OPERA measured the cosmic muon charge ratio

March 11, 2010 at 6:07 am 3 comments

Muons from cosmic rays rain down from the atmosphere all the time. If you were an empiricist, what would you do? You might compare the number of positive to the number of negative muons, and find that the ratio (pos/neg) is not one – it is about 1.3.

Why is that interesting now, many decades after the first studies of cosmic rays were conducted? Answer: this ratio is different from one due to identity of the cosmic particles that impinge upon the atmosphere, and due to the particles physics of the cascades they cause. Specifically, the production of pions, kaons and even charmed hadrons play a role that varies with the energy of the cascade. A high charge ratio may be linked to kaons, since there is an asymmetry in the production of K+ and K, or to a pure proton flux; a ratio close to one hints at heavy nuclei with a nearly equal number of protons and neutrons, and a predominant production of pions in the cascade for which there is no charge asymmetry.

Let me point out that the “chemical composition” of cosmic rays is an interesting topic – see an earlier post about extra-galactic iron nuclei detected by the Pierre Auger Collaboration.

The OPERA experiment was designed and built to study neutrino oscillations. It was installed deep underground in the Gran Sasso Laboratory (Italy), so the cosmic rays that pass through the apparatus have a high energy, on the order of a TeV. During the course of four months, they recorded a few thousand good events with a trajectory that allowed the authors to measure the momentum and charge. They posted their paper on the archives yesterday (arXiv:1003.1907).

For the purposes of this measurement, the OPERA detector is essentially a double-arm spectrometer which can give two measurements of the deflection of a muon in a 1.53 T magnetic field. The size of the deflection tells you the momentum, while the direction of the deflection tells you the charge of the muon. The trajectory is constructed from hits recorded in resistive plate chambers. The problem of false charge measurements due to bad tracking or large multiple scattering can be controlled adequately by comparing the two measurements. The simulation underestimates these effects somewhat, but not enough to spoil the measurement. Special attention is paid to the alignment of the chambers.

Here is the measurement by the OPERA Collaboration, compared to other recent measurements:

OPERA measurement of cosmic muon charge ratio

Ratio (pos/neg) in bins of Eμ cos(θ*).

The vertical axis is the ratio Rμ of positive to negative muons at the surface of the earth – the authors corrected their observations made in the underground cavern in Gran Sasso for the propagation of muons through the rock above. The horizontal axis is not just the muon energy Eμ, it includes a factor cos(θ*) which takes into account the inclination of the cascade, the radius of the earth and the height of the cascade.

In the figure, the OPERA points are five filled circles above 103 GeV. The curves represent the predictions of four models of cascades in the atmosphere produced by cosmic rays. The OPERA measurements are not able to distinguish those models, but they do agree with and extend prior measurements by MINOS (another underground neutrino experiment) and an experiment in Utah (1975).

This is a nice measurement which adds incrementally to our empirical knowledge of cosmic rays.


Entry filed under: Particle Physics.

C.S. Wu and the lack of a Nobel Prize b jets are hard to count!

3 Comments Add your own

  • 1. Cruton  |  March 11, 2010 at 8:04 am

    Any comment about the data point at 4,000 GeV?

    • 2. Michael Schmitt  |  March 11, 2010 at 8:42 am

      The point has large error bars, so the fact that is falls below the others and from the curves is not very significant. We should keep in mind, too, that very high momentum muons are the ones for which an accurate charge measurement is hardest, and for which a significant correction is needed. I don’t want to say that the OPERA Collaboration did a wrong analysis, but I would not get excited about the apparent deviation unless is was confirmed with much better accuracy by some other experiment.

  • 3. Twenty-three papers: Commissioning CMS « Collider Blog  |  March 20, 2010 at 11:24 am

    […] let me point out that there is some interest in cosmic ray characteristics and one can hope that CMS will use their cosmic ray data to perform some physics measurements, too. […]


Leave a Reply

Fill in your details below or click an icon to log in:

WordPress.com Logo

You are commenting using your WordPress.com account. Log Out /  Change )

Google+ photo

You are commenting using your Google+ account. Log Out /  Change )

Twitter picture

You are commenting using your Twitter account. Log Out /  Change )

Facebook photo

You are commenting using your Facebook account. Log Out /  Change )


Connecting to %s

Trackback this post  |  Subscribe to the comments via RSS Feed

March 2010
« Feb   Apr »

%d bloggers like this: