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1. Solar Neutrinos Spectroscopy with Borexino Phase-II

Author

Lino Miramonti, Matteo Agostini, Konrad Altenmueller, Simon Appel, Victor Atroshchenko, Zara Bagdasarian, Davide Basilico, Gianpaolo Bellini, Jay Benziger, Daniel Bick, Irene Bolognino, Giuseppe Bonfini, David Bravo, Barbara Caccianiga, Frank Calaprice, Alessio Caminata, Silvia Caprioli, Marco Carlini, Paolo Cavalcante, Francesca Cavanna, Alexander Chepurnov, Koun Choi, Laura Collica, Stefano Davini, Alexander Derbin, XueFeng Ding, Antonio Di Ludovico, Lea Di Noto, Ilia Drachnev, Kirill Fomenko, Andrey Formozov, Davide Franco, Federico Gabriele, Cristiano Galbiati, Michael Gschwender, Chiara Ghiano, Marco Giammarchi, Augusto Goretti, Maxim Gromov, Daniele Guffanti, Caren Hagner, Thibaut Houdy, Ed Hungerford, Aldo Ianni, Andrea Ianni, Anna Jany, Dominik Jeschke, Vladislav Kobychev, Denis Korablev, Gyorgy Korga, Tobias Lachenmaier, Matthias Laubenstein, Evgeny Litvinovich, Francesco Lombardi, Paolo Lombardi, Livia Ludhova, Georgy Lukyanchenko, Liudmila Lukyanchenko, Igor Machulin, Giulio Manuzio, Simone Marcocci, Jelena Maricic, Johann Martyn, Emanuela Meroni, Mikko Meyer, Marcin Misiaszek, Valentina Muratova, Birgit Neumair, Lothar Oberauer, Bjoern Opitz, Vsevolod Orekhov, Fausto Ortica, Marco Pallavicini, Laszlo Papp, Omer Penek, Lidio Pietrofaccia, Nelly Pilipenko, Andrea Pocar, Alessio Porcelli, Georgy Raikov, Gioacchino Ranucci, Alessandro Razeto, Alessandra Re, Mariia Redchuk, Aldo Romani, Nicola Rossi, Sebastian Rottenanger, Stefan Schöenert, Dmitrii Semenov, Mikhail Skorokhvatov, Oleg Smirnov, Albert Sotnikov, Lee F. F. Stokes, Yura Suvorov, Roberto Tartaglia, Gemma Testera, Jan Thurn, Maria Toropova, Evgenii Unzhakov, Alina Vishneva, Bruce Vogelaar, Franz von Feilitzsch, Stefan Weinz, Marcin Wojcik, Michael Wurm, Zachary Yokley, Oleg Zaimidoroga, Sandra Zavatarelli, Kai Zuber, and Grzegorz Zuzel

Subjects
solar neutrinos, neutrino oscillation, Borexino, Elementary particle physics, QC793-793.5
Abstract

Solar neutrinos have played a central role in the discovery of the neutrino oscillation mechanism. They still are proving to be a unique tool to help investigate the fusion reactions that power stars and further probe basic neutrino properties. The Borexino neutrino observatory has been operationally acquiring data at Laboratori Nazionali del Gran Sasso in Italy since 2007. Its main goal is the real-time study of low energy neutrinos (solar or originated elsewhere, such as geo-neutrinos). The latest analysis of experimental data, taken during the so-called Borexino Phase-II (2011-present), will be showcased in this talk—yielding new high-precision, simultaneous wide band flux measurements of the four main solar neutrino components belonging to the “pp„ fusion chain (pp, pep, 7 Be, 8 B), as well as upper limits on the remaining two solar neutrino fluxes (CNO and hep).

Published
2018
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2. First direct evidence of the CNO fusion cycle in the Sun with Borexino

