• USLHC
  • USLHC
  • USA

Latest Posts

  • Frank
  • Simon
  • MPI for Physics
  • Germany

Latest Posts

  • Aidan
  • Randle-Conde
  • USLHC
  • USA

Latest Posts

  • TRIUMF
  • Vancouver, BC
  • Canada

Latest Posts

  • Richard
  • Ruiz
  • UW - Madison
  • U.S.A.

Latest Posts

  • Byron
  • Jennings
  • TRIUMF
  • Canada

Latest Posts

  • Seth
  • Zenz
  • USLHC
  • USA

Latest Posts

  • Anna
  • Phan
  • USLHC
  • USA

Latest Posts

  • Alexandre
  • Fauré
  • CEA/IRFU
  • FRANCE

Latest Posts

  • Jim
  • Rohlf
  • USLHC
  • USA

Latest Posts

  • Zoe Louise
  • Matthews
  • ASY-EOS
  • UK

Latest Posts

  • Ken
  • Bloom
  • USLHC
  • USA

Latest Posts

Posts Tagged ‘astrophysics’

Turtles all the way down?

Tuesday, March 20th, 2012

I recently got an interesting e-mail about the Big Bang. The writer said she didn’t see how you could make something out of nothing. She collects creation myths and thought that, no matter how you sliced it, it’s always “turtles all the way down.” This is a reference to creation myths where the world is poised on top of a turtle, which is itself poised on top of something else, but raises the issue: Is there any firm ground?

This is worth addressing because it illustrates the gulf between the understandings in people’s minds about the Big Bang on one hand, and how physicists deal with it on the other. To be clear – we have a wealth of observations that support the Big Bang, but you have to be careful. We can only look back into the universe to a moment 300,000 years after the ‘start,’ as best we can discern it. At this early moment, the universe went from being opaque to transparent. Before this moment, ionized gas kept light from traveling any distance, but once protons and electrons cooled enough to form neutral hydrogen, light (photons) could travel long distances. The remnant photons from this time are seen as the so-called cosmic microwave radiation. These photons were first observed by Arno Penzias and Robert Wilson in the 1960’s and continues to be a rich source of information about the early universe.

What do we see? We see galaxies moving away from each other. The further away we look, the faster they appear to recede. Einstein’s gravity has a number of solutions for possible universe structures. One of these solutions describes the expanding universe very well, and, if taken at face value, would extrapolate back in time to an initial state when all matter in the universe existed as a single point of infinite density. But, does a point of infinite density make sense? The author of the e-mail question thinks not, that it’s like pulling a rabbit out of the hat. You can’t make something from nothing, and this apparent absurdity invalidates the Big Bang model.

The main issue is that, although our observations are very consistent with this model of a Big Bang universe, we cannot actually see the initial moment. It’s hidden from view. We strongly suspect that the laws of physics might change dramatically when distances scales and energy densities approach the conditions very close to initial moment. We know that when the classical laws of physics are combined with quantum mechanics, new phenomena emerge. This was the case of our theory of electromagnetism. When we incorporated quantum mechanics with electromagnetism, the phenomenon of anti-matter became apparent. We have yet to find a satisfactory theory of gravity that combines quantum mechanics. The manifestations of quantum mechanics in gravity will only emerge at extremely high energy densities, such as those in the very early universe, near the time of this infinite density, and will likely modify our current models. For all we know, space-time might resemble some Escher print, eluding the concept of an infinite density starting point through a twisted configuration that folds in on itself.

Rather than dealing with a concept that seems almost theological in nature, physicists try to reconcile models against data. We fully realize that our models will extrapolate to conditions that raise difficult issues, like infinite densities. More often than not, the difficult conditions are something we avoid talking about, because, largely, we cannot really test or measure these. If it is inaccessible, it is inaccessible. The work can be perhaps more likened to the work of explorers. Our job is to map new territories, and, if anything, we can only report on territories we’ve explored. What lies beyond the horizon is a matter of speculation.
Responses? Questions? Contact me on Twitter @JohnHuth1

Can We “Point” the LHC, Too?

Wednesday, January 28th, 2009

The Bad Astronomy blog is publicizing a chance to choose what the Hubble Space Telescope looks at.  The basic idea is that there’s going to be an internet vote between six objects that Hubble has never looked at, and Hubble will be pointed at the winner and send out pictures of it by April.  It seems like a fun way to get the public to learn more about, and feel more involved in, the Hubble project.

I’ll let you read more details at one of the links above, but I have another question to consider: can we do something similar with the LHC? That is, could we put up some kind of page where people could vote on what kind of physics we would study over the course of some particular week?  Maybe a choice between searching for Supersymmetry, or a high-mass Higgs boson, or a low-mass Higgs boson?  At first glance, the answer would seem to be “no.”  We obviously have no control over what kind of physics happens when the protons of the LHC collide — we just look at what comes out.  And it seems unlikely that any physicist would volunteer to put their work hours into a particular analysis because of a public vote, and anyway we’ll have people working on all the high-profile analyses and many low-profile ones besides.

But there actually is a sense in which ATLAS or CMS could to something similar.  Remember that our detectors can only record a few hundred events every second, out of the almost forty million times the beams cross during that second.  There are lots of collisions we have to throw out because we can’t store enough data, and it’s the trigger system that decides which few we keep.  In practice, there are a number of different signals that we program the trigger system to be interested in: we take a certain number of random low-energy events to help us calibrate what we see in our other events, and we have separate “trigger paths” for hadronic jets, for muons, for electrons, and so on.  We try to record all the events that might represent interesting new physics, but as the collision rate at the LHC increases, we’ll have to throw away even some of those.  When the committee meets to decide how to balance the different possible triggers, what is at issue is precisely which kinds of events the detector will “point at,” i.e. recognize as important and save.  People with different interests in terms of physics might make different choices about how to achieve that balance, and every study would always love more trigger bandwidth if it were available, and that’s why we have committees to argue about it in the first place.

