A. A. Kwiatkowski

'Searching for a needle in a haystack;' A Ba-tagging approach for an upgraded nEXO experiment

H. Rasiwala, K. Murray, Y. Lan, C. Chambers, M. Cvitan, T. Brunner, R. Collister, T. Daniels, R. Elmansali, W. Fairbank, R. Gornea, G. Gratta, T. Koffas, A. A. Kwiatkowski, K. G. Leach, A. Lennarz, C. Malbrunot [1], D. Ray [1], R. Shaikh [1], L. Yang [1]

Abstract

nEXO is a proposed experiment that will search for neutrinoless double-beta decay (0$νββ$) in 5-tonnes of liquid xenon (LXe), isotopically enriched in $^{136}$Xe. A technique called Ba-tagging is being developed as a potential future upgrade for nEXO to detect the $^{136}$Xe double-beta decay daughter isotope, $^{136}$Ba. An efficient Ba-tagging technique has the potential to boost nEXO's 0$νββ$ sensitivity by essentially suppressing non-double-beta decay background events. A conceptual approach for the extraction from the detector volume, trapping, and identification of a single Ba ion from 5 tonnes of LXe is presented, along with initial results from the commissioning of one of its subsystems, a quadrupole mass filter.

Collision-Induced Dissociation at TRIUMF's Ion Trap for Atomic and Nuclear science

A. Jacobs, C. Andreoiu, J. Bergmann, T. Brunner, T. Dickel, I. Dillmann, E. Dunling, J. Flowerdew, L. Graham, G. Gwinner, Z. Hockenbery, B. Kootte, Y. Lan, K. G. Leach, E. Leistenschneider, E. M. Lykiardopoulou, V. Monier, I. Mukul, S. F. Paul, W. R. Plaß, M. P. Reiter, C. Scheidenberger, R. Thompson, J. L Tracy, C. Will, M. E. Wieser, M. Yavor, J. Dilling [1], A. A. Kwiatkowski

Abstract

The performance of high-precision mass spectrometry of radioactive isotopes can often be hindered by large amounts of contamination, including molecular species, stemming from the production of the radioactive beam. In this paper, we report on the development of Collision-Induced Dissociation (CID) as a means of background reduction for experiments at TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN). This study was conducted to characterize the quality and purity of radioactive ion beams and the reduction of molecular contaminants to allow for mass measurements of radioactive isotopes to be done further from nuclear stability. This is the first demonstration of CID at an ISOL-type radioactive ion beam facility, and it is shown that molecular contamination can be reduced up to an order of magnitude.

Summit of the N=40 Island of Inversion: precision mass measurements and ab initio calculations of neutron-rich chromium isotopes

R. Silwal, C. Andreoiu, B. Ashrafkhani, J. Bergmann, T. Brunner, J. Cardona, K. Dietrich, E. Dunling, G. Gwinner, Z. Hockenbery, J. D. Holt, C. Izzo, A. Jacobs, A. Javaji, B. Kootte, Y. Lan, D. Lunney, E. M. Lykiardopoulou, T. Miyagi, M. Mougeot, I. Mukul, T. Murbock, W. S. Porter [1], M. Reiter [1], J. Ringuette [1], J. Dilling, A. A. Kwiatkowski

Abstract

Mass measurements continue to provide invaluable information for elucidating nuclear structure and scenarios of astrophysical interest. The transition region between the $Z = 20$ and $28$ proton shell closures is particularly interesting due to the onset and evolution of nuclear deformation as nuclei become more neutron rich. This provides a critical testing ground for emerging ab-initio nuclear structure models. Here, we present high-precision mass measurements of neutron-rich chromium isotopes using the sensitive electrostatic Multiple-Reflection Time-Of-Flight Mass Spectrometer (MR-TOF-MS) at TRIUMF's Ion Trap for Atomic and Nuclear Science (TITAN) facility. Our high-precision mass measurements of $^{59, 61-63}$Cr confirm previous results, and the improved precision in measurements of $^{64-65}$Cr refine the mass surface beyond N=40. With the ab initio in-medium similarity renormalization group, we examine the trends in collectivity in chromium isotopes and give a complete picture of the N=40 island of inversion from calcium to nickel.