Author

Kumaran, S., Agostini, M., Altenmüller, K., Appel, S., Atroshchenko, V., Bagdasarian, Z., Basilico, D., Bellini, G., Benziger, J., Biondi, R., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chepurnov, A., D’angelo, D., Davini, S., Derbin, A., Di Giacinto, A., Di Marcello, V., Ding, X. F., Di Ludovico, A., Di Noto, L., Drachnev, I., Formozov, A., Franco, D., Galbiati, C., Ghiano, C., Giammarchi, M., Goretti, A., Göttel, A. S., Gromov, M., Guffanti, D., Ianni, A., Jany, A., Jeschke, D., Vladislav Kobychev, Korga, G., Laubenstein, M., Litvinovich, E., Lombardi, P., Lomskaya, I., Ludhova, L., Lukyanchenko, G., Lukyanchenko, L., Machulin, I., Martyn, J., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Muratova, V., Neumair, B., Nieslony, M., Nugmanov, R., Oberauer, L., Orekhov, V., Ortica, F., Pallavicini, M., Papp, L., Pelicci, L., Penek, Ö, Pietrofaccia, L., Pilipenko, N., Pocar, A., Raikov, G., Ranalli, M. T., Ranucci, G., Razeto, A., Re, A., Redchuk, M., Romani, A., Rossi, N., Schönert, S., Semenov, D., Settanta, G., Skorokhvatov, M., Singhal, A., Smirnov, O., Sotnikov, A., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Unzhakov, E., Villante, F. L., Vishneva, A., Vogelaar, R. B., Feilitzsch, F., Wojcik, M., Wurm, M., Zavatarelli, S., Zuber, K., and Zuzel, G.

Subjects
Physics, Fusion, Direct evidence, Settore FIS/01 - Fisica Sperimentale, Astronomy, Borexino
Abstract

Proceedings of 37th International Cosmic Ray Conference - Sissa Medialab Trieste, Italy, 2021 37th International Cosmic Ray Conference, PoS(ICRC2021), Berlin, Germany - Online, 12 Jul 2021 - 23 Jul 2021; Sissa Medialab Trieste, Italy (2021). doi:10.22323/1.395.1109, The Borexino experiment has recently provided the first direct experimental evidence of the sub-dominant CNO-cycle in the Sun, which is assumed to be the main energy production mechanism in heavier stars. Borexino is a liquid scintillator detector located at the Laboratori Nazionali del Gran Sasso, Italy with the main goal to measure solar neutrinos. The extreme radiopurity of the scintillator and the successful thermal stabilisation of the detector have proven to be valuable assets in the quest for CNO neutrinos.The low abundance of CNO neutrinos and the similarity of its spectral shape to that of \emph{pep} solar neutrinos and the intrinsic 210Bi background, make CNO neutrino detection challenging. Therefore, it is necessary to constrain these backgrounds independently. The energy and radial distribution of the events can then be exploited to perform a multivariate fit, which requires a careful evaluation of the systematic uncertainty associated with the Monte-Carlo spectral shapes used. Borexino has successfully rejected the null hypothesis of CNO-cycle neutrinos in the Sun with greater than 5.0σ significance with 99% C.L. This article will present the overview of the strategy and methods used to achieve this result and the consequence of this result for solar and stellar physics., Published by Sissa Medialab Trieste, Italy

Published
2022

3. Status of cupid-mo

Author

Zolotarova, A., Armengaud, E., Augier, C., Barabash, A., Bellini, F., Benato, G., Benoît, A., Bergé, L., Besson, N., Billard, J., Bourgeois, C., Briere, M., Brudanin, V., Camus, P., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Charlieux, F., Combarieu, M., Dafinei, I., Danevich, F., Dumoulin, L., Eitel, K., Ferri, F., Fujikawa, B., Gascon, J., Gironi, L., Giuliani, A., Gros, M., Guerard, E., Huang, R., Huang, H. Z., Jesus, M., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Vladislav Kobychev, Kolomensky, Yu, Konovalov, S., Leder, A., Loaiza, P., Ma, L., Maisonobe, R., Marcillac, P., Marnieros, S., Navick, X. F., Nones, C., Novati, V., Olivieri, E., Ouellet, J., Pagnanini, L., Pari, P., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D., Polischuk, O., Previtali, E., Queguiner, E., Redon, T., Rozov, S., Rusconi, C., Sanglard, V., Schäffner, K., Schmidt, B., Shlegel, V., Siebenborn, B., Singh, V., Tomei, C., Tretyak, V., Vagneron, L., Velázquez, M., Vignati, M., Weber, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., Yumatov, V., Zolotarova, A, Armengaud, E, Augier, C, Barabash, A, Bellini, F, Benato, G, Benoit, A, Berge, L, Besson, N, Billard, J, Bourgeois, C, Briere, M, Brudanin, V, Camus, P, Cardani, L, Casali, N, Cazes, A, Chapellier, M, Charlieux, F, de Combarieu, M, Dafinei, I, Danevich, F, Dumoulin, L, Eitel, K, Ferri, F, Fujikawa, B, Gascon, J, Gironi, L, Giuliani, A, Gros, M, Guerard, E, Huang, R, Huang, H, de Jesus, M, Johnston, J, Juillard, A, Khalife, H, Kleifges, M, Kobychev, V, Kolomensky, Y, Konovalov, S, Leder, A, Loaiza, P, Ma, L, Maisonobe, R, de Marcillac, P, Marnieros, S, Navick, X, Nones, C, Novati, V, Olivieri, E, Ouellet, J, Pagnanini, L, Pari, P, Paul, B, Pavan, M, Peng, H, Pessina, G, Pirro, S, Poda, D, Polischuk, O, Previtali, E, Queguiner, E, Redon, T, Rozov, S, Rusconi, C, Sanglard, V, Schaffner, K, Schmidt, B, Shlegel, V, Siebenborn, B, Singh, V, Tomei, C, Tretyak, V, Vagneron, L, Velazquez, M, Vignati, M, Weber, M, Welliver, B, Winslow, L, Xue, M, Yakushev, E, and Yumatov, V

