Collider music November 10, 2009
Posted by apetrov in Funny, Near Physics, Particle Physics.add a comment
The Internet is “like a box of chocolates — you never know what you’re gonna get.” Apparently, colliders inspire songwriters of different styles: from educational rap to 60-style love songs… Enjoy…
Ginzburg November 9, 2009
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One of the most famous Russian physicists, 2003 Nobel Prize winner Vitaly L. Ginzburg died yesterday in Moscow. He was 94. He received his Nobel Prize “for pioneering contributions to the theory of superconductors and superfluids” (e.g. Landau-Ginzburg theory is taught in any statistical mechanics class). He was a truly universal physicist — with over 400 works in physics, radio-physics and astrophysics. He will be greatly missed.
2009 Nobel Prize in Physics October 6, 2009
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The 2009 Nobel Prize in Physics went to Charles K. Kao of Standard Telecommunication Laboratories Harlow (UK) “for groundbreaking achievements concerning the transmission of light in fibers for optical communication” and to Willard S. Boyle and George E. Smith of Bell Labs “for the invention of an imaging semiconductor circuit – the CCD sensor”. For more info see the announcement.
Another very applied Noble Prize – this time in optics. The first half is given for a low-loss optical fiber cables (he suggested fused silica as a material for fiber cables) — it is interesting that Nobel committee states that “An interesting example of the use of fiber-optic communication in science is the advanced fiber optics network developed at the Large Hadron Collider at CERN in Geneva that will transfer large amounts of information obtained by the particle detectors to computer centers all over the world.” I guess it is one way to connect fundamental physics with applied. Or maybe underline the importance of the very applied prize.
The second half of the prize is given for a device that is a heart of your digital camera (the charged-coupled device or CCD). The idea is simple — a CCD is a device that can record a picture by accumulating light-induced charges over its semiconductor surface, which can be read-off at the edge of the light sensitive area. Boyle and Smith invented those n 1970. Besides everyday use in small cameras, CCD’s are used, for instance, in the Hubble Space Telescope’s cameras to make great scientific discoveries.
Maybe next year the Nobel Committee can consider invention of cars and buses that take great scientists to work to make their discoveries or jet engines that are used in the airplanes that take them to the conferences where those results are discussed. Or maybe some ground-breaking technology in oil extraction that is used to fuel those engines that take those great scientists to work on their “fundamental projects.” Those inventions are definitely worthy of Nobel Prize in Physics. Stay tuned!
2009 Nobel week (which follows 2009 Ig Nobel) October 6, 2009
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Tomorrow (Oct 6) the 2009 Nobel prize in physics will be announced. Before that happens, I want to put my 2 cents in predicting it. Don’t worry, it never works for those kind of things, I should really leave my predictions to physics. But in case it works:
* My bet (drum roll…): Adam Reiss, Saul Perlmutter and Robert Kischner for discovery of accelerating Universe.
Now, apparently that totally contradicts predictions of Thompson Scientific, who claim the following:
===========================================
Who do you think will win the Nobel Prize in Physics?
Yakir Aharonov and
Sir Michael V. Berry – 24%
Juan Ignacio Cirac and
Peter Zoller – 27%
Andre K. Geim and
Kostya Novoselov – 14%
Sumio Iijima – 14%
Other – 20%
===========================================
But don’t worry, they never get it right either. Although I like the graphene idea for a Nobel Prize (Geim and Novoselov)…
P.S. The 2009 Ig Nobel prize in physics was given to Liza Shapiro, Kathleen Whitcome and Daniel Lieberman on why pregnant women don’t tip over. Actually, that paper was published in the journal Nature. Serious research (this is not a joke).
One day that started the arms race August 30, 2009
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There are two two days in the history of the world that started the (nuclear) arms race between the USA and the Soviet Union in the second half of the last century. The first day is July 16, 1945 — the day of the Trinity Test. The second one is August 29, 1949. So exactly 60 years ago today Soviet Union exploded its own atomic device (the so-called RDS-1 (“Rocket Engine of Stalin-1″), or Joe-1, as it was known in the West). Some of the brightest physicists of that time worked on the Manhattan Project and Soviet Atomic Project. Did the result save the world from another World War? Or paved the way for future political instabilities? Or simply gave us another source of energy? Time will tell. If you interested in the historico-technical side of this story, the model of that RDS-1 device is in the museum of nuclear weapons in Sarov.
LHC to start with 3.5 TeV beams August 6, 2009
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It looks like things at LHC are progressing quite fast. Last week, at DPF-2009, we heard a talk from Lyn Evans that LHC will start in November with energies “as close as possible to, but not above 5TeV” per beam. Now, Interactions.org reported that the start-up energy would be 3.5 TeV per beam. I’m curious how many physics projections will need to be updated for this first lower-energy scenario. And when LHC will ramp up to full 7 TeV x 7 TeV design energy…
DPF-2009 is underway! July 28, 2009
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The DPF-2009 conference started yesterday at Wayne State University in Detroit. This particular conference is close to my heart because I’m a chair of the Organizing Committee. And because of that I will not be able to report on my impressions of that conference — for one, I’m very much biased. Oh, and I’m also a bit busy with making sure that it runs smoothly.
So, we have a very nice program with a variety of talks — it started with the LHC machine status talk by Lyn Evans from CERN and will end on Friday with a talk by the Fermilab Director Pier Oddone. Please check our DPF-2009 website for the program of plenary and parallel sessions and other things (note that all of the talks are there thanks to the Indico system)! And for those readers, who are present at this conference — please do write about your impressions.
