Related Experiment Video
Updated: Jul 4, 2026

10:42
Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
Published on: May 3, 2019
Nuclear structure relevant to neutrinoless double beta decay: 76Ge and 76Se
J P Schiffer1, S J Freeman, J A Clark
1Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA. schiffer@anl.gov
Physical Review Letters
|June 4, 2008
Summary
Neutrinoless double beta decay research is crucial for determining neutrino mass. New measurements reveal significant differences in nucleon orbit occupations between germanium-76 and selenium-76, challenging current theoretical models.
Area of Science:
- Nuclear Physics
- Particle Physics
- Astroparticle Physics
Background:
- Neutrinoless double beta decay (0νββ) is a hypothetical radioactive decay.
- Observing 0νββ would determine the effective neutrino mass, a fundamental property of neutrinos.
- Accurate nuclear matrix elements are essential for interpreting 0νββ experiments, but theoretical calculations have uncertainties.
Purpose of the Study:
- To experimentally determine the occupation of valence neutron orbits in the ground states of 76Ge and 76Se.
- To provide crucial data for refining theoretical calculations of nuclear matrix elements relevant to 0νββ decay.
Main Methods:
- Precise measurement of cross sections for neutron-adding and neutron-removing transfer reactions.
- Utilizing 76Ge as a candidate for 0νββ decay and 76Se as its daughter nucleus.
- Analyzing reaction data to deduce the populations of specific nucleon orbits.
Main Results:
- The Fermi surface in 76Ge and 76Se is found to be significantly more diffuse than predicted by theoretical models.
- Populations of at least three valence neutron orbits show substantial changes between the ground states of 76Ge and 76Se.
- Theoretical calculations predominantly predict changes in only one orbit, highlighting a discrepancy with experimental findings.
Conclusions:
- Experimental data on valence orbit occupations provide critical insights into nuclear structure relevant to 0νββ decay.
- The observed diffuse Fermi surface and multi-orbit changes necessitate revisions in theoretical models for nuclear matrix elements.
- Improved theoretical calculations based on these findings will enhance the interpretation of future 0νββ experiments and neutrino mass determination.
Related Concept Videos
Nuclear Stability
Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively charged protons together in the...
To hold positively charged protons together in the...
Types of Radioactivity
The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Radioactivity and Nuclear Equations
Nuclear chemistry is the study of reactions that involve changes in nuclear structure. The nucleus of an atom is composed of protons and, except for hydrogen, neutrons. The number of protons in the nucleus is called the atomic number (Z) of the element, and the sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are isotopes of the same element.
A nuclide of an element has a specific number of protons and...
A nuclide of an element has a specific number of protons and...
Nuclear Transmutation
Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed protons being...
Atomic Nuclei: Nuclear Spin State Population Distribution
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
Nuclear Binding Energy
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound together;...

