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90 results on '"Sanglard V"'

1. Searching for beyond the Standard Model physics using the improved description of 100Mo 2νββ decay spectral shape with CUPID-Mo

Author: Augier, C., Barabash, A. S., Bellini, F., Benato, G., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu. A., Cardani, L., Casali, N., Cazes, A., Celi, E., Chapellier, M., Chiesa, D., Dafinei, I., Danevich, F. A., De Jesus, M., Dixon, T., Dumoulin, L., Eitel, K., Ferri, F., Fujikawa, B. K., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Helis, D. L., Huang, H. Z., Huang, R., Imbert, L., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S. I., Kotila, J., Loaiza, P., Ma, L., Makarov, E. P., de Marcillac, P., Mariam, R., Marini, L., Marnieros, S., Navick, X. F., Nones, C., Norman, E. B., Olivieri, E., Ouellet, J. L., Pagnanini, L., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D. V., Polischuk, O. G., Pozzi, S., Previtali, E., Redon, Th., Rojas, A., Rozov, S., Sanglard, V., Scarpaci, J. A., Schmidt, B., Shen, Y., Shlegel, V. N., Šimkovic, F., Singh, V., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Velázquez, M., Ware, B., Welliver, B., Winslow, L., Xue, M., Yakushev, E., Zarytskyy, M., and Zolotarova, A. S.
Published: 2024
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2. Ricochet Progress and Status

Author: Augier, C., Beaulieu, G., Belov, V., Berge, L., Billard, J., Bres, G., Bret, J. -L., Broniatowski, A., Calvo, M., Cazes, A., Chaize, D., Chapellier, M., Chaplinsky, L., Chemin, G., Chen, R., Colas, J., de Jesus, M., de Marcillac, P., Dumoulin, L., Exshaw, O., Ferriol, S., Figueroa-Feliciano, E., Filippini, J. -B., Formaggio, J. A., Fuard, S., Gascon, J., Giuliani, A., Goupy, J., Goy, C., Guerin, C., Hirjibehedin, C. F., Harrington, P., Heine, S. T., Hertel, S. A., Heusch, M., Hoarau, C., Hong, Z., Ianigro, J. -C., Jin, Y., Johnston, J. P., Juillard, A., Kazarcev, S., Lamblin, J., Lattaud, H., Lubashevskiy, A., Mayer, D. W., Marnieros, S., Minet, J., Misiak, D., Monfardini, A., Mounier, F., Olivieri, E., Oriol, C., Patel, P. K., Perbet, E., Pinckney, H. D., Ponomarev, D., Poda, D., Rarbi, F., Real, J. -S., Ricol, J. -S., Redon, T., Robert, A., Rozov, S., Rozova, I., Salagnac, T., Sanglard, V., Schmidt, B., Shevchik, Ye., Sibille, V., Soldner, T., Stachurska, J., Stutz, A., Vagneron, L., van de Pontseele, W., Vezzu, F., Weber, S., Winslow, L., Yakushev, E., and Zinatulina, D.
Published: 2023
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3. High Impedance TES Bolometers for EDELWEISS

Author: Marnieros, S., Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Billard, J., Broniatowski, A., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., De Jésus, M., Dumoulin, L., Eitel, K., Fillipini, J.-B., Filosofov, D., Gascon, J., Giuliani, A., Gros, M., Jin, Y., Juillard, A., Kleifges, M., Lattaud, H., Misiak, D., Navick, X.-F., Nones, C., Olivieri, E., Oriol, C., Pari, P., Paul, B., Poda, D., Rozov, S., Salagnac, T., Sanglard, V., Vagneron, L., Yakushev, E., and Zolotarova, A.
Published: 2022
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4. Machine Learning Techniques for Pile-Up Rejection in Cryogenic Calorimeters

Author: Fantini, G., Armatol, A., Armengaud, E., Armstrong, W., Augier, C., Avignone, III, F. T., Azzolini, O., Barabash, A., Bari, G., Barresi, A., Baudin, D., Bellini, F., Benato, G., Beretta, M., Bergé, L., Biassoni, M., Billard, J., Boldrini, V., Branca, A., Brofferio, C., Bucci, C., Camilleri, J., Capelli, S., Cappelli, L., Cardani, L., Carniti, P., Casali, N., Cazes, A., Celi, E., Chang, C., Chapellier, M., Charrier, A., Chiesa, D., Clemenza, M., Colantoni, I., Collamati, F., Copello, S., Cova, F., Cremonesi, O., Creswick, R. J., Cruciani, A., D’Addabbo, A., D’Imperio, G., Dafinei, I., Danevich, F. A., de Combarieu, M., De Jesus, M., de Marcillac, P., Dell’Oro, S., Domizio, S. Di, Dompè, V., Drobizhev, A., Dumoulin, L., Fasoli, M., Faverzani, M., Ferri, E., Ferri, F., Ferroni, F., Figueroa-Feliciano, E., Formaggio, J., Franceschi, A., Fu, C., Fu, S., Fujikawa, B. K., Gascon, J., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Gotti, C., Gras, P., Gros, M., Gutierrez, T. D., Han, K., Hansen, E. V., Heeger, K. M., Helis, D. L., Huang, H. Z., Huang, R. G., Imbert, L., Johnston, J., Juillard, A., Karapetrov, G., Keppel, G., Khalife, H., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S., Liu, Y., Loaiza, P., Ma, L., Madhukuttan, M., Mancarella, F., Mariam, R., Marini, L., Marnieros, S., Martinez, M., Maruyama, R. H., Mauri, B., Mayer, D., Mei, Y., Milana, S., Misiak, D., Napolitano, T., Nastasi, M., Navick, X. F., Nikkel, J., Nipoti, R., Nisi, S., Nones, C., Norman, E. B., Novosad, V., Nutini, I., O’Donnell, T., Olivieri, E., Oriol, C., Ouellet, J. L., Pagan, S., Pagliarone, C., Pagnanini, L., Pari, P., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pettinacci, V., Pira, C., Pirro, S., Poda, D. V., Polakovic, T., Polischuk, O. G., Pozzi, S., Previtali, E., Puiu, A., Ressa, A., Rizzoli, R., Rosenfeld, C., Rusconi, C., Sanglard, V., Scarpaci, J., Schmidt, B., Sharma, V., Shlegel, V., Singh, V., Sisti, M., Speller, D., Surukuchi, P. T., Taffarello, L., Tellier, O., Tomei, C., Tretyak, V. I., Tsymbaliuk, A., Vedda, A., Velazquez, M., Vetter, K. J., Wagaarachchi, S. L., Wang, G., Wang, L., Welliver, B., Wilson, J., Wilson, K., Winslow, L. A., Xue, M., Yan, L., Yang, J., Yefremenko, V., Yumatov, V., Zarytskyy, M. M., Zhang, J., Zolotarova, A., and Zucchelli, S.
Published: 2022
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5. The background model of the CUPID-Mo 0νββ experiment

Author: Augier, C., Barabash, A. S., Bellini, F., Benato, G., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu. A., Cardani, L., Casali, N., Cazes, A., Celi, E., Chapellier, M., Chiesa, D., Dafinei, I., Danevich, F. A., De Jesus, M., de Marcillac, P., Dixon, T., Dumoulin, L., Eitel, K., Ferri, F., Fujikawa, B. K., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Helis, D. L., Huang, H. Z., Huang, R., Imbert, L., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S. I., Kotila, J., Loaiza, P., Ma, L., Makarov, E. P., Mariam, R., Marini, L., Marnieros, S., Navick, X.-F., Nones, C., Norman, E. B., Olivieri, E., Ouellet, J. L., Pagnanini, L., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D. V., Polischuk, O. G., Pozzi, S., Previtali, E., Redon, Th., Rojas, A., Rozov, S., Sanglard, V., Scarpaci, J. A., Schmidt, B., Shen, Y., Shlegel, V. N., Singh, V., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Velázquez, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., Zarytskyy, M., and Zolotarova, A. S.
Published: 2023
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6. Fast neutron background characterization of the future Ricochet experiment at the ILL research nuclear reactor

Author: Augier, C., Baulieu, G., Belov, V., Berge, L., Billard, J., Bres, G., Bret, J-. L., Broniatowski, A., Calvo, M., Cazes, A., Chaize, D., Chapellier, M., Chaplinsky, L., Chemin, G., Chen, R., Colas, J., De Jesus, M., de Marcillac, P., Dumoulin, L., Exshaw, O., Ferriol, S., Figueroa-Feliciano, E., Filippini, J. -B., Formaggio, J. A., Fuard, S., Gascon, J., Giuliani, A., Goupy, J., Goy, C., Guerin, C., Guy, E., Harrington, P., Heine, S. T., Hertel, S. A., Heusch, M., Hirjibehedin, C. F., Hong, Z., Ianigro, J.-C., Jin, Y., Johnston, J. P., Juillard, A., Karaivanov, D., Kazarcev, S., Lamblin, J., Lattaud, H., Li, M., Lubashevskiy, A., Marnieros, S., Mayer, D. W., Minet, J., Misiak, D., Mocellin, J-.L., Monfardini, A., Mounier, F., Oliver, W. D., Olivieri, E., Oriol, C., Patel, P. K., Perbet, E., Pinckney, H. D., Poda, D., Ponomarev, D., Rarbi, F., Real, J.-S., Redon, T., Robert, A., Rozov, S., Rozova, I., Salagnac, T., Sanglard, V., Schmidt, B., Shevchik, Ye., Sibille, V., Soldner, T., Stachurska, J., Stutz, A., Vagneron, L., Van De Pontseele, W., Vezzu, F., Weber, S., Winslow, L., Yakushev, E., and Zinatulina, D.
Published: 2023
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7. Final results on the 0νββ100 decay half-life limit of 0νββ100Mo from the CUPID-Mo experiment

Author: Augier, C., Barabash, A. S., Bellini, F., Benato, G., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu. A., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Chiesa, D., Dafinei, I., Danevich, F. A., De Jesus, M., de Marcillac, P., Dixon, T., Dumoulin, L., Eitel, K., Ferri, F., Fujikawa, B. K., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Helis, D. L., Huang, H. Z., Huang, R., Imbert, L., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S. I., Loaiza, P., Ma, L., Makarov, E. P., Mariam, R., Marini, L., Marnieros, S., Navick, X.-F., Nones, C., Norman, E. B., Olivieri, E., Ouellet, J. L., Pagnanini, L., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D. V., Polischuk, O. G., Pozzi, S., Previtali, E., Redon, Th., Rojas, A., Rozov, S., Sanglard, V., Scarpaci, J. A., Schmidt, B., Shen, Y., Shlegel, V. N., Singh, V., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Velázquez, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., Zarytskyy, M., and Zolotarova, A. S.
Published: 2022
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8. Characterization of cubic Li2100421004MoO21004 crystals for the CUPID experiment

Author: Armatol, A., Armengaud, E., Armstrong, W., Augier, C., Avignone, III, F. T., Azzolini, O., Barabash, A., Bari, G., Barresi, A., Baudin, D., Bellini, F., Benato, G., Beretta, M., Bergé, L., Biassoni, M., Billard, J., Boldrini, V., Branca, A., Brofferio, C., Bucci, C., Camilleri, J., Capelli, S., Cappelli, L., Cardani, L., Carniti, P., Casali, N., Cazes, A., Celi, E., Chang, C., Chapellier, M., Charrier, A., Chiesa, D., Clemenza, M., Colantoni, I., Collamati, F., Copello, S., Cremonesi, O., J. Creswick, R., Cruciani, A., D’Addabbo, A., D’Imperio, G., Dafinei, I., A. Danevich, F., de Combarieu, M., De Jesus, M., de Marcillac, P., Dell’Oro, S., Di Domizio, S., Dompè, V., Drobizhev, A., Dumoulin, L., Fantini, G., Faverzani, M., Ferri, E., Ferri, F., Ferroni, F., Figueroa-Feliciano, E., Formaggio, J., Franceschi, A., Fu, C., Fu, S., Fujikawa, B. K., Gascon, J., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Gotti, C., Gras, P., Gros, M., Gutierrez, T. D., Han, K., Hansen, E. V., Heeger, K. M., Helis, D. L., Huang, H. Z., Huang, R. G., Imbert, L., Johnston, J., Juillard, A., Karapetrov, G., Keppel, G., Khalife, H., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S., Liu, Y., Loaiza, P., Ma, L., Madhukuttan, M., Mancarella, F., Mariam, R., Marini, L., Marnieros, S., Martinez, M., Maruyama, R. H., Mauri, B., Mayer, D., Mei, Y., Milana, S., Misiak, D., Napolitano, T., Nastasi, M., Navick, X. F., Nikkel, J., Nipoti, R., Nisi, S., Nones, C., Norman, E. B., Novosad, V., Nutini, I., O’Donnell, T., Olivieri, E., Oriol, C., Ouellet, J. L., Pagan, S., Pagliarone, C., Pagnanini, L., Pari, P., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pettinacci, V., Pira, C., Pirro, S., V. Poda, D., Polakovic, T., Polischuk, O. G., Pozzi, S., Previtali, E., Puiu, A., Ressa, A., Rizzoli, R., Rosenfeld, C., Rusconi, C., Sanglard, V., Scarpaci, J. A., Schmidt, B., Sharma, V., Shlegel, V., Singh, V., Sisti, M., Speller, D., Surukuchi, P. T., Taffarello, L., Tellier, O., Tomei, C., Tretyak, V. I., Tsymbaliuk, A., Velazquez, M., Vetter, K. J., Wagaarachchi, S. L., Wang, G., Wang, L., Welliver, B., Wilson, J., Wilson, K., Winslow, L. A., Xue, M., Yan, L., Yang, J., Yefremenko, V., Yumatov, V., Zarytskyy, M. M., Zhang, J., Zolotarova, A., and Zucchelli, S.
Published: 2021
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9. Measurement of the cosmogenic activation of germanium detectors in EDELWEISS-III

