Physics Archives

May 5, 2008December 24, 2015 by Ian O'Neill

Digging for Dark Matter: The Large Underground Xenon (LUX) Detector

The Hubble Space Telescope distribution of dark matter - indirect observations (HST)

How do you catch a WIMP? No, I’m not talking about bullying the weakest kid in class, I’m talking about Weakly Interacting Massive Particles (those WIMPs). Well, it isn’t easy. Although they are “massive” by definition, they do not interact with the electromagnetic force (via photons) so they cannot be “seen” and they do not interact with the strong nuclear force, so they cannot be “felt” by atomic nuclei. If we cannot detect WIMPs via these two forces, how can we possibly ever hope to detect them? After all, WIMPs are theorized to be flying through the Earth without hitting anything, they are that weakly interacting. But sometimes, they might collide with atomic nuclei but only if they collide head-on. This is a very rare occurrence, but the Large Underground Xenon (LUX) detector will be buried 4,800 feet (1,463 meters, or nearly a mile) underground in an old South Dakota goldmine and scientists are hopeful that when an unlucky WIMP bumps into a xenon atom, a flash of light will be captured, signifying the first ever experimental evidence of dark matter…

Galaxies observed from Earth have some strange qualities. The biggest problem for cosmologists has been to explain why galaxies (including the Milky Way) appear to have more mass than can be observed by counting stars and accounting for interstellar dust alone. In fact, 96% of the Universe’s mass cannot be observed. 22% of this missing mass is thought to be held in “dark matter” (74% is held as “dark energy”). Dark matter is theorized to take on many forms. Massive Astronomical Compact Halo Objects (astronomical bodies containing ordinary baryonic material that cannot be observed; like neutron stars or orphaned planets), neutrinos and WIMPS all are thought to contribute toward this missing mass. Many experiments are in progress to detect each contributor. Black holes can be indirectly detected by observing the interactions in the centre of galaxies (or gravitational lensing effects), neutrinos can be detected in huge tanks of fluid buried deep underground, but how can WIMPs be detected? It seems a WIMP detector needs to take a leaf out of the neutrino detector’s books – it needs to start digging.

To avoid interference from radiation such as cosmic rays, low energy detectors such as neutrino “telescopes” are buried well below the Earth’s surface. Old mine shafts make ideal candidates as the hole is already there for the instrumentation to be set up. Neutrino detectors are huge containers of water (or some other agent) with highly sensitive detectors positioned around the outside. One such example is the Super Kamiokande neutrino detector in Japan which contains a vast amount of ultra-purified water, weighing in at 50,000 tons (pictured left). As a weakly interacting neutrino hits a water molecule in the tank, a flash of Cherenkov radiation is emitted and a neutrino is detected. This is the basic principal behind the new Large Underground Xenon (LUX) detector that will use 600 pounds (272 kg) of liquid xenon suspended in a 25 foot high tank of pure water. If WIMPs exist beyond the realms of theory, it is hoped that these weakly interacting massive particles will collide head-on with a xenon atom, and like their light-weight cousins, emit a flash of light.

Robert Svoboda and Mani Tripathi, UC Davis professors, have secured $1.2 million in National Science Foundation (NSF) and U.S. Department of Energy funding for the project (this is 50% of the total required). When compared with the Large Hadron Collider (LHC) costing billions of Euros to build, LUX is a highly economic project considering the scope of what it might discover. Should there be experimental evidence of a WIMP interaction, the consequences will be enormous. We will be able to begin to understand the origins of WIMPs and their distribution as the Earth sweeps through the possible dark matter halo that is indirectly observed to exist in the Milky Way.

Detecting dark matter “would be the biggest deal since finding antimatter in the 1930s.” – Professor Mani Tripathi, LUX co-investigator, UC Davis.

The gold mine in South Dakota was closed in 2000 and in 2004 work began to develop the site into an underground laboratory. LUX will be the first large experiment to be housed there. It is hoped that the installation will start late summer, after water has been pumped out of the mine.

