The HP Team includes Bill Munroe and Kae Nemoto - who were both working at UQ when I was a student there. It's always great to see people I know in the news.
Read more at www.physorg.com/news953...
The best Physics Articles, Glossary and sites on the web including quantum physics, relativity philosophy of physics and biographies of famous physicists. A resource for homework help, worked physics problems and examples, physics discussion board, Resources for science teachers, Experiments that anyone can carry out, Resources for Teachers, Physicists, Worked problems and examples, electromagnetism, thermodynamics, quantum mechanics, experiments, physics experiments, physics humor.
Read more at www.physorg.com/news953...
Gaithersburg, Md.—Raw code for “unbreakable” encryption, based on the principles of quantum physics, has been generated at record speed over optical fiber at the Commerce Department’s National Institute of Standards and Technology (NIST). The work, reported today at the SPIE Defense & Security Symposium in Orlando, Fla., is a step toward using conventional high-speed networks such as broadband Internet and local-area networks to transmit ultra-secure video for applications such as surveillance.
The NIST quantum key distribution (QKD) system uses single photons, the smallest particles of light, in different orientations to produce a continuous binary code, or "key," for encrypting information. The rules of quantum mechanics ensure that anyone intercepting the key is detected, thus providing highly secure key exchange. The laboratory system produced this “raw” key at a rate of more than 4 million bits per second (4 million bps) over 1 kilometer (km) of optical fiber, twice the speed of NIST’s previous record, reported just last month. The system also worked successfully, although more slowly, over 4 km of fiber.
Read more at www.nist.gov/public_aff...
Light Pipes
6 April 2006 Funnelling daylight deep inside offices, factories and even homes is a challenge; dark corners are often too far away from the outside world for sunlight to penetrate. Now two resourceful groups in Brisbane and Sydney have devised ingenious methods for piping sunlight almost anywhere in a building, replacing the need for electrical lighting. These revolutionary inventions could save energy and reduce CO2 emissions, all courtesy of the sun
Read more at www.abc.net.au/catalyst...
A US researcher says the number of stupid mistakes made playing on the tennis court can be reduced by applying the laws of physics.
Professor Howard Brody of the University of Pennsylvania shows knowledge of the laws of matter and motion can lift a player's game in one of three main ways.
It can cut errors of latitude (hitting the ball wide), depth (hitting the net) and force (hitting the ball too hard), Professor Brody says in the current issue of the British Journal of Sports Medicine.
Australian Associate Professor of Physics Rod Cross of the University of Sydney has written a book on the science of tennis with Professor Brody.
He says physics can more accurately describe what happens when a player hits a ball than the player is aware of.
"The idea is that a physicist can tell a coach what the player's supposed to be doing and why, and the coach can translate that to a player," Professor Cross said.
"I tried it myself. I phoned up [professional tennis player] Jelena Dokic and told her she wasn't serving properly - she didn't hang up straight away."
Read more at www.abc.net.au/news/new...
The Showgirl, the Comic Strip and the Physicists
Monday 24 April 2006
Cross-dressing singers and The Beano are not the sorts of topics you'd expect to hear discussed at a physics conference. But that's exactly what will happen at the Institute of Physics in London on Monday 24 and Tuesday 25 April when the latest methods of conserving and digitising photographs and artworks will be described.
The two-day meeting on “Preservation and Conservation Issues Related to Digital Printing and Digital Photography” will bring together physicists, conservators and chemists from museums, universities and photographic companies. Participants will hear about the latest research into the longevity of digital prints and storage methods, which we are all increasingly using to document the important events in our lives, as well as the rise of digital reproductions of fine art, and what should be considered “an original”.