Author: Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Billard, J., Blümer, J., de Boissière, T., Broniatowski, A., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., De Jésus, M., Dumoulin, L., Eitel, K., Foerster, N., Gascon, J., Giuliani, A., Gros, M., Hehn, L., Heuermann, G., Jin, Y., Juillard, A., Kéfélian, C., Kleifges, M., Kozlov, V., Kraus, H., Kudryavtsev, V.A., Le-Sueur, H., Marnieros, S., Navick, X.-F., Nones, C., Olivieri, E., Pari, P., Paul, B., Piro, M.-C., Poda, D., Queguiner, E., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Siebenborn, B., Tcherniakhovski, D., Vagneron, L., Weber, M., and Yakushev, E.
Published: 2017
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10. Precise measurement of 2νββ100 decay of 2νββ100Mo with the CUPID-Mo detection technology

Author: Armengaud, E., Augier, C., Barabash, A. S., Bellini, F., Benato, G., Benoît, A., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu. A., Bourgeois, Ch., Briere, M., Brudanin, V., Camus, P., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Charlieux, F., de Combarieu, M., Dafinei, I., Danevich, F. A., De Jesus, M., Dumoulin, L., Eitel, K., Elkhoury, E., Ferri, F., Fujikawa, B. K., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Guerard, E., Helis, D. L., Huang, H. Z., Huang, R., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S. I., Leder, A., Kotila, J., Loaiza, P., Ma, L., Makarov, E. P., de Marcillac, P., Marini, L., Marnieros, S., Misiak, D., Navick, X.-F., Nones, C., Novati, V., Olivieri, E., Ouellet, J. L., Pagnanini, L., Pari, P., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D. V., Polischuk, O. G., Previtali, E., Redon, Th., Rozov, S., Rusconi, C., Sanglard, V., Schäffner, K., Schmidt, B., Shen, Y., Shlegel, V. N., Siebenborn, B., Singh, V., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Velázquez, M., Weber, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., and Zolotarova, A. S.
Published: 2020
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11. The background model of the CUPID-Mo $0\nu\beta\beta$ experiment

Author: Collaboration, CUPID-Mo, Augier, C., Barabash, A. S., Bellini, F., Benato, G., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu. A., Cardani, L., Casali, N., Cazes, A., Celi, E., Chapellier, M., Chiesa, D., Dafinei, I., Danevich, F. A., De Jesus, M., de Marcillac, P., Dixon, T., Dumoulin, L., Eitel, K., Ferri, F., Fujikawa, B. K., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Helis, D. L., Huang, H. Z., Huang, R., Imbert, L., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S. I., Kotila, J., Loaiza, P., Ma, L., Makarov, E. P., Mariam, R., Marini, L., Marnieros, S., Navick, X. F., Nones, C., Norman, E. B., Olivieri, E., Ouellet, J. L., Pagnanini, L., Pattavina, L., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D. V., Polischuk, O. G., Pozzi, S., Previtali, E., Redon, Th., Rojas, A., Rozov, S., Sanglard, V., Scarpaci, J. A., Schmidt, B., Shen, Y., Shlegel, V. N., Singh, V., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Velázquez, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., Zarytskyy, M., Zolotarova, A. S., Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Science et Ingénierie des Matériaux et Procédés (SIMaP), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), and CUPID-Mo
Subjects: Physics - Instrumentation and Detectors, model, bolometer, background, technology, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], particle identification, scintillation counter, High Energy Physics - Experiment, crystal
Abstract: International audience; CUPID-Mo, located in the Laboratoire Souterrain de Modane (France), was a demonstrator for the next generation $0\nu\beta\beta$ decay experiment, CUPID. It consisted of an array of 20 enriched Li$_{2}$$ ^{100}$MoO$_4$ bolometers and 20 Ge light detectors and has demonstrated that the technology of scintillating bolometers with particle identification capabilities is mature. Furthermore, CUPID-Mo can inform and validate the background prediction for CUPID. In this paper, we present a detailed model of the CUPID-Mo backgrounds. This model is able to describe well the features of the experimental data and enables studies of the $2\nu\beta\beta$ decay and other processes with high precision. We also measure the radio-purity of the Li$_{2}$$^{100}$MoO$_4$ crystals which are found to be sufficient for the CUPID goals. Finally, we also obtain a background index in the region of interest of 3.7$^{+0.9}_{-0.8}$(stat)$^{+1.5}_{-0.7}$(syst)$\times10^{-3}$counts/$\Delta$E$_{FWHM}$/mol$_{iso}$/yr, the lowest in a bolometric $0\nu\beta\beta$ decay experiment.
Published: 2023

12. Final results on the $$0\nu \beta \beta $$ <math> <mrow> <mn>0</mn> <mi>ν</mi> <mi>β</mi> <mi>β</mi> </mrow> </math> decay half-life limit of $$^{100}$$ <math> <msup> <mrow></mrow> <mn>100</mn> </msup> </math> Mo from the CUPID-Mo experiment

Author: Augier, C., Barabash, A., Bellini, F., Benato, G., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Chiesa, D., Dafinei, I., Danevich, F., Jesus, M., Marcillac, P., Dixon, T., Dumoulin, L., Eitel, K., Ferri, F., Fujikawa, B., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V., Gros, M., Helis, D., Huang, H., Huang, R., Imbert, L., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V., Kolomensky, Yu., Konovalov, S., Loaiza, P., Ma, L., Makarov, E., Mariam, R., Marini, L., Marnieros, S., Navick, X.F., Nones, C., Norman, E., Olivieri, E., Ouellet, J., Pagnanini, L., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D., Polischuk, O., Pozzi, S., Previtali, E., Redon, Th., Rojas, A., Rozov, S., Sanglard, V., Scarpaci, J., Schmidt, B., Shen, Y., Shlegel, V., Singh, V., Tomei, C., Tretyak, V., Umatov, V., Vagneron, L., Velázquez, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., Zarytskyy, M., and Zolotarova, A.
Abstract: The CUPID-Mo experiment to search for 0 $$\nu \beta \beta $$ ν β β decay in $$^{100}$$ 100 Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0 $$\nu \beta \beta $$ ν β β decay experiment. CUPID-Mo was comprised of 20 enriched $$\hbox {Li}_{{2}}$$ Li 2 $$^{100}$$ 100 $$\hbox {MoO}_4$$ MoO 4 scintillating calorimeters, each with a mass of $$\sim 0.2$$ ∼ 0.2 kg, operated at $$\sim 20$$ ∼ 20 mK. We present here the final analysis with the full exposure of CUPID-Mo ( $$^{100}$$ 100 Mo exposure of 1.47 $$\hbox {kg} \times \hbox {year}$$ kg × year ) used to search for lepton number violation via 0 $$\nu \beta \beta $$ ν β β decay. We report on various analysis improvements since the previous result on a subset of data, reprocessing all data with these new techniques. We observe zero events in the region of interest and set a new limit on the $$^{100}$$ 100 Mo 0 $$\nu \beta \beta $$ ν β β decay half-life of $$T_{1/2}^{0\nu }$$ T 1 / 2 0 ν $$> {1.8}\times 10^{24}$$ > 1.8 × 10 24 year (stat. + syst.) at 90% CI. Under the light Majorana neutrino exchange mechanism this corresponds to an effective Majorana neutrino mass of $$\left$$ m β β $$ < ( 0.28 - 0.49 ) eV, dependent upon the nuclear matrix element utilized.
Published: 2022

13. Improved EDELWEISS-III sensitivity for low-mass WIMPs using a profile likelihood approach

Author: Hehn, L., Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Billard, J., Blümer, J., de Boissière, T., Broniatowski, A., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., De Jésus, M., Dumoulin, L., Eitel, K., Foerster, N., Gascon, J., Giuliani, A., Gros, M., Heuermann, G., Jin, Y., Juillard, A., Kéfélian, C., Kleifges, M., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Le-Sueur, H., Marnieros, S., Navick, X.-F., Nones, C., Olivieri, E., Pari, P., Paul, B., Piro, M.-C., Poda, D., Queguiner, E., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Siebenborn, B., Tcherniakhovski, D., Vagneron, L., Weber, M., and Yakushev, E.
Published: 2016
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14. Background studies for the EDELWEISS dark matter experiment

Author: Armengaud, E., Augier, C., Benoıˆt, A., Bergé, L., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Censier, B., Chapellier, M., Charlieux, F., Couedo, F., Coulter, P., Cox, G.A., De Jesus, M., Domange, J., Drilien, A.-A., Dumoulin, L., Eitel, K., Filosofov, D., Fourches, N., Gascon, J., Gerbier, G., Gros, M., Henry, S., Hervé, S., Heuermann, G., Holtzer, N., Juillard, A., Kleifges, M., Kluck, H., Kozlov, V., Kraus, H., Kudryavtsev, V.A., Le Sueur, H., Loaiza, P., Marnieros, S., Menshikov, A., Navick, X-F., Nones, C., Olivieri, E., Pari, P., Paul, B., Rigaut, O., Robinson, M., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Siebenborn, B., Semikh, S., Tcherniakhovski, D., Torrento-Coello, A.S., Vagneron, L., Walker, R.J., Weber, M., Yakushev, E., and Zhang, X.
Published: 2013
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15. Muon-induced background in the EDELWEISS dark matter search

Author: Schmidt, B., Armengaud, E., Augier, C., Benoit, A., Bergé, L., Bergmann, T., Blümer, J., Bres, G., Broniatowski, A., Brudanin, V., Censier, B., Chapellier, M., Charlieux, F., Collin, S., Coulter, P., Cox, G.A., Crauste, O., Domange, J., Dumoulin, L., Eitel, K., Filosofov, D., Fourches, N., Garde, G., Gascon, J., Gerbier, G., Gros, M., Hehn, L., Henry, S., Hervé, S., Heuermann, G., Juillard, A., Kluck, H., Kozlov, V.Y., Kleifges, M., Kraus, H., Kudryavtsev, V.A., Loaiza, P., Marnieros, S., Menshikov, A., Navick, X.-F., Nieder, H., Nones, C., Olivieri, E., Pari, P., Paul, B., Robinson, M., Rodenas, H., Rozov, S., Sanglard, V., Siebenborn, B., Tcherniakhovski, D., Torrentó-Coello, A.S., Vagneron, L., Walker, R.J., Weber, M., Yakushev, E., and Zhang, X.
Published: 2013
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16. Search for sub-GeV Dark Matter via Migdal effect with an EDELWEISS germanium detector with NbSi TES sensors

Author: Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Billard, J., Broniatowski, A., Camus, P., Caze, A., Chapellier, M., Charlieux, F., De Jésus, M., Dumoulin, L., Eitel, K., Filippini, J. B., Filosofov, D., Gascon, J., Giuliani, A., Gros, M., Guy, E., Jin, Y., Juillard, A., Kleifges, M., Lattaud, H., Marnieros, S., Misiak, D., Navick, X. F., Nones, C., Olivieri, E., Oriol, C., Pari, P., Paul, B., Poda, D., Rozov, S., Salagnac, T., Sanglard, V., Vagneron, L., Yakushev, E., Zolotarova, A., and Kavanagh, B. J.
Subjects: Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences, Astrophysics - Astrophysics of Galaxies
Abstract: The EDELWEISS collaboration reports on the search for Dark Matter (DM) particle interactions via Migdal effect with masses between $32$ MeV$\cdot$c$^{-2}$ to $2$ GeV$\cdot$c$^{-2}$ using a $200$ g cryogenic Ge detector sensitive to simultaneously heat and ionization signals and operated underground at the Laboratoire Souterrain de Modane in France. The phonon signal was read out using a Transition Edge Sensor made of a NbSi thin film. The detector was biased at $66$ V in order to benefit from the Neganov-Trofimov-Luke amplification and resulting in a resolution on the energy of electron recoils of $4.46$ eV$_{ee}$ (RMS) and an analysis threshold of $30$ eV$_{ee}$. The sensitivity is limited by a dominant background not associated to charge creation in the detector. The search constrains a new region of parameter space for cross-sections down to $10^{-29}$ cm$^2$ and masses between $32$ and $100$ MeV$\cdot$c$^{-2}$. The achieved low threshold with the NbSi sensor shows the relevance of its use for athermal-phonon sensitive devices for low-mass DM searches., 10 pages, 9 figures
Published: 2022