Original source: UC Davis News

April 23, 2008December 24, 2015 by Ian O'Neill

Solar Sail Space Travel One Step Closer to Reality

An artist concept of the solar sail. The center package contains the solar panels powering an electron gun that keeps the many tethers charged. (Allt om vetenskap)

Solar sails were once thought to belong in the realms of science fiction. Huge canopies of lightweight tin foil catching the solar photon breeze, slowly allowing spacecraft to cruise around our solar system propelled by the small but continuous radiation pressure. Recent years however have shown that solar sail spacecraft could be engineered in reality, and a new solar sail invention from the Finnish Meteorological Institute could push this goal one step closer. Rather than using solar radiation pressure, this new concept makes use of the highly charged particles in the solar wind to give the craft its propulsion. Additionally, through radio wave electron excitation, the system may amplify the solar wind acceleration effects, giving the spacecraft a “boost” function…

Traditionally, solar sails make use for the momentum carried by photons of electromagnetic radiation from the Sun. Using a huge canopy of ultra-lightweight (but robust) material, the sail experiences a force from the incident sunlight. Some advanced concepts also theorized the use of planetary lasers to propel solar sail-powered spacecraft from A to B. Opting for solar propulsion would be the ultimate energy conservation method yet, optimizing payload transportation, maximizing fuel efficiency. Make a solar sail big enough, steady momentum can be transferred from the solar photons, accelerating the spacecraft. There are of course many hurdles to this design, but prototypes have been built (although many failed to make it into space due to rocket launch failures).

In a departure from the photon-powered solar sail, scientists and engineers have started to look into the properties of solar wind particles as a possible source of propulsion. The advantages of using solar wind particles are they a) are electrically charged, b) have high velocity (interplanetary scintillation observations have deduced velocities as high as 800 km/s, or 1.8 million miles per hour), and c) are abundant in interplanetary space throughout the solar system (particularly at solar maximum). So the new Finnish concept will take full advantage of this highly charged interplanetary medium. Using a fan of very long, electrically charged cables (stretching many kilometres from the central spacecraft), the similarly charged solar wind particles (mainly positively-charged protons) will hit the fan of positively-charged cables (generating a repulsive electric field), giving the cables a small proton-sized “kick”, exchanging their momentum into spacecraft thrust. Cable charge is maintained by a solar-powered electron gun, using two conventional solar panels as an energy source. A radio-frequency “boost” will also be tested in the prototype model. Radio waves will cause electron heating, possibly enhancing the solar sail’s thrust.

The project is currently being engineered and researchers from Finland, Germany, Sweden, Russia, and Italy are currently developing various components of the solar sail. Successful implementation of the prototype that could be launched in three years depends on securing $8 million (5 million euros) in funding.

Sources: Finnish Meteorological Institute, Live Science

April 22, 2008December 24, 2015 by Fraser Cain

Will the Large Hadron Collider Destroy the Earth?

Question: Will the Large Hadron Collider Destroy the Earth?

Answer: No.

As you might have heard in the news recently, several people are suing to try and get the Large Hadron Collider project canceled. When it finally comes online, the LHC will be the largest, most powerful particle accelerator ever constructed.

If there’s something wrong with it, the LHC might have the power to damage itself, but it can’t do anything to the Earth, or the Universe in general.

There are two worries that people have: black holes and strange matter.

One of the goals of the Large Hadron Collider is to simulate microscopic black holes that might have been generated in the first few moments of the Big Bang. Some people are worried that these artificial black holes might get loose, and then consume the Earth from within, eventually moving on to destroy the Solar System.

The physicists are confident that any black holes they create will evaporate almost instantaneously into a shower of particles. In fact, the theories that predict that black holes can be created also predicts that black holes will evaporate. The two concepts go hand in hand.

The other worry is that the Large Hadron Collider will create a theorized material called strangelets. This “strange matter” would then be able to infect other matter, turning the entire planet into a blog of strange matter.

This strange matter is completely theoretical, and once again, the same theories that say it might be produced in the Large Hadron Collider also rule out any risks from it.

One of the most important considerations is the fact that the Moon is struck by high energy cosmic rays that dwarf the power of the Large Hadron Collider. They were likely blasted out of the environment around a supermassive black hole.

These have been raining down on the Moon for billions of years, and so far, it hasn’t turned into a black hole or strange matter.

You can read more about the Large Hadron Collider lawsuit here. Or how it might create wormholes, a view into other dimensions, or unparticles.

