Tikalon Header Blog Logo

Tachyons

September 26, 2011

When I was in graduate school, I would often see papers about tachyons during my frequent literature searches in the library. A tachyon, named from the Greek word, ταχυς (swift), is a superluminal particle; that is, a particle that travels faster than light. None of those papers were about the discovery of tachyons. They were descriptions of experiments that set limits on how impossible they might be (See, for example, refs. 1-2).

Since the speed of light has always been considered to be the speed limit for our universe of normal, slowpoke matter, tachyons would need to have some unusual properties. Tachyons must always move at the speed of light, or higher. Motion at the speed of light would be nearly impossible since tachyons need to gain energy to slow down. A tachyon would need to attain infinite energy to slow to the speed of light, just as ordinary matter would need infinite energy to travel as fast as the speed of light.

Tachyons create a fundamental problem in causality if they might be used to transmit information faster than light. Reception of charged tachyons is possible, since they will lose energy via Cherenkov radiation. Cherenkov radiation is the blue glow observed in the cooling water of nuclear reactors. It's caused by charged particles exceeding the phase velocity of light in a medium. There is no known method for generation of tachyons, so a companion transmitter is not yet possible, and causality is saved. There is, however, a patent on another method of faster-than-light communication.[3]

One interesting idea about tachyons, proposed by Alan Chodosa, Avi I. Hausera and V. Alan Kostelecký in 1985, is that neutrinos could have a tachyonic component.[4] Through many observations, it's fairly well established that neutrinos oscillate between flavors; that is, a muon neutrinos emitted in a reaction may be detected at a later time as a tau neutrino. Somewhere in this oscillation there might be some hidden tachyons. Naturally, there were naysayers to this proposal.[5]

Hydrogen bubble chamber image of a neutrino



The first Argonne National Laboratory hydrogen bubble chamber image of the neutrino, taken on November 13, 1970.

In this image, a neutrino hits the proton nucleus of hydrogen)


The neutrino was discovered by the Cowan–Reines neutrino experiment in 1956. (Via Wikimedia Commons).

One major neutrino experiment is OPERA that I described in a previous article (Morphing Neutrinos, June 2, 2010). In the OPERA experiment, a beam of muon neutrinos is produced at the CERN Super Proton Synchrotron in Geneva and sent to an underground laboratory in a mountain called Gran Sasso in Italy 730 km (453 miles) away. The neutrinos are produced when protons hit a graphite target. The supposed transit time for the muon neutrinos, 2.4 milliseconds, is enough time for some to change to tau neutrinos.

The Opera experiment has been ongoing since 2006, and it's estimated that about 1018 muon neutrinos have been sent its way. Now, Antonio Ereditato, spokesperson for the OPERA team, has announced that a small fraction of this huge number (15,000) have arrived at the detector 60 nanoseconds sooner than expected.[6-9] It's important to note that only a fraction of neutrinos arrive early, so errors in the exact distance from CERN to Gran Sasso and timing can be discounted. In fact, timing accuracy between the sites is established at nanosecond accuracy, and the distance is known to within 20 centimeters.[6]

Any physicist would be timid in making the claim that his particles were traveling faster than the "cosmic speed limit." Says Ereditato,
"This result comes as a complete surprise... After many months of studies and cross checks we have not found any instrumental effect that could explain the result of the measurement. While OPERA researchers will continue their studies, we are also looking forward to independent measurements to fully assess the nature of this observation."[6]
Of course, such a discovery requires independent confirmation, but in the field of neutrino physics, there are few laboratories situated to make such a test. These are Fermilab, still reeling from its loss of pivotal position to CERN's Large Hadron Collider, and the Japanese Super-Kamiokande. The measurement capability of these facilities would need to be upgraded in order to see CERN's result. CERN Research Director, Sergio Bertolucci, announced in a press release that CERN welcomes such scrutiny.
"When an experiment finds an apparently unbelievable result and can find no artefact of the measurement to account for it, it's normal procedure to invite broader scrutiny, and this is exactly what the OPERA collaboration is doing, it's good scientific practice... If this measurement is confirmed, it might change our view of physics, but we need to be sure that there are no other, more mundane, explanations. That will require independent measurements."[6]

As Yogi Berra said, "It's déjà vu all over again." Another experiment, MINOS at Fermilab, saw the same thing in 2007. The MINOS data, however, were not accurate enough to make any claims.[8] MINOS may be up and running again in just six months.[8] It took OPERA three years of data collection to come to its conclusion, so don't throw out (or delete) your relativity books just yet.

It's appropriate to repeat the exclamation of I.I. Rabi at the discovery of the muon, "Who ordered that?"

References:

  1. C. Baltay, G. Feinberg, N. Yeh and R. Linsker, "Search for Uncharged Faster-than-Light Particles," Phys. Rev. D, vol. 1, no. 3 (February 1, 1970), pp. 759-770.
  2. D. F. Bartlett, D. Soo and M. G. White, "Search for tachyon monopoles in cosmic rays," Phys. Rev. D, vol. 18, no. 7 (October 1, 1978), pp. 2253-2261.
  3. David L. Strom, "Hyper-light-speed antenna," US Patent No. 6,025,810, February 15, 2000.
  4. Alan Chodosa, Avi I. Hausera and V. Alan Kostelecký, "The neutrino as a tachyon," Physics Letters vol. B150, no. 6 (January 24, 1985), pp. 431-435.
  5. Richard J. Hughes and G.J. Stephenson Jr., "Against tachyonic neutrinos," Physics Letters vol. B244, no. 1 (July 12, 1990), pp. 95-100.
  6. OPERA experiment reports anomaly in flight time of neutrinos from CERN to Gran Sasso, CERN Press Release No. PR19.11, September 23, 2011.
  7. Jason Palmer, "Speed-of-light experiments give baffling result at Cern," BBC News, September 22, 2011.
  8. Eryn Brown and Amina Khan, "Faster than light? CERN findings bewilder scientists," Los Angeles Times, September 23, 2011.
  9. Particles found to break speed of light, Reuters, September 22, 2011.
  10. Opera Experiment Web Site.                                   

Permanent Link to this article

Linked Keywords: Graduate school; tachyons; Greek; superluminal; light; speed of light; causality; information; charged; Cherenkov radiation; nuclear reactor; phase velocity; neutrino; oscillation; flavor; muon neutrino; tau neutrino; Argonne National Laboratory; hydrogen bubble chamber; Cowan–Reines neutrino experiment; Wikimedia Commons; OPERA; CERN Super Proton Synchrotron; Gran Sasso; Italy; proton; graphite; millisecond; Antonio Ereditato; nanosecond; centimeter; neutrino physics; laboratory; Fermilab; CERN; Large Hadron Collider; Japanese; Super-Kamiokande; Yogi Berra; It's déjà vu all over again; MINOS; relativity; I.I. Rabi; muon.

RSS Feed

Google Search


Latest Books by Dev Gualtieri

LGM by Dev Gualtieri
LGM by Dev Gualtieri, paperback LGM by Dev Gualtieri, Kindle

Thanks to Cory Doctorow of BoingBoing for his favorable review of Secret Codes!

Secret Codes & Number Games by Dev Gualtieri
Secret Codes & Number Games by Dev Gualtieri, paperback

Other Books

Other Books by Dev Gualtieri