17. A detection system to measure muon-induced neutrons for direct dark matter searches

Author: Kozlov, V.Yu., Armengaud, E., Augier, C., Benoit, A., Bergé, L., Besida, O., Blümer, J., Broniatowski, A., Brudanin, V., Chantelauze, A., Chapellier, M., Chardin, G., Charlieux, F., Collin, S., Defay, X., De Jésus, M., Di Stefano, P., Dolgorouki, Y., Domange, J., Dumoulin, L., Eitel, K., Gascon, J., Gerbier, G., Gros, M., Hannawald, M., Hervé, S., Juillard, A., Kluck, H., Lemrani, R., Loaiza, P., Lubashevskiy, A., Marnieros, S., Navick, X.-F., Olivieri, E., Pari, P., Paul, B., Rozov, S., Sanglard, V., Scorza, S., Semikh, S., Torrentó-Coello, A.S., Vagneron, L., Verdier, M.-A., and Yakushev, E.
Published: 2010
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18. Characterization of cubic Li $$_{2}$$ <math> <msub> <mrow></mrow> <mn>2</mn> </msub> </math> $$^{100}$$ <math> <msup> <mrow></mrow> <mn>100</mn> </msup> </math> MoO $$_4$$ <math> <msub> <mrow></mrow> <mn>4</mn> </msub> </math> crystals for the CUPID experiment

Author: Armatol, A., Armengaud, E., Armstrong, W., Augier, C., Avignone, F., Azzolini, O., Barabash, A., Bari, G., Barresi, A., Baudin, D., Bellini, F., Benato, G., Beretta, M., Bergé, L., Biassoni, M., Billard, J., Boldrini, V., Branca, A., Brofferio, C., Bucci, C., Camilleri, J., Capelli, S., Cappelli, L., Cardani, L., Carniti, P., Casali, N., Cazes, A., Celi, E., Chang, C., Chapellier, M., Charrier, A., Chiesa, D., Clemenza, M., Colantoni, I., Collamati, F., Copello, S., Cremonesi, O., J. Creswick, R., Cruciani, A., D’Addabbo, A., D’Imperio, G., Dafinei, I., A. Danevich, F., de Combarieu, M., De Jesus, M., de Marcillac, P., Dell’Oro, S., Di Domizio, S., Dompè, V., Drobizhev, A., Dumoulin, L., Fantini, G., Faverzani, M., Ferri, E., Ferri, F., Ferroni, F., Figueroa-Feliciano, E., Formaggio, J., Franceschi, A., Fu, C., Fu, S., Fujikawa, B., Gascon, J., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Gotti, C., Gras, P., Gros, M., Gutierrez, T., Han, K., Hansen, E., Heeger, K., Helis, D., Huang, H., Huang, R., Imbert, L., Johnston, J., Juillard, A., Karapetrov, G., Keppel, G., Khalife, H., Kobychev, V., Kolomensky, Yu., Konovalov, S., Liu, Y., Loaiza, P., Ma, L., Madhukuttan, M., Mancarella, F., Mariam, R., Marini, L., Marnieros, S., Martinez, M., Maruyama, R., Mauri, B., Mayer, D., Mei, Y., Milana, S., Misiak, D., Napolitano, T., Nastasi, M., Navick, X., Nikkel, J., Nipoti, R., Nisi, S., Nones, C., Norman, E., Novosad, V., Nutini, I., O’Donnell, T., Olivieri, E., Oriol, C., Ouellet, J., Pagan, S., Pagliarone, C., Pagnanini, L., Pari, P., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pettinacci, V., Pira, C., Pirro, S., V. Poda, D., Polakovic, T., Polischuk, O., Pozzi, S., Previtali, E., Puiu, A., Ressa, A., Rizzoli, R., Rosenfeld, C., Rusconi, C., Sanglard, V., Scarpaci, J., Schmidt, B., Sharma, V., Shlegel, V., Singh, V., Sisti, M., Speller, D., Surukuchi, P., Taffarello, L., Tellier, O., Tomei, C., Tretyak, V., Tsymbaliuk, A., Velazquez, M., Vetter, K., Wagaarachchi, S., Wang, G., Wang, L., Welliver, B., Wilson, J., Wilson, K., Winslow, L., Xue, M., Yan, L., Yang, J., Yefremenko, V., Yumatov, V., Zarytskyy, M., Zhang, J., Zolotarova, A., and Zucchelli, S.
Abstract: The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of ( $$6.7\pm 0.6$$ 6.7 ± 0.6 ) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of $$\alpha $$ α particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this $$\alpha $$ α -induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector.
Published: 2021

19. A new limit for neutrinoless double-beta decay of 100 Mo from the CUPID-Mo experiment (CUPID-Mo Collaboration)

Author: Armengaud, E., Augier, C., Barabash, A.S., Bellini, F, Benato, G, Benoit, Alain, Beretta, M, Bergé, L., Billard, J., Borovlev, Yu, Bourgeois, Ch, Brudanin, V, Camus, P, Cardani, L, Casali, N, Cazes, A., Chapellier, M, Charlieux, F., Chiesa, D, De Combarieu, M, Dafinei, I, Danevich, F, De Jesus, M., Dixon, T, Dumoulin, L, Eitel, K, Ferri, F, Fujikawa, B, Gascon, J., Gironi, L, Giuliani, A, Grigorieva, V, Gros, M, Guerard, E, Helis, D, Huang, H, Huang, R, Johnston, J, Juillard, A., Khalife, H, Kleifges, M, Kobychev, V, Kolomensky, Yu, Konovalov, S, Leder, A, Loaiza, P, Ma, L, Makarov, E, De Marcillac, P, Mariam, R, Marini, L, Marnieros, S, Misiak, D, Navick, X.-F, Nones, C, Norman, E, Novati, V, Olivieri, E, Ouellet, J, Pagnanini, L, Pari, P, Pattavina, L, Paul, B, Pavan, M, PENG, H, Pessina, G, Pirro, S, Poda, D, Polischuk, O, Pozzi, S, Previtali, E, Redon, Th, Rojas, A, Rozov, S, Rusconi, C, Sanglard, V., Scarpaci, J.A., Schäffner, K, Schmidt, B, Shen, Y, Shlegel, V, Siebenborn, B, Singh, V, Tomei, C, Tretyak, V, Umatov, V, Vagneron, L., Velázquez, M, Welliver, B, Winslow, L, Xue, M, Yakushev, E, Zarytskyy, M, Zolotarova, A. S., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Cryogénie (Cryo), Laboratoire Souterrain de Modane (LSM - UMR 6417), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), CUPID, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institute of Theoretical and Experimental Physics [Moscow] (ITEP), National Research Center 'Kurchatov Institute' (NRC KI), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Laboratori Nazionali di Frascati (INFN), LABORATORY NAZIONALI DI FRASCATI, Hélium : du fondamental aux applications (NEEL - HELFA), University of California [Berkeley] (UC Berkeley), University of California (UC), Nikolaev Institute of Inorganic Chemistry [Novosibirsk] (NIC), Siberian Branch of the Russian Academy of Sciences (SB RAS), Dzhelepov Laboratory of Nuclear Problems [Dubna] (DLNP), Joint Institute for Nuclear Research (JINR), Cryogénie (NEEL - Cryo), Istituto Nazionale di Fisica Nucleare [Sezione di Roma 1] (INFN), Istituto Nazionale di Fisica Nucleare, Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), Institut Rayonnement Matière de Saclay (IRAMIS), Institute for Nuclear Research of NAS of Ukraine, National Academy of Sciences of Ukraine (NASU), Karlsruhe Institute of Technology (KIT), Université Paris-Saclay, Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Fudan University [Shanghai], Massachusetts Institute of Technology (MIT), Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari (INFN, Sezione di Cagliari), Istituto Nazionale di Fisica Nucleare (INFN), University of Science and Technology of China [Hefei] (USTC), Istituto Nazionale di Fisica Nucleare, Sezione di Milano (INFN), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), University of Southern California (USC), Science et Ingénierie des Matériaux et Procédés (SIMaP), and Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )
Subjects: [PHYS]Physics [physics], [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], ComputingMilieux_MISCELLANEOUS
Abstract: International audience
Published: 2021

20. Precise measurement of $$2\nu \beta \beta $$ <math><mrow><mn>2</mn><mi>ν</mi><mi>β</mi><mi>β</mi></mrow></math> decay of $$^{100}$$ <math><msup><mrow></mrow><mn>100</mn></msup></math> Mo with the CUPID-Mo detection technology

Author: Armengaud, E., Augier, C., Barabash, A., Bellini, F., Benato, G., Benoît, A., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu., Bourgeois, Ch., Briere, M., Brudanin, V., Camus, P., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Charlieux, F., Combarieu, M., Dafinei, I., Danevich, F., Jesus, M., Dumoulin, L., Eitel, K., Elkhoury, E., Ferri, F., Fujikawa, B., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V., Gros, M., Guerard, E., Helis, D., Huang, H., Huang, R., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V., Kolomensky, Yu., Konovalov, S., Leder, A., Kotila, J., Loaiza, P., Ma, L., Makarov, E., Marcillac, P., Marini, L., Marnieros, S., Misiak, D., Navick, X.F., Nones, C., Novati, V., Olivieri, E., Ouellet, J., Pagnanini, L., Pari, P., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D., Polischuk, O., Previtali, E., Redon, Th., Rozov, S., Rusconi, C., Sanglard, V., Schäffner, K., Schmidt, B., Shen, Y., Shlegel, V., Siebenborn, B., Singh, V., Tomei, C., Tretyak, V., Umatov, V., Vagneron, L., Velázquez, M., Weber, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., and Zolotarova, A.
Abstract: We report the measurement of the two-neutrino double-beta ($$2\nu \beta \beta $$ 2νββ ) decay of $$^{100}$$ 100 Mo to the ground state of $$^{100}$$ 100 Ru using lithium molybdate ($$\hbox {Li}_2^{\;\;100}\hbox {MoO}_4$$ Li2100MoO4 ) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory (France). From a total exposure of 42.235 kg$$\times $$ × day, the half-life of $$^{100}$$ 100 Mo is determined to be $$T_{1/2}^{2\nu }=[7.12^{+0.18}_{-0.14}\,\mathrm {(stat.)}\pm 0.10\,\mathrm {(syst.)}]\times 10^{18}$$ T1/22ν=[7.12-0.14+0.18(stat.)±0.10(syst.)]×1018 years. This is the most accurate determination of the $$2\nu \beta \beta $$ 2νββ half-life of $$^{100}$$ 100 Mo to date.
Published: 2020

21. Identification of backgrounds in the EDELWEISS-I dark matter search experiment

Author: Fiorucci, S., Benoit, A., Bergé, L., Blümer, J., Broniatowski, A., Censier, B., Chantelauze, A., Chapellier, M., Chardin, G., Collin, S., Defay, X., De Jésus, M., Deschamps, H., Di Stefano, P., Dolgorouky, Y., Dumoulin, L., Eitel, K., Fesquet, M., Gascon, J., Gerbier, G., Goldbach, C., Gros, M., Horn, M., Juillard, A., Lemrani, R., de Lesquen, A., Lubashevskiy, A., Luca, M., Marnieros, S., Mosca, L., Navick, X.-F., Nollez, G., Olivieri, E., Pari, P., Sanglard, V., Schoeffel, L., Schwamm, F., Stern, M., and Yakushev, E.
Published: 2007
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22. EURECA — the European Future of Dark Matter Searches with Cryogenic Detectors

Author: Kraus, H., Bauer, M., Bavykina, I., Benoit, A., Blümer, J., Broniatowski, A., Brudanin, V., Burghart, G., Camus, P., Chantelauze, A., Chapellier, M., Chardin, G., Christ, P., Ciemniak, C., Coppi, C., De Jésus, M., De Lesquen, A., Deschamps, H., Di Stefano, P., Dumoulin, L., Eitel, K., von Feilitzsch, F., Fesquet, M., Gascon, J., Gerbier, G., Goldbach, C., Gros, M., Hauff, D., Henry, S., Horn, M., Imber, J., Isaila, C., Jochum, J., Juillard, A., Kimmerle, M., Lanfranchi, J.-C., Lemrani, R., Lubashevsky, A., Luca, M., Malek, M., Marnieros, S., McGowan, R., Mikhailik, V., Navick, X.-F., Niinikoski, T., Nollez, G., Pantic, E., Pari, P., Perevoshchikov, L., Petricca, F., Pfister, S., Potzel, W., Pröbst, F., Rau, W., Ritter, F., Rottler, K., Sanglard, V., Scholl, S., Schwamm, F., Seidel, W., Smolnikov, A., Stern, M., Teshima, M., Tolhurst, B., Westphal, W., Wikus, P., Wolf, J., and Yakushev, E.
Published: 2007
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23. EDELWEISS-II : Status and Future

Author: Sanglard, V.
Published: 2007
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24. Measurement of the response of heat-and-ionization germanium detectors to nuclear recoils

Author: Benoit, A., Bergé, L., Blümer, J., Broniatowski, A., Censier, B., Chantelauze, A., Chapellier, M., Chardin, G., Collin, S., Defay, X., De Jésus, M., Deschamps, H., Di Stefano, P., Dolgorouky, Y., Dumoulin, L., Eitel, K., Fesquet, M., Fiorucci, S., Gascon, J., Gerbier, G., Goldbach, C., Gros, M., Horn, M., Juillard, A., Lemrani, R., de Lesquen, A., Luca, M., Marnieros, S., Mosca, L., Navick, X.-F., Nollez, G., Olivieri, E., Pari, P., Sanglard, V., Schoeffel, L., Schwamm, F., and Stern, M.
Published: 2007
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25. Looking for SUSY with EDELWEISS-I and-II

