| Literature DB >> 31656452 |
Sarah Pfaff1, Cécile Philippe1, Lukas Nics1, Neydher Berroterán-Infante1, Katharina Pallitsch2, Christina Rami-Mark1, Ana Weidenauer3, Ulrich Sauerzopf3, Matthäus Willeit3, Markus Mitterhauser1,4, Marcus Hacker1, Wolfgang Wadsak1,5, Verena Pichler1.
Abstract
(+)-[11C]PHNO, a dopamine D2/3 receptor agonistic radiotracer, is applied for investigating the dopaminergic system via positron emission tomography (PET). An improved understanding of neuropsychiatric disorders associated with dysfunctions in the dopamine system and the underlying mechanism is a necessity in order to promote the development of new potential therapeutic drugs. In contrast to other broadly applied 11C-radiopharmaceuticals, the production of this radiotracer requires a challenging four-step radiosynthesis involving harsh reaction conditions and reactants as well as an inert atmosphere. Consequently, the production is prone to errors and troubleshooting after failed radiosyntheses remains time consuming. Hence, we aimed to optimize the radiosynthesis of (+)-[11C]PHNO for achieving better activity yields without loss of product quality. Therefore, we synthesized (+)-[11C]PHNO and omitted all heating and cooling steps leading to higher activity yields. As a result, radiosynthesis fully conducted at room temperature led to a time-reduced production procedure that saves about 5 min, which is an appreciable decay-prevention of around 15% of the activity yield. Additionally, we established a troubleshooting protocol by investigating reaction intermediates, byproducts, and impurities. Indeed, partial runs enabled the assignment of byproducts to their associated error source. Finally, we were able to generate a decision tree facilitating error detection in (+)-[11C]PHNO radiosynthesis.Entities:
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Year: 2019 PMID: 31656452 PMCID: PMC6791232 DOI: 10.1155/2019/4292596
Source DB: PubMed Journal: Contrast Media Mol Imaging ISSN: 1555-4309 Impact factor: 3.161
Figure 1Synthesis scheme for the four-step radiosynthesis of (+)-[11C]PHNO starting from cyclotron-produced [11C]CO2 and ethylmagnesium bromide.
Figure 2Chemical structure of the desired intermediate amide (compound 3) as well as nonreduced form of the side products (compounds 4 and 5) and reduced side products (compounds 6 and 7).
Figure 3Reaction scheme of partial runs A–E for investigation of reaction intermediates formed during (+)-[11C]PHNO radiosynthesis.
Figure 4Reaction scheme of partial runs G–J for investigation of reaction intermediates formed during (+)-[11C]PHNO radiosynthesis.
Figure 5Reaction steps of (+)-[11C]PHNO production according to Rami-Mark et al. [21] with the corresponding main risk for each reaction step.
Figure 6(a) Comparison of the synthesis duration of (+)-[11C]PHNO synthesis at room temperature (n = 16) and according to our previously published method including heating and cooling (n = 9). (b) Influence of the temperature at LAH addition on the isolated radiochemical yield not corrected for decay (22°C: n = 16, −15°C: n = 9, −40°C: n = 3).
Starting activity, activity yield, number of experiments, and success rate of the studied experimental setups.
| Temperature at LAH addition (°C) | Starting activity (EOB) (GBq) | Activity yield (GBq) |
| Success rate (%) |
|---|---|---|---|---|
| 22 | 120 ± 15 | 1.7 ± 1.0 | 16 | 89 |
| −15 | 122 ± 13 | 0.7 ± 0.2 | 9 | 82 |
| −40 | 113 ± 8 | 0.6 ± 0.1 | 3 | 100 |
Figure 7Analytical HPLC chromatograms of the crude reaction mixtures obtained by addition of LAH at room temperature (a) or at −40°C (b).
Figure 8Chromatogram of semipreparative HPLC of full synthesis at room temperature (a), route A synthesis without TEA and LAH (b), route E without LAH (c), and route F in which the reaction is quenched after Grignard reaction (d).
Figure 9Semipreparative HPLC chromatogram of partial run G and the corresponding analytical chromatograms of the respective peak.
Figure 10(a) UV/Vis chromatogram of [natC]propionic acid. (b) Radio-channel chromatogram of [11C]CO2.
Figure 11Schematic decision tree aiding troubleshooting after a failed (+)-[11C]PHNO formation.