Related Experiment Video
Updated: Dec 17, 2025

06:20
Irradiator Commissioning and Dosimetry for Assessment of LQ α and β Parameters, Radiation Dosing Schema, and in vivo Dose Deposition
Published on: March 11, 2021
7.6K
Do we really need the "detriment" for radiation protection?
1Institute of Medical Physics and Radiation Protection (IMPS), University of Applied Sciences, THM, Giessen, Germany. joachim.breckow@mni.thm.de.
Radiation and Environmental Biophysics
|June 26, 2020
Summary
The International Commission on Radiological Protection
Area of Science:
- Radiological Protection
- Radiation Biology
- Medical Physics
Background:
- The International Commission on Radiological Protection (ICRP) detriment concept quantifies stochastic radiation damage across organs.
- This involves weighting organ-specific risk coefficients by a function reflecting disease severity.
Purpose of the Study:
- To evaluate the necessity of the ICRP's complex detriment concept for radiation protection.
- To explore simpler alternative methods for quantifying radiation damage.
Main Methods:
- Analysis of the ICRP detriment concept's components.
- Comparison of the current detriment definition with potential simpler models.
Main Results:
- The current detriment concept incorporates disease-specific variables unrelated to radiation parameters.
- The study questions the necessity of this complexity for radiation protection.
Conclusions:
- A simpler approach to quantifying radiation damage may be sufficient or even superior for radiation protection.
- Re-evaluation of the ICRP detriment concept's complexity is warranted.
Related Concept Videos
Biological Effects of Radiation
17.3K
All radioactive nuclides emit high-energy particles or electromagnetic waves. When this radiation encounters living cells, it can cause heating, break chemical bonds, or ionize molecules. The most serious biological damage results when these radioactive emissions fragment or ionize molecules. For example, α and β particles emitted from nuclear decay reactions possess much higher energies than ordinary chemical bond energies. When these particles strike and penetrate matter, they...
17.3K
Nuclear Power
9.1K
Controlled nuclear fission reactions are used to generate electricity. Any nuclear reactor that produces power via the fission of uranium or plutonium by bombardment with neutrons has six components: nuclear fuel consisting of fissionable material, a nuclear moderator, a neutron source, control rods, reactor coolant, and a shield and containment system.
Nuclear Fuels
Nuclear fuel consists of a fissile isotope, such as uranium-235, which must be present in sufficient quantity to provide a...
Nuclear Fuels
Nuclear fuel consists of a fissile isotope, such as uranium-235, which must be present in sufficient quantity to provide a...
9.1K
Radiation Pressure: Problem Solving
702
The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
702
Diamagnetic Shielding of Nuclei: Local Diamagnetic Current
1.3K
An applied magnetic field causes the electrons present in the molecule to circulate, setting up a local diamagnetic current within the molecule. The local diamagnetic current arising from circulating sigma-bonding electrons induces a magnetic field, Blocal that opposes the applied magnetic field, B0. The effective magnetic field experienced by these nuclei is given by the difference between the applied and local magnetic fields in a phenomenon called local diamagnetic shielding. Essentially,...
1.3K
Absorption of Radiation
1.1K
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
1.1K
Radiation: Applications
1.6K
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
1.6K

