Related Experiment Video
Updated: Mar 31, 2026

06:28
Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
Published on: January 30, 2020
13.4K
Observation of the competitive double-gamma nuclear decay
C Walz1, H Scheit1, N Pietralla1
1Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany.
Nature
|October 16, 2015
Summary
Researchers observed double-gamma (γγ)-decay in excited nuclear states, a rare quantum process. This finding expands our understanding of nuclear structure and quantum electrodynamics beyond previously studied 0(+) to 0(+) transitions.
Area of Science:
- Nuclear Physics
- Quantum Electrodynamics
Background:
- Double-gamma (γγ)-decay is a fundamental second-order quantum electrodynamics process involving simultaneous emission of two gamma quanta.
- Previously, γγ-decay was only observed for specific nuclear transitions (J(π) = 0(+) → 0(+)) where single-gamma decay is forbidden.
- Single-gamma (γ)-decay is the primary experimental challenge for observing γγ-decay.
Purpose of the Study:
- To report the observation of γγ-decay from an excited nuclear state with J(π) = 11/2(-).
- To investigate γγ-decay competing directly with allowed single γ-decay.
- To determine the branching ratio and multipolarities of the γγ-decay process.
Main Methods:
- Experimental observation of γγ-decay in the 11/2(-) isomer of Barium-137 ((137)Ba).
- Measurement of angular correlation and energy spectra of emitted gamma rays.
- Calculation of transition matrix elements using the quasiparticle-phonon model.
Main Results:
- The γγ-decay of the 11/2(-) isomer of (137)Ba was observed competing with allowed γ-decay to the 3/2(+) ground state.
- The branching ratio for this competitive γγ-decay was determined to be (2.05 ± 0.37) × 10(-6).
- Analysis of angular correlations and energy spectra allowed determination of contributing multipolarities.
Conclusions:
- The observed γγ-decay provides a new pathway to probe nuclear structure.
- This decay mode offers access to previously unexplored nuclear properties, including generalized nuclear electric polarizabilities and magnetic susceptibilities.
- The quasiparticle-phonon model successfully reproduces the experimental measurements.
Related Concept Videos
Types of Radioactivity
21.4K
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:
21.4K
Radioactivity and Nuclear Equations
29.7K
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...
29.7K
Nuclear Stability
24.3K
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...
To hold positively charged protons together...
24.3K
Nuclear Binding Energy
15.2K
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...
15.2K
Nuclear Fission
12.9K
Many heavier elements with smaller binding energies per nucleon can decompose into more stable elements that have intermediate mass numbers and larger binding energies per nucleon—that is, mass numbers and binding energies per nucleon that are closer to the “peak” of the binding energy graph near 56. Sometimes neutrons are also produced. This decomposition of a large nucleus into smaller pieces is called fission. The breaking is rather random with the formation of a large...
12.9K
Nuclear Transmutation
21.0K
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...
21.0K