April 21, 2008December 24, 2015 by Ian O'Neill

X-Ray Flare Echo Reveals Supermassive Black Hole Torus

The echo of X-ray emissions from a black hole swallowing a star can be observed as light echos (MPE/ESA)

The light echo of an X-ray flare from the nucleus of a galaxy has been observed. The flare almost certainly originates from a single star being gravitationally ripped apart by a supermassive black hole in the galactic core. As the star was being pulled into the black hole, its material was injected into the black hole accretion disk, causing a sudden burst of radiation. The resulting X-ray flare emission was observed as it hit local stellar gases, producing the light echo. This event gives us a better insight to how stars are eaten by supermassive black holes and provides a method to map the structure of galactic nuclei. Scientists now believe they have observational evidence for the elusive molecular torus that is thought to surround active supermassive black holes.

Light echoes from distant galaxies have been observed before. The echoes from a supernova that occurred 400 years ago (that is now observed as the supernova remnant SNR 0509-67.5) were only just observed here on Earth, after the supernova emissions bounced off galactic matter. This is the first time however that the energetic emissions from a sudden influx of matter into a supermassive black hole accretion disk has been observed echoing off gases within galactic nuclei. This is a major step toward understanding how stars are consumed by supermassive black holes. Additionally, the echo acts like a searchlight, highlighting the dark stellar matter between the stars, revealing a structure we have never seen before.

This new research was carried out by an international team led by Stefanie Komossa from the Max Planck Institute for extraterrestrial Physics in Garching, Germany, using data from the Sloan Digital Sky Survey. Komossa likens this observation to illuminating a dark city with a firework burst:

“To study the core of a normal galaxy is like looking at the New York skyline at night during a power failure: You can’t learn much about the buildings, roads and parks. The situation changes, for example, during a fireworks display. It’s exactly the same when a sudden burst of high-energy radiation illuminates a galaxy.” – Stefanie Komossa

A strong X-ray burst such as this can be very hard to observe as they are short-lived emissions, but a huge amount of information can be gained by seeing such an event if astronomers are quick enough. By analysing the degree of ionization and velocity data in the spectroscopic emission lines of the echoed light, the Max Planck physicists were able to deduce the flare location. Held within the emission lines are the cosmic “fingerprints” of the atoms at the source of the emission, leading them to the galactic core where a supermassive black hole is believed to live.

The standard model for galactic nuclei (a.k.a. unified model of active galaxies) predict a “molecular torus” surrounding the black hole accretion disk. These new observations of the galaxy named SDSSJ0952+2143 appear to show the X-ray flare was reflected by the galactic molecular torus (with strong iron emission lines). This is the first time the presence of a possible torus has been seen, and if confirmed, astrophysicists will have their observational evidence of this theoretical possibility, strengthening the standard model. What’s more, using accretion disk flares may aid scientists when attempting to map the structure of other molecular toruses.

Strengthening the observation of echoed X-ray emission from the torus is the possibility of seeing variable infrared emissions. This emission signifies a “last call for help” by the dusty cloud being rapidly heated by the incident X-rays. The dust will have been vaporized soon after.

But how do they know it was a star that fell into the accretion disk? In addition to the strong iron lines, there are strange hydrogen emission lines which have never been seen before. This is a strong piece of evidence that it is the debris from a star that came too close to the black hole, stripping away its hydrogen fuel.

Although the X-ray flare has subsided, the galaxy continues to be observed by the X-ray satellite Chandra. Faint but measurable X-ray emissions are being observed perhaps signifying that the star is still being fed to the accretion disk. It seems possible that measuring this faint emission may also be of use, allowing researchers to continue to map the molecular torus long after the initial strong X-ray emission has ended.

Sources: arXiv, Max Planck Institute for Extraterrestrial Physics

April 16, 2008December 24, 2015 by Nancy Atkinson

Inflation Theory Takes a Little Kick in the Pants

Inflation theory proposes that the universe underwent a period of exponential expansion right after the Big Bang. One of the key predictions of inflation theory is the presence of a particular spectrum of “gravitational radiation”â€”ripples in the fabric of space-time that are really hard to detect but thought to exist. But a team of researchers has now found that gravitational radiation can be produced by a mechanism other than inflation. So this type of radiation, if eventually detected, wonâ€™t provide the conclusive evidence for inflation theory that was once was thought to be a certainty.

“If we see a primordial gravitational wave background, we can no longer say for sure it is due to inflation,” said noted astronomer Lawrence Krauss, from Case Western Reserve University.