To infinity and beyond or to the Moon in back July 21, 2009
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Today (20 July that is) is a 40-year anniversary of people landing on the Moon. Incredible event? Absolutely! Useful? Well, it depends. But incredible nonetheless. There are plenty news stories and personal recollections that could be found on websites of any more-or-less major TV or radio stations. A nice source is, of course, Wikipedia – it has the whole story of Soviet-American competition on who gets there first.
It is interesting that Moon landing was not shown on TV in USSR or China in 1969. Of course, the technical capabilities for that were present, but, besides a handful space science and engineering specialists in TsUP (Flight Control Center), no one in USSR saw the Armstrong to step on the Moon. The whole Soviet program was classified — and it was later communicated to the people that Soviet automatic stations completed all needed research on the Moon. And that it was decided that there is no point in sending people there.
Guess what — some news agencies are still saying that! Here is the latest press-release from RIA Novosti (Russian Information Service) that says just that (here is the English translation). C’est la vie.
Meanwhile, here is a picture of the Soviet spacesuit Krechet that was supposed to be used on the Moon. This picture was taken at the Smithsonian National Air and Space Museum in Washington DC.

The image is rather large, I apologize to those of you with slower connection…
Physics rap is becoming popular… June 18, 2009
Posted by apetrov in Funny, Near Physics, Science.add a comment
Apparently, rapping about physics becomes increasingly popular. While major label producers are still not considering those for their star performers like Usher or Six Cents (?), physics rap star AlpineKat (widely praised for her recent single “LHCRap“) has released a new single. This time she tackles nuclear physics at NSCL, which is located at the Michigan State University. The piece actually made it to the New York Times and can be found here.
Would it bring more participants to DPF-2009?
CHARM-2009 May 22, 2009
Posted by apetrov in Particle Physics, Physics, Science.2 comments
I am at the CHARM-2009 conference in Leiman (a suburb of Heidelberg, Germany). This is the third charm conference that I’m participating in since the rebirth of the series in 2006. That year the conference was in Beijing and it finally made it to Germany by the way of Cornell University. All of those places have rich connections to charm (BESII/III experiment in Beijing, CLEO-c at Cornell and the upcoming PANDA at GSI just a short drive from Leimen). The conference is winding down, so I wanted to update you on what happened. Please see the talks posted on the website next week.
The program of talks has three days of plenary presentations. The first day is mainly devoted to hidden charm states, both conventianl and exotic. So everything you wanted to know about states from J/psi to X, Y, and Z was discussed. The second day is all about open charm states, with strong and electroweak studies of all of those with a main concentration on mixing of DDbar mesons and CP-violation. The topic continued today (during the third day), gradually moving to “future hardware” — i.e. how upcoming data from current BESIII and upcoming PANDA, LHCb, and SuperFlavor factories will change the world.
The first day had a lot of discussions on QCD studies with charmonia. The main reason one wants to study QCD with heavy quarkonium states is the fact that this is one of the simplest QCD systems, kina like positronium in QED. But unlike QED, QCD is much more complicated, so one can study quite non-trivial systems such as molecules built of heavy mesons that behave just like hidden charm states. The cool thing is that those things are actually experimentally observed!!! In fact, most of discoveries (not “anomalies” as in cosmic ray physics) done in the past seven years were done in charm systems.Pierre Artoisenet, Antonio Vairo, Gunnar Bali, Steve Olsen, Helmut Vogel,Kay Yi, Daniel Gamermann,Ruslan Chistov, and Claudia Patrigiani talked about various experimental and theoretical issues in quarkonium states. I wanted to mention that, according to Pierre Artoisenet, there problem of chamonium polarization in ppbar collisions has been solved. The problem is (was) that in non-relativistic QCD (NRQCD), at the leading order, one predicts that a J/psi state that is transvesely polarized. This comes from the fact that the dominant mechanism is gluon fragmentation to charm-anticharm pair — so J/psi retains polarization of a gluon, which is transverse (as gluon is a massless particle). Now the problem was that experiment (CDF) saw J/psi’s being quite an opposite condition – longitudinally polarized. So he claimed that at higher orders in QCD one gets new channels (new machainisms for J/psi production) that for some reason (?) makes J/psi polarized longtudinally. Steve Olsen reported a (yet another) new charmonium state, X(3915). It’s amazing that some years ago people talked about the fact that experimentally we see too few charmonium states. Now I think we have too many. Helmut Vogel pointed out an intersting problem in radiative decays of J/psi and psi(2s) into eta and eta’ mesons. In addition, charmonia production in heavy ion collisions was discussed by Carlos Lourenco, Hermine Woehri, and Peter Petreczky.
The second day was mainly about DDbar mixing. It is the last meson-antimeson mixing observed experimentally (in total agreement with theoretical predictions
). Tina Cartaro, Marko Staric, Paras Naik, Angelo di Canto gave talks on DDbar measurments from different experiments, AlanS chwartz gave an HFAG (Heavy Flavor Averaging Group) take on that — and provided us with most recent averages of mixing and CP-violating parametres. Ikaros Bigi and I gave theoretical reviews on mixing and CP-violation. Then it was an area of Dalitz plot analyses… It’s interesting that there are not so many people who know how to “work” Dalitz plots…
And today we talked about open charm exotic states. An interesting discussion came after Christoph Hanhart’s claims about mlecular nature of some states and Fulvia de Fazio’s statements about their “conventioal” nature. Leptonic and semileptonic decays of charm were also discussed, with the recent controvercy about f_Ds, the observation vs. lattice computation of leptonic decay constants… And then there are “machine” talks. BESIII was just over. What I also learned from Yifang Wang’s talk, besides the current status of BESSIII (they are slowly getting to their design lumnocity of 10^33 cm^-2 s^-1, now getting a third of it), is ajoke that they wanted to buy a beampipe in the US, but they wouldn’t sell it to them. I wonder why…