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1. Search for low mass dark matter in DarkSide-50: the bayesian network approach

Author

Collaboration, The DarkSide-50, Agnes, P., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Ave, M., Back, H. O., Batignani, G., Biery, K., Bocci, V., Bonivento, W. M., Bottino, B., Bussino, S., Cadeddu, M., Cadoni, M., Calaprice, F., Caminata, A., Campos, M. D., Canci, N., Caravati, M., Cargioli, N., Cariello, M., Carlini, M., Cataudella, V., Cavalcante, P., Cavuoti, S., Chashin, S., Chepurnov, A., Cicalò, C., Covone, G., D'Angelo, D., Davini, S., De Candia, A., De Cecco, S., De Filippis, G., De Rosa, G., Derbin, A. V., Devoto, A., D'Incecco, M., Dionisi, C., Dordei, F., Downing, M., D'Urso, D., Fairbairn, M., Fiorillo, G., Franco, D., Gabriele, F., Galbiati, C., Ghiano, C., Giganti, C., Giovanetti, G. K., Goretti, A. M., di Cortona, G. Grilli, Grobov, A., Gromov, M., Guan, M., Gulino, M., Hackett, B. R., Herner, K., Hessel, T., Hosseini, B., Hubaut, F., Hungerford, E. V., Ianni, An., Ippolito, V., Keeter, K., Kendziora, C. L., Kimura, M., Kochanek, I., Korablev, D., Korga, G., Kubankin, A., Kuss, M., La Commara, M., Lai, M., Li, X., Lissia, M., Longo, G., Lychagina, O., Machulin, I. N., Mapelli, L. P., Mari, S. M., Maricic, J., Messina, A., Milincic, R., Monroe, J., Morrocchi, M., Mougeot, X., Muratova, V. N., Musico, P., Nozdrina, A. O., Oleinik, A., Ortica, F., Pagani, L., Pallavicini, M., Pandola, L., Pantic, E., Paoloni, E., Pelczar, K., Pelliccia, N., Piacentini, S., Pocar, A., Poehlmann, D. M., Pordes, S., Poudel, S. S., Pralavorio, P., Price, D. D., Ragusa, F., Razeti, M., Razeto, A., Renshaw, A. L., Rescigno, M., Rode, J., Romani, A., Sablone, D., Samoylov, O., Sandford, E., Sands, W., Sanfilippo, S., Savarese, C., Schlitzer, B., Semenov, D. A., Shchagin, A., Sheshukov, A., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stracka, S., Suvorov, Y., Tartaglia, R., Testera, G., Tonazzo, A., Unzhakov, E. V., Vishneva, A., Vogelaar, R. B., Wada, M., Wang, H., Wang, Y., Westerdale, S., Wojcik, M. M., Xiao, X., Yang, C., Zuzel, G., Royal Holloway [University of London] (RHUL), Escola Politecnica da Universidade de Sao Paulo [Sao Paulo], Pacific Northwest National Laboratory (PNNL), Augustana University, Istituto Nazionale di Fisica Nucleare [Pisa] (INFN), Istituto Nazionale di Fisica Nucleare (INFN), Fermi National Accelerator Laboratory (Fermilab), Istituto Nazionale di Fisica Nucleare [Sezione di Roma 1] (INFN), Istituto Nazionale di Fisica Nucleare, Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari (INFN, Sezione di Cagliari), Università degli studi di Genova = University of Genoa (UniGe), Princeton University, Istituto Nazionale di Fisica Nucleare, Sezione di Genova (INFN, Sezione di Genova), King‘s College London, University of Naples Federico II = Università degli studi di Napoli Federico II, D.V. Skobeltsyn Institute of Nuclear Physics (SINP), Lomonosov Moscow State University (MSU), Università degli Studi di Milano = University of Milan (UNIMI), INFN Laboratori Nazionali del Gran Sasso, Istituto Nazionale di Fisica Nucleare, Sezione di Roma 3 (INFN, Sezione di Roma 3), University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS), Università degli Studi di Sassari = University of Sassari [Sassari] (UNISS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), National Research Center 'Kurchatov Institute' (NRC KI), Moscow State Engineering Physics Institute (MEPhI), Institute of High Energy Physics [Beijing] (IHEP), Chinese Academy of Sciences [Changchun