Author: Gerbier, G., Benoît, A., Bergé, L., Broniatowski, A., Chabert, L., Chambon, B., Chardin, B., Chapellier, M., Charvin, P., De Jésus, M., Deschamps, H., Di Stefano, P., Drain, D., Dumoulin, L., Fiorucci, S., Gascon, J., Gerlic, E., Goldbach, C., Goyot, M., Gros, M., Hadjout, J. P., Hervé, S., Juillard, A., de Lesquen, A., Mallet, J., Marnieros, S., Martineau, O., Mosca, L., Navick, X. -F., Nollez, G., Pari, P., Riccio, C., Sanglard, V., Schoeffel, L., Stern, M., and Vagneron, L.
Published: 2004
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26. 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

27. EDELWEISS dark matter search update

Author: Di Stefano, P.C.F., Benoit, A., Bergé, L., Blümer, J., Broniatowski, A., Censier, B., Chabert, L., Chambon, B., Chapellier, M., Chardin, G., Charvin, P., De Jésus, M., Drain, D., Dumoulin, L., Eitel, K., Fesquet, M., Fiorucci, S., Gascon, J., Gerbier, G., Gerlic, E., Goldbach, C., Goyot, M., Gros, M., Habermahl, F., Horn, M., Hadjout, J.P., Hervé, S., Juillard, A., Kikuchi, C., de Lesquen, A., Luca, M., Mallet, J., Marnieros, S., Martineau, O., Mosca, L., Navick, X.F., Nollez, G., Pari, P., Riccio, C., Sanglard, V., Stern, M., Vagneron, L., and Villard, V.
Published: 2005
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28. CUPID pre-CDR

Author: Armstrong, W.R., Chang, C., Hafidi, K., Lisovenko, M., Novosad, V., Pearson, J., Polakovic, T., Wang, G., Yefremenko, V., Zhang, J., Bucci, C., Canonica, L., Cappelli, L., Caracciolo, V., Copello, S., D'Addabbo, A., Gorla, P., Nisi, S., Orlandi, D., Pagliarone, C.E., Pattavina, L., Pirro, S., Schaffner, K., Benato, G., Drobizhev, A., Fujikawa, B.K., Huang, R., Kolomensky, Yu.G., Marini, L., Norman, E., Sakai, M., Schmidt, B., Singh, V., Vetter, K., Wagaarachchi, S., Wallig, J., Welliver, B., Dell'oro, S., O'Donnell, T., Zucchelli, S., Moggi, N., Boldrini, V., Mancarella, F., Rizzi, R., Johnston, J., Ouellet, J., Formaggio, J., Winslow, L., Avignone, F., Rusconi, C., Creswick, R., Wilson, K., Franceschi, A., Napolitano, T., Caminata, A., Di Domizio, S., Pallavicni, M., Velazquez, M., Peng, H., Xue, M., Danevich, F., Kobychev, V., Polischuk, O., Tretyak, V., Azzolini, O., Keppel, G., Pira, C., Ferroni, F., Dompè, V., Fantini, G., Alfonso, K., Huang, H.Z., Arnaud, Q., Augier, C., Billard, J., Cazes, A., Charlieux, F., Elkhoury, E., Gascon, J., De Jesus, M., Juillard, A., Misiak, D., Sanglard, V., Vagneron, L., Beretta, M., Biassoni, M., Brofferio, C., Capelli, S., Carniti, P., Chiesa, D., Clemenza, M., Cremonesi, O., Faverzani, M., Ferri, E., Giachero, A., Gironi, L., Gotti, C., Nastasi, M., Nutini, I., Pagnanini, L., Pavan, M., Pessina, G., Pozzi, S., Previtali, E., Puiu, A., Sisti, M., Barabash, A., Konovalov, S., Yumatov, V., Heeger, K., Maruyama, R., Nikkel, J., Speller, D., Surukuchi, P.T., Shlegel, V., Bergé, L., Chapellier, M., Dumoulin, L., Giuliani, A., Khalife, H., De Marcillac, P., Marnieros, S., Olivieri, E., Poda, D., Redon, T., Zolotarova, A., Brière, M., Bourgeois, C., Guerard, E., Loaiza, P., Taffarello, L., Karapetrov, G., Bellini, F., Cardani, L., Casali, N., Cruciani, A., Dafinei, I., Pettinacci, V., D'Imperio, G., Tomei, C., Vignati, M., Colantoni, I., Armengaud, E., Charrier, A., De Combarieu, M., Ferri, F., Gras, Ph., Gros, M., Helis, D., Navick, X.F., Nones, C., Pari, P., Paul, B., Gutierrez, T., Han, K., Ma, L., Shen, Y., He, W., Martinez, M., Science et Ingénierie des Matériaux et Procédés (SIMaP ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), CUPID, Science et Ingénierie des Matériaux et Procédés (SIMaP), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National Polytechnique de Grenoble (INPG)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: Physics - Instrumentation and Detectors, data acquisition, FOS: Physical sciences, fabrication, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), double-beta decay: (0neutrino), [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), Nuclear Experiment, lepton number: violation, activity report, detector: design, CUORE, molybdenum: nuclide, Instrumentation and Detectors (physics.ins-det), calibration, molybdenum: oxygen, cryogenics, lithium, electronics: readout, scintillation counter: crystal, control system, performance, electronics: design
Abstract: International audience; CUPID is a proposed future tonne-scale bolometric neutrinoless double beta decay ($0\nu\beta\beta$) experiment to probe the Majorana nature of neutrinos and discover Lepton Number Violation in the so-called inverted hierarchy region of the neutrino mass. CUPID will be built on experience, expertise and lessons learned in CUORE, and will exploit the current CUORE infrastructure as much as possible. In order to achieve its ambitious science goals, CUPID aims to dramatically reduce the backgrounds in the region of interest introducing a high efficiently $\alpha$/$\beta$ discrimination techniques, also demonstrated by the CUPID-0 and CUPID-Mo experiments, and using a high transition energy double beta decay nucleus, $^{100}$Mo. This document describe the main concepts related with the design of the CUPID experiment and indicates the projected sensitivities and the global scientific goal of the experiment.
Published: 2019

29. Searching for low-mass dark matter particles with a massive Ge bolometer operated above ground

Author: Armengaud, E., Augier, C., Benoît, A., Benoit, A., Bergé, L., Billard, J., Broniatowski, A., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., Ducimetière, D., Dumoulin, L., Eitel, K., Filosofov, D., Gascon, J., Giuliani, A., Gros, M., De Jésus, M., Jin, Y., Juillard, A., Kleifges, M., Maisonobe, R., Marnieros, S., Misiak, D., Navick, X.-F., Nones, C., Olivieri, E., Oriol, C., Pari, P., Paul, B., Poda, D., Queguiner, E., Rozov, S., Sanglard, V., Siebenborn, B., Vagneron, L., Weber, M., Yakushev, E., Zolotarova, A., Kavanagh, B.J., GRAPPA (ITFA, IoP, FNWI), IoP (FNWI), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Nanosciences et de Nanotechnologies [Orsay] (C2N), Université Paris-Sud - Paris 11 (UP11)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Institut Rayonnement Matière de Saclay (IRAMIS), EDELWEISS, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Hélium : du fondamental aux applications (NEEL - HELFA), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), and Cryogénie (NEEL - Cryo)
Subjects: Physics - Instrumentation and Detectors, detector: cryogenics, Dark matter, energy resolution, FOS: Physical sciences, chemistry.chemical_element, S030DI5, Context (language use), Cosmic ray, Germanium, EDELWEISS, 01 natural sciences, 7. Clean energy, Cosmology, law.invention, thermal, Nuclear physics, energy: threshold, particle: massive, bolometer, cosmic rays, law, 0103 physical sciences, surface, Experiments in gravity, Neutron, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Nuclear Experiment, Instrumentation and Methods for Astrophysics (astro-ph.IM), nucleus: recoil, Physics, cross section, S030DP5, 010308 nuclear & particles physics, shielding, background, dark matter: mass, Bolometer, Instrumentation and Detectors (physics.ins-det), Astrophysics - Astrophysics of Galaxies, S030DN5, chemistry, Astrophysics of Galaxies (astro-ph.GA), germanium: target, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], cosmology
Abstract: The EDELWEISS collaboration has performed a search for dark matter particles with masses below the GeV-scale with a 33.4-g germanium cryogenic detector operated in a surface lab. The energy deposits were measured using a neutron-transmutation-doped Ge thermal sensor with a 17.7~eV (RMS) baseline heat energy resolution leading to a 60~eV analysis energy threshold. Despite a moderate lead shielding and the high-background environment, the first sub-GeV spin-independent dark matter limit based on a germanium target has been achieved. The experiment provides the most stringent, nuclear recoil based, above-ground limit on spin-independent interactions above 600~MeV/c$^{2}$. The experiment also provides the most stringent limits on spin-dependent interactions with protons and neutrons below 1.3~GeV/c$^{2}$. Furthermore, the dark matter search results were studied in the context of Strongly Interacting Massive Particles, taking into account Earth-shielding effects, for which new regions of the available parameter space have been excluded. Finally, the dark matter search has also been extended to interactions via the Migdal effect, resulting for the first time in the exclusion of particles with masses between 45 and 150~MeV/c$^{2}$ with spin-independent cross sections ranging from $10^{-29}$ to $10^{-26}$~cm$^2$., 16 pages, 8 figures. New figure added for Spin-Dependent interactions. Accepted in Phys. Rev. D
Published: 2019

30. Calibration of the EDELWEISS cryogenic heat-and-ionization germanium detectors for dark matter search

Author: Martineau, O., Benoı̂t, A., Bergé, L., Broniatowski, A., Chabert, L., Chambon, B., Chapellier, M., Chardin, G., Charvin, P., De Jésus, M., Di Stefano, P., Drain, D., Dumoulin, L., Gascon, J., Gerbier, G., Gerlic, E., Goldbach, C., Goyot, M., Gros, M., Hadjout, J.P., Hervé, S., Juillard, A., de Lesquen, A., Loidl, M., Mallet, J., Marnieros, S., Mirabolfathi, N., Mosca, L., Navick, X.-F., Nollez, G., Pari, P., Riccio, C., Sanglard, V., Schoeffel, L., Stern, M., and Vagneron, L.
Published: 2004
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31. Latest results from the EDELWEISS WIMP search

Author: Marnieros, S., Benoit, A., Bergé, L., Broniatowski, A., Censier, B., Chabert, L., Chambon, B., Chapellier, M., Chardin, G., Charvin, P., Jésus, M.De, Stefano, P.Di, Drain, D., Dumoulin, L., Fesquet, M., Fiorucci, S., Gascon, J., Gerbier, G., Gerlic, E., Goldbach, C., Goyot, M., Gros, M., Hadjout, J.P., Hervé, S., Juillard, A., Kikuchi, C., de Lesquen, A., Mallet, J., Martineau, O., Mosca, L., Navick, X.F., Nollez, G., Pari, P., Riccio, C., Sanglard, V., Stern, M., Vagneron, L., and Villard, V.
Published: 2004
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32. Development of $^{100}$Mo-containing scintillating bolometers for a high-sensitivity neutrinoless double-beta decay search

