High Energy K X-Ray Hypersatellites

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Zewdu Alamineh Fetene
Zewdu Alamineh Fetene
α Debre Tabor University

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High Energy K X-Ray Hypersatellites

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Abstract

This study focus on the weak lines that appear on high energy side of the diagram lines which is called High Energy K X-ray hypersatellites i.e., a particular category of characteristic Xray due to splitting of fine structure levels. It’s resulted from the interaction of spin of an electron with the spin of the nucleus. They are emitted when an atom that has undergone a spontaneous transitions from the higher hyperfine level to the lower one to a radiation of ≈ 1.42 × 10 9 𝐻𝐻𝐻𝐻 frequency and ≈ 21 𝑐𝑐𝑐𝑐 wavelength. Simultaneous double ionization in the K-shell and multiple ionization in the L-shell gives rise to K α X-ray hypersatellites. These can be studied only by high energy resolution instruments like WDXRF spectrometry. Fundamental experimental procedures were outlined in this field by several workers due to different excitation modes. The theoretical models to predict their energies and intensities were developed. And also this review can show a clear discrepancy between theoretical and experimental results in the case of hyper satellites formation from different shells. In case of experimental instrumentation, WDXRF is the most accurate for determining the energy and intensity of X-ray hypersatellites. All sources of data was literature done by different scholars.

References

29 Cites in Article
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Funding

No external funding was declared for this work.

Conflict of Interest

The authors declare no conflict of interest.

Ethical Approval

No ethics committee approval was required for this article type.

Data Availability

Not applicable for this article.

How to Cite This Article

Zewdu Alamineh Fetene. 2015. \u201cHigh Energy K X-Ray Hypersatellites\u201d. Global Journal of Science Frontier Research - A: Physics & Space Science GJSFR-A Volume 15 (GJSFR Volume 15 Issue A4): .

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Journal Specifications

Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

Keywords
Classification
GJSFR-A Classification: FOR Code: 020199p
Version of record

v1.2

Issue date

September 8, 2015

Language
en
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This study focus on the weak lines that appear on high energy side of the diagram lines which is called High Energy K X-ray hypersatellites i.e., a particular category of characteristic Xray due to splitting of fine structure levels. It’s resulted from the interaction of spin of an electron with the spin of the nucleus. They are emitted when an atom that has undergone a spontaneous transitions from the higher hyperfine level to the lower one to a radiation of ≈ 1.42 × 10 9 𝐻𝐻𝐻𝐻 frequency and ≈ 21 𝑐𝑐𝑐𝑐 wavelength. Simultaneous double ionization in the K-shell and multiple ionization in the L-shell gives rise to K α X-ray hypersatellites. These can be studied only by high energy resolution instruments like WDXRF spectrometry. Fundamental experimental procedures were outlined in this field by several workers due to different excitation modes. The theoretical models to predict their energies and intensities were developed. And also this review can show a clear discrepancy between theoretical and experimental results in the case of hyper satellites formation from different shells. In case of experimental instrumentation, WDXRF is the most accurate for determining the energy and intensity of X-ray hypersatellites. All sources of data was literature done by different scholars.

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High Energy K X-Ray Hypersatellites

Zewdu Alamineh Fetene
Zewdu Alamineh Fetene Debre Tabor University

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