Archive for the ‘Physics’ Category

Shortest LHC FAQ Ever

Wednesday, September 10th, 2008

The Large Hadron Collider reached a major milestone today with the first beam sent down the pipe, but like most interesting things, a lot of the Internet chatter is revolving around fundamental misconceptions.  I’d like to clear those up briefly:

Q: Does this prove the LHC won’t kill everyone?

A: No, this was a 450 GeV beam test without beam-on-beam collisions.  Nothing even close to the LHC design energy was reached.  No new evidence was given on the doomsday question today, as these energies were reached 20 years ago.

Q: So, the LHC will kill us?

A: No, this is a silly idea that keeps getting news play because it sounds like a good science-fiction plot and leverages the evil scientist stereotype for dramatic effect.  The LHC is not going to make new particles as far as the universe is concerned; it is going to make particles in a controlled environment that we probably haven’t documented before.  There is a difference.

Q: Is the LHC awesome?

A: Yes.

Four Languages

Saturday, May 31st, 2008

Inspired by the Slashdot story, Programming as Part of a Science Education?, I have to agree with the author, mostly. These days, every scientist and engineer should be fluent in four kinds of languages:

  1. Verbal: English still works, but the way things are going, Mandarin Chinese is becoming a useful #2.
  2. Pictorial: Each field has its own way to visualize information. In physics, the art of the histogram is paramount.
  3. Mathematical: Calculus the most relevant language for most sciences, but the language of graph theory and abstract algebra can be handy in some niches.
  4. Computational: FORTRAN was king for a while, and C++ is the current king, but on a very slow decline. Personally, I think all scientists would benefit from learning Python first, and then supplement with whatever compiled language is used by their colleagues.

Some people might argue that the first two are languages, and the second two are tools, but I disagree. Both math and programming are ways to express ideas, one symbolic and one procedural. (Unless you do your data analysis in PROLOG, in which case you are impressively loony.) On the physics experiment I work on, our 15-year-old simulation program (woo FORTRAN!) is in many respects the most precise, unambiguous description of how our experiment actually functions. Sure there are piles of words, plots, and equations also documenting everything, but sometimes when I want to know something behaves, I go straight for the code and read it.

In effect, we have built a procedural description of our particle detector, and it is worth recognizing the code as a form of communication. It certainly changes the way you think about programming.

G4TessellatedSolid and G4ExtrudedSolid are broken

Wednesday, November 7th, 2007

Update: This bug has been fixed in GEANT 4.9.1, released on December 14, 2007. Go get it!

Apologies to people reading this (all 3 of you) who don’t care about the GEANT4 simulation library.

I’m pitching this out there in the hopes that Google will index it and help some confused physicist:

G4TessellatedSolid, and therefore the subclass G4ExtrudedSolid, are broken in GEANT 4.9, and most likely earlier releases as well. Geometry optimization (which is enabled in G4LogicalVolume by default) requires the voxelizer to divide the detector geometry into rectangular regions in order to speed up tracking. The voxel generator needs to be able to determine which volumes in your detector overlap with each voxel region. To do this, it calls the G4Tessellated::CalculateExtent() (or G4ExtrudedSolid::CalculateExtent()) passing in an affine transformation describing the solid’s current orientation in the global coordinate system.

The implementation of CalculateExtent() first checks for the easy case, which is a transformation that is pure translation, and behaves correctly in that case. However, if the current transformation has any rotation component at all, then the if statement takes the other branch which is empty! The method obviously does not behave correctly in that case, and the voxelizer will give you nutty results, including mysteriously appearing, disappearing, or clipped volumes.

This problem is now being tracked as bug #983 in the GEANT4 bug database. The workaround is to either disable optimization in the parent G4LogicalVolume of your tessellated or extruded solids, or to patch the G4TessellatedSolid::CalculateExtent() method as described in the bug report.

Always remember to visualize your GEANT4 detector volumes with the raytracer, or you might not catch problems like this!pornstar karina
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Torrents of hep-th!

