Related Experiment Video
Updated: Dec 14, 2025

08:03
Study of Protein Dynamics via Neutron Spin Echo Spectroscopy
Published on: April 13, 2022
2.4K
Sequential Nature of (p,3p) Two-Proton Knockout from Neutron-Rich Nuclei
A Frotscher1, M Gómez-Ramos1, A Obertelli1,2,3
1Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt, Germany.
Physical Review Letters
|July 18, 2020
Summary
Researchers measured two-proton knockout reactions in neutron-rich nuclei. The findings confirm sequential proton-proton collisions, offering insights into nuclear structure and reactions.
Area of Science:
- Nuclear Physics
- High-Energy Nuclear Reactions
- Atomic and Molecular Physics
Background:
- Understanding nuclear structure is crucial for nuclear physics.
- Proton knockout reactions provide insights into nuclear dynamics.
Purpose of the Study:
- To measure two-proton knockout (p,3p) cross sections from neutron-rich nuclei.
- To determine the angular distribution of emitted protons in (p,3p) reactions.
- To investigate the reaction mechanism in neutron-rich nuclei.
Main Methods:
- Measurements were conducted in inverse kinematics using neutron-rich nuclei.
- Proton knockout cross sections were determined at approximately 250 MeV/nucleon.
- Angular distributions of three emitted protons were analyzed.
Main Results:
- The angular distribution of three emitted protons was determined for the first time.
- Kinematics indicate two sequential proton-proton collisions within the projectile nucleus.
- Ratios of (p,3p) to (p,2p) cross sections support a sequential reaction mechanism.
Conclusions:
- The (p,3p) reaction mechanism in neutron-rich nuclei is consistent with sequential proton-proton collisions.
- These findings reinforce the understanding of many-nucleon removal reactions.
- The study provides valuable data for nuclear structure models.
More Related Videos
Related Concept Videos
Nuclear Transmutation
20.2K
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...
20.2K
Nuclear Stability
22.3K
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...
22.3K
Types of Radioactivity
19.1K
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:
19.1K
Radioactivity and Nuclear Equations
26.2K
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...
26.2K
Atomic Nuclei: Nuclear Spin State Population Distribution
2.2K
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.
2.2K
Atomic Nuclei: Nuclear Spin State Overview
1.8K
NMR-active nuclei have energy levels called 'spin states' that are associated with the orientations of their nuclear magnetic moments. In the absence of a magnetic field, the nuclear magnetic moments are randomly oriented, and the spin states are degenerate. When an external magnetic field is applied, the spin states have only 2 + 1 orientations available to them. A proton with = ½ has two available orientations. Similarly, for a quadrupolar nucleus with a nuclear spin value of one, the...
1.8K

