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  • November 4, 2010
  • 05:22 AM
  • 998 views

Nanotechnology on ice - novel lithography approach to nanodevice fabrication

by Michael Berger in nanowerk

Researchers at Harvard University have shown that nanostructures can be patterned with focused electron or ion beams in thin, stable, conformal films of water ice grown on silicon. They demonstrated ice lithography as a lithographic technique for patterning e.g. metal wires down to 20 nm wide. What's interesting about this technique is that patterning with ices of any condensed gas is a straightforward and practical process. Ice resist does not require spinning or baking. All processing and patterning steps can occur in a single evacuated chamber and be monitored at high resolution. The final removal of unexposed resist leaves minimal residues. Environmentally harmful solvents are not required and complete dry removal of the ice layer can be performed by in situ sublimation. Also, ice lithography makes it possible to nanopattern chemical modifications into silicon and other substrates. The team has now reported the successful application of ice lithography to the fabrication of nanoscale devices.... Read more »

Han, A., Vlassarev, D., Wang, J., Golovchenko, J., & Branton, D. (2010) Ice Lithography for Nanodevices. Nano Letters, 2147483647. DOI: 10.1021/nl1032815  

  • November 4, 2010
  • 05:07 AM
  • 993 views

A galaxy far, far away…

by Kelly Oakes in Basic Space

When we look up into the sky at night, we see stars (even in London I can usually spot a few!). But there haven’t always been stars and galaxies in the universe. In a period known as the dark ages – not to be confused with the other dark ages – there was no light [...]... Read more »

M. D. Lehnert, N. P. H. Nesvadba, J. -G. Cuby, A. M. Swinbank, S. Morris, B. Clement, C. J. Evans, M. N. Bremer, & S. Basa. (2010) Spectroscopic confirmation of a galaxy at redshift z. Nature. arXiv: 1010.4312v1

  • November 3, 2010
  • 02:03 PM
  • 824 views

Real-time holographic video displays could be near

by Joerg Heber in All That Matters

Holograms may seem like an original invention from some science fiction films. A famous scene often mentioned in this context is that from Star Wars where Princess Leia records an important holographic message, ending with the words “Help me, Obi-Wan Kenobi“. Such visions of holograms aren’t fiction. In a paper published in Nature, Nasser Peyghambarian, [...]... Read more »

Blanche, P., Bablumian, A., Voorakaranam, R., Christenson, C., Lin, W., Gu, T., Flores, D., Wang, P., Hsieh, W., Kathaperumal, M.... (2010) Holographic three-dimensional telepresence using large-area photorefractive polymer. Nature, 468(7320), 80-83. DOI: 10.1038/nature09521  

  • November 2, 2010
  • 05:04 PM
  • 1,030 views

Standing on the shoulders of tyrants

by Duncan Hull in O'Really?

There are at least two ways of looking at the history of Science: If we have seen farther it is by standing on the shoulders of giants. If we have seen farther it is by standing on the shoulders of tyrants. Take Isaac Newton for example, a giant whose shoulders we all stand on today. [...]... Read more »

  • November 2, 2010
  • 04:57 PM
  • 361 views

Cell Traction Forces Independent of Intracellular Biochemistry

by Michael Long in Phased

How may cell shape regulate cell adhesion and spreading, important to many physiological processes, independent of intracellular biochemistry? A predictive model has been developed by Christopher Lemmon (Duke University Medical Center, United States) and Lewis Romer (John Hopkins Medical Institutions, United States) to answer this question.... Read more »