Branch] (CAS), INFN---Laboratori Nazionali del Sud (LNS), Via S. Sofia 62, 95123 Catania, Italy, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), University of Houston, Black Hills State University, Nicolaus Copernicus Astronomical Cente (AstroCeNT), Joint Institute for Nuclear Research (JINR), Belgorod National Research University, 308015 Belgorod, Russia, Kurchatov NBIC Centre, National Research Centre, Kurchatov Institute, University of California (UC), University of Hawai'i [Honolulu] (UH), Laboratoire National Henri Becquerel (LNHB), Département Métrologie Instrumentation & Information (DM2I), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département d'instrumentation Numérique (DIN (CEA-LIST)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Università degli Studi di Perugia = University of Perugia (UNIPG), University of California [Davis] (UC Davis), Laboratori Nazionali del Sud (INFN), Uniwersytet Jagielloński w Krakowie = Jagiellonian University (UJ), University of Manchester [Manchester], Istituto Nazionale di Fisica Nucleare, Sezione di Milano (INFN), Virginia Tech [Blacksburg], Università degli Studi di Cagliari = University of Cagliari (UniCa), University of California [Riverside] (UC Riverside), the IN2P3-COPIN consortium (Grant No. 20-152), DarkSide-50 Collaboration, ANR-10-LABX-0023,UnivEarthS,Earth - Planets - Universe: observation, modeling, transfer(2010), ANR-18-IDEX-0001,Université de Paris,Université de Paris(2018), European Project: 952480,DarkWave, Agnes, P., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Ave, M., Back, H. O., Batignani, G., Biery, K., Bocci, V., Bonivento, W. M., Bottino, B., Bussino, S., Cadeddu, M., Cadoni, M., Calaprice, F., Caminata, A., Campos, M. D., Canci, N., Caravati, M., Cargioli, N., Cariello, M., Carlini, M., Cataudella, V., Cavalcante, P., Cavuoti, S., Chashin, S., Chepurnov, A., Cical??, C., Covone, G., D'Angelo, D., Davini, S., De Candia, A., De Cecco, S., De Filippis, G., De Rosa, G., Derbin, A. V., Devoto, A., D'Incecco, M., Dionisi, C., Dordei, F., Downing, M., D'Urso, D., Fairbairn, M., Fiorillo, G., Franco, D., Gabriele, F., Galbiati, C., Ghiano, C., Giganti, C., Giovanetti, G. K., Goretti, A. M., Grilli di Cortona, G., Grobov, A., Gromov, M., Guan, M., Gulino, M., Hackett, B. R., Herner, K., Hessel, T., Hosseini, B., Hubaut, F., Hungerford, E. V., Ianni, An., Ippolito, V., Keeter, K., Kendziora, C. L., Kimura, M., Kochanek, I., Korablev, D., Korga, G., Kubankin, A., Kuss, M., La Commara, M., Lai, M., Li, X., Lissia, M., Longo, G., Lychagina, O., Machulin, I. N., Mapelli, L. P., Mari, S. M., Maricic, J., Messina, A., Milincic, R., Monroe, J., Morrocchi, M., Mougeot, X., Muratova, V. N., Musico, P., Nozdrina, A. O., Oleinik, A., Ortica, F., Pagani, L., Pallavicini, M., Pandola, L., Pantic, E., Paoloni, E., Pelczar, K., Pelliccia, N., Piacentini, S., Pocar, A., Poehlmann, D. M., Pordes, S., Poudel, S. S., Pralavorio, P., Price, D. D., Ragusa, F., Razeti, M., Razeto, A., Renshaw, A. L., Rescigno, M., Rode, J., Romani, A., Sablone, D., Samoylov, O., Sandford, E., Sands, W., Sanfilippo, S., Savarese, C., Schlitzer, B., Semenov, D. A., Shchagin, A., Sheshukov, A., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stracka, S., Suvorov, Y., Tartaglia, R., Testera, G., Tonazzo, A., Unzhakov, E. V., Vishneva, A., Vogelaar, R. B., Wada, M., Wang, H., Wang, Y., Westerdale, S., Wojcik, M. M., Xiao, X., Yang, C., Zuzel, G., INFN Laboratori Nazionali del Gran Sasso, (INFN), Saint Petersburg Nuclear Physics Institute RAS, St Petersburg Nuclear Physics Institute, and DarkSide-50

