Loading menu…

High Energy K X-Ray Hypersatellites

Β§ Debre Tabor University

Send Message

To: Author

High Energy K X-Ray Hypersatellites

Article Fingerprint

ReserarchID

SFR565JV

High Energy K X-Ray Hypersatellites Banner

Key Research Insights

Synthesized scholarly intelligence & interactive research assistant
  • English
  • Afrikaans
  • Albanian
  • Amharic
  • Arabic
  • Armenian
  • Azerbaijani
  • Basque
  • Belarusian
  • Bengali
  • Bosnian
  • Bulgarian
  • Catalan
  • Cebuano
  • Chichewa
  • Chinese (Simplified)
  • Chinese (Traditional)
  • Corsican
  • Croatian
  • Czech
  • Danish
  • Dutch
  • Esperanto
  • Estonian
  • Filipino
  • Finnish
  • French
  • Frisian
  • Galician
  • Georgian
  • German
  • Greek
  • Gujarati
  • Haitian Creole
  • Hausa
  • Hawaiian
  • Hebrew
  • Hindi
  • Hmong
  • Hungarian
  • Icelandic
  • Igbo
  • Indonesian
  • Irish
  • Italian
  • Japanese
  • Javanese
  • Kannada
  • Kazakh
  • Khmer
  • Korean
  • Kurdish (Kurmanji)
  • Kyrgyz
  • Lao
  • Latin
  • Latvian
  • Lithuanian
  • Luxembourgish
  • Macedonian
  • Malagasy
  • Malay
  • Malayalam
  • Maltese
  • Maori
  • Marathi
  • Mongolian
  • Myanmar (Burmese)
  • Nepali
  • Norwegian
  • Pashto
  • Persian
  • Polish
  • Portuguese
  • Punjabi
  • Romanian
  • Russian
  • Samoan
  • Scots Gaelic
  • Serbian
  • Sesotho
  • Shona
  • Sindhi
  • Sinhala
  • Slovak
  • Slovenian
  • Somali
  • Spanish
  • Sundanese
  • Swahili
  • Swedish
  • Tajik
  • Tamil
  • Telugu
  • Thai
  • Turkish
  • Ukrainian
  • Urdu
  • Uzbek
  • Vietnamese
  • Welsh
  • Xhosa
  • Yiddish
  • Yoruba
  • Zulu
Reading Preferences
Font Size
Line Spacing
Background
This converted HTML version may contain rendering inconsistencies. Please refer to the PDF for the authoritative version, or click here to provide feedback.