  • November 2, 2010
  • 11:38 AM
  • 1,305 views

This Week in the Universe: October 26th – November 1st

by S.C. Kavassalis in The Language of Bad Physics

Astrophysics and Gravitation:
Hubble Tries to See into the Future
Illustration Credit: NASA, ESA, and G. Bacon (STScI), Science Credit: NASA, ESA, and J. Anderson and R. van der Marel (STScI)
From NASA, ESA, and J. Anderson and R. van der Marel (STScI):
The multicolor snapshot, at top, taken with Wide Field Camera 3 aboard NASA’s Hubble Space Telescope, captures the central region of the giant globular cluster Omega Centauri. All the stars in the image are moving in random directions, like a swarm of bees. Astronomers used Hubble’s exquisite resolving power to measure positions for stars in 2002 and 2006.
From these measurements, they can predict the stars’ future movement. The bottom illustration charts the future positions of the stars highlighted by the white box in the top image. Each streak represents the motion of the star over the next 600 years. The motion between dots corresponds to 30 years.
By precisely observing the stars in Omega Centauri, a 10 million star globular cluster within our galaxy, the NASA/ESA team has been able to predict the stars’ movements over the next 10,000 years.  Considering how many variables are in this system, this is an awfully impressive achievement.
For more, see Hubble Data Used to Look 10,000 Years into the Future.
High Energy Physics and Particles:
ANITA Balloon sees Cosmic Rays by Accident
Hoover, S., & et al. (2010). Observation of Ultrahigh-Energy Cosmic Rays with the ANITA Balloon-Borne Radio Interferometer Physical Review Letters, 105 (15) DOI: 10.1103/PhysRevLett.105.151101
Credit: Physical Review Letters » Covers » Vol. 105, Iss. 15- Locations of direct (black) and reflected (red) detection of ultrahigh energy cosmic ray events by the ANITA balloon experiment over Antarctica. The field of view is delineated by the dashed blue line.
From the abstract:
We report the observation of 16 cosmic ray events with a mean energy of 1.5×1019 eV via radio pulses originating from the interaction of the cosmic ray air shower with the Antarctic geomagnetic field, a process known as geosynchrotron emission. We present measurements in the 300–900 MHz range, which are the first self-triggered, first ultrawide band, first far-field, and the highest energy sample of cosmic ray events collected with the radio technique. Their properties are inconsistent with current ground-based geosynchrotron models.
The ANITA Experiment, while on the hunt for cosmic neutrinos, ended up seeing 16 exceptionally high energy cosmic ray events (particles with energy several orders of magnitude greater than those made in the LHC).  Accidental observations are always fun, especially when they suggest a new technique for observing known phenomena.  Perhaps radio interferometer equipped balloons will now be used to detect these rare cosmic ray events.
For more, see Antarctic balloon sees particles with a million times more energy than the Large Hadron Collider.
Confirmed Top Quark Observation in the LHC
CMS Collaboration (2010). First Measurement of the Cross Section for Top-Quark Pair Production in Proton-Proton Collisions at sqrt(s)=7 TeV arXiv arXiv: 1010.5994v1
Exciting news! The CMS Collaboration has published their first confirmed observations of top quark production at the LHC this week.  This is especially exciting because it means that we’ll be able to study top quarks in multi-TeV proton-proton collisions for the first time.  At the Tevatron, top quark pairs are mainly produced via quark-antiquark annihilation, while at the LHC top quark pair production is expected to be dominated by a gluon fusion process.  Thus, observing top quark production is crucial to our understanding of this new mechanism. This is an important step in the early physics program at the LHC, since, “many signatures of new physics models accessible at the LHC either suffer from top-quark production as a significant background or contain top quarks themselves.”
The US at the Large Hadron Collider Photo of the Week

Credit: US/LHC - Candidate W-boson decay to tau and neutrino in ATLAS
The US/LHC has started an Event of the Week flickr account, showcasing an exciting and beautiful particle event from the current LHC runs every week.  This weeks was a candidate W-boson decaying into a tau and a neutrino within the ATLAS detector!
General Relativity, Quantum Gravity, et al.:
Want to Learn More about Gauge Gravity?
Andrew Randono (2010). Gauge Gravity: a forward-looking introduction arXiv arXiv: 1010.5822v1
... Read more »

  • October 28, 2010
  • 01:24 PM
  • 738 views

Teaching new tricks to insulators

by Joerg Heber in All That Matters

    Insulators might seem pretty boring materials for an electronic device such as a computer memory, because by the very nature of their definition, they don’t conduct any electrical current. But some insulators show some pretty intriguing properties. Amongst them are the so-called ferroelectrics. A ferroelectric is a material where positive and negative electrical [...]... Read more »

  • October 27, 2010
  • 09:06 AM
  • 608 views

Graphene research at Cal: Close, but no Nobel

by Anna Goldstein in Berkeley Science Review Blog



Fans of the Nobel Prize in Physics know that this year's honors went to a pair of U.K.-based researchers for the discovery of graphene, a.k.a., The World's Thinnest Material. While neither winner has a significant connection to UC Berkeley (the last Cal professor to win the physics Nobel was George Smoot in 2006), many here in the physics department can rightly claim at least some stake in this year's prize. That's because graphene's discovery in 2004 sparked a huge burst of high-impact research around the globe, much of which has been influenced by the work of Berkeley scientists.