Subjects
instrumentation, detector response, Cosmology and Nongalactic Astrophysics (astro-ph.CO), dark matter, mass, low, detector, Markov chain, FOS: Physical sciences, parametric, spectrum analysis, background, spectrum, Bayesian, dark matter, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Monte Carlo, Markov chain, particle transport, network, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Bayesian Networks, distribution function, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], signal processing, Monte Carlo, Statistical inference, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present a novel approach for the search of dark matter in the DarkSide-50 experiment, relying on Bayesian Networks. This method incorporates the detector response model into the likelihood function, explicitly maintaining the connection with the quantity of interest. No assumptions about the linearity of the problem or the shape of the probability distribution functions are required, and there is no need to morph signal and background spectra as a function of nuisance parameters. By expressing the problem in terms of Bayesian Networks, we have developed an inference algorithm based on a Markov Chain Monte Carlo to calculate the posterior probability. A clever description of the detector response model in terms of parametric matrices allows us to study the impact of systematic variations of any parameter on the final results. Our approach not only provides the desired information on the parameter of interest, but also potential constraints on the response model. Our results are consistent with recent published analyses and further refine the parameters of the detector response model., Comment: 24 pages, 12 figures, 1 table

Published
2023

2. Measurements and computational analysis on the natural decay of $^{176}$Lu

Author

Quarati, F. G. A., Bollen, G., Dorenbos, P., Eibach, M., Gulyuz, K., Hamaker, A., Izzo, C., Keblbeck, D. K., Mougeot, X., Puentes, D., Redshaw, M., Ringle, R., Sandler, R., Surbrook, J., Yandow, I., Delft University of Technology (TU Delft), National Superconducting Cyclotron Laboratory (NSCL), Michigan State University [East Lansing], Michigan State University System-Michigan State University System, Facility for Rare Isotope Beams and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824 (FRIB), Central Michigan University (CMU), Universität Greifswald - University of Greifswald, Michigan State University System, Laboratoire National Henri Becquerel (LNHB), Département Métrologie Instrumentation & Information (DM2I), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département d'instrumentation Numérique (DIN (CEA-LIST)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), and European Project: 605728,EC:FP7:PEOPLE,FP7-PEOPLE-2013-COFUND,P.R.I.M.E.(2014)

Subjects
instrumentation, spectroscopy, [PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th], Decay data measurement, FOS: Physical sciences, Primary activity measurement, 176Lu, spectrum analysis, Lutetium, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], High Energy Physics - Experiment, spectrometry, High Energy Physics - Experiment (hep-ex), metrology, radioactivity, beta-rays, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), ionizing radiation, beta spectrum, Nuclear Experiment, nuclear instrumentation
Abstract

International audience; Background: Mainly because of its long half-life and despite its scientific relevance, spectroscopic measurements of 176Lu beta decays are very limited and lack formulation of shape factors. Direct measurement of its Q-value is also presently unreported. In addition, the description of forbidden decays provides interesting challenges for nuclear theory. The comparison of precise experimental results with theoretical calculations for these decays can help to test underlying models and can aid the interpretation of data from other experiments.Purpose: Perform the first precision measurement of 176Lu beta-decay spectrum and attempt the observation of its electron capture decays, as well as perform the first precision direct measurement of the 176Lu beta-decay Q-value. Compare the shape of the precisely determined experimental beta-spectrum to theoretical calculations, and compare the end-point energy to that obtained from an independent Q-value measurement.Method: The 176Lu beta-decay spectra and the search for electron capture decays were measured with an experimental set-up that employed lutetium-based scintillator crystals and an NaI(Tl) spectrometer for coincidence counting. The beta-decay Q-value was determined via high-precision Penning trap mass spectrometry (PTMS) with the LEBIT facility at the National Superconducting Cyclotron Laboratory. The beta-spectrum calculations were performed within the Fermi theory formalism with nuclear structure effects calculated using a shell model approach.Results: Both beta transitions of 176Lu were experimentally observed and corresponding shape factors formulated in their entire energy ranges. Search for electron captures decay branches led to an experimental upper limit of 6.3x10-6 compared to its beta decays. The 176Lu beta-decay and electron capture Q-values were measured using PTMS to be 1193.0(6) keV and 108.9(8) keV, respectively. This enabled precise beta end-point energies of 596.2(6) keV and 195.3(6) keV for the primary and secondary beta-decays, respectively, to be determined. The conserved vector current hypothesis was applied to calculate the relativistic vector matrix elements. The beta-spectrum shape was shown to significantly depend on the Coulomb displacement energy and on the value of the axial vector coupling constant gA, which was extracted according to different assumptions.