Wednesday, July 27th, 2005

It looks like Joanna Karczmarek at Harvard has set up a BitTorrent tracker serving up the hep-th arXiv papers. The main set of papers goes from 1991 (the start) up through March 2005, a total of 8 GB of PDFs. Since completing the download myself earlier in the day, I haven’t had anyone download from me. I guess these aren’t exactly hot items. :)

For those of you who don’t know what I’m talking about, the arXiv is a massive, free online repository of research papers (technically “pre-prints,” but in this age when software never gets out of beta, a pre-print is almost as good as the real thing). It did for physics pretty much what SourceForge did for open source software. There are different categories on the arXiv (still pronounced “arr-kive”) with cryptic abbreviations like “hep-th” or “gr-qc”. hep-th is the theoretical physics section, and is pretty busy these days. I see about 20-30 papers announced in each nightly update email. Interestingly enough, it’s become fairly common to post papers to the arXiv at the same time that you send them to journals for publication. As a result, quite a lot of serious published research (and not just random articles that no one peer reviewed) is in there. Not a bad catch for your hard drive.

Now we just need a torrent for hep-ex (experimental physics)….

Quantum Gravity and Background Independence

Tuesday, July 26th, 2005

Just finished reading a fascinating paper by Lee Smolin posted last night on the arXiv:

The case for background independence: hep-th/0507235.

While the paper is occassionally too jargon-laden for us non-quantum gravity researchers to follow, most of it is a very clearly written review of how our view of the “background” impacts the way we do physics. It’s really quite a journey, starting from the classic arguments between Newton and Leibniz about absolute vs. relational notions of space and time. Space and time were just early forms of “the background,” which is anything static and unchanging in your theory. We’ve moved from space and time separately, to spacetime, to fixing the dimensionality and topology of space, and so on. Field theories not only live in a fixed spacetime background, but also have conserved charges related to symmetries on a background. Fixed masses and coupling constants are all backgrounds in the Standard Model.

Smolin’s major point is that moving from background dependent to background independent theories is going to be necessary to address the problems of quantum gravity AND will lead to more predictive theories. You need only wander into one of the heated discussions on string theory that physicists frequently have to see that what we could really use is some falsifiable predictions paired with some data.

The philosophy of science aspect of this paper is a nice change from relentless pummelling of your subject with complex math you usually find on the arXiv. Not that I am complaining about math, of course. It serves as a nice anchor to prevent the hot air in your philosophies from carrying you off to crackpot-land.

One unexpected gem in the paper was the discussion of how the notion of background-independence relates to natural selection. Smolin even lays out a (very sketchy) description of what natural selection might look like when applied to cosmology. In his words (from page 35 of the paper):

  • The space of parameters is the space of parameters of the standard models of physics
    and cosmology. This is the analogue of phenotype. At a deeper level, this is to be
    explained by a space analogous to genotypes such as the space of possible string
    theories. This leads to the term the string theory landscape.
  • The mechanism of reproduction is the formation of black holes. It is long conjec-
    tured that black hole singularities bounce, leading to the formation of new universes
    through new big bangs. There is increasing evidence that this is true in loop quan-
    tum gravity.
  • We may conjecture that the low energy parameters do change in such a bounce.
    There are a few calculations that support this.
  • The mechanism of differentiation is that universes with different parameters will
    have different numbers of black holes.

He finishes this discussion by pointing out that this isn’t just idle speculation, but actually can lead to testable predictions. One prediction which he mentions is that no neutron star can have a mass bigger than 1.6 times the mass of our sun, and the largest neutron star observed so far is 1.45 solar masses. How exactly this prediction is made is a mystery to me, but he does cite another paper of his, hep-th/0407213, for more details.
(Disclaimer: This is far from an accepted theory, but is just an interesting idea that should be investigated.)

Overall, there were too many big ideas in this paper for me to absorb in one reading. It will take a couple passes to get it, I think. :)

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