Continue reading →... Read more »

Zhou SY, Gweon GH, Fedorov AV, First PN, de Heer WA, Lee DH, Guinea F, Castro Neto AH, & Lanzara A. (2007) Substrate-induced bandgap opening in epitaxial graphene. Nature Materials, 6(10), 770-5. PMID: 17828279  

Son YW, Cohen ML, & Louie SG. (2006) Half-metallic graphene nanoribbons. Nature, 444(7117), 347-9. PMID: 17108960  

Son YW, Cohen ML, & Louie SG. (2006) Energy gaps in graphene nanoribbons. Physical Review Letters, 97(21), 216803. PMID: 17155765  

Zhang, Y., Brar, V., Girit, C., Zettl, A., & Crommie, M. (2009) Origin of spatial charge inhomogeneity in graphene. Nature Physics, 5(10), 722-726. DOI: 10.1038/nphys1365  

Levy N, Burke SA, Meaker KL, Panlasigui M, Zettl A, Guinea F, Castro Neto AH, & Crommie MF. (2010) Strain-induced pseudo-magnetic fields greater than 300 tesla in graphene nanobubbles. Science, 329(5991), 544-7. PMID: 20671183  

Girit, C., Meyer, J., Erni, R., Rossell, M., Kisielowski, C., Yang, L., Park, C., Crommie, M., Cohen, M., Louie, S.... (2009) Graphene at the Edge: Stability and Dynamics. Science, 323(5922), 1705-1708. DOI: 10.1126/science.1166999  

Zhang Y, Tang TT, Girit C, Hao Z, Martin MC, Zettl A, Crommie MF, Shen YR, & Wang F. (2009) Direct observation of a widely tunable bandgap in bilayer graphene. Nature, 459(7248), 820-3. PMID: 19516337  

  • October 26, 2010
  • 05:23 PM
  • 1,092 views

Groundbreaking method for computer simulation: Car-Parrinello Molecular Dynamics turns 25

by Olexandr Isayev in olexandrisayev.com

Twenty five years ago two budding scientists, Roberto Car and Michele Parrinello, used their expert knowledge, coupled with enthusiasm and a healthy dose of naivety, to develop a groundbreaking method for computer simulation. ... Read more »

Editorial. (2010) A model approach to modelling. Nature Materials, 9(9), 687-687. DOI: 10.1038/nmat2852  

Hafner, J. (2010) A joint effort with lasting impact. Nature Materials, 9(9), 690-692. DOI: 10.1038/nmat2838  