Mass Measurements of Neutron-Rich Gallium Isotopes Refine Production of Nuclei of the First r-Process Abundance Peak in Neutron Star Merger Calculations

M. P. Reiter, S. Ayet San Andrés, S. Nikas [3,4], J. Lippuner [5,6,7], C. Andreoiu [8], C. Babcock [2], B. R. Barquest, J. Bollig [2,9], T. Brunner [2,10], T. Dickel [1,3], J. Dilling [2,11], I. Dillmann [2,12], E. Dunling [2,13], G. Gwinner [14], L. Graham [2], C. Hornung [1], R. Klawitter [2,15], B. Kootte [2,14,12], A. A. Kwiatkowski, Y. Lan [2,11], D. Lascar [2,16,17], K. G. Leach, E. Leistenschneider [2,11,3,4,12,9,1], G. Martínez-Pinedo, J. E. McKay, S. F. Paul, W. R. Plaß, L. Roberts [18], H. Schatz [7,18,19], C. Scheidenberger [1,3], A. Sieverding [3,4,20,2], R. Steinbrügge, R. Thompson [21], M. E. Wieser, C. Will [1], D. Welch [18]

Abstract

We report mass measurements of neutron-rich Ga isotopes $^{80-85}$Ga with TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN). The measurements determine the masses of $^{80-83}$Ga in good agreement with previous measurements. The masses of $^{84}$Ga and $^{85}$Ga were measured for the first time. Uncertainties between $25-48$ keV were reached. The new mass values reduce the nuclear uncertainties associated with the production of A $\approx$ 84 isotopes by the \emph{r}-process for astrophysical conditions that might be consistent with a binary neutron star (BNS) merger producing a blue kilonova. Our nucleosynthesis simulations confirm that BNS merger may contribute to the first abundance peak under moderate neutron-rich conditions with electron fractions $Y_e=0.35-0.38$.

Dawning of the N=32 shell closure seen through precision mass measurements of neutron-rich titanium isotopes

E. Leistenschneider [1,2,3,4], M. P. Reiter, S. Ayet San Andrés, B. Kootte [1,5], J. D. Holt, P. Navrátil, C. Babcock [1], C. Barbieri [6,1], B. R. Barquest, J. Bergmann [3], J. Bollig [1,7], T. Brunner [1,8], E. Dunling [1,9], A. Finlay [1,2], H. Geissel [3,4], L. Graham [1], F. Greiner [3], H. Hergert [10], C. Hornung [3], C. Jesch [3], R. Klawitter [1,11], Y. Lan [1,2], D. Lascar [1,12], K. G. Leach, W. Lippert [3,1,13,7], J. E. McKay, S. F. Paul, A. Schwenk [11,14,15], D. Short [1,16], J. Simonis [17,18,1,19], V. SomÃ, R. Steinbrügge, S. R. Stroberg, R. Thompson [20], M. E. Wieser, C. Will [3], M. Yavor [21], C. Andreoiu [16], T. Dickel [3,4], I. Dillmann [1,13], G. Gwinner [5,3,4], W. R. Plaß, C. Scheidenberger [3,4,1,13], A. A. Kwiatkowski, J. Dilling [1,2]

Abstract

A precision mass investigation of the neutron-rich titanium isotopes $^{51-55}$Ti was performed at TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN). The range of the measurements covers the $N=32$ shell closure and the overall uncertainties of the $^{52-55}$Ti mass values were significantly reduced. Our results confirm the existence of a weak shell effect at $N=32$, establishing the abrupt onset of this shell closure. Our data were compared with state-of-the-art \textit{ab-initio} shell model calculations which, despite very successfully describing where the $N=32$ shell gap is strong, overpredict its strength and extent in titanium and heavier isotones. These measurements also represent the first scientific results of TITAN using the newly commissioned Multiple-Reflection Time-of-Flight Mass Spectrometer (MR-TOF-MS), substantiated by independent measurements from TITAN's Penning trap mass spectrometer.

