Comparison of Martian meteorites with earth composition: Study of effective atomic numbers in the energy range 1 keV-100 GeV

Journal Article · Mon Apr 18 00:00:00 EDT 2016 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.4945945· OSTI ID:22591198

Ün, Adem; Han, İbrahim ^[1]; Ün, Mümine ^[2]

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1. Ağrı İbrahim Çeçen University, Faculty of Arts and Sciences, Department of Physics, 04100 Ağrı (Turkey)
2. Ağrı İbrahim Çeçen University, Vocational School, Department of Electricity and Energy, 04100 Ağrz (Turkey)

Effective atomic (Z{sub eff}) and electron numbers (N{sub eff}) for 24 Martian meteorites have been determined in the energy range from 1 keV to 100 GeV and also for sixteen significant energies of commonly used radioactive sources. The values of Z{sub eff} and N{sub eff} for all sample were obtained from the DirectZeff program. The obtained results for Martian meteorites have been compared with the results for Earth composition and similarities or differences also evaluated.

• OSTI ID: 22591198
• Journal Information: AIP Conference Proceedings, Vol. 1726, Issue 1; Conference: ICANAS 2016: International conference on advances in natural and applied sciences, Antalya (Turkey), 21-23 Apr 2016; Other Information: (c) 2016 Author(s); Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ATOMIC NUMBER
COMPARATIVE EVALUATIONS
COMPUTER CALCULATIONS
D CODES
EARTH PLANET
ELECTRONIC STRUCTURE
GEV RANGE
KEV RANGE
MARS PLANET
METEORITES
RADIATION SOURCES