  • October 26, 2010
  • 11:24 AM
  • 1,119 views

This “Week” in the Universe: October 12th – October 25th

by S.C. Kavassalis in The Language of Bad Physics

Two weeks of news in one!
Astrophysics and Gravitation:
Did We Already Have the Data to Show Dark Matter Annihilation?
Dan Hooper, & Lisa Goodenough (2010). Dark Matter Annihilation in The Galactic Center As Seen by the Fermi Gamma Ray Space Telescope arXiv arXiv: 1010.2752v1
Analyzing old data from the Fermi Gamma Ray Space Telescope, the authors have noticed gamma ray emissions consistent with predictions for a certain type of dark matter.  Unfortunately, these things are never nice, clear problems where they’ve definitely seen dark matter or have definitely not seen it, but it’s an exciting collection of data points for astrophysicists who are on the dark matter hunt.  It could turn out to be the evidence that people have been looking for, but it’s too early to say anything definitively.
For more, see Signs of Destroyed Dark Matter Found in Milky Way’s Core, Fermilab theorist sees dark matter evidence in public data.
Weighing Planets with Pulsars
Champion, D., et al. (2010). MEASURING THE MASS OF SOLAR SYSTEM PLANETS USING PULSAR TIMING The Astrophysical Journal, 720 (2) DOI: 10.1088/2041-8205/720/2/L201
What can’t pulsars do? The team, using an array of pulsars (PSRs J0437–4715, J1744–1134, J1857+0943, J1909–3744), have identified the masses of the planetary system from Mercury to Saturn, in agreement with the best-known masses determined by spacecraft and other observations.  This new method relies on the incredibly predictable nature of pulsars and solar system ephemeris (the past and future positions of the Sun, Moon, and nine planets in three-dimensional space).
From the authors:
While spacecraft are likely to produce the most accurate measurements for individual solar system bodies, the pulsar technique is sensitive to planetary system masses and has the potential to provide the most accurate values of these masses for some planets.
Practical!
For more, see A New Way to Weigh Planets.
A New Standard Candle?
Poznanski, D., Nugent, P., & Filippenko, A. (2010). TYPE II-P SUPERNOVAE AS STANDARD CANDLES: THE SDSS-II SAMPLE REVISITED The Astrophysical Journal, 721 (2), 956-959 DOI: 10.1088/0004-637X/721/2/956
For years, Type Ia supernovae have been used as standard candles to measure cosmic distances; they were especially important for the measurements that determined that the expansion of the universe ws accelerating.  Now, some astrophysicists are suggesting that for even higher accuracy, we use Type II supernovae as well.  Initially, Type II supernovae weren’t used as standard candles because we weren’t as sure about their properties and actual brightness as we were for Type Ia supernovae.  Using additional markers to gauge cosmic distances could help confirm and strengthen current observations, as well as discover inconsistencies.
Adam Burrows, astrophysicist at Princeton University:
It is unlikely that this technique will be able to compete with Ia, but it can contribute complementary cosmic information. It is coming into its own.
For more, see Alternative yardstick to measure the universe.
Dark Matter in the Sun, Revisited
Lopes, I., & Silk, J. (2010). Neutrino Spectroscopy Can Probe the Dark Matter Content in the Sun Science, 330 (6003), 462-462 DOI: 10.1126/science.1196564
The abstract:
After being gravitationally captured, low-mass cold dark-matter particles (mass range from 5 to ~50 x 109 electron volts) are thought to drift to the center of the Sun and affect its internal structure. Solar neutrinos provide a way to probe the physical processes occurring in the Sun’s core. Solar neutrino spectroscopy, in particular, is expected to measure the neutrino fluxes produced in nuclear reactions in the Sun. Here, we show how the presence of dark-matter particles inside the Sun will produce unique neutrino flux distributions in 7Be- and 8B-, as well as 13N-, 15O-, and 17F-.
Finally, a credible sounding experiment to test this dark-matter-in-the-sun-hypothesis, discover that there is no cold dark matter in the sun, and convince people to stop taking things seriously just because they technically “could” be possible.  We’re not 100% sure of the consistency of the moon either, therefore I propose it’s full of anaerobic unicorns.
For more, see Neutrino Spectroscopy Can Probe the Dark Matter Content in the Sun.
New Oldest/Farthest Object in the Universe*
... Read more »

Champion, D., Hobbs, G., Manchester, R., Edwards, R., Backer, D., Bailes, M., Bhat, N., Burke-Spolaor, S., Coles, W., Demorest, P.... (2010) MEASURING THE MASS OF SOLAR SYSTEM PLANETS USING PULSAR TIMING. The Astrophysical Journal, 720(2). DOI: 10.1088/2041-8205/720/2/L201  

Lehnert, M., Nesvadba, N., Cuby, J., Swinbank, A., Morris, S., Clément, B., Evans, C., Bremer, M., & Basa, S. (2010) Spectroscopic confirmation of a galaxy at redshift z . Nature, 467(7318), 940-942. DOI: 10.1038/nature09462  

Raphael Bousso, Ben Freivogel, Stefan Leichenauer, & Vladimir Rosenhaus. (2010) Eternal inflation predicts that time will end. arXiv. arXiv: 1009.4698v1

Sabine Hossenfelder. (2010) Experimental Search for Quantum Gravity. arXiv. arXiv: 1010.3420v1

Henrique Gomes, Sean Gryb, & Tim Koslowski. (2010) Einstein gravity as a 3D conformally invariant theory. arXiv. arXiv: 1010.2481v1

  • October 25, 2010
  • 08:04 AM
  • 678 views

Meteorite tea, and the failures of genius

by Lab Lemming in Lounge of the Lab Lemming

In the early 1970’s, Io, the innermost large moon of Jupiter, was somewhat of an enigma. Unlike Europa and Ganymede, it did not exhibit water ice adsorption bands it its IR spectra. Its density suggested that it was a rock and metal planet, but the surface reflectance was unlike anything known to science. This problem was addressed brilliantly in a Science paper by Fanale, Johnson, and Matson,... Read more »