Read more at www.iop.org/news/1111
The American Institute of Physics Bulletin of Physics News
Number 774 April 19, 2006 by Phillip F. Schewe, Ben Stein, and
Davide Castelvecchi
INDICATIONS OF A CHANGE IN THE PROTON-TO-ELECTRON MASS RATIO have
shown up in comparisons of the spectra of hydrogen gas as recorded
in a lab with spectra of light coming from hydrogen clouds at the
distance of quasars. This is another of those tests of so-called
physical constants that might not be absolutely constant. For
example, the steadiness of the fine structure constant (denoted by
the letter alpha), defined as the square of the electron's charge
divided by the speed of light times Planck's constant, has been in
dispute (http://www.aip.org/pnu/1999/split/pnu410-1.htm ). Some
tests say it's changing, others say it isn't. This is an
important
issue since alpha sets the overall strength of the electromagnetic
force, the force that holds atoms together. Similarly, the
proton-to-electron mass ratio (denoted by the letter mu) figures in
setting the scale of the strong nuclear force. There is at present
no explanation why the proton's mass should be 1836 times that of
the electron's. The new search for a varying mu was carried out by
Wim Ubachs of the Vrije Universiteit Amsterdam. He and his
colleagues approach their task by studying hydrogen gas in the lab,
performing ultra-high-resolution spectroscopy in the
difficult-to-access extreme-ultraviolet range. This data is compared
to accurate observations of absorption spectra of distant hydrogen
(which absorbs light from even more distant quasars) as recorded
with the European Southern Observatory (ESO) in Chile. The
astronomical hydrogen is essentially hydrogen as it was 12 billion
years ago, so one can seek hints of a changing value for mu. Why
the comparison? Because the position of a particular spectral line
depends on the value of mu; locate the spectral line accurately
(that is, its wavelength) and you can infer a value for mu. In
this way, the researchers report that they see evidence that mu has
decreased by 0.002% over those 12 billion years. According to Ubachs
(wimu@nat.vu.nl, www.nat.vu.nl/~wimu ), the statistical confidence
of his spectroscopic comparison is at the level of 3.5 standard
deviations. (Reinhold et al., Physical Review Letters, 21 April
2006, laser website at www.nat.vu.nl/~laser )
NUCLEAR QUANTUM OPTICS. Normally the atomic realm, characterized by
an energy scale of electron volts or less, is very much removed from
the nuclear realm, where energy levels are measured in thousands and
millions of eV. Some laser interactions in nuclei can be achieved
indirectly by using light to create plasmas, whose secondary
particles either interact with nuclei or, in a tertiary step,
produce gamma rays which then influence nuclear states. Scientists
at the Max-Planck-Institut fur Kernphysik have now studied how
present and future x-ray laser facilities will make possible direct
laser intervention in the nucleus and how this will open up a new
branch of quantum optics. X-ray sources such as the TESLA device at
the DESY lab in Hamburg will not only deliver high-intensity,
high-energy beams but will, at least partially, consist of coherent
(laserlike) radiation. One doesn't need coherent light to excite a
nucleus, but coherence can be important in exercising greater
control over optical phenomena analogous to those in atomic
systems. Examples include exciting a complete population inversion
of the target nuclei or even producing some kind of nuclear
"electromagnetically induced transparency." One of the
researchers,
Thomas Burvenich (buervenich@fias.uni-frankfurt.de), says that an
additional benefit of nuclear quantum optics will be the direct
measurement of specific nuclear facts, such as nuclear dipole
moments and the energy levels of nuclei. (Burvenich et al.,
Physical Review Letters, 14 April 2006; lab website at
http://www.mpi-hd.mpg.de/keitel/evers/ )
The American Institute of Physics Bulletin of Physics News
Number 773 April 12, 2006 by Phillip F. Schewe, Ben Stein, and
Davide Castelvecchi
SHARPER FOCUSING OF HARD X RAYS has been achieved with a device
developed at Argonne National Lab. Because of their high energy, x
rays are hard to focus: they can be reflected from a surface but
only at a glancing angle (less than a tenth of a degree); they can
be
refracted but the index of refraction is very close to 1, so that
making efficient lenses becomes a problem; and they can be
diffracted, but the thick, variable pitch grating required for
focusing is tricky to achieve. The Argonne device is of the
diffraction type, and it consists of a stack of alternating layers
of metal and silicon, made by depositing progressively thicker
layers (see figure at http://www.aip.org/png/2006/258.htm ). When
the x rays fall on such a structure, nearly edge-on, what they see
is a grating pattern (called a linear zone plate) consisting of a
sort of bar-code pattern. The Argonne device succeeds so well in
focusing x rays because the position of the zones can be controlled
to within nanometer tolerances through the deposition process, and
the depth of the zones that the x rays experience can be made
arbitrarily long---microns long---by merely cutting a thicker
section of the multilayer wafer. In tests so far, one of these zone
plates, very slightly tilted to the x rays coming out of a
synchrotron source, has focused 20-keV x rays to a line only 30 nm
wide, better than previously possible. According to Argonne
researcher Brian Stephenson (stephenson@anl.gov, 630-252-3214), an
ideal version of this kind of x-ray lens, which they call a
Multilayer Laue Lens (MLL), should be able to focus x rays to a spot
of 1 nm or less. The likely uses for a better x-ray lens are in
full-field microscopy (making a magnified x-ray image of a sample)
or in scanning probe microscopy (by scanning the beam across a
sample). (Kang et al., Physical Review Letters, 31 March 2006)
NANO-EARTHQUAKES: ACOUSTIC WAVES EXCITE ARTIFICIAL MOLECULES. By
absorbing photons from a laser, an atom can be excited to any of
various discrete energy levels allowed by quantum mechanics. What
about artificial atoms? A quantum dot, created by the same
lithographic methods used to prepare electronic chips, is nearly a
zero-dimensional zone of semiconducting material; as with electrons
inside atoms, electrons inside the confinement of a quantum dot will
also possess only a restricted menu of allowed energies. The same
is true for a pair of quantum dots 200 nm apart; with just the right
voltage applied, electrons can tunnel from one dot to the other. In
fact, an electron, considered as a spread-out quantum wave
phenomenon, can be considered to reside in both dots at the same
time, a property which makes the quantum-dot "molecule"
potentially
useful for carrying out quantum computing operations.