Author: Armengaud, E., Augier, C., Barabash, A.S., Beeman, J.W., Bekker, T.B., Bellini, F., Benoît, A., Bergé, L., Bergmann, T., Billard, J., Boiko, R.S., Broniatowski, A., Brudanin, V., Camus, P., Capelli, S., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Charlieux, F., Chernyak, D.M., De Combarieu, M., Coron, N., Danevich, F.A., Dafinei, I., De Jesus, M., Devoyon, L., Di Domizio, S., Dumoulin, L., Eitel, K., Enss, C., Ferroni, F., Fleischmann, A., Foerster, N., Gascon, J., Gastaldo, L., Gironi, L., Giuliani, A., Grigorieva, V.D., Gros, M., Hehn, L., Hervé, S., Humbert, V., Ivannikova, N.V., Ivanov, I.M., Jin, Y., Juillard, A., Kleifges, M., Kobychev, V.V., Konovalov, S.I., Koskas, F., Kozlov, V., Kraus, H., Kudryavtsev, V.A., Laubenstein, M., Le Sueur, H., Loidl, M., Magnier, P., Makarov, E.P., Mancuso, M., De Marcillac, P., Marnieros, S., Marrache-Kikuchi, C., Nagorny, S., Navick, X-F., Nikolaichuk, M.O., Nones, C., Novati, V., Olivieri, E., Pagnanini, L., Pari, P., Pattavina, L., Pavan, M., Paul, B., Penichot, Y., Pessina, G., Piperno, G., Pirro, S., Plantevin, O., Poda, D.V., Queguiner, E., Redon, T., Rodrigues, M., Rozov, S., Rusconi, C., Sanglard, V., Schäffner, K., Scorza, S., Shlegel, V.N., Siebenborn, B., Strazzer, O., Tcherniakhovski, D., Tomei, C., Tretyak, V.I., Umatov, V.I., Vagneron, L., Vasiliev, Ya.V., Velazquez, M., Vignati, M., Weber, M., Yakushev, E., Zolotarova, A.S., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre de Nanosciences et de Nanotechnologies [Orsay] (C2N), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Saclay, 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), Institut de Chimie de la Matière Condensée de Bordeaux (ICMCB), Université de Bordeaux (UB)-Institut Polytechnique de Bordeaux-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Université Paris-Saclay-Direction de Recherche Technologique (CEA) (DRT (CEA)), Université de Bordeaux (UB)-Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique (CNRS), Armengaud, E, Augier, C, Barabash, A, Beeman, J, Bekker, T, Bellini, F, Benoît, A, Bergé, L, Bergmann, T, Billard, J, Boiko, R, Broniatowski, A, Brudanin, V, Camus, P, Capelli, S, Cardani, L, Casali, N, Cazes, A, Chapellier, M, Charlieux, F, Chernyak, D, de Combarieu, M, Coron, N, Danevich, F, Dafinei, I, Jesus, M, Devoyon, L, Domizio, S, Dumoulin, L, Eitel, K, Enss, C, Ferroni, F, Fleischmann, A, Foerster, N, Gascon, J, Gastaldo, L, Gironi, L, Giuliani, A, Grigorieva, V, Gros, M, Hehn, L, Hervé, S, Humbert, V, Ivannikova, N, Ivanov, I, Jin, Y, Juillard, A, Kleifges, M, Kobychev, V, Konovalov, S, Koskas, F, Kozlov, V, Kraus, H, Kudryavtsev, V, Laubenstein, M, Sueur, H, Loidl, M, Magnier, P, Makarov, E, Mancuso, M, de Marcillac, P, Marnieros, S, Marrache-Kikuchi, C, Nagorny, S, Navick, X, Nikolaichuk, M, Nones, C, Novati, V, Olivieri, E, Pagnanini, L, Pari, P, Pattavina, L, Pavan, M, Paul, B, Penichot, Y, Pessina, G, Piperno, G, Pirro, S, Plantevin, O, Poda, D, Queguiner, E, Redon, T, Rodrigues, M, Rozov, S, Rusconi, C, Sanglard, V, Schäffner, K, Scorza, S, Shlegel, V, Siebenborn, B, Strazzer, O, Tcherniakhovski, D, Tomei, C, Tretyak, V, Umatov, V, Vagneron, L, Vasiliev, Y, Velázquez, M, Vignati, M, Weber, M, Yakushev, E, Zolotarova, A, Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Institut de Physique Nucléaire de Lyon ( IPNL ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Néel ( NEEL ), Université Grenoble Alpes [Saint Martin d'Hères]-Centre National de la Recherche Scientifique ( CNRS ), Centre de Sciences Nucléaires et de Sciences de la Matière ( CSNSM ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut d'astrophysique spatiale ( IAS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Intégration des Systèmes et des Technologies ( LIST ), Institut de Chimie de la Matière Condensée de Bordeaux ( ICMCB ), Université de Bordeaux ( UB ) -Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique ( CNRS ), Kurchatov NBIC Centre, National Research Centre, Kurchatov Institute, Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Sobolev Institute of Geology and Mineralogy [Novosibirsk], Siberian Branch of the Russian Academy of Sciences (SB RAS), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Hélium : du fondamental aux applications (NEEL - HELFA), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Karlsruhe Institute of Technology (KIT), Kiev Institute for Nuclear Research, Joint Institute for Nuclear Research (JINR), Cryogénie (NEEL - Cryo), Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), Istituto Nazionale di Fisica Nucleare [Sezione di Roma 1] (INFN), Istituto Nazionale di Fisica Nucleare, Kiev Institute for Nuclear Research (KINR), Ukrainian Academy of Sciences, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Università degli studi di Genova = University of Genoa (UniGe), Kirchhoff Institute for Physics, Universität Heidelberg [Heidelberg] = Heidelberg University, Universitá degli Studi dell’Insubria = University of Insubria [Varese] (Uninsubria), University of Oxford, University of Sheffield [Sheffield], Laboratori Nazionali del Gran Sasso (LNGS), Istituto Nazionale di Fisica Nucleare (INFN), Laboratoire National Henri Becquerel (LNHB), Département Métrologie Instrumentation & Information (DM2I), 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)-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)), Nikolaev Institute of Inorganic Chemistry [Novosibirsk] (NIC), Laboratori Nazionali di Frascati (LNF), and National Research Centre 'Kurchatov Institute': Petersburg Nuclear Physics Institute
Subjects: Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), energy resolution, Double-beta decay, FOS: Physical sciences, fabrication, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], high optical quality, quality: optical, engineering (miscellaneous), physics and astronomy (miscellaneous), 100 Mo -enriched scintillating bolometers, boule recrystallization, lithium molybdate detectors, 23.40.-s, bolometer, double-beta decay: (0neutrino), ddc:530, Scintillating bolometer, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear Experiment (nucl-ex), Engineering (miscellaneous), [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment, Enriched $^{100}$Mo, Zinc molybdate, S076H2N, Lithium molybdate, CUORE, molybdenum: nuclide, Physics, zinc, Instrumentation and Detectors (physics.ins-det), 29.40.Mc, molybdenum: oxygen, Physics and Astronomy, lithium, scintillation counter: crystal, performance
Abstract: This paper reports on the development of a technology involving $^{100}$Mo-enriched scintillating bolometers, compatible with the goals of CUPID, a proposed next-generation bolometric experiment to search for neutrinoless double-beta decay. Large mass ($\sim$1~kg), high optical quality, radiopure $^{100}$Mo-containing zinc and lithium molybdate crystals have been produced and used to develop high performance single detector modules based on 0.2--0.4~kg scintillating bolometers. In particular, the energy resolution of the lithium molybdate detectors near the $Q$-value of the double-beta transition of $^{100}$Mo (3034~keV) is 4--6~keV FWHM. The rejection of the $\alpha$-induced dominant background above 2.6~MeV is better than 8$\sigma$. Less than 10~$\mu$Bq/kg activity of $^{232}$Th ($^{228}$Th) and $^{226}$Ra in the crystals is ensured by boule recrystallization. The potential of $^{100}$Mo-enriched scintillating bolometers to perform high sensitivity double-beta decay searches has been demonstrated with only 10~kg$\times$d exposure: the two neutrino double-beta decay half-life of $^{100}$Mo has been measured with the up-to-date highest accuracy as $T_{1/2}$ = [6.90 $\pm$ 0.15(stat.) $\pm$ 0.37(syst.)] $\times$ 10$^{18}$~yr. Both crystallization and detector technologies favor lithium molybdate, which has been selected for the ongoing construction of the CUPID-0/Mo demonstrator, containing several kg of $^{100}$Mo., Comment: 25 pages, 12 figures, 8 tables; submitted to EPJC
Published: 2017

33. Complete event-by-event α/γ(β) separation in a full-size TeO2 CUORE bolometer by simultaneous heat and light detection

Author: Bergé, L., Chapellier, M., Combarieu, M.D., Dumoulin, L., Giuliani, A., Gros, M., Marcillac, P.D., Marnieros, S., Nones, C., Novati, V., Olivieri, E., Paul, B., Poda, D.V., Redon, T., Siebenborn, B., Zolotarova, A.S., Armengaud, E., Augier, C., Benoît, A., Billard, J., Broniatowski, A., Camus, P., Cazes, A., Charlieux, F., Jesus, M.D., Eitel, K., Foerster, N., Gascon, J., Jin, Y., Juillard, A., Kleifges, M., Kozlov, V., Kraus, H., Kudryavtsev, V.A., Sueur, H.L., Maisonobe, R., Navick, X-F., Pari, P., Queguiner, E., Rozov, S., Sanglard, V., Vagneron, L., Weber, M., and Yakushev, E.
Abstract: The CUORE project began recently a search for neutrinoless double-beta decay ($0\nu\beta\beta$) of $^{130}$Te with a $\mathcal{O}$(1 ton) TeO$_2$ bolometer array. In this experiment, the background suppression relies essentially on passive shielding, material radiopurity and anti-coincidences. The lack of particle identification in CUORE makes $\alpha$ decays at the detector surface the dominant background, at the level of $\sim$0.01 counts/(keV kg y) in the region of interest ($Q$-value of $0\nu\beta\beta$ of the order of 2.5 MeV). In the present work we demonstrate, for the first time with a CUORE-size (5$\times$5$\times$5 cm) TeO$_2$ bolometer and using the same technology as CUORE for the readout of the bolometric signals, an efficient $\alpha$ particle discrimination (99.9\%) with a high acceptance of the $0\nu\beta\beta$ signal (about 96\%). This unprecedented result was possible thanks to the superior performance (10 eV RMS baseline noise) of a Neganov-Luke-assisted germanium bolometer used to detect a tiny (70 eV) light signal dominated by $\gamma$($\beta$)-induced Cherenkov radiation in the TeO$_2$ detector. The obtained results represent a major breakthrough towards the TeO$_2$-based version of CUPID, a ton-scale cryogenic $0\nu\beta\beta$ experiment proposed as a follow-up to CUORE with particle identification.
Published: 2018

34. Complete event-by-event $\alpha/\gamma(\beta)$ separation in a full-size ${\mathrm{TeO}}_{2}$ CUORE bolometer by Neganov-Luke-magnified light detection

Author: Bergé , L., Chapellier , M., De Combarieu , M., Dumoulin , L., Giuliani , A., Gros , M., De Marcillac , P., Marnieros , S., Nones , C., Novati , V., Olivieri , E., Paul , B., Poda , D.V., Redon , T., Siebenborn , B., Zolotarova , A.S., Armengaud , E., Augier , C., Benoît , A., Billard , J., Broniatowski , A., Camus , P., Cazes , A., Charlieux , F., De Jesus , M., Eitel , K., Foerster , N., Gascon , J., Jin , Y., Juillard , A., Kleifges , M., Kozlov , V., Kraus , H., Kudryavtsev , V.A., Le Sueur , H., Maisonobe , R., Navick , X-F., Pari , P., Queguiner , E., Rozov , S., Sanglard , V., Vagneron , L., Weber , M., Yakushev , E., Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut Rayonnement Matière de Saclay (IRAMIS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut Néel (NEEL), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Centre de Nanosciences et de Nanotechnologies [Orsay] (C2N), Université Paris-Sud - Paris 11 (UP11)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Cryogénie (NEEL - Cryo), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Centre de Sciences Nucléaires et de Sciences de la Matière ( CSNSM ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Rayonnement Matière de Saclay ( IRAMIS ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Institut de Physique Nucléaire de Lyon ( IPNL ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Néel ( NEEL ), and Université Grenoble Alpes [Saint Martin d'Hères]-Centre National de la Recherche Scientifique ( CNRS )
Subjects: CUORE, Physics - Instrumentation and Detectors, electron: particle identification, radiation: Cherenkov, tellurium: oxygen, helium: particle identification, photon: particle identification, High Energy Physics - Experiment, helium: background, bolometer, double-beta decay: (0neutrino), [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], tellurium: nuclide, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], performance, background: suppression
Abstract: In the present work, we describe the results obtained with a large ($\approx 133$ cm$^3$) TeO$_2$ bolometer, with a view to a search for neutrinoless double-beta decay ($0\nu\beta\beta$) of $^{130}$Te. We demonstrate an efficient $\alpha$ particle discrimination (99.9\%) with a high acceptance of the $0\nu\beta\beta$ signal (about 96\%), expected at $\approx 2.5$ MeV. This unprecedented result was possible thanks to the superior performance (10 eV rms baseline noise) of a Neganov-Luke-assisted germanium bolometer used to detect a tiny (70 eV) light signal from the TeO$_2$ detector, dominated by $\gamma$($\beta$)-induced Cherenkov radiation but exhibiting also a clear scintillation component. The obtained results represent a major breakthrough towards the TeO$_2$-based version of CUORE Upgrade with Particle IDentification (CUPID), a ton-scale cryogenic $0\nu\beta\beta$ experiment proposed as a follow-up to the CUORE project with particle identification. The CUORE experiment began recently a search for neutrinoless double-beta decay of $^{130}$Te with an array of 988 125-cm$^3$ TeO$_2$ bolometers. The lack of $\alpha$ discrimination in CUORE makes $\alpha$ decays at the detector surface the dominant background component, at the level of $\approx 0.01$ counts/(keV kg y) in the region of interest. We show here, for the first time with a CUORE-size bolometer and using the same technology as CUORE for the readout of both heat and light signals, that surface $\alpha$ background can be fully rejected., Comment: The second version reflects the changes made after PRC referees' comments
Published: 2018

35. Development of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{100}\hbox {Mo}$$\end{document}100Mo-containing scintillating bolometers for a high-sensitivity neutrinoless double-beta decay search