Subjects
double beta decay, scintillating bolometers
Abstract

CUPID-Mo is a bolometric experimental demonstrator searching for neutrinoless double beta (0ν2β) decay of 100Mo. The observation of this process, which is not allowed by the Standard Model, would determine the Majorana nature of neutrino and its mass scale. The CUPID-Mo detector array consists of 20 scintillating bolometers made of Li2100MoO4 crystals (2.34 kg of 100Mo), assembled in a compact structure of 5 suspended towers. Data taking will start soon in the EDELWEISS cryostat at the Underground Laboratory of Modane (LSM, France). The main goal of the CUPID-Mo experiment is to demonstrate “zero-background” conditions in the region of the expected 0ν2β decay signal of 100Mo over six months of measurement. The reproducibility of Li2100MoO4 scintillating bolometers with high performance should be confirmed, demonstrating the applicability of the CUPID-Mo technology for the future ton-scale 0ν2β decay bolometric experiment CUPID.

Published
2018

5. Low background scintillation setup to investigate radiopurity of materials

Author

Kasperovych, D. V., Danevich, F. A., Vladislav Kobychev, Kropivyansky, B. N., Sokur, N. V., and Tymoshenko, A. I.

Subjects
Чистые материалы и вакуумные технологии
Abstract

Background of 2.128 kg CdWO₄ scintillation detector was reduced by 3 orders of magnitude in the energy region 0.5…2.6 MeV, and one order of magnitude above 3 MeV in the low background scintillation setup located in the basement floor of a laboratory building at the Institute for Nuclear Research (Kyiv, Ukraine). It was achieved by application of radiopure passive shield, plastic scintillators to veto cosmic rays, and pulse-shape discrimination to reject fast Cherenkov signals in the quartz light-guide of the detector. Sensitivity of the setup to radioactive contamination of different materials were estimated. For instance, for a 3.36 kg titanium sample over 30 days of measurements detection limits are on the level of 2.9 mBq/kg (⁴⁰K); 0.6 mBq/kg (¹³⁷Cs); 2 mBq/kg (²²⁶Ra), and 0.5 mBq/kg (²²⁸Th). Зниження фону низькофонової сцинтиляційної установки із сцинтиляційним кристалом CdWO₄ масою 2,128 кг складає три порядки в області енергій 0,5…2,6 МеВ і один порядок для енергій більше 3 МеВ. Придушення фону було досягнуто встановленням радіоактивно чистого пасивного захисту, пластикових сцинтиляторів для відкидання сигналів від космічних частинок і розділенням сигналів від черенковського свічення у світловоді детектора за формою. Оцінено чутливість установки до радіоактивних забруднень різних матеріалів (з довірчою ймовірністю 68%), наприклад, на рівні 2,9 мБк/кг (⁴⁰K); 0,6 мБк/кг (¹³⁷Cs); 2 мБк/кг (²²⁶Ra) і 0,5 мБк/кг (²²⁸Th) для зразку титану масою 3,36 кг протягом 30 діб вимірювання. Снижение фона низкофоновой сцинтилляционной установки со сцинтилляционным кристаллом CdWO₄ массой 2,128 кг составило три порядка в области энергий 0,5…2,6 МэВ и один порядок при энергиях больше 3 МэВ. Подавление фона было достигнуто путем установки радиоактивно чистой пассивной защиты, пластиковых сцинтилляторов для отбрасывания сигналов от космических частиц и разделением сигналов от черенковского свечения в световоде детектора по форме. Оценена чувствительность установки к радиоактивным загрязнениям разных материалов (с доверительной вероятностью 68%), например, на уровне 2,9 мБк/кг (⁴⁰K); 0,6 мБк/кг (¹³⁷Cs); 2 мБк/кг (²²⁶Ra) и 0,5 мБк/кг (²²⁸Th) для образца титана массой 3,36 кг за время измерения 30 сут.