Now, a group of scientists have been able to probe, and to change,
the quantum energy states of a double quantum dot with sound waves,
or more particularly surface acoustic waves excited in the substrate
supporting the dots. The acoustic waves, less than1 nm in
amplitude, ripple through the surface for distances as long as
hundreds of microns as a sort of nano-earthquake, are created
through the process of piezoelectricity; a small voltage is sent
into a series of tiny electrodes painted onto the surface. This
excites the faint acoustic waves (see figure at
http://www.aip.org/png/2006/259.htm ). The acoustic-dot
arrangement, mediated by the delicate interactions between electrons
and phonons, can work in both directions: the quantum dots can be
used to monitor the acoustic waves (which, because of their tiny
energy, are otherwise difficult to detect) or the acoustic waves can
be used to interrogate the electronic status of the dots, which
makes possible the aforesaid quantum-information applications. The
researchers involved work at the University of Twente and the Delft
University of Technology (Netherlands), NTT Corporation, Tokyo
Institute of Technology, and University of Tokyo (Japan), and Jilin
University (China). (Naber et al., Physical Review Letters, April 7
2006; contact Wouter Naber, W.J.M.Naber@utwente.nl)
Related Resources
Outrage at Attacks on NASA Science
The Universe in a Single Atom - The Convergence of Science and Spirituality
The Physics of Friendship
A Short History of Nearly Everything
Elsewhere on the Web
Understanding Evolution
Wired: The Crusade Against Evolution
Lawrence Krauss: Science Under Attack
In two reports today in the journal Nature, a team of scientists led by Neil H. Shubin of the University of Chicago say they have uncovered several well-preserved skeletons of the fossil fish in sediments of former streambeds in the Canadian Arctic, 600 miles from the North Pole.The skeletons have the fins, scales and other attributes of a giant fish, four to nine feet long. But on closer examination, the scientists found telling anatomical traits of a transitional creature, a fish that is still a fish but has changes that anticipate the emergence of land animals — and is thus a predecessor of amphibians, reptiles and dinosaurs, mammals and eventually humans.
In the fishes' forward fins, the scientists found evidence of limbs in the making. There are the beginnings of digits, proto-wrists, elbows and shoulders. The fish also had a flat skull resembling a crocodile's, a neck, ribs and other parts that were similar to four-legged land animals known as tetrapods."
There cna be no argument that this is a transitional fossil - removing one of the arguments used by anti-scientific "creationists." This article, by John Noble Wilford, is a commendable piece of science journalism - rather than trying to "find the other side" of evolution, he presents the evidence that exists. As Larry Krauss has recently stated, there is no other side to evolution.Read more at www.nytimes.com/2006/04... (free registration required)
Related Resources
AIP Physics News Articles
Antigravity with magnets and liquid nitrogen
Quantum Entanglement
Physics 101 - Basic Information
Elsewhere on the Web
Extensive Visuals and Explanations of Leidenfrost Experiments
Quantum Entanglement and Information
How Light Emitting Diodes Work
***********
PHYSICS NEWS UPDATE
The American Institute of Physics Bulletin of Physics News
Number 772 April 5, 2006 by Phillip F. Schewe, Ben Stein, and
Davide Castelvecchi
Related Resources
NASA - Ringside Seat to the Universe's First Split Second Moon Dust - Could Electrically Charged Dust Have Formed a Layer Around the Moon and Swallowed the Apollo Lander? Elsewhere on the Web NASA
Thirty-plus years ago on the moon, Apollo astronauts made an important discovery: Moondust can be a major nuisance. The fine powdery grit was everywhere and had a curious way of getting into things. Moondust plugged bolt holes, fouled tools, coated astronauts' visors and abraded their gloves. Very often while working on the surface, they had to stop what they were doing to clean their cameras and equipment using large--and mostly ineffective--brushes.
Dealing with "the dust problem" is going to be a priority for the next generation of NASA explorers. But how? Professor Larry Taylor, director of the Planetary Geosciences Institute at the University of Tennessee, believes he has an answer: "Magnets".
Read more at science.nasa.gov/headli...