Inflation theory first was proposed by cosmologist Alan Guth in 1981 as a means to explain some features of the universe that had previously baffled astronomers, such as why the universe is so close to being flat and why it is so uniform. Today, inflation remains the best way to theoretically understand many aspects of the early Big Bang universe, but most of the theoryâ€™s predictions are somewhat vague enough that even if the predictions were observed, they probably wouldnâ€™t provide a clear-cut confirmation of the theory.

But gravitational radiation was considered one of the key predictions of inflation theory, and detection of this spectrum was regarded among physicists as “smoking gun” evidence that inflation did in fact occur, billions of years ago.

Gravitational radiation is a prediction of Einstein’s Theory of General Relativity. According to the theory, whenever large amounts of mass or energy are shifting around, it disrupts the surrounding space-time and ripples emanate from the region where the shift occurs. These ripples arenâ€™t easily detected, but there is one experiment designed to look directly for this radiation, the Laser Interferometer Gravitational Wave Observatory (LIGO) in Livingston, Louisiana. The upcoming Planck Mission, set to launch in 2009 will look for it indirectly by looking at the cosmic microwave background.

Until now it was widely believed that detecting gravitational radiation in the form of polarized light from the CMB would confirm inflation theory, since it was thought inflation would be the only way this radiation could be produced. But Krauss and his team have raised the issue of whether this radiation can be unmistakably tied to inflation.

Kraussâ€™s team proposes that a phenomenon called “symmetry breaking,” can also produce gravitational radiation. Symmetry breaking is a central part of fundamental particle physics, where a system goes from being symmetrical to a low energy state that is not symmetrical. Kraussâ€™s explanation is that a “scalar field” (similar to an electric or magnetic field) becomes aligned as the universe expands. But as the universe expands, each region over which the field is aligned comes into contact with other regions where the field has a different alignment. When that happens the field relaxes into a state where it is aligned over the entire region and in the process of relaxing it emits gravitational radiation.

This is all fairly confusing, but the sweetened condensed version is that if gravitational radiation is ever detected, that event wonâ€™t necessarily verify inflation theory. Therefore, whether inflation theory can ever be confirmed remains to be seen.

Kraussâ€™s paper “Nearly Scale Invariant Spectrum of Gravitational Radiation from Global Phase Transitions” is published in the Aprill 2008 Physical Review Letters.

Original News Source: Case Western Reserve University press release

April 16, 2008December 24, 2015 by Ian O'Neill

The Pioneer Anomaly: A Deviation from Einstein Gravity?

Artist impression of the Pioneer 10 probe (NASA)

Both Pioneer probes are approximately 240,000 miles (386,000 km) closer to the Sun than predicted by calculation. Scientists have been arguing over the cause of this mysterious force for a decade and reasons for the Pioneer anomaly range from the bizarre to the sublime. Is it a simple fuel leak, pushing the probes of course? Is it phantom dark matter dragging them down? Or do the gravity textbooks need to be re-written? Unfortunately there’s still no one answer, but some researchers believe there might be a small deviation in the large-scale space-time Einstein described in his famous theory of general relativity. See, I knew there would be a simple explanation…

The Pioneer 10 and 11 deep space probes were launched in 1972 and 1973, visiting Jupiter and Saturn before pushing on toward interplanetary space, into the unknown. The Pioneer program really lived up to its name, pioneering deep space exploration. But a few years on, as the probes passed the through the 20-70 AU mark, something strange happened… not suddenly, but gradually. Ten years ago Pioneer scientists noticed that something was wrong; the probes were slightly off course. Not by much, but both were experiencing a slight but constant sunward acceleration. The Pioneer probes had been measured some 240,000 miles (386,000 km) closer to the Sun than predicted. This might sound like a long way, but in astronomical terms it’s miniscule. 240,000 miles is a tiny deviation after 6.5 billion miles (10.5 billion km) of travel (it would take light 10 hours to cover this distance), but it’s a deviation all the same and physicists are having a very hard time trying to work out what the problem is.

