapplesage)
The Theory of ‘Most Things’ (Revised introduction to my theory of Dark Matter)
I decided not to bother hiding it anymore. It’s incomplete, but here is the WIP.
Sir Isaac Newton (25 December 1642 [NS: 4 January 1643] – 20 March 1727 [NS: 31 March 1727]) was an English physicist, mathematician, astronomer, natural philosopher, alchemist and theologian, who has been considered by many to be the greatest and most influential scientist who ever lived. Although his career was long and littered with success, there were four discoveries that were considered to be his most important.
Law of universal gravitation
Thoughts of gravitation entered Newton’s head as result of a certain apple tree and the tree’s falling fruit. In 1666, while Newton was sitting in the manor house garden at Woolsthorpe, he saw an apple fall from a tree. This triggered certain thoughts that he had been having about gravitation. Despite popular belief, the apple did not fall on his head. What actually happened was that he saw an apple fall from an apple tree and he began to wonder why it fell. From there his thoughts broadened to the rotation of the moon. It was already common knowledge that the moon revolved around the Earth and the planets revolved around the sun. This was caused by gravity. What Newton wanted to know was why the moon revolved around the earth instead of simply being pulled into the earth like the apple was. This brainstorm (which some scholars suspect Newton may have invented late in life) ultimately led to his law of universal gravitation. The law says that all particles of matter in the universe attract every other particle, that gravitational attraction is a property of all matter. The law explained many things, from the orbits of the planets around the sun to the influence of the moon and sun on the tides. And it held sway as the accepted description of terrestrial and celestial mechanics for almost 200 years, until Einstein came along and rocked the boat with relativity.
Three laws of motion
Newton’s laws of motion are three physical laws that form the basis for classical mechanics. They describe the relationship between the forces acting on a body and its motion due to those forces. They have been expressed in several different ways over nearly three centuries and can be summarized as follows:
- First law: If an object experiences no net force, then its velocity is constant: the object is either at rest (if its velocity is zero), or it moves in a straight line with constant speed (if its velocity is nonzero).
- Second law: The acceleration a of a body is parallel and directly proportional to the net force F acting on the body, is in the direction of the net force, and is inversely proportional to the mass m of the body, i.e., F = ma.
- Third law: When a first body exerts a force F1 on a second body, the second body simultaneously exerts a force F2 = −F1 on the first body. This means that F1 and F2 are equal in magnitude and opposite in direction.
Theory of light and color
Newton became stuck while trying to figure out what the radius of the earth was in order to help him prove his Universal Law of Gravitation. Rather than guess and take a chance that he might be wrong, he decided to put the project on hold and study something else. That something else optics, or the study of color and light. From 1670 to 1672, Newton lectured on optics. During this period he investigated the refraction of light, demonstrating that a prism could decompose white light into a spectrum of colours, and that a lens and a second prism could recompose the multicoloured spectrum into white light.
He also showed that the coloured light does not change its properties by separating out a coloured beam and shining it on various objects. Newton noted that regardless of whether it was reflected or scattered or transmitted, it stayed the same colour. Thus, he observed that colour is the result of objects interacting with already-coloured light rather than objects generating the colour themselves.
From this work, he concluded that the lens of any refracting telescope would suffer from the dispersion of light into colours (chromatic aberration). As a proof of the concept, he constructed a telescope using a mirror as the objective to bypass that problem.
Calculus
When Newton began to muse on the problem of the motion of the planets and what kept them in their orbits around the sun, he realized that the mathematics of the day weren’t sufficient to the task. Properties such as direction and speed, by their very nature, were in a continuous state of flux, constantly changing with time and exhibiting varying rates of change. So he invented a new branch of mathematics, which he called the fluxions (later known as calculus). Calculus allowed him to draw tangents to curves, determine the lengths of curves, and solve other problems that classical geometry could not help him solve. Interestingly, Newton’s masterwork, the Principia, doesn’t include the calculus in the form that he’d invented years before, simply because he hadn’t yet published anything about it. But he did combine related methods with a very high level of classical geometry, making no attempt to simplify it for his readers. The reason was, he said, “to avoid being baited by little Smatterers in Mathematicks.”
Research Team Discerns Atomic Bond Types From Image
A team of researchers at IBM has had astounding success at imaging things on the smallest of scales, and once again they have worked their magic and produced something completely out of this world. After producing an image of a molecule shaped like the Olympic Rings earlier this year, they have published this image and a paper in the journal, Science, in which the detail is so high that they are able to discern the types of atomic bonds present.
Using a technique called atomic force microscopy (AFM), the team was able to create this picture. Atomic force microscopy works through using a carbon monoxide molecule which effectively works as a recording needle (read: record player needle), as to pick up the minute vibrations.
In order to get a clear picture instead of a fuzzy mess, the experiment must be isolated from any vibrations in the lab. This means that too much warmth would lead to distortion also, so the experiment is kept at a chilly -268C.
In the image you can see just how long the atomic bonds are, with the bright and dark spots corresponding to higher and lower densities of electrons respectively.