Related Resources
Physics News
Black Holes
Microscopes
Elsewhere on the Web
Hundreds of Science Fair Projects for Students
Science Fair Central offers ideas for science fair projects and experiments
BLACK HOLE MERGER MOVIE. Accurate calculations of the gravitational waveforms emitted during the collision of black holes can now be made. A new computer study of how a pair of black holes, circling each other, disturbs the surrounding space and sends huge gusts of
gravitational waves outwards, should greatly benefit the experimental search for those waves with detectors like LIGO and LISA. The relative difficulty of computer modeling of complicated physical behavior depends partly on the system in question and on the equations that describe the forces at work. To describe the complicated configuration of charges and currents, one uses Maxwell's equations to determine the forces at work. In the case of black-hole binaries, the equations are those from Albert Einstein's theory of general relativity. Black holes encapsulate the ultimate in gravitational forces, and this presents difficulties for
computations attempting to model behavior nearby. Nevertheless, some physicists at the University of Texas at Brownsville have now derived an algorithm that not only produces accurate estimates of the gravity waves of the inspiraling black holes, even over the short time intervals leading up to the final merger, but also is
easily implemented on computers (see figures and movie at www.aip.org/png/2006/256.htm ). "The importance of this work," says
Carlos Lousto, one of the authors of the new study, "is that it gives an accurate prediction to the gravitational wave observatories, such as LIGO, of what they are going to observe." The new results are part of a larger study of numerical relativity carried out at the University of Texas, work referred to as the
Lazarus Project (http://www.phys.utb.edu/numrel/research_dir/lazarus.html ).
(Campanelli, Lousto, Marronetti, and Zlochower; Physical Review Letters, 24 March 2006; contact information, lousto@phys.utb.edu, 956-882-6651)
A SUBMERSIBLE HOLOGRAPHIC MICROSCOPE. A new device allows scientists to form 3D images of tiny marine organisms at depths as great as 100 m. The device allows the recording of behavioral characteristics of zooplankton and other marine organisms in their natural environment without having to bring specimens to the surface for examination. Scientists at Dalhousie University in Halifax, Canada, used the hologram arrangement originally invented by Denis Gabor: light from a laser is focused on a pinhole that acts as a point source of light if the size of the hole is comparable to the wavelength of light. The spherical waves that emanate from the
pinhole illuminate a sample of sea water. Waves scattered by objects in the sea water then combine at the chip of a CCD camera with un-scattered waves (the reference wave) from the pin hole to form a digitized interference pattern or hologram. The digital holograms are then sent to a computer where they are digitally
reconstructed with specially developed software to provide images of the objects. The Dalhousie researchers packaged their holography apparatus in such a way that the laser and digital camera parts are in separate watertight containers, while the object plane is left open (see figure at http://www.aip.org/png/2006/255.htm ). One
difficulty was to get container windows of optical quality that are thin enough for high resolution imaging but thick enough to resist sea pressure. The new submersible microscope can also record the trajectories of organisms in the sample volume so that movies of the swimming characteristics of micron size marine organisms can easily be produced. Holograms with1024 x 1024 pixels can be recorded at 7
to 10 frames/s. This requires a large bandwidth for data transmission to a surface vessel and was accomplished with water tight Ethernet cables. Imaging volumes can be several cubic centimeters depending on the desired resolution. The Gabor geometry
allowed the Dalhousie researchers to design a very simple instrument capable of wavelength limited resolution of marine organisms in their natural environment. Past generations of submersible holographic microscopes had lower resolution, weighed several tons, had to be deployed from large ships, and used high-resolution film
as the hologram recording medium. This meant that only a small number of holograms could be recorded. In contrast, the Dalhousie instrument only weighs 20 kg, can be deployed from small boats or even pleasure vessels, and can record thousands of holograms in a few minutes so that the motion of aquatic organisms can be captured
in detail. (Jericho et al., Review of Scientific Instruments, upcoming article; contact M.H. Jericho, Dalhousie University, jericho@fizz.phys.dal.ca, and also the Universidad Nacional de Columbia)
The American Institute of Physics Bulletin of Physics News
Number 771 March 29, 2006 by Phillip F. Schewe, Ben Stein, and
Davide Castelvecchi
Related Resources
Fluid
Elsewhere on the Web
Physics of Swimming
The Physics of Sport
The research will make use of the same software CSIRO uses for other fluid simulations such as animating water for movies and modelling volcanoes and tsunamis. Researchers are hoping to see some practical results in time to implement improvements for the London Olympics in 2012.
Read More at Virtual swimmer to speed up our athletes
Elsewhere on the Web
UQ Press Release
Bullet-Shaped SCRAMjet put to the Test - ABC Space and Astromony News
Scramjet Clocks Nearly Mach 10