Related Experiment Video
Updated: Dec 17, 2025

07:46
Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
8.9K
A new formulae study for the (n,2p) reaction cross-section systematics at 14-15 MeV
1Kahramanmaras Sutcu Imam University, Vocational School of Health Services, Department of Medical Imaging Techniques, Kahramanmaras, Turkey.
Summary
New empirical formulas accurately predict (n, 2p) reaction cross sections for nuclei between 29≤A≤159. These formulas, based on the (N-Z)/A asymmetry parameter, improve nuclear reaction calculations for incident neutron energies of 14-15 MeV.
Area of Science:
- Nuclear Physics
- Nuclear Reactions
- Cross-Section Calculations
Background:
- Accurate cross-section calculations are crucial for understanding particle-induced nuclear excitation.
- Systematics in nuclear reaction cross-sections require reliable empirical formulas for predictive power.
Purpose of the Study:
- To develop new empirical formulas for (n, 2p) reaction cross sections at 14-15 MeV incident neutron energy.
- To investigate the dependence of these cross sections on the (N-Z)/A asymmetry parameter.
- To reveal the systematics of (n, 2p) reactions within specific mass ranges.
Main Methods:
- Modification of the original Levkovski formula to obtain asymmetry parameters.
- Application of the least square fitting method to analyze EXFOR data.
- Examination of statistical dependence (R-squared) for the 29≤A≤159 mass range.
Main Results:
- New empirical formulas were derived for mass ranges 29≤A≤159, 29≤A≤103, and 133≤A≤159.
- The formulas demonstrate a clear dependence on the modified (N-Z)/A asymmetry parameter.
- Calculated results show good agreement with existing EXFOR data for 29≤A≤159 and 29≤A≤103.
Conclusions:
- The developed empirical formulas provide a reliable method for predicting (n, 2p) reaction cross sections.
- The study successfully established systematics for (n, 2p) reactions based on nuclear asymmetry.
- The findings contribute to a better understanding of nuclear reaction mechanisms and cross-section behavior.
Related Concept Videos
Nuclear Stability
22.4K
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...
22.4K
Radioactivity and Nuclear Equations
26.4K
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...
26.4K
Other Nuclides: 31P, 19F, 15N NMR
658
Many organic, inorganic, and biological molecules contain spin-half nuclei such as nitrogen-15, fluorine-19, and phosphorus-31. As a result, NMR studies of these nuclei have found extensive applications in chemical and biological research.
While fluorine-19 and phosphorous-31 have high natural abundances (100%) and positive gyromagnetic ratios, nitrogen-15 has a low natural abundance and a negative gyromagnetic ratio. However, nitrogen-15 is still preferred over nitrogen-14 (which has a...
While fluorine-19 and phosphorous-31 have high natural abundances (100%) and positive gyromagnetic ratios, nitrogen-15 has a low natural abundance and a negative gyromagnetic ratio. However, nitrogen-15 is still preferred over nitrogen-14 (which has a...
658
Nuclear Binding Energy
14.5K
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 are bound...
14.5K
Mass Spectrum: Interpretation
2.5K
An unknown compound can be established by identifying the molecular ion peak in the mass spectrum. The molecular ion peak is often weak or absent due to the predominance of fragmentation in high-energy electron beams. In such cases, a soft-energy electron beam can be used to scan the spectrum to enhance the intensity of the molecular ion peak. Additionally, chemical ionization, field ionization, and desorption ionization spectra are used to obtain a relatively intense molecular ion peak.To...
2.5K
Nuclear Transmutation
20.3K
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...
20.3K