Published
2023

3. Spectral unmixing applied to fast identification of γ-emitting radionuclides using NaI(Tl) detectors

Author

Thiam, C., Bobin, C., Lourenço, V., Chisté, V., Amiot, M.-N., Mougeot, X., Lacour, D., Rigoulay, F., Ferreux, L., Paradis, H., Bobin, J., Bouchard, J., André, R., de Vismes Ott, A., Thévenin, M., Laboratoire National Henri Becquerel (LNHB), Département Métrologie Instrumentation & Information (DM2I), Laboratoire d'Intégration des Systèmes et des Technologies (LIST), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Radioprotection et de Sûreté Nucléaire (IRSN), Laboratoire de Cosmologie et Statistiques (LCS - COSMOSTAT), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, IRSN - LABORATOIRE DE MESURE DE LA RADIOACTIVITE DANS L'ENVIRONNEMENT, IRSN - LABORATOIRE DE MESURE DE LA RADIOACTIVITE DANS L'ENVIRONNEMENT,Bois des Rames, 91400, Orsay, France, Service de physique de l'état condensé (SPEC - UMR3680), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département d'instrumentation Numérique (DIN (CEA-LIST)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire d'Électronique et Traitement du Signal (LETS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Institut Rayonnement Matière de Saclay (IRAMIS), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay

Subjects
Signal processing, Ionizing radiation, Monte Carlo method, Nuclear material, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 010403 inorganic & nuclear chemistry, 01 natural sciences, 030218 nuclear medicine & medical imaging, 03 medical and health sciences, 0302 clinical medicine, Optics, Multiplicative update algorithm, [INFO.INFO-TS]Computer Science [cs]/Signal and Image Processing, Automatic decision-making, Environmental analysis, Monte Carlo, nuclear instrumentation, ComputingMilieux_MISCELLANEOUS, gamma spectrometry, Physics, [PHYS]Physics [physics], Radionuclide, Radiation, business.industry, NaI(Tl) detector, Spectrometry, Detector, gamma-rays, Spectrum analysis, 0104 chemical sciences, Radioactivity, Inverse problem, business, [STAT.ME]Statistics [stat]/Methodology [stat.ME], Spectroscopic measurements, Spectral unmixing
Abstract

International audience; Spectral unmixing was investigated for fast spectroscopic identification in γ-emitter mixtures at low-statistics in the case of measurements performed to prevent illegal nuclear material trafficking or for in situ environmental analysis following a radiological or nuclear accident. For that purpose, a multiplicative update algorithm based on full-spectrum analysis was tested in the case of a 3″x3″ NaI(Tl) detector. Automatic decision-making was addressed using Monte Carlo calculations of decision thresholds and detection limits. The first results obtained with a portable instrument equipped with a 3″x3″ NaI(Tl) detector designed for the control of food samples by non-expert users following a radiological or nuclear accident, are also presented.

Published
2020

4. Direct determination of the $^{138}$La β-decay Q value using Penning trap mass spectrometry

Author

Sandler, R., Bollen, G., Dissanayake, J., Eibach, M., Gulyuz, K., Hamaker, A., Izzo, C., Mougeot, X., Puentes, D., Quarati, F. G. A., Redshaw, M., Ringle, R., Yandow, I., Central Michigan University (CMU), National Superconducting Cyclotron Laboratory (NSCL), Michigan State University [East Lansing], Michigan State University System-Michigan State University System, TRIUMF [Vancouver], Laboratoire National Henri Becquerel (LNHB), Département Métrologie Instrumentation & Information (DM2I), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département d'instrumentation Numérique (DIN (CEA-LIST)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Delft University of Technology (TU Delft), Laboratoire d'Intégration des Systèmes et des Technologies (LIST), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay

Subjects
instrumentation, data decay measurement, spectrum analysis, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear Structure, spectrometry, 138Ba, radioactivity, 138Ce, forbidden decays, beta-rays, 138La, ionizing radiation, Nuclear Experiment, nuclear instrumentation, mass spectrometry
Abstract