High-precision $Q_{EC}$-value measurement of the superallowed $β^+$ emitter $^{22}$Mg and an evaluation of the $A=22$ isobaric triplet

M. P. Reiter, K. G. Leach, O. M. Drozdowski [1,4], S. R. Stroberg, J. D. Holt, C. Andreoiu [5], C. Babcock [1], B. Barquest [1], M. Brodeur [6], A. Finlay [7,1], M. Foster [8,1,7,9], A. T. Gallant, G. Gwinner [10], R. Klawitter [1,11], B. Kootte [7,1,12], A. A Kwiatkowski, Y. Lan [7,1], D. Lascar [1], E. Leistenschneider [7,1], A. Lennarz [1,13], S. Paul [1,12,14], R. Steinbrügge, R. I. Thompson, M. Wieser [14], J. Dilling [1,7]

Abstract

A direct $Q_{EC}$-value measurement of the superallowed $β^+$ emitter $^{22}$Mg was performed using TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN). The direct ground-state to ground-state atomic mass difference between $^{22}$Mg and $^{22}$Na was determined to be $Q_{EC}=4781.40(22)$~keV, representing the most precise single measurement of this quantity to date. In a continued push towards calculating superallowed isospin-symmetry-breaking (ISB) corrections from first principles, ab-initio shell-model calculations of the $A=22$ IMME are also presented for the first time using the valence-space in-medium similarity renormalization group formalism. With particular starting two- and three-nucleon forces, this approach demonstrates a level of agreement with the experimental data that suggests reliable ab-initio calculations of superallowed ISB corrections are now possible.

Electroweak Decay Studies of Highly Charged Radioactive Ions with TITAN at TRIUMF

K. G. Leach, I. Dillmann [2], R. Klawitter [2,3], E. Leistenschneider [2,4], A. Lennarz [2], T. Brunner [2,5], D. Frekers [6], C. Andreiou [7,2], A. A. Kwiatkowski, J. Dilling [2]

Abstract

Several modes of electroweak radioactive decay require an interaction between the nucleus and bound electrons within the constituent atom. Thus, the probabilities of the respective decays are not only influenced by the structure of the initial and final states in the nucleus, but can also depend strongly on the atomic charge. Conditions suitable for the partial or complete ionization of these rare isotopes occur naturally in hot, dense astrophysical environments, but can also be artificially generated in the laboratory to selectively block certain radioactive decay modes. Direct experimental studies on such scenarios are extremely difficult due to the laboratory conditions required to generate and store radioactive ions at high charge states. A new electron-beam ion trap (EBIT) decay setup with the TITAN experiment at TRIUMF has successfully demonstrated such techniques for performing spectroscopy on the radioactive decay of highly charged ions.

Improvements to TITAN's Mass Measurement and Decay Spectroscopy Capabilities

D. Lascar, A. A. Kwiatkowski, M. Alanssari, U. Chowdhury, J. Even, A. Finlay, A. T. Gallant, M. Good, R. Klawitter, B. Kootte, T. Li K. G. Leach, A. Lennarz, E. Leistenschneider, A. J. Mayer, B. E. Schultz, R. Schupp [1], D. A. Short, C. Andreoiu [1], J. Dilling [1], G. Gwinner [1]