So why not reserve 5% of the ATLAS or CMS trigger bandwidth for a public vote on what physics to look for, to give a little extra oomph to one study or another?  Actually, I can think of several good and practical reasons why not — but it’s fun to think about!

Big Explosions

Sunday, May 25th, 2008

Hubble Telescope image of the Crab NebulaNow that I’ve gotten your attention with the entry title, I of course have to admit that there are no big explosions at CERN. That’s a good thing, too, because I’m talking about really big explosions.

CERN, like any big laboratory or university, has a fair number of lectures and colloquia on various topics in physics. One of the great things about being a physicist, and a physics student in particular, is that going to these lectures counts as work, at least if it doesn’t get in the way of things that have to be done. Since my work this week was mostly meetings about getting a new project and passing the old one off to another person, along with writing an ATLAS Infernal Internal Note on the old project, I had the opportunity and need for any educational breaks I could find.

As it happened, there were three very interesting talks by Princeton Professor Adam Burrows. Their nominal subject was “Black Holes and Neutron Stars,” but what he really wanted to show was stars exploding. The first talk, which was definitely my favorite, had a lot of movies and simulations of exactly that. A particularly pretty example is this movie of a Type Ia Supernova:

The neat thing about that video is that, not only does it look good, it’s also a real simulation. One of the main things I learned from the talks is that a substantial obstacle to understanding the details of supernovae is a lack of computing power: there are a lot of ideas about how they work exactly, but none of them come out quite right in simplified simulations. For example, Type II Supernovae probably need to lose their spherical symmetry so that the explosion can spread along one axis while new material collapses into the core from other directions, but it’s not clear exactly how this happens, and it can’t be simulated properly in only two dimensions.

Jokes about avoiding real work aside, it’s quite valuable for physicists to keep up with work in fields that are somewhat removed from our own work; you never know what interesting connections might come up. The details of supernovae have a lot of particle physics in them; for example, there are a tremendous number of neutrinos produced. In fact, neutrino detectors were the first instruments to “see” Supernova 1987a, because the weakly-interacting neutrinos escaped from the star a few hours ahead of the rest of the explosion.

[Image credit: NASA, ESA, J. Hester and A. Loll (Arizona State University)]

The LHC Astro-Lab

Monday, May 5th, 2008

A few weeks ago the physics community got shaken by an announcement of the DAMA project (no not the bad guys on ‘Lost’, they’re the DHARMA initiative), an underground experiment in the Gran Sasso tunnel, which claimed to have found experimental evidence for Dark Matter. The claim is based on the fact that the motion of the earth around the sun should produce a modulation in the dark matter count rate, because the earth’s velocity needs to be added (or subtracted) to the dark matter (or halo) escape velocity. DAMA has found indeed an eight sigma signal of a modulation in their candidate count rate. The question remains whether any background source could cause this signal, and it will take scientists some time to exclude all reasons why this measurement might not be significant. Nevertheless the possibility of experimental evidence for dark matter is exciting. But what does this have to do with the LHC and in particular ALICE ?

Well, throughout the past few years relativistic heavy ion and high energy physics have stressed their significance towards understanding QCD and electro-weak symmetry breaking, but the original quest for the heavy ion program at RHIC and the LHC was to find a state of matter which would have taught us a lot about the evolution of the universe shortly after the Big Bang, at a time where matter as we know it (luminous and dark) should have formed. This original link has been disfavored for some time because scientists felt that the ‘Little Bang’ can not be easily applied to the ‘Big Bang’; the system is too small, the evolution is too fast. But several speculative explanations of experimental measurements at RHIC gave new life to the ‘astro-connection’ of relativistic heavy ion physics (see for example Peter Steinberg’s blog entries on Anti-de-Sitter space and Hawking-Unruh radiation). D.J.Schwarz from CERN in his very instructive article: ‘The first second of the universe’ showed the anticipated evolution of matter formation, and pointed out the relevance of the so-called QCD phase transition from quarks and gluons to hadrons for the evolution of the universe.

It is interesting to note that the LHC offers a two-prong approach to accelerator based astrophysics. Not only can the high energy proton proton collisions likely probe the Higgs field, extra dimensions, super symmetry and dark matter candidates, but the relativistic heavy ion collisions can probe physics in the strong force sector that has traditionally been assumed to occur at higher energies, such as CP violationwhich is necessary for baryogenesis in the universe, anti-baryonic dark matter candidates and the infamous 5-d quantum black holes.

So this is an exciting time, and the diversity of the LHC programme, bringing high energy and heavy ion physicists together by offering proton-proton and Pb-Pb collisions, will lead not only to breakthroughs in the understanding of QCD and potentially new physics beyond the standard model. It will also make the LHC the premier astro-lab in the world. I am glad that all three big experiments (ATLAS, CMS and ALICE) now feature a pp and a PbPb program. Although ALICE is the most versatile heavy ion detector, both ATLAS and CMS have strong programs with heavy ions, and only together and with the necessary verification of each other’s results will we be able to crack some of the cosmic mysteries that I am most interested in. I am looking forward to that and to your attempts of taking aim at some of my claims in this and future blogs

Cheers