Background: The understanding and description of forbidden decays provides interesting challenges for nuclear theory. These calculations could help to test underlying nuclear models and interpret experimental data. Purpose: Compare a direct measurement of the $^{138}$La $\beta$-decay $Q$ value with the $\beta$-decay spectrum end-point energy measured by Quarati et al. using LaBr$_3$ detectors [Appl. Radiat. Isot. 108, 30 (2016)]. Use new precise measurements of the $^{138}$La $\beta$-decay and electron capture (EC) $Q$ values to improve theoretical calculations of the $\beta$-decay spectrum and EC probabilities. Method: High-precision Penning trap mass spectrometry was used to measure cyclotron frequency ratios of $^{138}$La, $^{138}$Ce and $^{138}$Ba ions from which $\beta$-decay and EC $Q$ values for $^{138}$La were obtained. Results: The $^{138}$La $\beta$-decay and EC $Q$ values were measured to be $Q$ = 1052.42(41) keV and $Q_{EC}$ = 1748.41(34) keV, improving the precision compared to the values obtained in the most recent atomic mass evaluation [Wang, et al., Chin. Phys. C 41, 030003 (2017)] by an order of magnitude. These results are used for improved calculations of the $^{138}$La $\beta$-decay shape factor and EC probabilities. New determinations for the $^{138}$Ce 2EC $Q$ value and the atomic masses of $^{138}$La, $^{138}$Ce, and $^{138}$Ba are also reported. Conclusion: The $^{138}$La $\beta$-decay $Q$ value measured by Quarati et al. is in excellent agreement with our new result, which is an order of magnitude more precise. Uncertainties in the shape factor calculations for $^{138}$La beta-decay using our new $Q$ value are reduced by an order of magnitude. Uncertainties in the EC probability ratios are also reduced and show improved agreement with experimental data., Comment: Nine pages, eight figures

Published
2019

5. Metallic Magnetic Calorimeters for Beta Spectrometry.

Author

Loidl, M., Rodrigues, M., Censier, B., Kowalski, S., Mougeot, X., Cassette, P., Branger, T., and Lacour, D.

Subjects
CALORIMETERS, DETECTORS, BETA ray spectrometry, SPECTRUM analysis, IONIZING radiation
Abstract

We are developing metallic magnetic calorimeters for beta spectrometry in the context of ionizing radiation metrology. The aim is the determination of the shape factors of beta spectra. Our latest detector has been designed to measure the spectrum of 241Pu, a pure beta emitter with an endpoint energy of 20.8 keV. We present the spectrum resulting from our first measurement and compare it with theoretical spectra. [ABSTRACT FROM AUTHOR]

Published
2009
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6. New excited states in the halo nucleus 6He

Author

Mougeot, X., Lapoux, V., Mittig, W., Alamanos, N., Auger, F., Avez, B., Beaumel, D., Blumenfeld, Y., Dayras, R., Drouart, A., Force, C., Gaudefroy, L., Gillibert, A., Guillot, J., Iwasaki, H., Al Kalanee, T., Keeley, N., Nalpas, L., Pollacco, E.C., and Roger, T.

Subjects
*HELIUM isotopes, *SPECTRUM analysis, *NEUTRON beams, *NUCLEAR reactions, *PARTICLES (Nuclear physics), *ANGULAR distribution (Nuclear physics), *MICROSCOPY
Abstract

Abstract: The low-lying spectroscopy of 6He was investigated via the 2-neutron transfer reaction with the 8He beam delivered by the SPIRAL facility at . The light charged particles produced by the direct reactions were measured using the MUST2 Si-strip telescope array. Above the known state, two new resonances were observed: at (width ) and at with . Through the analysis of the angular distributions, they correspond to a state and to an state, respectively. These new states, challenging the nuclear theories, could be used as benchmarks for checking the microscopic inputs of the newly improved structure models, and should trigger development of models including the treatments of both core excitation and continuum coupling effects. [Copyright &y& Elsevier]

Published
2012
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7. Study of the Influence of the Source Quality on the Determination of the Shape Factor of Beta Spectra.

Author

Le-Bret, C., Loidl, M., Rodrigues, M., Mougeot, X., and Bouchard, J.

Subjects
CALORIMETERS, NUCLEAR counters, SPECTRUM analysis, ABSORPTION, COMPARATIVE studies, SCIENTIFIC observation
Abstract

We are developing metallic magnetic calorimeters for beta spectrometry with the aim of determining the shape factors of beta spectra. The beta emitter is enclosed inside the detector absorber and the absorber size is chosen such that the detection efficiency is close to 100% for the entire spectrum. The nature of the deposit of the beta emitter is critical for precise measurement. A dependence of the shape of the spectrum on the quality of the source has been observed, supposedly due to interactions between the electrons and the deposit itself. We chose for this comparative study a nuclide with an allowed transition whose theoretical spectrum is relatively well-known, Ni, a pure beta emitter with an endpoint energy of 66.98 keV. Results of measurements of Ni deposited with different techniques are presented and compared to each other and to the theoretical spectrum. [ABSTRACT FROM AUTHOR]

Published
2012
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8. Consistent calculation of the screening and exchange effects in allowed β- transitions.