Author: Armengaud, E., Augier, C., Barabash, A. S., Beeman, J. W., Bekker, T. B., Bellini, F., Benoît, A., Bergé, L., Bergmann, T., Billard, J., Boiko, R. S., Broniatowski, A., Brudanin, V., Camus, P., Capelli, S., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Charlieux, F., Chernyak, D. M., de Combarieu, M., Coron, N., Danevich, F. A., Dafinei, I., Jesus, M. De, Devoyon, L., Domizio, S. Di, Dumoulin, L., Eitel, K., Enss, C., Ferroni, F., Fleischmann, A., Foerster, N., Gascon, J., Gastaldo, L., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Hehn, L., Hervé, S., Humbert, V., Ivannikova, N. V., Ivanov, I. M., Jin, Y., Juillard, A., Kleifges, M., Kobychev, V. V., Konovalov, S. I., Koskas, F., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Laubenstein, M., Sueur, H. Le, Loidl, M., Magnier, P., Makarov, E. P., Mancuso, M., de Marcillac, P., Marnieros, S., Marrache-Kikuchi, C., Nagorny, S., Navick, X-F., Nikolaichuk, M. O., Nones, C., Novati, V., Olivieri, E., Pagnanini, L., Pari, P., Pattavina, L., Pavan, M., Paul, B., Penichot, Y., Pessina, G., Piperno, G., Pirro, S., Plantevin, O., Poda, D. V., Queguiner, E., Redon, T., Rodrigues, M., Rozov, S., Rusconi, C., Sanglard, V., Schäffner, K., Scorza, S., Shlegel, V. N., Siebenborn, B., Strazzer, O., Tcherniakhovski, D., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Vasiliev, Ya. V., Velázquez, M., Vignati, M., Weber, M., Yakushev, E., and Zolotarova, A. S.
Subjects: Regular Article - Experimental Physics
Abstract: This paper reports on the development of a technology involving \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{100}\hbox {Mo}$$\end{document}100Mo-enriched scintillating bolometers, compatible with the goals of CUPID, a proposed next-generation bolometric experiment to search for neutrinoless double-beta decay. Large mass (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\sim 1~\hbox {kg}$$\end{document}∼1kg), high optical quality, radiopure \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{100}\hbox {Mo}$$\end{document}100Mo-containing zinc and lithium molybdate crystals have been produced and used to develop high performance single detector modules based on 0.2–0.4 kg scintillating bolometers. In particular, the energy resolution of the lithium molybdate detectors near the Q-value of the double-beta transition of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{100}\hbox {Mo}$$\end{document}100Mo (3034 keV) is 4–6 keV FWHM. The rejection of the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\alpha $$\end{document}α-induced dominant background above 2.6 MeV is better than \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$8\sigma $$\end{document}8σ. Less than \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10~\upmu \hbox {Bq/kg}$$\end{document}10μBq/kg activity of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{232}\hbox {Th}\, (^{228}\hbox {Th})$$\end{document}232Th(228Th) and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{226}\hbox {Ra}$$\end{document}226Ra in the crystals is ensured by boule recrystallization. The potential of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{100}\hbox {Mo}$$\end{document}100Mo-enriched scintillating bolometers to perform high sensitivity double-beta decay searches has been demonstrated with only \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10~\hbox {kg}\times \hbox {d}$$\end{document}10kg×d exposure: the two neutrino double-beta decay half-life of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{100}\hbox {Mo}$$\end{document}100Mo has been measured with the up-to-date highest accuracy as \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$T_{1/2}$$\end{document}T1/2 = [6.90 ± 0.15(stat.) ± 0.37(syst.)] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\times ~10^{18}~\hbox {years}$$\end{document}×1018years. Both crystallization and detector technologies favor lithium molybdate, which has been selected for the ongoing construction of the CUPID-0/Mo demonstrator, containing several kg of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{100}\hbox {Mo}$$\end{document}100Mo.
Published: 2017

36. Recent results on Low Mass WIMP search with the EDELWEISS-III experiment

Author: Sanglard, V., Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Matière noire (MANOIR), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), EDELWEISS-III, and Girod, Dominique
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], ComputingMilieux_MISCELLANEOUS
Abstract: International audience
Published: 2016

37. Scintillating bolometers based on ZnMoO4 and Zn100MoO4 crystals to search for 0ν2β decay of 100Mo (LUMINEU project): first tests at the Modane Underground Laboratory

Author: Poda, D.V., Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Boiko, R.S., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Camus, P., Cazes, A., Censier, B., Chapellier, M., Charlieux, F., Chernyak, D.M., Coron, N., Coulter, P., Cox, G.A., Danevich, F.A., Boissière, T.D., Decourt, R., Jesus, M.D., Devoyon, L., Drillien, A.-A., Dumoulin, L., Eitel, K., Enss, C., Filosofov, D., Fleischmann, A., Fourches, N., Gascon, J., Gastaldo, L., Gerbier, G., Giuliani, A., Gros, M., Hehn, L., Henry, S., Hervé, S., Heuermann, G., Humbert, V., Ivanov, I.M., Juillard, A., Kéfélian, C., Kleifges, M., Kluck, H., Kobychev, V.V., Koskas, F., Kozlov, V., Kraus, H., Kudryavtsev, V.A., Sueur, H.L., Loidl, M., Magnier, P., Makarov, E.P., Mancuso, M., Marcillac, P.D., Marnieros, S., Marrache-Kikuchi, C., Menshikov, A., Nasonov, S.G., Navick, X.-F., Nones, C., Olivieri, E., Pari, P., Paul, B., Penichot, Y., Pessina, G., Piro, M.C., Plantevin, O., Redon, T., Robinson, M., Rodrigues, M., Rozov, S., Sanglard, V., Schmidt, B., Shlegel, V.N., Siebenborn, B., Strazzer, O., Tcherniakhovski, D., Tenconi, M., Torres, L., Tretyak, V.I., Vagneron, L., Vasiliev, Y.V., Velazquez, M., Viraphong, O., Walker, R.J., Weber, M., Yakushev, E., Zhang, X., Zhdankov, V.N., Collaboration, L., and Collaboration, E.
Abstract: The technology of scintillating bolometers based on zinc molybdate (ZnMoO4) crystals is under development within the LUMINEU project to search for decay of 100Mo with the goal to set the basis for large scale experiments capable to explore the inverted hierarchy region of the neutrino mass pattern. Advanced ZnMoO4 crystal scintillators with mass of ∼0.3 kg were developed and Zn100MoO4 crystal from enriched 100Mo was produced for the first time by using the low-thermal-gradient Czochralski technique. One ZnMoO4 scintillator and two samples (59 g and 63 g) cut from the enriched boule were tested aboveground at milli-Kelvin temperature as scintillating bolometers showing a high detection performance. The first results of the low background measurements with three ZnMoO4 and two enriched detectors installed in the EDELWEISS set-up at the Modane Underground Laboratory (France) are presented.
Published: 2016

38. Constraints on low-mass WIMPs from the EDELWEISS-III dark matter search

Author: EDELWEISS Collaboration, Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Bergmann, T., Billard, J., Blümer, J., de Boissière, T., Bres, G., Broniatowski, A., Brudanin, V., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., Dumoulin, L., Eitel, K., Filosofov, D., Foerster, N., Fourches, N., Garde, G., Gascon, J., Gerbier, G., Giuliani, A., Grollier, M., Gros, M., Hehn, L., Hervé, S., Heuermann, G., Humbert, V., De Jésus, M., Jin, Y., Jokisch, S., Juillard, A., Kéfélian, C., Kleifges, M., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Le-Sueur, H., Lin, J., Mancuso, M., Marnieros, S., Menshikov, A., Navick, X. -F., Nones, C., Olivieri, E., Pari, P., Paul, B., Piro, M. -C., Poda, D. V., Queguiner, E., Robinson, M., Rodenas, H., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Siebenborn, B., Tcherniakhovski, D., Vagneron, L., Weber, M., Yakushev, E., Zhang, X., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Matière noire (MANOIR), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Electronique (ElecLab), Cryogénie (Cryo), Laboratoire de photonique et de nanostructures (LPN), Centre National de la Recherche Scientifique (CNRS), Institut Rayonnement Matière de Saclay (IRAMIS), EDELWEISS, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Hélium : du fondamental aux applications (NEEL - HELFA), Electronique (NEEL - ElecLab), and Cryogénie (NEEL - Cryo)
Subjects: Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Dark matter, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, EDELWEISS, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), WIMP, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Elastic scattering, Physics, Range (particle radiation), 010308 nuclear & particles physics, Scattering, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Weakly interacting massive particles, High Energy Physics::Experiment, Low Mass, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the results of a search for elastic scattering from galactic dark matter in the form of Weakly Interacting Massive Particles (WIMPs) in the 4-30 GeV/$c^2$ mass range. We make use of a 582 kg-day fiducial exposure from an array of 800 g Germanium bolometers equipped with a set of interleaved electrodes with full surface coverage. We searched specifically for $\sim 2.5-20$ keV nuclear recoils inside the detector fiducial volume. As an illustration the number of observed events in the search for 5 (resp. 20) GeV/$c^2$ WIMPs are 9 (resp. 4), compared to an expected background of 6.1 (resp. 1.4). A 90% CL limit of $4.3\times 10^{-40}$ cm$^2$ (resp. $9.4\times 10^{-44}$ cm$^2$) is set on the spin-independent WIMP-nucleon scattering cross-section for 5 (resp. 20) GeV/$c^2$ WIMPs. This result represents a 41-fold improvement with respect to the previous EDELWEISS-II low-mass WIMP search for 7 GeV/$c^2$ WIMPs. The derived constraint is in tension with hints of WIMP signals from some recent experiments, thus confirming results obtained with different detection techniques., Matches published version
Published: 2016

39. LUMINEU: A search for neutrinoless double beta decay based on ZnMoO₄ scintillating bolometers

Author: Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Boiko, S., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., Chernyak, D. M., Coron, N., Coulter, P., Danevich, F. A., De Boissiére, T., Decourt, R., De Jesus, M., Devoyon, L., Drillien, A.-A., Dumoulin, L., Eitel, K., Enss, C., Filosofov, D., Fleischmann, A., Foerster, N., Fourches, N., Gascon, J., Gastaldo, L., Gerbier, G., Giuliani, A., Gray, D., Gros, M., Hehn, L., Henry, S., Hervé, S., Heuermann, G., Humbert, V., Ivanov, I. M., Juillard, A., Kéfélian, C., Kleifges, M., Kluck, H., Kobychev, V. V., Koskas, F., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Le Sueur, H., Loidl, M., Magnier, P., Makarov, E. P., Mancuso, M., De Marcillac, P., Marnieros, S., Marrache-Kikuchi, C., Menshikov, A., Nasonov, S. G., Navick, X.-F., Nones, C., Olivieri, E., Pari, P., Paul, B., Penichot, Y., Pessina, G., Piro, M. C., Plantevin, O., Poda, D. V., Redon, T., Robinson, M., Rodrigues, M., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Shlegel, V. N., Siebenborn, B., Strazzer, O., Tcherniakhovski, D., Tenconi, M., Torres, L., Tretyak, V. I., Vagneron, L., Vasiliev, Ya V., Velazquez, M., Viraphong, O., Walker, R. J., Weber, M., Yakushev, E., Zhang, X., and Zhdankov, V. N.
Subjects: Physics, ddc:530
Abstract: The LUMINEU is designed to investigate the possibility to search for neutrinoless double beta decay in $^{100}$Mo by means of a large array of scintillating bolometers based on ZnMoO$_{4}$ crystals enriched in $^{100}$Mo. High energy resolution and relatively fast detectors, which are able to measure both the light and the heat generated upon the interaction of a particle in a crystal, are very promising for the recognition and rejection of background events. We present the LUMINEU concepts and the experimental results achieved aboveground and underground with large-mass natural and enriched crystals. The measured energy resolution, the α/β discrimination power and the radioactive internal contamination are all within the specifications for the projected final LUMINEU sensitivity. Simulations and preliminary results confirm that the LUMINEU technology can reach zero background in the region of interest (around 3 MeV) with exposures of the order of hundreds kg x years, setting the bases for a next generation 0ν2β decay experiment capable to explore the inverted hierarchy region of the neutrino mass pattern.
Published: 2016