That we can now see different physical properties of different bonds is really freaking awesome and this new ability will no doubt lend itself to future developments in many areas of science. (x)
(via physicsphysics)
The empathy machine
…Let’s dwell for a moment on ‘Silver Blaze’ (1892), Arthur Conan Doyle’s story of the gallant racehorse who disappeared, and his trainer who was found dead, just days before a big race. The hapless police are stumped, and Sherlock Holmes is called in to save the day. And save the day he does — by putting himself in the position of both the dead trainer and the missing horse. Holmes speculates that the horse is ‘a very gregarious creature’. Surmising that, in the absence of its trainer, it would have been drawn to the nearest town, he finds horse tracks, and tells Watson which mental faculty led him there. ‘See the value of imagination… We imagined what might have happened, acted upon that supposition, and find ourselves justified.’
Holmes takes an imaginative leap, not only into another human mind, but into the mind of an animal. This perspective-taking, being able to see the world from the point of view of another, is one of the central elements of empathy, and Holmes raises it to the status of an art.
Usually, when we think of empathy, it evokes feelings of warmth and comfort, of being intrinsically an emotional phenomenon. But perhaps our very idea of empathy is flawed. The worth of empathy might lie as much in the ‘value of imagination’ that Holmes employs as it does in the mere feeling of vicarious emotion. Perhaps that cold rationalist Sherlock Holmes can help us reconsider our preconceptions about what empathy is and what it does.
Though the scientific literature on empathy is complex, a recent review in Nature Neuroscience by a team of researchers from Harvard and Columbia including Jamil Zaki and Kevin Ochsner has distilled the phenomenon into three central stages. The first stage is ‘experience sharing’, or feeling someone else’s emotions as if they were your own — scared when they are scared, happy when they are happy, and so on. The second stage is ‘mentalising’, or consciously considering those states and their sources, and trying to work through understanding them. The final stage is ‘prosocial concern’, or being motivated to act — wanting, for example, to reach out to someone in pain. However, you don’t need all three to experience empathy. Instead, you can view these as three points on an empathetic continuum: first, you feel; then, you feel and you understand; and finally, you feel, understand, and are compelled to act on your understanding. It seems that the defining thing here is the feeling that accompanies all those stages.
Universal emotions like anger, sadness and happiness are expressed nearly the same in both music and movement across cultures, according to new research.
The researchers found that when Dartmouth undergraduates and members of a remote Cambodian hill tribe were asked to use sliding bars to adjust traits such as the speed, pitch, or regularity of music, they used the same types of characteristics to express primal emotions. What’s more, the same types of patterns were used to express the same emotions in animations of movement in both cultures.
“The kinds of dynamics you find in movement, you find also in music and they’re used in the same way to provide the same kind of meaning,” said study co-author Thalia Wheatley, a neuroscientist at Dartmouth University.
The findings suggest music’s intense power may lie in the fact it is processed by ancient brain circuitry used to read emotion in our movement.
“The study suggests why music is so fundamental and engaging for us,” said Jonathan Schooler, a professor of brain and psychological sciences at the University of California at Santa Barbara, who was not involved in the study. “It takes advantage of some very, very basic and, in some sense, primitive systems that understand how motion relates to emotion.”
Universal emotions
Why people love music has been an enduring mystery. Scientists have found that animals like different music than humans and that brain regions stimulated by food, sex and love also light up when we listen to music. Musicians even read emotions better than nonmusicians.
Past studies showed that the same brain areas were activated when people read emotion in both music and movement. That made Wheatley wonder how the two were connected.
To find out, Wheatley and her colleagues asked 50 Dartmouth undergraduates to manipulate five slider bars to change characteristics of an animated bouncy ball to make it look happy, sad, angry, peaceful or scared.
“We just say ‘Make Mr. Ball look angry or make Mr. Ball look happy,’” she told LiveScience.
To create different emotions in “Mr. Ball,” the students could use the slider bars to affect how often the ball bounced, how often it made big bounces, whether it went up or down more often and how smoothly it moved.
Another 50 students could use similar slider bars to adjust the pitch trajectory, tempo, consonance (repetition), musical jumps and jitteriness of music to capture those same emotions.
The students tended to put the slider bars in roughly the same positions whether they were creating angry music or angry moving balls.
To see if these trends held across cultures, Wheatley’s team traveled to the remote highlands of Cambodia and asked about 85 members of the Kreung tribe to perform the same task. Kreung music sounds radically different from Western music, with gongs and an instrument called a mem that sounds a bit like an insect buzzing, Wheatley said. None of the tribes’ people had any exposure to Western music or media, she added.
Interestingly, the Kreung tended to put the slider bars in roughly the same positions as Americans did to capture different emotions, and the position of the sliders was very similar for both music and emotions.
The findings suggest that music taps into the brain networks and regions that we use to understand emotion in people’s movements. That may explain why music has such power to move us — it’s activating deep-seated brain regions that are used to process emotion, Wheatley said.
“Emotion is the same thing no matter whether it’s coming in through our eyes or ears,” she said.
