Science Watch® - Tracking Trends and Performance in Basic Research
July/August 2004


Pentaquark Pursuit: Five-Quark Particle Charms Physicists
by Simon Mitton
WHAT'S HOT IN PHYSICS
Rank      Paper Citations This Period (Jan-Feb 04) Rank Last Period (Nov-Dec 03)
1 D.N. Spergel, et al., "First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters," Astrophys. J. Suppl. Ser., 148(1): 175-94, September 2003. [6 U.S. and Canadian institutions] *715BR
(Also read comments by Verde, L; co-author of this Hot Paper.)
102 1
2 C.L. Bennett, et al., "First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Preliminary maps and basic results," Astrophys. J. Suppl. Ser., 1(148): 1-27, September 2003. [7 U.S. and Canadian institutions] *715BR 52 4
3 K. Eguchi, et al., "First results from KamLAND: Evidence for reactor antineutrino disappearance," Phys. Rev. Lett., 90(2): 1802, 17 January 2003. [12 institutions worldwide] *636FP 48 2
4 Q.R. Ahmad, et al., "Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory," Phys. Rev. Lett., 89(1): 1301, 1 July 2002. [17 institutions worldwide] *563YN 39 3
5 Q.R. Ahmad, et al., "Measurement of day and night neutrino energy spectra at SNO and constraints on neutrino mixing parameters," Phys. Rev. Lett., 89(1): 1302, 1 July 2002. [17 institutions worldwide] *563YN 29 6
6 T. Nakano, et al., "Evidence for a narrow S = +1 baryon resonance in photoproduction from the neutron," Phys. Rev. Lett., 91(1): 2002, 4 July 2003. [19 institutions worldwide] *696YP 21
7 N.W. Halverson, et al., "Degree Angular Scale Interferometer first results: A measurement of the cosmic microwave background angular power spectrum," Astrophys. J., 568(1): 38-45, 20 March 2002. [U. Chicago, IL; U. Calif., Berkeley; JPL, Pasadena, CA; Caltech, Pasadena] *531VN 20
8 S. Fukuda, et al., "Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data," Physics Letters B, 539(3,4): 179-87, 18 July 2002. [29 institutions worldwide] *576WT 20
9 J. Park, et al., "Coulomb blockade and the Kondo effect in single-atom transistors," Nature, 417(6890): 722-5, 13 June 2002. [Cornell U., Ithaca, NY; U. Calif., Berkeley] *561QY 20
10 J.M. Kovac, et al., "Detection of polarization in the cosmic microwave background using DASI," Nature, 420(6917): 772-87, 19/26 December 2002. [U. Chicago, IL; U. Calif., Berkeley] *626WR 19
 SOURCE: ISI's Hot Paper Database. Read the full legend.

Quark physics makes the top newcomer this period, with the creation of a subatomic particle containing five quarks, rather than the normal two or three, described in #6. Quarks and leptons (the electron, muon, and tau particles) are the fundamental building blocks of nuclear matter. The quarks come in six "flavors": up and down, charmed and strange, and, top and bottom. Their electrical charge is either +2/3 or –1/3 the charge on the electron. All baryons are quark triplets: for example the proton has two up quarks and one down, while the neutron has one up and two down. The mesons are quark-antiquark pairs. Quark-quark interactions inside a particle are mediated by gluons, a name chosen because they are the glue holding everything together. Free quarks do not exist, so they can be studied only in combination with other quarks inside hadrons.

Soon after the genesis in 1964 of the quark model, theorists began to ask if particles could be made from more than three quarks. Quantum chromodynamics, the theory of how quarks interact, does not rule out higher combinations. Theorists soon speculated on the existence of assemblies of four or more quarks, triggering a long history of searches for exotic resonances in baryon collisions, without making any progress. This situation might have changed in 1997, when Maxim Polyakov, Dmitri Diakonov, and Victor Petrov at the Petersburg Nuclear Physics Institute in Russia proposed the pentaquark, as a new bound state of matter. However, their musings met great skepticism, and could easily have been forgotten. Then, in 2000, Dmitri Diakonov and Takashi Nakano (Osaka University, Research Center for Nuclear Physics) struck up conversations at the lunch counter while attending a conference in Copenhagen. Diakonov thought that the experiments then being conducted by Nakano and his team could produce a five-quark particle. Crucially, Diakonov suggested a new method of data analysis that should, he thought, reveal the pentaquark’s presence.

For their quest, the Japanese team used the Spring-8 synchrotron near Kobe, the world’s largest third-generation synchrotron radiation facility. They directed a beam of 2.4 GeV gamma rays at a carbon target, and studied the missing-mass spectrum of the nuclear reaction in which a neutron absorbs a gamma ray and then decays to a K+, and K- meson plus a neutron. The missing-mass spectrum has a sharp resonance at 1.54 GeV/c2, which indicates the formation of a particle of that mass, about 1.5 times the proton mass. This can be attributed to a meson-baryon molecular resonance, or, much more exciting, an exotic five-quark baryon composed of two ups, one down, one strange, and one anti-down quark. The half-life of the pentaquark, essentially a fleeting fusion of a neutron and a K+ meson, is 10-20 s.

For Science Watch, Nakano offers the following comments. "Our result is important because it indicates a new way to confine quarks in a particle. So far about 10 experimental groups have observed the peak, although there is still no observation which undeniably proves the existence of the pentaquark, which belongs to a rare species of the hadron family." He adds that in the early Big Bang universe free quarks existed, and the pentaquark "may give a clue to understand how quarks now form protons and neutrons and can never escape from them."

The early universe features in Hot Paper #10, which reports on polarization in the cosmic microwave background (CMB), as measured by the Degree Angular Scale Interferometer (DASI). This ground-based instrument is at the South Pole, where it profits from the very dry atmosphere. Paper #10 reports the first detection of polarization of the CMB, which University of Chicago astrophysicists first announced in September 2002. One of them, lead author John Kovac, tells Science Watch, "An initial detection of CMB polarization had long been sought; with its achievement cosmology passes a significant milestone." Many ongoing experiments are now taking up the challenge of precision polarization measurements, spurred on by the Chicago results. Looking to the future, Kovac adds, "A new generation of experiments will push into uncharted territory, where the polarization should contain the signatures of the physics of inflation and dark energy."

Hot Paper #8 from Super-Kamiokande deserves a brief mention. The annual results from this solar neutrino experiment have regularly made the Physics Top Ten. What’s new this time is the measurement of critical oscillation parameters to a high degree of confidence (up to 95% CL). The combined results of all solar neutrino experiment are used to determine a unique region of oscillation parameters that explains the famous solar neutrino problem.end 

Dr. Simon Mitton of St. Edmund’s College, University of Cambridge, U.K.,
is pursuing research on the history of 20th century astronomy.

Science Watch®, July/August 2004, Vol. 15, No. 4
Citing URL: http://www.sciencewatch.com/july-aug2004/sw_july-aug2004_page6.htm

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