Charged particle induced reaction cross section data for production of the emerging medically important positron emitter 64Cu: A comprehensive evaluation
Abstract The radionuclide 64Cu (T 1/2= 12.7 h) is an important non-standard positron
emitter, suitable for combining PET imaging and targeted therapy. Its production in no-carrier …
emitter, suitable for combining PET imaging and targeted therapy. Its production in no-carrier …
Upgrade of IAEA recommended data of selected nuclear reactions for production of PET and SPECT isotopes
A Hermanne, FT Tarkanyi, AV Ignatyuk, S Takács… - Nuclear Data …, 2021 - Elsevier
An IAEA research project was dedicated to the compilation, evaluation and recommendation
of cross-section data for the accelerator production of 11 C, 13 N, 15 O, 18 F, 64 Cu, and 124 …
of cross-section data for the accelerator production of 11 C, 13 N, 15 O, 18 F, 64 Cu, and 124 …
New measurement and evaluation of the excitation function of 64Ni (p, n) reaction for the production of 64Cu
RA Rebeles, P Van den Winkel, A Hermanne… - Nuclear Instruments and …, 2009 - Elsevier
One of the radioisotopes for which a growing interest exists in nuclear medicine is 64Cu. Its
branched decay makes it suitable for both diagnostic and therapeutic purposes. Activation …
branched decay makes it suitable for both diagnostic and therapeutic purposes. Activation …
Low-energy () reactions in Ni and Cu nuclei using a microscopic optical model
G Gangopadhyay - Physical Review C—Nuclear Physics, 2010 - APS
Radiative capture reactions for low-energy protons have been theoretically studied for Ni
and Cu isotopes using the microscopic optical model. The optical potential has been …
and Cu isotopes using the microscopic optical model. The optical potential has been …
Electron screening in nickel
J Gajević, A Cvetinović, A Likar, M Lipoglavšek… - The European Physical …, 2013 - Springer
In order to investigate the interplay between nuclei and their surroundings, we studied
proton-induced nuclear reactions over an energy range from 0.86 to 3.08 MeV for different …
proton-induced nuclear reactions over an energy range from 0.86 to 3.08 MeV for different …
Studies of the gamma-strength function and low energy levels in 65Ga using the (p, γ) average resonance method
K Nilson, L Spanier, B Erlandsson, K Vierinen… - Nuclear Physics A, 1987 - Elsevier
The 64Zn (p, γ) 65Ga reaction has been studied in the proton energy ranges Ep= 2.0–2.9
and 3.3–4.3 MeV. Using a three-crystal pair spectrometer, gamma-ray spectra of primary …
and 3.3–4.3 MeV. Using a three-crystal pair spectrometer, gamma-ray spectra of primary …
Electron screening in nickel
J Gajević, M Lipoglavšek, T Petrovič… - AIP Conference …, 2012 - pubs.aip.org
In order to investigate the interplay between nuclei and their surroundings we studied proton
induced nuclear reactions over an energy range from 1.35 to 3.08 MeV for different …
induced nuclear reactions over an energy range from 1.35 to 3.08 MeV for different …
[PDF][PDF] PROTON RADIATIVE CAPTURE BY NUCLEI 54Cr
SN Utenkov, KV Shebeko - Voprosy Atomnoj Nauki i Tekhniki …, 2005 - vant.kipt.kharkov.ua
The paper presents experimental results from proton capture reaction by nuclei 54Cr,
namely, partial cross-sections and radiative strength functions (RSF) simulated in the …
namely, partial cross-sections and radiative strength functions (RSF) simulated in the …
Radiative strength functions for nuclei in which the number of protons is close to the magic number of Z=28
ID Fedorets - Physics of Atomic Nuclei, 2001 - Springer
The distribution of the radiative strength in nuclei where the number of nucleons of one type
is nearly magic (Z= 28±1) and where there are a few valence nucleons of the other type is …
is nearly magic (Z= 28±1) and where there are a few valence nucleons of the other type is …
[PDF][PDF] Electron screening in Al and Ni metals
J Gajevic, M Škof, P Pelicon… - Proceedings of the VI …, 2011 - pos.sissa.it
Due to Coulomb repulsion, the cross-section σ for charged-particle-induced nuclear
reactions drops rapidly with decreasing beam energy. The astrophysical S-factor is usually …
reactions drops rapidly with decreasing beam energy. The astrophysical S-factor is usually …