That is until NASA physicist Slava Turyshev, co-discoverer of the anomaly, rescued a number of Pioneer magnetic data storage disks from being thrown out in 2006. These disks contain telemetric data, temperature and power readings that both Pioneer probes had transmitted back to mission control up to 2003 (when Pioneer 10 lost contact with Earth). From this, Turyshev and his colleagues teamed up with Viktor Toth, a computer programmer in Ottawa, Ontario, to design a new code designed to extract the vast quantity of raw binary code (1s and 0s), revealing the temperature and power readings from the crafts instruments. It sounds as if the search for the culprit of the Pioneer anomaly required a bit of forensic science.

Now the researchers have a valuable tool at their disposal. Turyshev and 50 other scientists are trying to match this raw data with modelled data in an effort to reconstruct the heat and electricity flow around the craft’s instrumentation. Electricity was supplied by the on-board plutonium generator, but this is only a small portion of the energy generated; the rest was converted to heat, lost to space and warmed up the probe’s bodywork. Heat lost to space and warming of the probe’s instruments are both thought to have a part to play in altering spacecraft momentum. So could this be the answer?

Tests are ongoing, and only a select few simulations have been run. However, early results indicate that around 30% of the Pioneer anomaly is down to the on-board heat distribution. The rest, it seems, still cannot be explained by probe dynamics alone. The team are currently processing a total of 50 years of telemetry data (from both Pioneer 10 and 11), so more simulations on the rich supply of transmissions from the probes may still uncover some surprises.

But on the back of everyone’s mind, and it keeps cropping up in every Pioneer anomaly article I find, that the fundamental physics of our universe may need to be brought into question. Sending long-distance deep space probes gives us a huge opportunity to see if what we observe locally is the same for other parts of the Solar System. Could Einstein’s general theory of relativity need to be “tweaked” when considering interplanetary (or interstellar) travel?

The researchers are excited if a mundane solution does not present itself (i.e. probe heat distribution effects), therefore indicating some other cosmic reason is behind this anomaly:

“If we actually had a means in the solar system here to measure deviations from Einstein’s gravity, that would be phenomenal.” – Viktor Toth

In the mean time, Pioneer 10 is drifting silently toward the red star of Aldebarran and (barring any more anomalous behaviour) will arrive there in 2 million years time…

Sources: Scientific American, Symmetry Breaking News

April 14, 2008December 24, 2015 by Ian O'Neill

What was Before the Big Bang? An Identical, Reversed Universe

The Big Bounce Theory — Graphic of the Big Bounce concept (Relativity4Engineers.com)

So what did exist before the Big Bang? This question would normally belong in the realms of deep philosophical thinking; the laws of physics have no right to probe beyond the Big Bang barrier. There can be no understanding of what was there before. We have no experience, no observational capability and no way of travelling back through it (we can’t even calculate it), so how can physicists even begin to think they can answer this question? Well, a new study of Loop Quantum Gravity (LQG) is challenging this view, perhaps there is a way of looking into the pre-Big Bang “universe”. And the conclusion? The Big Bang was more of a “Big Bounce”, and the pre-bounce universe had the same physics as our universe… just backwards… Confused? I am…

LQG is a tough theory to put into words, but it basically addresses the problems associated with the incompatibilities behind quantum theory and general relativity, two crucial theories that characterize our universe. If these two theories are not compatible with each other, the search for the “Theory Of Everything” will be hindered, disallowing gravity to merge with the “Grand Unified Theory” (a.k.a. the electronuclear force). LQG quantizes gravity, thereby providing a possible explanation for gravity and a possible key to unlocking the Theory Of Everything. However, from the outset, LQG has many critics as there is little direct or indirect evidence backing up the theory.

See the previous Universe Today article on Loop Quantum Gravity»

Regardless, much work is being done into this area of research. The primary consequence to come from LQG is that it predicts that the Big Bang which occurred 13.7 billion years ago was actually a “Big Bounce”; our universe is therefore the product of a contracting universe before the Big Bang. The previous universe (or our universe “twin”) contracted to a single point (which could be interpreted as a “Big Crunch”) and then rebounded in a Big Bounce to produce the Big Bang as we’ve learned to accept as the birth of the universe as we know it. But until now, although the pre-bounce universe has been predicted, its characteristics could not be known. No information about the pre-bounce universe could be observed in today’s universe, the Big Bounce causes a “cosmic amnesia”, destroying all information of the previous universe.