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 β‰ˆ 1.42 Γ— 10 9 𝐻𝐻𝐻𝐻 frequency and β‰ˆ 21 𝑐𝑐𝑐𝑐 wavelength. Simultaneous double ionization in the K-shell and multiple ionization in the L-shell gives rise to K Ξ± 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
  1. 1. J Briand,P Chevallitr,N Tavernivee,J Rozet (1971). Observation of K Hyper satellites and KL satellites in the X-ray spectrum of doubly K ionized Gallium. Phys. Rev. Letters, 27, 777.
  2. 2. (1982). interaction on K X-ray hyper satellite Spectra. Phys. Rev. A, 25, 391.
  3. 3. R Diamant,R Huotan,S Hamiainem,C Kao,M Deutch (2000). Cu K Ξ±(1,2) Hyper satellites threshold evolution of hollow atom X-ray spectrum. Super Phys.Rev.A, 62
  4. 4. J Hoszowska,J Cl,Y Dousse,W Kayser,J Cao,M Szlachetko,Kavcic (2007). Evolution of the electronelectron scattering contribution to the double 1s photo ionization cross-section for low-Z elements. physical review, 1-3.
  5. 5. M Berset,J.-Cl Dousse,K Fennane,J Hoszowska,J Szlachetko,M Szlachetko (2004). double K-shell photo ionization of Mg, Al and Si from threshold to saturation. Physical Riv, 2404, 1-3.
  6. 6. S Raju,B Seetharami,M Reddy,L Murti,Mombasawala (1992). A study of X-ray hyper satellites and KMM radiative auger effect of the elements 19 <Z <25 by photo excitation. Indian J.Phys, 66, 797.
  7. 7. Hannspeter Winter,Friedrich Aumayr (1999). Hollow atoms. Journal of Physics B: Atomic, Molecular and Optical Physics, 32(7), R39-R65.
  8. 8. Kengo Moribayashi,Akira Sasaki,T Tajima (1999). X-ray emission by ultrafast inner-shell ionization from vapors of Na, Mg, and Al. Physical Review A, 59(4), 2732-2737.
  9. 9. Ian Hughes (1995). Charge of the hollow atom. Physics World, 8(4), 43-48.
  10. 10. J Desclaux,C BrianΓ§on,J Thibaud,R Walen,R Walen (1974). Breit Interaction and DoubleKVacancies in Nuclear Transitions. Physical Review Letters, 32(9), 447-450.
  11. 11. W WΓΆlfli,Ch Stoller,G Bonani,M Suter,M StΓΆckli (1975). Two-Electron-One-Photon Transitions in Heavy-Ion Collisions. Physical Review Letters, 35(10), 656-659.
  12. 12. J Briand,L De Billy,P Charles,S Essabaa,P Briand,P Geller,J Desclaux,S Bliman,C Ristori (1990). production of hollowatoms by the excitation of highlycharged ions in interaction with ametallic surface. Phys. Rev. Lett, 65, 159.
  13. 13. J Briand,S Thuriez,G Giardino,G Borsoni,M Froment,M Eddrief,C Sebeene (1996). Unknown Title. Phys. Rev. Lett, 77, 1452.
  14. 14. E Kanter,R Dunford,B Krassig,S Southworth (1999). Double K-vacancy production in molybdenumby X-ray photoionization. phys. Rev. Lett, 83, 508.
  15. 15. L Kiernan,E Kennedy,J-P Mosnier,J Costello,B Sonntag (1994). First observation of a photon-induced triply excited state in atomic lithium. Physical Review Letters, 72(15), 2359-2362.
  16. 16. Patrick Richard,W Hodge,C Moore (1972). Direct Observation ofKΞ±Hypersatellites in Heavy-Ion Collisions. Physical Review Letters, 29(7), 393-395.
  17. 17. Y Awaya,M Akibe,T Katou,H Kumagai,Y Tendow,K Izumo,T Takahashi,M Okano,T Hamada (1977). Unknown Title. Phys. Lett, 61, 111.
  18. 18. J Briand,A Touai,M Frilley,P Chevallier,L Jhonson,J Rozet,M Taverllier,S Shafroth,M Krause (1976). The structure of K Ξ± hypersatellites Spectra of Cu, Ni and Fe as a test of intermediate coupling. J.Phy-B, 9, 1055.
  19. 19. O Keski-Rahkonen,J Saijonmaa,M Suvanen,A Servomaa (1977). KΞ±hHypersatellite Spectra and K Shell Double Photoionization Cross Sections of Elemental Mg, V, Cr, Mn, and Fe. Physica Scripta, 16(3-4), 105-108.
  20. 20. P Suresh,B Reddy,T Reddy,M Raju,B Rao,B Rao,M Murti (2000). K x-ray satellite spectrum of Al by photon excitation. Journal of Physics B: Atomic, Molecular and Optical Physics, 33(8), 1645-1652.
  21. 21. P Richard,C Moore (1972). Level structure of N=49 nuclei up to an excitation energy. Phys. Rev. Letts, 29, 395.
  22. 22. J Slater (1960). Quantum Theory of Atomic Structure. Quantum Theory of Atomic Structure
  23. 23. S Soni (1998). X-ray spectroscopy and allied area. J. Phys. B. At. Mol. Opt. Phys, 31, 1695.
  24. 24. Katarzyna Slabkowska,Marek Polasik (2009). Systematic multicon fugeration Dirac-Fock method study of the K X-ray spectra of silicon. J. Phys, 163, 12040.
  25. 25. M Krause,J Ferreira (1975). The structure of K Ξ± hyper satellite spectra of Cu, Niand Fe asatest of intermediate coupling. J.Phys, 88, 2007.
  26. 26. K Mvr Murti,V Rao,V Murthy,M Gopala Krishna,K Raju,Parthasaradhi (1988). Experimental values of K Ξ± L 1 /K Ξ± L 0 intensity ratio. Indian J. Phys, 62, 90.
  27. 27. Krvosm Kawatsura (1977). X-ray emissionspectrainduced by ion atom collisions II or effects of chemical bonding and multiple ionization on X-ray spectra. Phys. Rev, 47(2)
  28. 28. R Watson,F Jonson,T Chiao (1974). Z dependance of K X-ray satellite structure in heavy ion atom collisions. Phys. Rev, 10, 4.
  29. 29. K Narayana,B Reddy,S Raju,T Reddy,S Narayana,K Premachand,B Rao,M Murti,L Mombasawala (2005). Evidence for resonance electron transfer in photon excited X-ray satellite spectra of fluorine compounds. Pramana, 65(2), 285-290.

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. "High Energy K X-Ray Hypersatellites". Global Journal of Science Frontier Research - A: Physics & Space Science GJSFR-A Volume 15 (GJSFR Volume 15 Issue 31 (A4)).

More Citation Formats

Download Citation

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
August 3, 2015

Language
English
Order Article Reprint
Experience in AR

Explore published articles in an immersive Augmented Reality environment. Our platform converts research papers into interactive 3D books, allowing readers to view and interact with content using AR and VR compatible devices.

Read in 3D

Your published article is automatically converted into a realistic 3D book. Flip through pages and read research papers in a more engaging and interactive format.

Article Matrices
Total Views: 1.1K
Total Downloads: 92
All Trends

Request Access

Please fill out the form below to request access to this research paper. Your request will be reviewed by the editorial or author team.
X

This is the heading

Lorem ipsum dolor sit amet, consectetur adipiscing elit. Ut elit tellus, luctus nec ullamcorper mattis, pulvinar dapibus leo.

High-quality academic research articles on global topics and journals.

High Energy K X-Ray Hypersatellites

Zewdu Fetene
Zewdu Fetene Debre Tabor University