Abstract

The study of nuclei farther from the valley of $β$-stability goes hand-in-hand with shorter-lived nuclei produced in smaller abundances than their more stable counterparts. The measurement, to high precision, of nuclear masses therefore requires innovations in technique in order to keep up. TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN) facility deploys three ion traps, with a fourth in the commissioning phase, to perform and support Penning trap mass spectrometry and in-trap decay spectroscopy on some of the shortest-lived nuclei ever studied. We report on recent advances and updates to the TITAN facility since the 2012 EMIS Conference. TITAN's charge breeding capabilities have been improved and in-trap decay spectroscopy can be performed in TITAN's electron beam ion trap (EBIT). Higher charge states can improve the precision of mass measurements, reduce the beam-time requirements for a given measurement, improve beam purity and opens the door to access, via in-trap decay and recapture, isotopes not available from the ISOL method. This was recently demonstrated during TITAN's mass measurement of $^{30}$Al. The EBIT's decay spectroscopy setup was commissioned with a successful branching ratio and half-life measurement of $^{124}$Cs. Charge breeding in the EBIT increases the energy spread of the ion bunch sent to the Penning trap for mass measurement so a new Cooler Penning Trap (CPET), which aims to cool highly charge ions with an electron plasma, is undergoing online commissioning. Already, CPET has demonstrated the trapping and self-cooling of a room-temperature electron plasma which was stored for several minutes. A new detector has been installed inside the CPET magnetic field which will allow for in-magnet charged particle detection.

Low-Background In-Trap Decay Spectroscopy with TITAN at TRIUMF

K. G. Leach, A. Lennarz [1,3], A. Grossheim [1], R. Klawitter [1,4], T. Brunner [1,5], A. Chaudhuri [1], U. Chowdhury [1,6,4,7], J. R. Crespo López-Urrutia, A. T. Gallant, A. A. Kwiatkowski, T. D. Macdonald, B. E. Schultz, S. Seeraji [2], C. Andreoiu [2], D. Frekers [3], J. Dilling [1]

Abstract

An in-trap decay spectroscopy setup has been developed and constructed for use with the TITAN facility at TRIUMF. The goal of this device is to observe weak electron-capture (EC) branching ratios for the odd-odd intermediate nuclei in the $ββ$ decay process. This apparatus consists of an up-to 6 Tesla, open-access spectroscopy ion-trap, surrounded radially by up to 7 planar Si(Li) detectors which are separated from the trap by thin Be windows. This configuration provides a significant increase in sensitivity for the detection of low-energy photons by providing backing-free ion storage and eliminating charged-particle-induced backgrounds. An intense electron beam is also employed to increase the charge-states of the trapped ions, thus providing storage times on the order of minutes, allowing for decay-spectroscopy measurements. The technique of multiple ion-bunch stacking was also recently demonstrated, which further extends the measurement possibilities of this apparatus. The current status of the facility and initial results from a $^{116}$In measurement are presented.

The TITAN in-trap decay spectroscopy facility at TRIUMF

K. G. Leach, A. Grossheim, A. Lennarz, T. Brunner, J. R. Crespo López-Urrutia, A. T. Gallant, M. Good, R. Klawitter, A. A. Kwiatkowski, T. Ma, T. D. Macdonald, S. Seeraji, M. C. Simon, C. Andreoiu, J. Dilling [1], D. Frekers [1]

Abstract

This article presents an upgraded in-trap decay spectroscopy apparatus which has been developed and constructed for use with TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN). This device consists of an open-access electron-beam ion-trap (EBIT), which is surrounded radially by seven low-energy planar Si(Li) detectors. The environment of the EBIT allows for the detection of low-energy photons by providing backing-free storage of the radioactive ions, while guiding charged decay particles away from the trap centre via the strong (up to 6 T) magnetic field. In addition to excellent ion confinement and storage, the EBIT also provides a venue for performing decay spectroscopy on highly-charged radioactive ions. Recent technical advancements have been able to provide a significant increase in sensitivity for low-energy photon detection, towards the goal of measuring weak electron-capture branching ratios of the intermediate nuclei in the two-neutrino double beta ($2νββ$) decay process. The design, development, and commissioning of this apparatus are presented together with the main physics objectives. The future of the device and experimental technique are discussed.