Author

Mougeot, X. and Bisch, C.

Subjects
*ATOMS, *ELECTRON waveguides, *SPECTRUM analysis, *SPATIAL analysis (Statistics), *PARTICLES, *ACCURACY
Abstract

The atomic exchange effect has previously been demonstrated to have a great influence at low energy on the 241 Pu β- transition. The screening effect has been given as a possible explanation for a remaining discrepancy. Improved calculations have been made to consistently evaluate these two atomic effects, compared here to the recent high-precision measurements of 241 Pu and 63Ni β spectra. In this paper a screening correction has been defined to account for the spatial extension of the electron wave functions. Excellent overall agreement of about 1% from 500 eV to the end-point energy has been obtained for both β spectra, which demonstrates that a rather simple ß decay model for allowed transitions, including atomic effects within an independent-particle model, is sufficient to describe well the current most precise measurements. [ABSTRACT FROM AUTHOR]

Published
2014
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9. Beta spectrometry with metallic magnetic calorimeters.

Author

Loidl, M., Rodrigues, M., Le-Bret, C., and Mougeot, X.

Subjects
*BETA ray spectrometry, *CALORIMETRY, *MAGNETIC properties of metals, *CRYOGENICS, *SPECTRUM analysis, *ELECTROPLATING
Abstract

Abstract: Metallic magnetic calorimeters are a specific type of cryogenic detectors that have been shown to enable precise measurement of the shape of low energy beta spectra. The aim of their use at LNHB is the determination of the shape factors of beta spectra. The beta source is enclosed in the detector absorber, allowing for very high detection efficiency. It has turned out that the type of source is of crucial importance for the correctness of the measured spectrum. Spectra of 63Ni measured with several sources prepared by drying a NiCl2 solution differ from one another and from theory, whereas spectra measured with electroplated sources are reproducible and agree with theory. With these latter measurements we could confirm the atomic exchange effect down to very low energy (200eV). [Copyright &y& Elsevier]

Published
2014
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10. First measurement of the beta spectrum of 241Pu with a cryogenic detector

Author

Loidl, M., Rodrigues, M., Censier, B., Kowalski, S., Mougeot, X., Cassette, P., Branger, T., and Lacour, D.

Subjects
*BETA decay, *LOW temperature engineering, *METALLIC composites, *RADIOACTIVITY measurements, *SPECTRUM analysis, *IONIZING radiation, *PLUTONIUM isotopes
Abstract

Abstract: The LNE-LNHB is developing metallic magnetic calorimeters, a specific type of cryogenic detectors, for beta spectrometry. The aim is the determination of the shape factors of beta spectra. Our latest detector has been designed to measure the spectrum of 241Pu, a pure beta emitter with an endpoint energy of 20.8keV. In this paper, the detection principle of metallic magnetic calorimeters is explained and a detailed description is given of the realization of the detector enclosing a 241Pu source inside the detector absorber. A spectrum resulting from our first measurement is shown and compared with a theoretical spectrum. [Copyright &y& Elsevier]

Published
2010
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11. Shell gap reduction in neutron-rich nuclei

Author

Obertelli, A., Gillibert, A., Alamanos, N., Alvarez, M., Auger, F., Dayras, R., Drouart, A., de France, G., Jurado, B., Keeley, N., Lapoux, V., Mittig, W., Mougeot, X., Nalpas, L., Pakou, A., Patronis, N., Pollacco, E.C., Rejmund, F., Rejmund, M., and Roussel-Chomaz, P.

Subjects
*PARTICLES (Nuclear physics), *SPECTRUM analysis, *NUCLEAR physics, *MATHEMATICS
Abstract

Abstract: The spectroscopy of 27Ne has been investigated through the one-neutron transfer reaction 26Ne()27Ne in inverse kinematics at 9.7 MeV/nucleon. The results strongly support the existence of a low-lying negative parity state in 27Ne, which is a signature of a reduced sd–fp shell gap in the neutron-rich region, at variance with stable nuclei. [Copyright &y& Elsevier]

Published
2006
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