Now, physicists Alejandro Corichi from Universidad Nacional AutÃ³noma de MÃ©xico and Parampreet Singh from the Perimeter Institute for Theoretical Physics in Ontario are working on a simplified Loop Quantum Gravity (sLQG) theory where they approximate the value of the “quantum constraint”, a key equation in the LQG theory. What happens next is a little surprising. From their calculations, it would appear that a universe, identical to our own, with identical mechanics, existed before the Big Bounce.

“…the twin universe will have the same laws of physics and, in particular, the same notion of time as in ours. The laws of physics will not change because the evolution is always unitary, which is the nicest way a quantum system can evolve. In our analogy, it will look identical to its twin when seen from afar; one could not distinguish them.” – Parampreet Singh

We are not talking about an alternate dimension; we are talking about an identical universe with the same space-time and quantum characteristics as our own. If we look at our universe now (13.7 billion years post-bounce), it would be identical to the universe 13.7 billion years before the Big Bounce. The only difference being the direction of time would be opposite; the pre-bounce universe would be reversed.

“In the universe before the bounce, all the general features will be the same. It will follow the same dynamical equations, the Einstein’s equations when the universe is large. Our model predicts that this happens when the universe becomes of the order 100 times larger than the Planck size. Further, the matter content will be the same, and it will have the same evolution. Since the pre-bounce universe is contracting, it will look as if we were looking at ours backward in time.” – Parampreet Singh

Analysing what happened before the Big Bang is only part of the story. By making this approximation of a key LQG equation, Singh and Corichi are working on models where galaxies and other physical structures leave an imprint in the pre-bounce universe to influence the post-bounce universe. Would these structures be distributed in similar ways? Will the structures in one universe be similar or identical to structures in the other universe? There may also be an opportunity to look into the future of this universe and predict whether the conditions are right for another Big Bounce (once can imagine repeated bounces, producing a cycle of universes).

For now, this research is highly theoretical and any observational evidence will remain sparse for the time being. Although this is the case, it does begin to probe the big question and may push physics a bit closer toward describing what existed before the Big Bang…

Source: Physorg.com

April 11, 2008April 26, 2016 by Ian O'Neill

Shortest Single-Photon Pulse Generated: Implications for Quantum Communications in Space

Equipment used by Oxford scientists to produce the pulses (Oxford Uni.)

Scientists at Oxford University have developed a method to generate the shortest ever single-photon pulse by removing the interference of quantum entanglement. So how big are these tiny record-breakers? They are 20 microns long (or 0.00002 metres), with a period of 65 femtoseconds (65 millionths of a billionth of a second). This experiment smashes the previous record for the shortest single-photon pulse; the Oxford photon is 50 times shorter. While this sounds pretty cool, what is all the fuss about? How can these tiny electromagnetic wave-particles be of any use? In two words: quantum computing. And in an additional three words: quantum satellite communications…

Quantum entanglement is a tough situation to put into words. In a nutshell: If a photon is absorbed by a type of material, two photons may be re-emitted. These two photons are of a lower energy than the original photon, but they are emitted from the same source and therefore entangled. This entangled pair is inextricably linked; regardless of the distance they are separated. Should the quantum state of one be changed, the other will experience that change. In theory, no matter how far away these photons are separated, the quantum change of one will communicated to the other instantly. Einstein called this quantum phenomenon “spooky action at a distance” and didn’t believe it possible, but experiment has proven otherwise.

So, in a recent publication, the Oxford group are trying to remove the entangled state of photons, this experiment isn’t about using this “spooky action”, it is to get rid of it. This is to remove the interference caused when one of the photon pair is detected. Once one of the twins is detected, the quantum state of the other is altered, contaminating the signal. If this effect can be removed, very short-period “pure” photons can be generated, heralding a new phase of quantum computing. If scientists have very definite, identical single photons at their disposal, highly accurate information can be carried with no interference from the quirky nature of quantum physics.

“Our technique minimises the effects of this entanglement, enabling us to prepare single photons that are extremely consistent and, to our knowledge, have the shortest duration of any photon ever generated. Not only is this a fascinating insight into fundamental physics but the precise timing and consistent attributes of these photons also makes them perfect for building photonic quantum logic gates and conducting experiments requiring large numbers of single photons.” – Peter Mosley, Co-Investigator, Oxford University.