40. LUMINEU: a search for neutrinoless double beta decay based on ZnMoO$_4$ scintillating bolometers

Author: Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Boiko, S., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., Chernyak, D. M., Coron, N., Coulter, P., Danevich, F. A., De Boissiére, T., Decourt, R., De Jesus, M., Devoyon, L., Drillien, A. A., Dumoulin, L., Eitel, K., Enss, C., Filosofov, D., Fleischmann, A., Foerster, N., Fourches, N., Gascon, J., Gastaldo, L., Gerbier, G., Giuliani, ANDREA ERNESTO GUIDO, Gray, D., Gros, M., Hehn, L., Henry, S., Hervé, S., Heuermann, G., Humbert, V., Ivanov, I. M., Juillard, A., Kéfélian, C., Kleifges, M., Kluck, H., Kobychev, V. V., Koskas, F., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Le Sueur, H., Loidl, M., Magnier, P., Makarov, E. P., Mancuso, Michele, De Marcillac, P., Marnieros, S., Marrache Kikuchi, C., Menshikov, A., Nasonov, S. G., Navick, X. F., Nones, C., Olivieri, E., Pari, P., Paul, B., Penichot, Y., Pessina, G., Piro, M. C., Plantevin, O., Poda, D. V., Redon, T., Robinson, M., Rodrigues, M., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Shlegel, V. N., Siebenborn, B., Strazzer, O., Tcherniakhovski, D., Tenconi, M., Torres, L., Tretyak, V. I., Vagneron, L., Vasiliev, Y. a. V., Velazquez, M., Viraphong, O., Walker, R. J., Weber, M., Yakushev, E., Zhang, X., Zhdankov, V. N., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Bordeaux (UB), 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), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Université Paris-Saclay-Direction de Recherche Technologique (CEA) (DRT (CEA)), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Institut de Physique Nucléaire de Lyon ( IPNL ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Centre de Sciences Nucléaires et de Sciences de la Matière ( CSNSM ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Néel ( NEEL ), Université Grenoble Alpes [Saint Martin d'Hères]-Centre National de la Recherche Scientifique ( CNRS ), Institut d'astrophysique spatiale ( IAS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Université de Bordeaux ( UB ), Laboratoire d'Intégration des Systèmes et des Technologies ( LIST ), Hélium : du fondamental aux applications (NEEL - HELFA), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Karlsruhe Institute of Technology (KIT), Joint Institute for Nuclear Research (JINR), Cryogénie (NEEL - Cryo), Kiev Institute for Nuclear Research (KINR), Ukrainian Academy of Sciences, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), University of Oxford, Kirchhoff Institut für Physik, Universität Heidelberg [Heidelberg] = Heidelberg University, Nikolaev Institute of Inorganic Chemistry [Novosibirsk] (NIC), Siberian Branch of the Russian Academy of Sciences (SB RAS), University of Sheffield [Sheffield], Laboratoire National Henri Becquerel (LNHB), Département Métrologie Instrumentation & Information (DM2I), 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)-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)), Istituto Nazionale di Fisica Nucleare, Sezione di Milano (INFN), Istituto Nazionale di Fisica Nucleare (INFN), CML Ltd., University of Torino, INFN, and Fornengo, Nicolao (ed.) (University of Torino and INFN)
Subjects: History, Physics - Instrumentation and Detectors, design, hierarchy, 7. Clean energy, 01 natural sciences, neutrino mass, law.invention, Crystal, molybdenum, law, energy resolution: measured, beta-rays, neutrino: mass, Nuclear Experiment (nucl-ex), [ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear Experiment, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], nuclear instrumentation, Physics, instrumentation, Detector, Resolution (electron density), double-beta decay, Instrumentation and Detectors (physics.ins-det), high energy resolution, 3. Good health, Computer Science Applications, particle: interaction, experimental equipment, radioactivity, technology, Neutrino, ionizing radiation, performance, FOS: Physical sciences, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Education, crystal, Nuclear physics, interaction particle, Physics and Astronomy (all), bolometer, double-beta decay: (0neutrino), Double beta decay, 0103 physical sciences, Sensitivity (control systems), [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, scintillation counter, detector, 010308 nuclear & particles physics, background, Bolometer, Neutrinoless, sensitivity, energy resolution: high, Energy (signal processing), experimental results
Abstract: The LUMINEU is designed to investigate the possibility to search for neutrinoless double beta decay in $^{100}$Mo by means of a large array of scintillating bolometers based on ZnMoO$_4$ crystals enriched in $^{100}$Mo. High energy resolution and relatively fast detectors, which are able to measure both the light and the heat generated upon the interaction of a particle in a crystal, are very promising for the recognition and rejection of background events. We present the LUMINEU concepts and the experimental results achieved aboveground and underground with large-mass natural and enriched crystals. The measured energy resolution, the $\alpha/\beta$ discrimination power and the radioactive internal contamination are all within the specifications for the projected final LUMINEU sensitivity. Simulations and preliminary results confirm that the LUMINEU technology can reach zero background in the region of interest (around 3 MeV) with exposures of the order of hundreds kg$\times$years, setting the bases for a next generation $0\nu2\beta$ decay experiment capable to explore the inverted hierarchy region of the neutrino mass pattern., Comment: 5 pages, 3 figures, submitted as proceedings of the TAUP 2015 conference
Published: 2015

41. Scintillating bolometers based on ZnMoO$_4$ and Zn$^{100}$MoO$_4$ crystals to search for 0$\nu$2$\beta$ decay of $^{100}$Mo (LUMINEU project): first tests at the Modane Underground Laboratory

Author: Poda, D. V., Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Boiko, R. S., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Camus, P., Cazesb, A., Chapellier, M., Charlieux, F., Chernyak, D. M., Coron, N., Coulter, P., Danevich, F. A., de Boissière, T., Decourt, R., De Jesus, M., Devoyon, L., Drillien, A. A., Dumoulin, L., Eitel, K., Enss, C., Filosofov, D., Fleischmann, A., Foerster, N., Fourches, N., Gascon, J., Gastaldo, L., Gerbier, G., Giuliani, ANDREA ERNESTO GUIDO, Gray, D., Gros, M., Hehn, L., Henry, S., Hervé, S., Heuermann, G., Humbert, V., Ivanov, I. M., Juillard, A., Kéfélian, C., Kleifges, M., Kluck, H., Kobychev, V. V., Koskas, F., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Le Sueur, H., Loidl, M., Magnier, P., Makarov, E. P., Mancuso, M., de Marcillac, P., Marnieros, S., Marrache Kikuchi, C., Menshikov, A., Nasonov, S. G., Navick, X. F., Nones, C., Olivieri, E., Pari, P., Paul, B., Penichot, Y., Pessina, G., Piro, M. C., Plantevin, O., Redon, T., Robinson, M., Rodrigues, M., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Shlegel, V. N., Siebenborn, B., Strazzer, O., Tcherniakhovski, D., Tenconi, M., Torres, L., Tretyak, V. I., Vagneron, L., Vasiliev, Y. a. V., Velazquez, M., Viraphong, O., Walker, R. J., Weber, M., Yakushev, E., Zhang, X., Zhdankov, V. N., Girod, Dominique, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CSNSM PS1, Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), CSNSM INSTRU, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CSNSM MECA, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), EDELWEISS, LUMINEU program, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Particle physics, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Zinc molybdate, [PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], Scintillator, EDELWEISS, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 7. Clean energy, 01 natural sciences, law.invention, Nuclear physics, Crystal, chemistry.chemical_compound, law, Double beta decay, 0103 physical sciences, Scintillating bolometer, 010306 general physics, Nuclear Experiment, Physics, 010308 nuclear & particles physics, Bolometer, Low counting experiment, ZnMoO4 crystal scintillator, chemistry, Underground laboratory, Neutrino
Abstract: The technology of scintillating bolometers based on zinc molybdate (ZnMoO$_4$) crystals is under development within the LUMINEU project to search for 0$\nu$2$\beta$ decay of $^{100}$Mo with the goal to set the basis for large scale experiments capable to explore the inverted hierarchy region of the neutrino mass pattern. Advanced ZnMoO$_4$ crystal scintillators with mass of $\sim$~0.3 kg were developed and Zn$^{100}$MoO$_4$ crystal from enriched $^{100}$Mo was produced for the first time by using the low-thermal-gradient Czochralski technique. One ZnMoO$_4$ scintillator and two samples (59 g and 63 g) cut from the enriched boule were tested aboveground at milli-Kelvin temperature as scintillating bolometers showing a high detection performance. The first results of the low background measurements with three ZnMoO$_4$ and two enriched detectors installed in the EDELWEISS set-up at the Modane Underground Laboratory (France) are presented., Comment: 7 pages, 5 figures, Contribution to the proceedings of the 37th International Conference on High Energy Physics (ICHEP 2014), Valencia, Spain, 2-9 July 2014
Published: 2014

42. EURECA Conceptual Design Report

Author: Angloher, G., Armengaud, E., Augier, C., Benoit, A., Bergmann, T., Bluemer, J., Broniatowski, A., Brudanin, V., Camus, P., Cazes, A., Chapellier, M., Coron, N., Cox, G.A., Cuesta, C., Danevich, F.A., de Jesus, M., Dumoulin, L., Eitel, K., Erb, A., Ertl, A., von Feilitzsch, F., Filosofov, D., Fourches, N., Garcia, E., Gascon, J., Gerbier, G., Ginestra, C., Gironnet, J., Giuliani, A., Gros, M., Guetlein, A., Hauff, D., Henry, S., Heuermann, G., Jochum, J., Jokisch, S., Juillard, A., Kister, C., Kleifges, M., Kluck, H., Korolkova, E.V., Kozlov, Y., Kraus, H., Kudryavtsev, V.A., Lanfranchi, J-C., Loaiza, P., Loebell, J., Machulin, I., Marnieros, S., Martinez, M., Menshikov, A., Muenster, A., Navick, X-F., Nones, C., Ortigoza, Y., Pari, P., Petricca, F., Potzel, W., Povinec, P.P., Proebst, F., Puimedon, J., Reindl, F., Robinson, M., Rolon, T., Roth, S., Rottler, K., Rozov, S., Sailer, C., Salinas, A., Sanglard, V., Sarsa, M.L., Schaeffner, K., Schmidt, B., Scholl, S., Schoenert, S., Seidel, W., Siebenborn, B., Sivers, M.V., Strandhagen, C., Strauss, R., Tanzke, A., Tretyak, V.I., Turad, M., Ulrich, A., Usherov, I., Veber, P., Velazquez, M., Villar, J.A., Viraphong, O., Walker, R.J., Wawoczny, S., Weber, M., Willers, M., Wuestrich, M., Yakushev, E., Zhang, X., Zoeller, A., Collaboration, EURECA, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Matière noire (MANOIR), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Cryogénie (Cryo), Laboratoire Souterrain de Modane (LSM - UMR 6417), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Hélium : du fondamental aux applications (NEEL - HELFA), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Cryogénie (NEEL - Cryo), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Institut de Chimie de la Matière Condensée de Bordeaux (ICMCB), and Université de Bordeaux (UB)-Institut Polytechnique de Bordeaux-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Cryostat, Direct detection, Dark matter, Cryogenics, 01 natural sciences, 7. Clean energy, EURECA experiment, law.invention, Conceptual design, law, Cryogenic bolometers, 0103 physical sciences, ddc:530, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Aerospace engineering, 010306 general physics, ComputingMilieux_MISCELLANEOUS, Physics, Calorimeter (particle physics), 010308 nuclear & particles physics, business.industry, Bolometer, Electrical engineering, Astronomy and Astrophysics, WIMPs, Semiconductor detector, Space and Planetary Science, European Underground Rare Event Calorimeter Array, business
Abstract: The EURECA (European Underground Rare Event Calorimeter Array) project is aimed at searching for dark matter particles using cryogenic bolometers. The proponents of the present project have decided to pool their strengths and expertise to build a facility to house up to 1000 kg of detectors, EURECA, consisting in the first instance of germanium and CaWO4 crystals. The shielding will be provided through a large water tank in which the cryostat with detectors will be immersed. The EURECA infrastructure will be an essential tool for the community interested in using cryogenic detectors for dark matter searches. Beyond European detectors, it will be designed to host other types of similar cryogenic detectors, requiring millikelvin operating temperatures. In particular, this includes the germanium detectors currently in use by the SuperCDMS team, following the current collaborative work performed by the EURECA and SuperCDMS collaborations. EURECA will have two stages. The first phase aims at a sensitivity of 3 10-10pb and will involve building the infrastructure, cryostat and shielding, and operating 150kg of detectors. The second phase will be completed with 850kg of additional detectors, the relative weight between the different detectors being decided by the collaboration according to the physics reach. A sensitivity of 2.10-11 pb is aimed for atthe second stage. EURECA will ideally benefit from the planned extension of the deepest underground laboratory in Europe - LSM. With a site-independent design, it can also be hosted in other locations at similar or deeper sites such as SNOLAB. © 2014 The Authors.
Published: 2014

43. EDELWEISS-‐II WIMP search at low energy

Author: Sanglard, V., Matière noire (MANOIR), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), EDELWEISS, and Flores, Sylvie
Subjects: [SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.ASTR.IM] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Published: 2013

44. A search for low-mass WIMPs with EDELWEISS-II heat-and-ionization detectors

Author: EDELWEISS Collaboration, Armengaud, E., Augier, C., Benoît, A., Bergé, L., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Censier, B., Chapellier, M., Charlieux, F., Couëdo, F., Coulter, P., Cox, G. A., Domange, J., Drillien, A. A., Dumoulin, L., Eitel, K., Filosofov, D., Fourches, N., Gascon, J., Gerbier, G., Gironnet, J., Gros, M., Heuermann, G., Henry, S., Hervé, S., Juillard, A., Kleifges, M., Kluck, H., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Sueur, H. Le, Loaiza, P., Marnieros, S., Menshikov, A., Navick, X. -F., Nones, C., Olivieri, E., Pari, P., Paul, B., Robinson, M., Rozov, S., Sanglard, V., Schmidt, B., Siebenborn, B., Tcherniakhovski, D., Torrento-Coello, A. S., Vagneron, L., Walker, R. J., Weber, M., Yakushev, E., Zhang, X., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), CSNSM INSTR, Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), CSNSM PS1, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Souterrain de Modane (LSM - UMR 6417), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), EDELWEISS, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])
Subjects: Nuclear and High Energy Physics, Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Dark matter, FOS: Physical sciences, EDELWEISS, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), WIMP, Ionization, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Nuclear Experiment, Elastic scattering, Physics, 010308 nuclear & particles physics, Scattering, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Semiconductor detector, Weakly interacting massive particles, High Energy Physics::Experiment, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We report on a search for low-energy (E < 20 keV) WIMP-induced nuclear recoils using data collected in 2009 - 2010 by EDELWEISS from four germanium detectors equipped with thermal sensors and an electrode design (ID) which allows to efficiently reject several sources of background. The data indicate no evidence for an exponential distribution of low-energy nuclear recoils that could be attributed to WIMP elastic scattering after an exposure of 113 kg.d. For WIMPs of mass 10 GeV, the observation of one event in the WIMP search region results in a 90% CL limit of 1.0x10^-5 pb on the spin-independent WIMP-nucleon scattering cross-section, which constrains the parameter space associated with the findings reported by the CoGeNT, DAMA and CRESST experiments., PRD rapid communication accepted
Published: 2012

45. Final results of the EDELWEISS-II WIMP search using a 4-kg array of cryogenic germanium detectors with interleaved electrodes