Fanale, F., Johnson, T., & Matson, D. (1974) Io: A Surface Evaporite Deposit?. Science, 186(4167), 922-925. DOI: 10.1126/science.186.4167.922  

  • October 22, 2010
  • 01:13 PM
  • 567 views

The State of Confined Water in the Ribosome Exit Tunnel

by Michael Long in Phased

Vijay Pande (Stanford University, United States) and coworkers have used computer simulations to show that water confined within the ribosome exit tunnel has unique properties, which may explain certain aspects of protein synthesis, and provide insight into how certain antibiotics work.... Read more »

Lucent, D., Snow, C. D., Aitken, C. E., & Pande, V. S. (2010) Non-Bulk-Like Solvent Behavior in the Ribosome Exit Tunnel. PLoS Computational Biology, 6(10). DOI: 10.1371/journal.pcbi.1000963  

  • October 22, 2010
  • 08:24 AM
  • 594 views

Geim and Novoselov Isolate Graphene, Win 2010 Nobel Prize in Physics

by A. Goldstein in WiSci

It is 100 times stronger than steel and the best heat conductor known to man. Most people have produced this substance unwittingly, yet it could be used to substantially improve computer chips, solar cells, and even satellites. What is this astonishing material? The first truly 2-dimensional crystalline material: graphene. This year, two pioneering physicists received [...]... Read more »

Tsoukleri, G., Parthenios, J., Papagelis, K., Jalil, R., Ferrari, A., Geim, A., Novoselov, K., & Galiotis, C. (2009) Subjecting a Graphene Monolayer to Tension and Compression. Small, 5(21), 2397-2402. DOI: 10.1002/smll.200900802  

  • October 22, 2010
  • 03:45 AM
  • 1,346 views

The Physics of Wet Dogs

by GrrlScientist in GrrlScientist

Dog owners no longer have to lay awake at night, wondering how rapidly a wet dog should oscillate its body to dry its fur. Presumably, dogs already know, and now, thanks to slo-mo photography, physicists know, too... Read more »

Andrew Dickerson, Grant Mills, Jay Bauman, Young-Hui Chang, & David Hu. (2010) The Wet-Dog Shake. Fluid Dynamics. info:/arxiv.org/abs/1010.3279

  • October 20, 2010
  • 03:33 AM
  • 390 views

Critical mass or is mass critical?

by Shaun Hendy in A Measure of Science







In research and development, it’s often taken for granted that teams require a certain critical mass to be successful.  Indeed, in a recent paper [1] two European researchers claim to have seen the effects of critical mass in the UK Research Assessment Exercise (RAE) and its French equivalent (HT: Mark Wilson).  However, I think that [...]... Read more »

Kenna, R., & Berche, B. (2010) The extensive nature of group quality. EPL (Europhysics Letters), 90(5), 58002. DOI: 10.1209/0295-5075/90/58002  

  • October 18, 2010
  • 12:00 PM
  • 1,105 views

Guest Post: The fine-structure constant is probably constant by Sean Carroll

by S.C. Kavassalis in The Language of Bad Physics

This is the first guest post on The Language of Bad Physics by Cosmic Variance‘s Sean Carroll.  This post is cross-posted on Cosmic Variance.
A few weeks ago there was a bit of media excitement about a somewhat surprising experimental result. Observations of quasar spectra indicated that the fine structure constant, the parameter in physics that describes the strength of electromagnetism, seems to be slightly different on one side of the universe than on the other. The preprint is here.
Remarkable, if true. The fine structure constant, usually denoted α, is one of the most basic parameters in all of physics, and it’s a big deal if it’s not really constant. But how likely is it to be true? This is the right place to trot out the old “extraordinary claims require extraordinary evidence” chestnut. It’s certainly an extraordinary claim, but the evidence doesn’t really live up to that standard. Maybe further observations will reveal truly extraordinary evidence, but there’s no reason to get excited quite yet.
Chad Orzel does a great job of explaining why an experimentalist should be skeptical of this result. It comes down to the figure below: a map of the observed quasars on the sky, where red indicates that the inferred value of α is slightly lower than expected, and blue indicates that it’s slightly higher. As Chad points out, the big red points are mostly circles, while the big blue points are mostly squares. That’s rather significant, because the two shapes represent different telescopes: circles are Keck data, while squares are from the VLT (“Very Large Telescope”). Slightly suspicious that most of the difference comes from data collected by different instruments.

