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Radiation: Applications01:17

Radiation: Applications

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...
Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

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 per...
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
Radioactivity and Nuclear Equations03:18

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...
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container. Nichols...
Atomic Absorption Spectroscopy: Radiation and Light Sources01:13

Atomic Absorption Spectroscopy: Radiation and Light Sources

Atomic absorption spectroscopy (AAS) relies on the Beer-Lambert law, which requires that the radiation source emits a narrow range of wavelengths to match the absorption characteristics of the analyte atom. The primary criteria for choosing an appropriate radiation source in AAS is to provide a precise and intense emission at specific wavelengths that will allow accurate detection of the analyte.
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...

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Related Experiment Video

Updated: May 30, 2026

Laser-heating and Radiance Spectrometry for the Study of Nuclear Materials in Conditions Simulating a Nuclear Power Plant Accident
09:18

Laser-heating and Radiance Spectrometry for the Study of Nuclear Materials in Conditions Simulating a Nuclear Power Plant Accident

Published on: December 14, 2017

Geant4 hadronic physics for space radiation environment.

Anton V Ivantchenko1, Vladimir N Ivanchenko, Jose-Manuel Quesada Molina

  • 1Université Bordeaux 1, CNRS/IN2P3, Centre d'Etudes Nucléaires de Bordeaux Gradignan, CENBG, 33175 Gradignan, France. Anton.Ivantchenko@cern.ch

International Journal of Radiation Biology
|August 12, 2011
PubMed
Summary
This summary is machine-generated.

This study tested Geant4 (Geometry And Tracking version 4) Monte Carlo hadronic models for space radiation environments. An optimal configuration was proposed for simulating particle interactions with matter.

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Last Updated: May 30, 2026

Laser-heating and Radiance Spectrometry for the Study of Nuclear Materials in Conditions Simulating a Nuclear Power Plant Accident
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Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera

Published on: January 30, 2020

Area of Science:

  • Nuclear Physics
  • Particle Physics
  • Astrophysics

Background:

  • Space radiation poses significant risks to electronic systems and astronauts.
  • Accurate simulation of particle interactions with matter is crucial for radiation shielding and risk assessment.

Purpose of the Study:

  • To test and develop Geant4 (Geometry And Tracking version 4) Monte Carlo hadronic models.
  • To optimize these models for simulating the space radiation environment.

Main Methods:

  • Utilized the Geant4 toolkit for Monte Carlo simulations.
  • Employed Binary (BIC), BIC-ion, and Bertini (BERT) cascades as primary generators.
  • Validated models against experimental data using a hadronic testing suite.

Main Results:

  • Revised and improved Geant4 pre-compound (PRECO) and de-excitation (DEE) models.
  • Simulated proton, neutron, pion, and ion nuclear interactions using Geant4 version 9.4.
  • Compared simulation results with experimental data from thin and thick target experiments.

Conclusions:

  • Geant4 provides a comprehensive set of models for simulating particle-matter interactions.
  • An optimal Geant4 model configuration for space radiation environment simulations has been identified.