Author: Armengaud, E, Augier, C, Benoit, A, Berge, L, Bluemer, J, Broniatowski, A, Brudanin, V, Censier, B, Chardin, G, Chapellier, M, Charlieux, F, Coulter, P, Cox, GA, Defay, X, De Jesus, M, Dolgorouki, Y, Domange, J, Dumoulin, L, Eitel, K, Filosofov, D, Fourches, N, Gascon, J, Gerbier, G, Gironnet, J, Gros, M, Henry, S, Herve, S, Juillard, A, Kluck, H, Kozlov, V, Kraus, H, Kudryavtsev, VA, Loaiza, P, Marnieros, S, Navick, X-F, Nones, C, Olivieri, E, Pari, P, Pattavina, L, Paul, B, Robinson, M, Rozov, S, Sanglard, V, Schmidt, B, Scorza, S, Semikh, S, Torrento-Coello, AS, Vagneron, L, Verdier, M-A, Walker, RJ, Yakushev, E, Collaboration, EDELWEISS, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Souterrain de Modane (LSM - UMR 6417), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Institut Rayonnement Matière de Saclay (IRAMIS), EDELWEISS, HELFA - Hélium : du fondamental aux applications, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Hélium : du fondamental aux applications (HELFA), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
Subjects: Cryogenic Ge detectors, Nuclear and High Energy Physics, Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Physics::Instrumentation and Detectors, Dark matter, FOS: Physical sciences, WIMP searches, chemistry.chemical_element, Germanium, EDELWEISS, 7. Clean energy, 01 natural sciences, Particle detector, High Energy Physics - Experiment, Nuclear physics, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], High Energy Physics - Experiment (hep-ex), Recoil, WIMP, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Nuclear Experiment, 010306 general physics, Physics, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, 3. Good health, Semiconductor detector, chemistry, High Energy Physics::Experiment, Nucleon, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The EDELWEISS-II collaboration has completed a direct search for WIMP dark matter with an array of ten 400-g cryogenic germanium detectors in operation at the Laboratoire Souterrain de Modane. The combined use of thermal phonon sensors and charge collection electrodes with an interleaved geometry enables the efficient rejection of gamma-induced radioactivity as well as near-surface interactions. A total effective exposure of 384 kg.d has been achieved, mostly coming from fourteen months of continuous operation. Five nuclear recoil candidates are observed above 20 keV, while the estimated background is 3.0 events. The result is interpreted in terms of limits on the cross-section of spin-independent interactions of WIMPs and nucleons. A cross-section of 4.4x10^-8 pb is excluded at 90%CL for a WIMP mass of 85 GeV. New constraints are also set on models where the WIMP-nucleon scattering is inelastic., 23 pages, 5 figures; matches published version
Published: 2011

46. Combined limits on WIMPs from the CDMS and EDELWEISS experiments

Author: Ahmed, Z, Akerib, DS, Armengaud, E, Arrenberg, S, Augier, C, Bailey, CN, Balakishiyeva, D, Baudis, L, Bauer, DA, Benoît, A, Bergé, L, Blümer, J, Brink, PL, Broniatowski, A, Bruch, T, Brudanin, V, Bunker, R, Cabrera, B, Caldwell, DO, Censier, B, Chapellier, M, Chardin, G, Charlieux, F, Cooley, J, Coulter, P, Cox, GA, Cushman, P, Daal, M, Defay, X, De Jesus, M, Dejongh, F, Di Stefano, PCF, Dolgorouki, Y, Domange, J, Dumoulin, L, Dragowsky, MR, Eitel, K, Fallows, S, Figueroa-Feliciano, E, Filippini, J, Filosofov, D, Fourches, N, Fox, J, Fritts, M, Gascon, J, Gerbier, G, Gironnet, J, Golwala, SR, Gros, M, Hall, J, Hennings-Yeomans, R, Henry, S, Hertel, SA, Hervé, S, Holmgren, D, Hsu, L, Huber, ME, Juillard, A, Kamaev, O, Kiveni, M, Kluck, H, Kos, M, Kozlov, V, Kraus, H, Kudryavtsev, VA, Leman, SW, Liu, S, Loaiza, P, Mahapatra, R, Mandic, V, Marnieros, S, Martinez, C, McCarthy, KA, Mirabolfathi, N, Moore, D, Nadeau, P, Navick, XF, Nelson, H, Nones, C, Ogburn, RW, Olivieri, E, Pari, P, Pattavina, L, Paul, B, Phipps, A, Pyle, M, Qiu, X, Rau, W, Reisetter, A, Ricci, Y, Robinson, M, Rozov, S, Saab, T, Sadoulet, B, Sander, J, and Sanglard, V
Abstract: The CDMS and EDELWEISS collaborations have combined the results of their direct searches for dark matter using cryogenic germanium detectors. The total data set represents 614kg•days equivalent exposure. A straightforward method of combination was chosen for its simplicity before data were exchanged between experiments. The results are interpreted in terms of limits on spin-independent weakly interacting, massive particle (WIMP)-nucleon cross section. For a WIMP mass of 90GeV/c2, where this analysis is most sensitive, a cross section of 3.3×10-44cm2 is excluded at 90% C.L. At higher WIMP masses, the combination improves the individual limits, by a factor 1.6 above 700GeV/c2. Alternative methods of combining the data provide stronger constraints for some ranges of WIMP masses and weaker constraints for others. © 2011 American Physical Society.
Published: 2011

47. EURECA

Author: Kraus, H, Armengaud, E, Augier, C, Bauer, M, Bechtold, N, Benoit, A, Bento, A, Berge, L, Blümer, J, Bornschein, L, Broniatowski, A, Brown, A, Camus, P, Censier, B, Chantelauze, A, Chapellier, M, Chardin, G, Ciemniak, C, Collin, S, Coron, N, Coulter, P, Cox, A, Crauste, O, Danevich, FA, Daw, E, De Jésus, M, De Marcillac, P, Deuter, G, Domange, J, Drexlin, G, Dumoulin, L, Eitel, K, Feilitzsch, FV, Filosofov, D, Gandit, P, García, E, Gascon, J, Gerbier, G, Gironnet, J, Godfrin, H, Graffin, P, Grohmann, S, Gros, M, Hauff, D, Henry, S, Huff, P, Ingleby, S, Isaila, C, Jochum, J, Juillard, A, Kiefer, M, Kikuchi, C, Kimmerle, M, Kluck, H, Kobychev, VV, Kozlov, V, Kudovbenko, VM, Kudryavtsev, VA, Lanfranchi, J-C, Loaiza, P, Lubashevsky, A, Marnieros, S, Martinez, M-L, Mikhailik, VM, Monfardini, A, Nagorny, SS, Navick, X-F, Nieder, H, Niinikoski, T, Nikolaiko, AS, Olivieri, E, Ortigoza, Y, Pari, P, Pattavina, L, Paul, B, Petricca, F, Pfeiffer, M, Pfister, S, Pobes, C, Poda, DV, Podviyanuk, RB, Polischuk, OG, Ponsot, P, Potzel, W, Pröbst, F, Puimedón, J, Robinson, M, Rolón, T, Roth, S, Rottler, K, Rozov, S, Sailer, C, Salinas, A, Sanglard, V, Sarsa, M-L, Schäffner, K, Schmaler, J, Schmidt, B, Scholl, S, Scorza, S, Seidel, W, Semikh, S, Sivers, MV, Stodolsky, L, Strandhagen, C, Strauss, R, Sullivan, P, Teshima, M, Torrento, A, Torres, L, Tretyak, VI, Usherov, I, Veber, P, Velázquez, M, Villar, JA, Walker, R, Wolf, J, and Yakushev, E
Abstract: EURECA (European Underground Rare Event Calorimeter Array) is an astro-particle physics facility aiming to directly detect galactic dark matter. The Laboratoire Souterrain de Modane has been selected as host laboratory. The EURECA collaboration unites CRESST, EDELWEISS and the Spanish-French experiment ROSEBUD, thus concentrating and focussing effort on cryogenic detector research in Europe into a single facility. EURECA will use a target mass of up to one ton, enough to explore WIMP - nucleon scalar scattering cross sections in the region of 10-9 - 10-10 picobarn. A major advantage of EURECA is the planned use of more than just one target material (multi target experiment for WIMP identification). © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
Published: 2010

48. Full Inter-Digitized Detectors For The EDELWEISS-II Dark Matter Search

Author: Marnieros, S., Armengaud, E., Augier, C., Berge, L., Benoit, Angélique, Besida, O., Blumer, J., Broniatowski, A., Chantelauze, A., Chapellier, M., Chardin, G., Charlieux, F., Collin, S., Crauste, O., Defay, X., De Jesus, M., Di Stefano, P., Dolgorouki, Y., Domange, J., Dumoulin, L., Eitel, K., Gascon, J., Gerbier, G., Gros, M., Hannawald, M., Herve, S., Juillard, A., Kluck, H., Kozlov, V., Lemrani, R., Lubashevskiy, A., Marrache, C., Ricci, Y., Sanglard, V., Scorza, S., Semikh, S., A. Verdier, M., Vagneron, L., Yakushev, E., Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Matière noire (MANOIR), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), EDELWEISS, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)
Subjects: EDELWEISS, Dark Matter, Cryogenic detectors, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Abstract: International audience; A new design for the Ge bolometers of the EDELWEISS project is described here, based on innovative interleaved charge collection electrodes with high background discrimination capabilities. The measured surface event rejection is compatible with WIMP sensitivity levels down to 10(-) 9 picobarn (pb). Use of interleaved electrodes on the overall surface of the Ge crystal, including its lateral surface, results to a high fiducial volume of the order of 80%. Electronic setup is fairly simple with a total of five JFET based read-out amplifiers, one for the NTD-Ge heat channel and four for the ionization signal. Fabrication process is quite simple and the design is easily scalable to higher mass bolometers (1 kg Ge crystal), making it very appealing for the future 1 ton scale EUREKA Dark Matter experiment.
Published: 2009

49. Dark Matter Searches with the experiment EDELWEISS-II

Author: Sanglard, V., Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and EDELWEISS
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], ComputingMilieux_MISCELLANEOUS
Abstract: International audience
Published: 2009

50. EURECA – setting the scene for scintillators

Author: Kraus, H., Eric Armengaud, Bauer, M., Bavykina, I., Benoit, A., Bento, A., Blümer, J., Bornschein, L., Broniatowski, A., Burghart, G., Camus, P., Chantelauze, A., Chapellier, M., Chardin, G., Ciemniak, C., Coppi, C., Coron, N., Crauste, O., Danevich, F. A., Daw, E., Defay, X., Jésus, M., Marcillac, P., Deuter, G., Domange, J., Stefano, P. Di, Drexlin, G., Dumoulin, L., Eitel, K., Feilitzsch, F., Filosofov, D., Gandit, P., Garcia, E., Gascon, J., Gerbier, G., Gironnet, J., Godfrin, H., Grohmann, S., Gros, M., Hannewald, M., Hauff, D., Haug, F., Henry, S., Huff, P., Imber, J., Ingleby, S., Isaila, C., Jochum, J., Juillard, A., Kiefer, M., Kimmerle, M., Kluck, H., Kobychev, V. V., Kozlov, V., Kudovbenko, V. M., Kudryavtsev, V. A., Lachenmaier, T., Lanfranchi, J. -C, Lang, R. F., Loaiza, P., Lubashevsky, A., Malek, M., Marnieros, S., Mcgowan, R., Mikhailik, V., Monfardini, A., Navick, X. -F, Niinikoski, T., Nikolaiko, A. S., Oberauer, L., Olivieri, E., Ortigoza, Y., Pantic, E., Pari, P., Paul, B., Perinic, G., Petricca, F., Pfister, S., Pobes, C., Poda, D. V., Podviyanuk, R. B., Polischuk, O. G., Potzel, W., Pröbst, F., Puimedon, J., Robinson, M., Roth, S., Rottler, K., Rozov, S., Sailer, C., Salinas, A., Sanglard, V., Sarsa, M. L., Schäffner, K., Scholl, S., Scorza, S., Seidel, W., Semikh, S., Smolnikov, A., Stern, M., Stodolsky, L., Teshima, M., Tomasello, V., Torrento, A., Torres, L., Tretyak, V. I., Usherov, I., Verdier, M. A., Villar, J. A., Wolf, J., Yakushev, E., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Cryogénie (Cryo), Institut Rayonnement Matière de Saclay (IRAMIS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Ultra-basses températures (UBT), Laboratoire Souterrain de Modane (LSM - UMR 6417), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Hélium : du fondamental aux applications (NEEL - HELFA), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Cryogénie (NEEL - Cryo), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Ultra-basses températures (NEEL - UBT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), HELFA - Hélium : du fondamental aux applications, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Cryo - Cryogénie, UBT - Ultra-basses températures, Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Girod, Dominique
Subjects: [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA], [PHYS.PHYS.PHYS-INS-DET] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.ASTR.GA] Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Abstract: voir fichier complet des proceedings; International audience; EURECA (European Underground Rare Event Calorimeter Array) will be an astro-particle physics facility aiming to directly detect galactic dark matter. TheLaboratoire Souterrain de Modane has been selected as host laboratory. TheEURECA collaboration concentrates effort on cryogenic detector research inEurope into a single facility by bringing together colleagues from CRESST,EDELWEISS, ROSEBUD and additional new member institutes. EURECA will use atarget mass of up to one ton for exploring WIMP-nucleon scalar scattering crosssections in the region of 10 −9 – 10 −10 picobarn. A major advantage of EURECAis the planned use of more than just one target material (multi targetexperiment for WIMP identification).
Published: 2008

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