2020
DOI: 10.1016/j.nima.2019.163178
|View full text |Cite
|
Sign up to set email alerts
|

A facility for direct measurements for nuclear astrophysics at IFIN-HH - a 3 MV tandem accelerator and an ultra-low background laboratory

Abstract: We present a facility for direct measurements at low and very low energies typical for nuclear astrophysics. The facility consists of a small and robust tandem accelerator where irradiations are made and an ultra-low background laboratory located in a salt mine where very low radio-activities can be measured. Both belong to "Horia Hulubei" National Institute for Physics and Nuclear Engineering (IFIN-HH), but are situated 120 km apart. Their performances are shown using a few cases where they were used. We argu… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
3
0

Year Published

2021
2021
2023
2023

Publication Types

Select...
4

Relationship

1
3

Authors

Journals

citations
Cited by 4 publications
(3 citation statements)
references
References 21 publications
0
3
0
Order By: Relevance
“…Its unique characteristics provide great environmental conditions for ultralow background dose rate monitor calibrations. According to [35], the average underground dose rate was found to be (1.17 ± 0.14) nSv h -1 .…”
Section: Dose Ratementioning
confidence: 99%
“…Its unique characteristics provide great environmental conditions for ultralow background dose rate monitor calibrations. According to [35], the average underground dose rate was found to be (1.17 ± 0.14) nSv h -1 .…”
Section: Dose Ratementioning
confidence: 99%
“…Activation spectra (offline) can be afterward measured locally at GammaSpec [39] or in the nuclear astrophysics laboratory with BEGA. In order to increase the sensitivity of our measurements through background reduction, the irradiated samples can be taken to the MicroBecquerel (μBq) laboratory [40] that is located 210 m underground, inside the Slanic Salt mine [22].…”
Section: Nuclear Physics For Astrophysicsmentioning
confidence: 99%
“…The first tests with this method were done in 2013, and since then, a number of reactions have been studied successfully [21,22,41,42], with more currently ongoing or planned for the future. Given that proton and alpha capture reactions represent an important proxy in nucleosynthesis, two of the reactions that were studied are α + 64 Zn [41] and α + 58 Ni (paper in preparation).…”
Section: Nuclear Physics For Astrophysicsmentioning
confidence: 99%