Published
2017

6. Spectrometer for slow scintillation detectors with pulse shape digitizing

Author

Podviyanuk, R. B., Vladislav Kobychev, and Chernyak, D. N.

Subjects
Physics::Instrumentation and Detectors, digital signal processing, low-counting nuclear spectrometry, molybdates, lcsh:Atomic physics. Constitution and properties of matter, tungstates, lcsh:QC170-197
Abstract

PS4TD data acquisition system for nuclear physical low background detectors on slow scintillators is described. The system is based on the ADC125AS3 14-bit 100 MHz digitizer board operating on the PCI bus of IBM compatible personal computer. The software of the system is realized under Windows XP and allows to process scintillation signals online, to build and to analyze energy spectra. The data acquisition system improves energy resolution of scintillation spectra as compared to conventional spectrometers and is significantly less expensive.

Published
2009

7. Precision Measurement of theBe7Solar Neutrino Interaction Rate in Borexino

Author

Lino Miramonti, Davide Franco, Michael Wurm, Francesco Lombardi, Margherita Buizza Avanzini, Albert Sotnikov, Valentina Muratova, Luca Grandi, Matthias Laubenstein, Marco Pallavicini, Livia Ludhova, Stefan Schönert, Richard Saldanha, Alexander Derbin, Gioacchino Ranucci, Alessandra Carlotta Re, Jingke Xu, Aldo Romani, Oleg Smirnov, Fausto Ortica, Cristiano Galbiati, Carlos Peña Garay, Aldo Ianni, Alessandro Razeto, Vladislav Kobychev, Davide D'Angelo, and Ben Loer

Subjects
Physics, Particle physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, Center (category theory), General Physics and Astronomy, 01 natural sciences, 7. Clean energy, Nuclear physics, 0103 physical sciences, High Energy Physics::Experiment, Sensitivity (control systems), Neutrino, 010306 general physics, Neutrino oscillation, Isotopes of beryllium, Borexino, Lepton
Abstract

The rate of neutrino-electron elastic scattering interactions from 862 keV {sup 7}Be solar neutrinos in Borexino is determined to be 46.0{+-}1.5(stat){sub -1.6}{sup +1.5}(syst) counts/(day{center_dot}100 ton). This corresponds to a {nu}{sub e}-equivalent {sup 7}Be solar neutrino flux of (3.10{+-}0.15)x10{sup 9} cm{sup -2} s{sup -1} and, under the assumption of {nu}{sub e} transition to other active neutrino flavours, yields an electron neutrino survival probability of 0.51{+-}0.07 at 862 keV. The no flavor change hypothesis is ruled out at 5.0 {sigma}. A global solar neutrino analysis with free fluxes determines {Phi}{sub pp}=6.06{sub -0.06}{sup +0.02}x10{sup 10} cm{sup -2} s{sup -1} and {Phi}{sub CNO}

Published
2011

8. Quest for neutrinoless double beta decay of 160Gd

Author

Danevich, F. A., Georgadze, A. Sh, Vladislav Kobychev, Kropivyansky, B. N., Kuts, V. N., Muzalevsky, V. V., Nikolaiko, A. S., Ponkratenko, O. A., Prokopets, A. G., Tretyak, V. I., and Zdesenko, Yu G.

10. Borexino: From the sun to the earth

Author

Roncin, R., Agostini, M., Altenmüller, K., Appel, S., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chepurnov, A., D Angelo, D., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., Empl, A., Etenko, A., Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Ghiano, C., Giammarchi, M., Göger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Hungerford, E., Ianni, A., Jedrzejczak, K., Kaiser, M., Vladislav Kobychev, Korablev, D., Korga, G., Kryn, D., Laubenstein, M., Lehnert, B., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pagani, L., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Schönert, S., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Unzhakov, E., Vogelaar, R. B., Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., and Zuzel, G.

Subjects
Multidisciplinary

12. Recent solar and geo-ν results from borexino

Author

Zavatarelli, S., Agostini, M., Altenmüller, K., Appel, S., Atroshchenko, V., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Carlini, M., Cavalcante, P., Chepurnov, A., Choi, K., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., Etenko, A., Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Ghiano, C., Giammarchi, M., Göger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Hungerford, E., Ianni, A., Jany, A., Jedrzejczak, K., Jeschke, D., Vladislav Kobychev, Korablev, D., Korga, G., Kryn, D., Laubenstein, M., Lehnert, B., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Marcocci, S., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Roncin, R., Rossi, N., Schrönert, S., Semenov, D., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Unzhakov, E., Vishneva, A., Vogelaar, R. B., Feilitzsch, F., Wang, H., Weinz, S., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zuber, K., and Zuzel, G.