But from a completely separate angle, there is also good reason for theorists to be skeptical, which is what I wanted to talk about. Theoretical considerations will always be trumped by rock-solid data, but when the data are less firm, it makes sense to take account of what we already think we know about how physics works.
The crucial idea here is the notion of a scalar field. That’s just fancy physics-speak for a quantity which takes on a unique numerical value at every point in spacetime. In quantum field theory, scalar fields lead to spinless particles; the Higgs field is a standard example. (Other particles, such as electrons and photons, arise from more complicated geometric objects — spinors and vectors, respectively.)
The fine structure constant is a scalar field. We don’t usually think of it that way, since we usually reserve the term “field” for something that actually varies from place to place rather than remaining constant, but strictly speaking it’s absolutely true. So, while it would be an amazing and Nobel-worthy result to show that the fine structure constant were varying, it wouldn’t be hard to fit it into the known structure of quantum field theory; you just take a scalar field that is traditionally thought of as constant and allow it to vary from place to place and time to time.
That’s not the whole story, of course, When a field varies from point to point, those variations carry energy. Think of pulling a spring, or twisting a piece of metal. For a scalar field, there are three important contributions to the energy: kinetic energy from the field varying in time, gradient energy from the field varying in space, and potential energy associated with the value of the field at every point, unrelated to how it is changing.
For the fine structure constant, the observations imply that it changes by only a very tiny bit from one end of the universe to the other. So we really wouldn’t expect the gradient energy to be very large, and there’s correspondingly no reason to expect the kinetic energy to matter much.
The potential energy is a different matter. The potential is similar to the familiar example of a ball rolling in a hill; how steep the potential is near its minimum is related to the mass of the field. For most scalar fields, like the Higgs field, the potential is extremely steep; this means that if you displace the field from the minimum of its potential by just a bit, it will tend to immediately roll back down.

A priori, we don’t know ahead of time what the potential should look like; specifying it is part of defining the theory. But quantum field theory gives us clues. At heart, the world is quantum, not classical; the “value” of the scalar field is actually the expectation value of a quantum operator. And such an operator gets contributions from the intrinsic vibrations of all the other fields that it couples to — in this case, every kind of charged particle in the universe. What we actually observe is not the “bare” form of the potential, but the renormalized value, which takes into account the accumulated effects of various forms of virtual particles popping in and out of the quantum vacuum.
The basic effect of renormalization on a scalar field potential is easy to summarize: it makes the mass large. So, if you didn’t know any better, you would expect the potential to be as steep as it could possibly be — probably up near the Planck scale. The Higgs boson probably has a mass of order a hundred times the mass of a proton, which sounds large — but it’s actually a big mystery why it isn’t enormously larger. That’s the hierarchy problem of particle physics.
So what about our friend the fine structure constant? Well, if these observations are correct, the field would have to have an extremely tiny mass — otherwise it wouldn’t vary smoothly over the universe, it would just slosh harmlessly around the bottom of its potential. Plugging in numbers, we find that the mass has to be something like 10-42 GeV or less, where 1 GeV is the mass of the proton. In other words: extremely, mind-bogglingly small.
But there’s no known reason for the mass of the scalar field underlying the fine structure constant to be anywhere near that small. This was established in some detail by Banks, Dine, and Douglas. They affirmed our intuition, that a tiny change in the fine structure constant should be associated with a huge change in potential energy.
Now, there are loopholes — there are always loopholes. In this case, you could possibly prevent those quantum fluctuations from renormalizing your scalar-field potential simply by shielding the field from interactions with other fields. That is, you can impose a symmetry that forbids the field from coupling to other forms of matter, or only lets it couple in certain very precise ways; then you could at least imagine keeping the mass small. That’s essentially the strategy behind the supersymmetric solution to the hierarchy problem.
Problem is, that route is a complete failure when we turn to the fine structure constant, for a very basic reason: we can’t prevent it from coupling to other fields, it’s the parameter that governs the strength of electromagnetism! So like it or not, it will couple to the electromagnetic field and all charged particles in nature. I talked about this in one of my own papers from a few years ago. I was thinking about time-dependent scalars, not spatially-varying ones, but the principles are precisely the same.
That’s why theorists are skeptical of this claimed result. Not that it’s impossible; if the data stand up, it will present a serious challenge to our theoretical prejudices, but that will doubtless goad theorists into being more clever than usual in trying to explain it. Rather, the point is that we have good reasons to suspect that the fine structure constant really is constant; it’s not just a fifty-fifty kind of choice. And given those good reasons, we need really good data to change our minds. That’s not what we have yet — but what we have is certainly more than enough motivation to keep searching.

