Zobrazeno 1 - 10
of 170
pro vyhledávání: '"I. Bikit"'
Autor:
J. Knezevic, D. Mrdja, J. Hansman, K. Bikit, S. Forkapic, I. Bikit, D. Velimirovic, P. Kuzmanovic
Publikováno v:
Applied radiation and isotopes : including data, instrumentation and methods for use in agriculture, industry and medicine. 189
Standard reference sources, used for efficiency curve calibration of detector, often contain radionuclides with complex decay schemes (such as 60Co, 88Y, 152Eu …), introducing a potential problem in gamma-ray spectrometry, due to the appearance of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::133d53942a2fa78c9dd8d9d226bb10b6
https://pubmed.ncbi.nlm.nih.gov/36037728
https://pubmed.ncbi.nlm.nih.gov/36037728
Akademický článek
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Akademický článek
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Akademický článek
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Autor:
D. Mrda, I. Bikit, M. Veskovic, J. Slivka, M. Krmar, N. Todorovic, S. Forkapic, N. Jovancevic, G. Soti, J. Papuga, Matko Milin, Tamara Niksic, Suzana Szilner, Dario Vretenar
Publikováno v:
AIP Conference Proceedings.
The MIREDO (Muon Induced Rare Event Dynamic Observatory) spectrometer system will be mainly devoted for the study of cosmic muon induced nuclear reactions. The system will be developed around the 100% nominal efficiency ultra low‐background HPGe sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4c61b178cdff8aa7e2bf75cc568b2cda
https://doi.org/10.1063/1.3232145
https://doi.org/10.1063/1.3232145
Autor:
N. Jovancevic, M. Krmar, I. Bikit, D. Mrda, M. Veskovic, J. Slivka, N. Todorovic, S. Forkapic, G. Soti, J. Papuga, Matko Milin, Tamara Niksic, Suzana Szilner, Dario Vretenar
Publikováno v:
AIP Conference Proceedings.
Cosmic‐rays induced neutrons can produce measurable activity in carefully selected materials used for construction of low‐background gamma spectroscopy systems. In order to improve shielding of low‐background systems, flux of neutrons inside th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9147fa880d74acb38c3d50ee2833cb52
https://doi.org/10.1063/1.3232147
https://doi.org/10.1063/1.3232147
Autor:
I. Bikit, T. Nemes, D. Mrdja, S. Forkapic, Matko Milin, Tamara Niksic, Suzana Szilner, Dario Vretenar
Publikováno v:
AIP Conference Proceedings.
In the present paper the activity of 60Co source was measured using the full absorption, sum and random coincidences (pile up) peaks and the total spectrum area in the gamma spectra. By the exact treatment of the chance coincidence and pile‐up even
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1c6b7be65e2427a084211bb6f3bdec44
https://doi.org/10.1063/1.3232146
https://doi.org/10.1063/1.3232146
Publikováno v:
AIP Conference Proceedings.
Muons have a small cross section for interactions and high energy, so they are very penetrating and give the significant contribution to the gamma spectra of Ge detectors, even in deep underground laboratories. One of the muon interaction effects wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02c6514a7eca9e7936f6e924cc9a4ce9
https://doi.org/10.1063/1.2733069
https://doi.org/10.1063/1.2733069
Contemporary theories of dark matter predict that weakly interacting massive particles interact with matter by nuclear recoils leaving in the detector energies up 50 keV. The bremsstrahlung of 210Pb contributes to this spectral region. The 46.5 keV g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::138877d597b6595e89f75546fab4c585
https://doi.org/10.1063/1.2733054
https://doi.org/10.1063/1.2733054
Publikováno v:
AIP Conference Proceedings.
The anticosmic veto system developed around the extended range HPGe detector is described. In order to maximize the vetoing effect in the low‐energy Ge spectrum region, the Ge fast output was amplified and the subsequent CFD threshold was set above
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b2e7aa119e56dcc3e03ee4e19ca1e792
https://doi.org/10.1063/1.2733053
https://doi.org/10.1063/1.2733053