13. Simulation of light collection in calcium tungstate scintillation detectors

Author

Danevich, F. A., Vladislav Kobychev, Kobychev, R. V., Kraus, H., Mikhailik, V. B., and Mokina, V. M.

Subjects
Physics::Instrumentation and Detectors, light collection efficiency, Physics::Optics, scintillation detector, CaWO4 crystal scintillator, lcsh:Atomic physics. Constitution and properties of matter, Monte Carlo simulation, lcsh:QC170-197
Abstract

Due to high operational properties, the oxide scintillators are perspective for cryogenic scintillation experiments with aim of study rare nuclear processes. In order to optimize light yield and the energy resolution we performed calculations of the efficiency of light collection for different geometries of scintillation detector with CaWO4 crystal by Monte-Carlo method using Litrani, Geant4 and Zemax packages. The calculations were compared with experimental data in the same configurations, depending on the crystal shape, surface treatment, material and shape of the reflector and presence of optical contact. The best results were obtained with crystals shaped as the right prism with triangle base, with completely diffused surfaces, using mirror reflector shaped as a truncated cone. Simulations by using Litrani have shown the best agreement with experimental results.

14. Solar neutrino physics with BOREXINO i

Author

Ludhova, L., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Avanzini, M. B., Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Cavalcante, P., Chavarria, A., D Angelo, D., Davini, S., Derbin, A., Etenko, A., Fomenko, K., Franco, D., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goger-Neff, M., Goretti, A., Grandi, L., Guardincerri, E., Hardy, S., Ianni, A., Kayunov, A., Vladislav Kobychev, Korablev, D., Korga, G., Koshio, Y., Kryn, D., Laubenstein, M., Lewke, T., Litvinovich, E., Loer, B., Lombardi, F., Lombardi, P., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Montanari, D., Mosteiro, P., Muratova, V., Oberauer, L., Obolenksy, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Perasso, S., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Re, A., Romani, P. A., Sabelnikov, A., Saldanha, R., Salvo, C., Schonert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., Feilitzsch, F., Winter, J., Wojcik, M., Wright, A., Wurm, M., Xu, J., Zaimidoroga, O., Zavatarelli, S., and Zuzel, G.

15. Measurement of 7Be and 8B solar neutrinos with Borexino

Author

Zavatarelli, S., Bellini, G., Benziger, J., Bonetti, S., Buizza-Avanzini, M., Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Chavarria, A., Dalnoki-Veress, F., D Angelo, D., Davini, S., Kerret, H., Derbin, A., Etenko, A., Fomenko, K., Franco, D., Galbiati, C., Gazzana, S., Giammarchi, M., Goeger-Neff, M., Goretti, A., Hardy, S., Ianni, A., Joyce, M., Vladislav Kobychev, Korga, G., Kryn, D., Laubenstein, M., Leung, M., Lewke, T., Litninovich, E., Loer, B., Lombardi, P., Ludhova, L., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Masetti, F., Mccarty, K., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Montanari, D., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Perasso, L., Perasso, S., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Risso, P., Romani, A., Rountree, D., Sabelnikov, A., Saldanha, R., Salvo, C., Schonert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., Feilitzsch, F., Wojcik, M., Wurm, M., Zaimidoroga, O., and Zuzel, G.

16. Investigation of β decay of 113Cd

Author

Belli, P., Bernabei, R., Bukilic, N., Cappella, F., Cerulli, R., Dai, C. J., Danevich, F. A., Laeter, J. R., Incicchitti, A., Vladislav Kobychev, Nagorny, S. S., Nisi, S., Nozzoli, F., Poda, D. V., Prosperi, D., Tretyak, V. I., and Yurchenko, S. S.

18. New results of 116Cd ββ decay experiment

Author

Bizzeti, P. G., Danevich, F. A., Fazzini, T. F., Georgadze, A., Vladislav Kobychev, Maurenzig, P. R., Nagorny, S. S., Nikolaiko, A. S., Ponkratenko, O. A., Tretyak, V. I., Zdesenko, S. Yu, and Zdesenko, Yu G.

19. CdWO4 scintillators with large volume

Author

Georgadze, A. Sh, Danevich, F. A., Sdesenko, Yu G., Kuts, V. N., Vladislav Kobychev, Kropivyanskij, B. N., Muzalevskij, V. V., Nikolajko, A. S., Pankratenko, O. A., and Tret Yak, V. I.

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