Related Experiment Video
Updated: Jul 16, 2025

12:19
Measurement of Quantum Interference in a Silicon Ring Resonator Photon Source
Published on: April 4, 2017
8.4K
First Measurement of the Nuclear-Recoil Ionization Yield in Silicon at 100 eV
M F Albakry1,2, I Alkhatib3, D Alonso4,5
1Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada.
Physical Review Letters
|September 18, 2023
Summary
Researchers explored nuclear-recoil ionization yield in silicon detectors. The study found no ionization threshold above 100 eV, prompting further investigation into detector response at low energies.
Area of Science:
- Nuclear physics
- Detector technology
Background:
- Understanding nuclear-recoil interactions is crucial for various physics experiments.
- Previous studies have explored ionization yield, but low-energy thresholds remain an area of interest.
Purpose of the Study:
- To measure the nuclear-recoil ionization yield in silicon at unprecedented low energies.
- To investigate the existence of an ionization production threshold above 100 eV.
Main Methods:
- Utilized a cryogenic phonon-sensitive gram-scale detector.
- Employed a monoenergetic neutron beam to scatter off silicon nuclei.
- Probed energy depositions ranging from 4 keV down to 100 eV.
Main Results:
- Successfully measured nuclear-recoil ionization yield in silicon.
- Observed no evidence of an ionization production threshold at energies above 100 eV.
- Achieved the lowest energy probing to date for this measurement.
Conclusions:
- The absence of a threshold challenges existing ionization yield theories.
- Further research is needed to refine detector response functions below the keV scale.
- Experimental results necessitate theoretical re-evaluation of low-energy nuclear interactions.
Related Concept Videos
Ionization Energy
33.8K
The amount of energy required to remove the most loosely bound electron from a gaseous atom in its ground state is called its first ionization energy (IE1). The first ionization energy for an element, X, is the energy required to form a cation with 1+ charge:
33.8K
Nuclear Binding Energy
12.5K
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...
12.5K
Nuclear Fission
9.7K
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...
9.7K
Thomson's e/m Experiment
3.8K
In a beam of charged particles created by a heated cathode, the particles move at different speeds. However, many applications need a beam with uniform particle speeds. An arrangement known as a velocity selector uses electric and magnetic fields to pick particles with a particular speed from the beam.
A particle with charge q, speed v, and mass m enters an area from the top, where the magnetic and electric fields are perpendicular both to the particle's motion and to one another. The...
A particle with charge q, speed v, and mass m enters an area from the top, where the magnetic and electric fields are perpendicular both to the particle's motion and to one another. The...
3.8K
Atomic Radii and Effective Nuclear Charge
51.7K
The elements in groups of the periodic table exhibit similar chemical behavior. This similarity occurs because the members of a group have the same number and distribution of electrons in their valence shells.
51.7K
Atomic Nuclei: Nuclear Magnetic Moment
1.2K
All atomic nuclei are positively charged. When they have a nonzero spin, they behave like rotating charges. As a consequence of their charge and spin, these nuclei generate a magnetic field (B). This, in turn, gives rise to a magnetic moment (μ), which is randomly oriented in the absence of an external magnetic field. When an external magnetic field (B0) is applied, the magnetic moment vectors can align with the field or against it in 2 + 1 orientations. A hydrogen nucleus, which is just a...
1.2K

