Cowan–Reines neutrino experiment

The Cowan–Reines neutrino experiment was performed by Clyde L. Cowan and Frederick Reines in 1956. This experiment confirmed the existence of the antineutrino—a neutrally charged subatomic particle with very low mass.

Background

During the 1910s and 1920s, through the study of electron spectra from the nuclear beta decay, it became apparent that, in addition to an electron, another particle with very small mass and with no electric charge is emitted in the beta-decay but not observed. The observed electron energy spectrum was continuous. Assuming energy conservation, this is only possible if the beta decay is a three-body rather than a two-body decay: the latter would produce a monochromatic peak rather than a continuous energy spectrum. This and other reasons led Wolfgang Pauli to postulate the existence of the neutrino in 1930.

Potential for experiment

Via the inverse beta decay, the predicted electron antineutrino ( ${\bar {\nu }}_{e}$ ), should interact with a proton (
p
) to produce a neutron (
n
) and positron ( $e^{+}$ ) – the antimatter counterpart of the electron.

{\bar {\nu }}_{e}+p\to n+e^{+}

The positron quickly finds an electron, and they annihilate each other. The two resulting gamma rays (
γ
) are detectable. The neutron can be detected by its capture on an appropriate nucleus, releasing a gamma ray. The coincidence of both events—positron annihilation and neutron capture—gives a unique signature of an antineutrino interaction.

Most hydrogen atoms bound in water molecules have a single proton for a nucleus. Those protons serve as a target for the antineutrinos from a reactor. For heavier nuclei, with several protons and neutrons, the interaction mechanism is more complicated and is not always well described by considering the constituent protons as free.

Setup

Cowan and Reines used a nuclear reactor, as advised by Los Alamos physics division leader J.M.B. Kellogg,^[1] as a source of a neutrino flux of 7013500000000000000♠5×10¹³ neutrinos per second per square centimeter;^[2] far higher than any attainable flux from other radioactive sources.

The neutrinos then interacted with protons in two tanks of water, creating neutrons and positrons. Each positron created a pair of gamma rays when it annihilated with an electron. The gamma rays were detected by sandwiching the water tanks between tanks filled with liquid scintillator. The scintillator material gives off flashes of light in response to the gamma rays, and these light flashes are detected by photomultiplier tubes.

This experiment was not conclusive enough, so they devised a second layer of certainty. They detected the neutrons by placing cadmium chloride in the tank. Cadmium is a highly effective neutron absorber and gives off a gamma ray when it absorbs a neutron.

n
+ 108
Cd
→ 109m
Cd
→ 109
Cd
+
γ

The arrangement was such that the gamma ray from the cadmium would be detected 5 microseconds after the gamma ray from the positron, if it were truly produced by a neutrino.

Results

They performed the experiment preliminarily at Hanford Site, but later moved the experiment to the Savannah River Plant in South Carolina near Aiken where they had better shielding against cosmic rays. This shielded location was 11 m from the reactor and 12 m underground.

They used two tanks with a total of about 200 liters of water with about 40 kg of dissolved CdCl₂. The water tanks were sandwiched between three scintillator layers which contained 110 five-inch (127 mm) photomultiplier tubes.

After months of data collection, they had accumulated data on about three neutrinos per hour in their detector. To be absolutely sure that they were seeing neutrino events from the detection scheme described above, they shut down the reactor to show that there was a difference in the number of detected events.

They had predicted a cross-section for the reaction to be about 6952600000000000000♠6×10⁻⁴⁴ cm² and their measured cross-section was 6952630000000000000♠6.3×10⁻⁴⁴ cm². Their results were published in the July 20, 1956 issue of Science.^[3]^[4]

Clyde Cowan died in 1974; Frederick Reines was honored with the Nobel Prize in 1995 for his work on neutrino physics.^[5]

References

↑ "The Reines-Cowan Experiments: Detecting the Poltergeist" (PDF). Los Alamos Science. 25: 3. 1997.
↑ Griffiths, David J. (1987). Introduction to Elementary Particles. John Wiley & Sons. ISBN 0-471-60386-4.
↑ C. L Cowan Jr.; F. Reines; F. B. Harrison; H. W. Kruse; A. D McGuire (July 20, 1956). "Detection of the Free Neutrino: a Confirmation". Science. 124 (3212): 103–4. Bibcode:1956Sci...124..103C. PMID 17796274. doi:10.1126/science.124.3212.103.
↑ Winter, Klaus (2000). Neutrino physics. Cambridge University Press. p. 38ff. ISBN 978-0-521-65003-8.
This source reproduces the 1956 paper.
↑ "The Nobel Prize in Physics 1995". The Nobel Foundation. Retrieved 201-06-29. Check date values in: |access-date= (help)