... Read more »

J. K. Webb, J. A. King, M. T. Murphy, V. V. Flambaum, R. F. Carswell, & M. B. Bainbridge. (2010) Evidence for spatial varia. arXiv. arXiv: 1008.3907v1

  • October 17, 2010
  • 03:48 PM
  • 1,201 views

I’ve got you under my skin

by Joerg Heber in All That Matters

Take a piece of silicon, try to bend it and it will break. Stretch a thin film of gold and it will rupture. Conventional metals and semiconductors are brittle and not elastic at all. But these are properties that you need when you want to use electronic devices in unusual places and for unusual applications. [...]... Read more »

  • October 17, 2010
  • 03:06 PM
  • 1,006 views

How the stuff from sun lotions became one of the hottest materials in physics

by Joerg Heber in All That Matters

  Even if you don’t know much about this compound, everybody is familiar with zinc oxide (ZnO). It is a white powder used as the UV-light absorbing component in many sun lotions (and the part of the sun lotion that leaves those white marks on clothes), as an antibacterial agent in some baby powders, in [...]... Read more »

Tsukazaki, A., Akasaka, S., Nakahara, K., Ohno, Y., Ohno, H., Maryenko, D., Ohtomo, A., & Kawasaki, M. (2010) Observation of the fractional quantum Hall effect in an oxide. Nature Materials. DOI: 10.1038/nmat2874  

  • October 12, 2010
  • 03:13 PM
  • 1,073 views

The kind of experimentalist I like

by Andrew Sun in On The Road

Boukany, P., Hemminger, O., Wang, S., & Lee, L. (2010). Molecular Imaging of Slip in Entangled DNA Solution Physical Review Letters, 105 (2) DOI: 10.1103/PhysRevLett.105.027802 About the paper Prof. Shiqing Wang (王十庆) have long been interested in observing the event … Continue reading →... Read more »

Boukany, P., Hemminger, O., Wang, S., & Lee, L. (2010) Molecular Imaging of Slip in Entangled DNA Solution. Physical Review Letters, 105(2). DOI: 10.1103/PhysRevLett.105.027802  

