ECRIS2024 - List of Keywords (detector)

Paper	Title	Other Keywords	Page
MOP15	Study of noble gas memory effect of ECR3 at ATLAS	ECR, ion-source, experiment, ECRIS	64
	R.H. Scott, J.T. McLain, R.C. Vondrasek ANL, Lemont, Illinois, USA M. Paul, S. Bhattacharya The Hebrew University of Jerusalem, Jerusalem, Israel
	Funding: This work was supported by the U.S. Department of Energy, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357. Over the past three decades a portion of the accelerated beam time at the Argonne Tandem Linac Accelerator System (ATLAS) has been reserved for ultra-sensitive detection of argon radioisotopes. A unique noble-gas accelerator mass spectrometry (NOGAMS) technique [1] at ATLAS combines electron cyclotron resonance ion source (ECRIS) positive ion production, acceleration up to ~6 MeV/u and detection methods for separating isobars and other m/q contaminants. The ECR3 ion source was chosen for such experiments due to the limited scope of material introduced into the plasma chamber, inferring a lower background production compared to ECR2. A recent ³⁹⸴⁴²Ar NOGAMS experiment has highlighted a need to understand the beam production of material that is no longer being actively introduced into the ECRIS, known as memory effect. A quantitative study of source memory was performed to determine the decay characteristics of argon in the ECR3 ion source. Results of this study as well as details of setup and operation of ECR3 for NOGAMS experiments are presented. [1] M. Paul et al., Nucl. Instr. and Methods in Phys. Res., Sect. B, vol. 456, p. 222, 2019. doi:10.1016/j.nimb.2019.04.003
DOI •	reference for this paper ※ doi:10.18429/JACoW-ECRIS2024-MOP15
About •	Received ※ 13 September 2024 — Revised ※ 20 September 2024 — Accepted ※ 29 May 2025 — Issued ※ 07 June 2025
Cite •	reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)

THA2	Numerical design of an innovative superconducting magnetic trap for probing β-decay in ECR plasmas	plasma, injection, electron, ECR	159
	G.S. Mauro, L. Celona, G. Torrisi, A. Pidatella, E. Naselli, F. Russo, B. Mishra, G. Finocchiaro, D. Santonocito, D. Mascali INFN-LNS, Catania, Italy A. Galatà INFN-LNL, Legnaro (PD), Italy
	The main aim of Plasmas for Astrophysics Nuclear Decays Observation and Radiation for Archaeometry (PANDORA) project is to build a flexible magnetic plasma trap where plasma reaches a density nₑ ∼ 10¹¹ – 10¹³ cm⁻³, and a temperature, in units of kT, kTₑ ∼ 0.1 – 30 keV in order to measure, for the first time, nuclear β-decay rates in stellar-like conditions. Here we present the numerical design of the PANDORA magnetic system, carried out by using the commercial simulators OPERA and CST Studio Suite. In particular, we discuss the design choices taken to: 1) obtain the required magnetic field levels at relevant axial and radial positions; 2) avoid the magnetic branches along the plasma chamber wall; 3) find the optimal position for the set of plasma diagnostics that will be employed. The magnetic trap has been conceived to be as large as possible, both in radial and axial directions, in order to exploit the plasma confinement mechanism on a bigger plasmoid volume. The plasma chamber will have a length of 700 mm and a diameter of 280 mm. The magnetic trap tender procedure has been completed in June 2024 and the structure realization is expected to start in late 2024.
	Slides THA2 [6.420 MB]
DOI •	reference for this paper ※ doi:10.18429/JACoW-ECRIS2024-THA2
About •	Received ※ 25 January 2025 — Revised ※ 28 January 2025 — Accepted ※ 30 January 2025 — Issued ※ 15 June 2025
Cite •	reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)

Paper

Title

Other Keywords

Page

MOP15

Study of noble gas memory effect of ECR3 at ATLAS

ECR, ion-source, experiment, ECRIS

64

R.H. Scott, J.T. McLain, R.C. Vondrasek
ANL, Lemont, Illinois, USA
M. Paul, S. Bhattacharya
The Hebrew University of Jerusalem, Jerusalem, Israel

Funding: This work was supported by the U.S. Department of Energy, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357.
Over the past three decades a portion of the accelerated beam time at the Argonne Tandem Linac Accelerator System (ATLAS) has been reserved for ultra-sensitive detection of argon radioisotopes. A unique noble-gas accelerator mass spectrometry (NOGAMS) technique [1] at ATLAS combines electron cyclotron resonance ion source (ECRIS) positive ion production, acceleration up to ~6 MeV/u and detection methods for separating isobars and other m/q contaminants. The ECR3 ion source was chosen for such experiments due to the limited scope of material introduced into the plasma chamber, inferring a lower background production compared to ECR2. A recent ³⁹⸴⁴²Ar NOGAMS experiment has highlighted a need to understand the beam production of material that is no longer being actively introduced into the ECRIS, known as memory effect. A quantitative study of source memory was performed to determine the decay characteristics of argon in the ECR3 ion source. Results of this study as well as details of setup and operation of ECR3 for NOGAMS experiments are presented.
[1] M. Paul et al., Nucl. Instr. and Methods in Phys. Res., Sect. B, vol. 456, p. 222, 2019. doi:10.1016/j.nimb.2019.04.003

DOI •

reference for this paper ※ doi:10.18429/JACoW-ECRIS2024-MOP15

About •

Received ※ 13 September 2024 — Revised ※ 20 September 2024 — Accepted ※ 29 May 2025 — Issued ※ 07 June 2025

Cite •

reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)

THA2

Numerical design of an innovative superconducting magnetic trap for probing β-decay in ECR plasmas

plasma, injection, electron, ECR

159

G.S. Mauro, L. Celona, G. Torrisi, A. Pidatella, E. Naselli, F. Russo, B. Mishra, G. Finocchiaro, D. Santonocito, D. Mascali
INFN-LNS, Catania, Italy
A. Galatà
INFN-LNL, Legnaro (PD), Italy

The main aim of Plasmas for Astrophysics Nuclear Decays Observation and Radiation for Archaeometry (PANDORA) project is to build a flexible magnetic plasma trap where plasma reaches a density nₑ ∼ 10¹¹ – 10¹³ cm⁻³, and a temperature, in units of kT, kTₑ ∼ 0.1 – 30 keV in order to measure, for the first time, nuclear β-decay rates in stellar-like conditions. Here we present the numerical design of the PANDORA magnetic system, carried out by using the commercial simulators OPERA and CST Studio Suite. In particular, we discuss the design choices taken to: 1) obtain the required magnetic field levels at relevant axial and radial positions; 2) avoid the magnetic branches along the plasma chamber wall; 3) find the optimal position for the set of plasma diagnostics that will be employed. The magnetic trap has been conceived to be as large as possible, both in radial and axial directions, in order to exploit the plasma confinement mechanism on a bigger plasmoid volume. The plasma chamber will have a length of 700 mm and a diameter of 280 mm. The magnetic trap tender procedure has been completed in June 2024 and the structure realization is expected to start in late 2024.

Slides THA2 [6.420 MB]

DOI •

reference for this paper ※ doi:10.18429/JACoW-ECRIS2024-THA2

About •

Received ※ 25 January 2025 — Revised ※ 28 January 2025 — Accepted ※ 30 January 2025 — Issued ※ 15 June 2025

Cite •

reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)