Inverse Beta Decay of $^{40}$Ar: A New Approach for Observing {MeV} Neutrinos From Laboratory and Astrophysical Sources - INSPIRE

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Inverse Beta Decay of $^{40}$ Ar: A New Approach for Observing {MeV} Neutrinos From Laboratory and Astrophysical Sources

R.S. Raghavan
(
- Bell Labs
)

1986

4 pages

Published in:

Phys.Rev.D 34 (1986) 2088-2091

DOI:

10.1103/PhysRevD.34.2088

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Abstract: (APS)

Inverse β− decay of Ar40 to its isobaric analog state in K40 should occur with a large cross section (σ) for neutrino (νe) capture above a threshold of Eth=5.885 MeV. The νe capture is distinguished by a characteristic γ-ray coincidence signature. With a σ typically larger than that for (e,νe) scattering, the new capture mode of detection should significantly enhance the sensitivity and usefulness of liquid-Ar chambers as νe spectrometers at meson factories and for astrophysical sources such as the Sun, cosmic rays, and collapsing stars.

NEUTRINO NUCLEUS: CAPTURE
CAPTURE: NEUTRINO NUCLEUS
ARGON
NEUTRINO: SOLAR
NEUTRINO: COSMIC RADIATION
CHANNEL CROSS SECTION
COUNTERS AND DETECTORS: PROPOSED

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