  • October 11, 2010
  • 06:59 PM
  • 1,148 views

This Week in the Universe: October 5th – October 11th

by S.C. Kavassalis in The Language of Bad Physics

Astrophysics and Gravitation:
Early Universe was Overheated, says NASA
Michael Shull, Kevin France, Charles Danforth, Britton Smith, & Jason Tumlinson (2010). Hubble/COS Observations of the Quasar HE 2347-4342: Probing the Epoch of He II Patchy Reionization at Redshifts z = 2.4-2.9 arXiv arXiv: 1008.2957v1
Credit: NASA/Michael Shull, University of Colorado
From the Press Release:
During a period of universal warming 11 billion years ago, quasars — the brilliant core of active galaxies — produced fierce radiation blasts that stunted the growth of some dwarf galaxies for approximately 500 million years.  This important conclusion comes from a team of astronomers that used the new capabilities of NASA’s Hubble Space Telescope to probe the invisible, remote universe. The team’s results will be published in… The Astrophysical Journal.
For more, see Hubble Astronomers Uncover an Overheated Early Universe.
Dark Matter, Neutron Stars, and Strange Quark Matter, Oh My!
Perez-Garcia, M., Silk, J., & Stone, J. (2010). Dark Matter, Neutron Stars, and Strange Quark Matter Physical Review Letters, 105 (14) DOI: 10.1103/PhysRevLett.105.141101
The abstract:
We show that self-annihilating weakly interacting massive particle (WIMP) dark matter accreted onto neutron stars may provide a mechanism to seed compact objects with long-lived lumps of strange quark matter, or strangelets, for WIMP masses above a few GeV. This effect may trigger a conversion of most of the star into a strange star. We use an energy estimate for the long-lived strangelet based on the Fermi-gas model combined with the MIT bag model to set a new limit on the possible values of the WIMP mass that can be especially relevant for subdominant species of massive neutralinos.
For more, see Does dark matter trigger strange stars?.
High Energy Physics and Particles:
Hey, this isn’t research news!
Yeah, it’s not… But, for anyone who will be in Manchester from October 23rd – 27th, 2010 should make sure they check out Super K Sonic Booooum!
This large installation consists of a 22 meter long ‘river’ of water running through a tunnel lined with thousands of silver balloons (photomultiplier tubes). Members of the public embark on a boat, pulled through the tunnel on a submerged track using a pulley system, with sound and lighting effects, and with an expert particle physicist navigator as a guide. On the journey they learn of neutrinos, their role in the Universe and how scientists detect them. All crew members must first don white Tyvek suits, wellies and hard hats or else face the wrath of Nelly the security chief, at the entrance of the tunnel. This installation is designed to deliver physically thrilling experiences; emerging the audience on a journey through the physics of the Universe.
Workshop on Sunday 24 October – 2pm – 4pm
Capture the Invisible: Craft and Science in particle physics.
In this workshop you will get the chance to make your own photomultiplier tube to capture the invisible in your own bedroom! Designed by Nelly Ben Hayoun in collaboration with Dr Jonathan Perkin, physicist and glassblower Jochen Holz
For more, see Super K Sonic Booooum.
SuperB Project Preparing for Construction!
SuperB Collaboration, E. Grauges et al., Francesco Forti, Blair N. Ratcliff, & David Aston (2010). SuperB Progress Reports — Detector arXiv arXiv: 1007.4241v1
It looks like funding for the SuperB Collaboration will come through and see the new experiment built in Frascati.  I hope the Italians take this great opportunity to make many “flavour country” jokes.
From the press release:
The most elementary components of matter, quarks and leptons, have been found, as the result of 100 years of research, to be organized into three replicating “families”. The reason for this specific number or organization remains a full mystery. Flavor physics, the detailed understanding of the relationship between these families and the comparison between properties of matter and antimatter, is one of the most promising ways to explore new physics, quite complementary to the energy frontier research most notably pursued at the CERN LHC collider. Different kinds of new physics have different effects on rare decays of bottom and charmed quarks and of heavy tau leptons. These particles are all produced at SuperB in unparalleled abundance, making possible for the first time measurements of the precision required to be sensitive to the details of new physics uncovered at CERN.
For more, see SuperB project moves forward, preparing for construction.
Bonner Nuclear Lab to Study Quark-Gluon Plasma
Credit: Frank Geurts/Rice University
It was a good week to get funding for high-energy experiments.
From the Press Release:
Rice University’s Bonner Nuclear Lab has won a $1.175 million grant that will support its research on high-density and hot nuclear matter.  Rice physicist Frank Geurts, who has spent his career looking for clues to the basic elements of the universe by smashing the nuclear contents of gold, lead and other heavy atoms, said the Department of Energy grant will facilitate his group’s transition from constructing and commissioning a highly complex detector system to using that machinery to do basic research.
Video: Quark gluon plasma (QGP)
For more, see Grant advances quark-gluon ... Read more »

Michael Shull, Kevin France, Charles Danforth, Britton Smith, & Jason Tumlinson. (2010) Hubble/COS Observations of the Quasar HE 2347-4342: Probing the Epoch of He II Patchy Reionization at Redshifts z . arXiv. arXiv: 1008.2957v1

Perez-Garcia, M., Silk, J., & Stone, J. (2010) Dark Matter, Neutron Stars, and Strange Quark Matter. Physical Review Letters, 105(14). DOI: 10.1103/PhysRevLett.105.141101  

SuperB Collaboration, E. Grauges et al., Francesco Forti, Blair N. Ratcliff, & David Aston. (2010) SuperB Progress Reports -- Detector. arXiv. arXiv: 1007.4241v1

Gary Felder, & Stephanie Erickson. (2010) CurvedLand: An Applet for Illustrating Curved Geometry without Embedding. arXiv. arXiv: 1010.1426v1

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