The Oxford University blog reporting this news highlights how useful these regimented photons will be to quantum computing, quantum communications in space could also be a major benefactor. Imagine sending pulses of quantum-identical photons through space, to satellites at first, later through interplanetary space. Space scientists will have an extremely powerful resource so data can be sent though the vacuum, encrypted in a small number of photons, indecipherable to everything other than its destination…

Source: University of Oxford

April 10, 2008December 24, 2015 by Fraser Cain

Podcast: Wave Particle Duality

Have you ever heard that photons behave like both a particle and a wave and wondered what that meant? It’s true. Sometimes light acts like a wave, and other times it behaves like a little particle. It’s both. This week we discuss the experiments that demonstrate this, explain how scientists figured it all out in the first place. What does wave/particle duality have to do with astronomy? Well, everything, since light is the only way astronomers can see out into the Universe.

Click here to download the episode

Wave Particle Duality – Show notes and transcript

Or subscribe to: astronomycast.com/podcast.xml with your podcatching software.

March 28, 2008December 26, 2015 by Ian O'Neill

Hawaiian Man Files Lawsuit Against the Large Hadron Collider (LHC)

The Large Hadron Collider (LHC) is set to go online in May of this year. This magnificent machine will accelerate particles and collide them at such high energies that scientists expect to make some of the biggest discoveries ever about the very small (exotic sub-atomic particles) and the very large (the structure of the Universe itself).

But not everyone is happy. Particle accelerators have always been the source of controversy; at the end of the day, we can only predict the outcome of the LHC experiments. But what if scientists have overlooked something? What if the theories are wrong? A guy living on the other side of the planet to the LHC believes the world may come to an end and he’s begun filing a lawsuit against the completion of the accelerator. The concern? A massive black hole might be created, or vast amounts of antimatter will destroy the Earth. And where’s the scientificÂ basis for allÂ this panic? Hmmm… didn’t think so…

Through fear that the LHC is going to unleash death and destruction on the world, Walter Wagner from Hawaii has filed a lawsuit against an impressive array of defendants. The U.S. Department of Energy, the Fermilab particle-accelerator near Chicago, CERN and the National Science Foundation (NSF) are all named.

Wagner and his associate Luis Sancho have a pretty dubious (and quite frankly, weak) argument against the LHC, as they describe in the lawsuit:

“The compression of the two atoms colliding together at nearly light speed will cause an irreversible implosion, forming a miniature version of a giant black hole. […] Any matter coming into contact with it would fall into it and never be able to escape. Eventually, all of earth would fall into such growing micro-black-hole, converting earth into a medium-sized black hole, around which would continue to orbit the moon, satellites, the ISS, etc.” Walter F. Wagner and Luis Sancho lawsuit, filed in U.S. District Court in Honolulu.

There is no evidence to suggest that colliding particles will create a black hole that will swallow the planet. I do however like their description that the International Space Station will continue to orbit the Earth-mass black hole – at least we’ll have somewhere to hide as the rampaging black hole eats the ground from under us!

The credentials of the plaintiffs are also pretty sketchy. Wagner has worked in nuclear medicine and has a minor degree in physics from Berkley, but he has nothing more advanced than that. His colleague Sancho has an even more sketchy physics background.

Wagner wants the opening of the LHC to be delayed until further safety studies are carried out. Its cases like these that scientists have had to combat for many years. Unfounded predictions of the “end of the world” and fear of the unknown have been published only to be debunked through correct scientific thinking. If the world listened to alarmists such as Wagner and co, weÂ would advance no further.

I for one hope that the LHC does produce micro-black holes. I hope that this time next year we’ll be looking in awe at images of particle tracks from the sensors at the LHC showing the point of creation and the point of evaporation of micro-black holes. Peering very closely we see particle emission as if from nowhere, the evaporating particles from the tiny event horizon. The image will be entitled Hawking Radiation Experiment.

Even if the accelerator energies are not high enough to create mini-black holes, thereby giving Stephen Hawking some experimental evidence for his radiation, we are pretty sure we’ll find some other exotic and exciting particles to help us understand our universe a little bit better. We might gain a better grasp of other dimensions, detect some exotic particles, and lets not forget the possibility of discovering the Higgs Boson.

If we give into the fear of the unknown, scientific advancement will be stopped in its tracks and we may be restricted to scratching at the surface of space-time and string theory, rather than physically proving its existence with tools like the LHC.

Source: FOXnews.com