Lowering the CUORE energy threshold

© Published under licence by IOP Publishing Ltd. The Cryogenic Underground Observatory for Rare Events (CUORE) is a ton-scale double beta decay experiment based on TeO 2 cryogenic bolometers and is currently in the last construction stage at the Gran Sasso National Laboratory (LNGS). Its primary go...

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Main Authors: Copello, S., Alduino, C., Alfonso, K., Artusa, D. R., Avignone, F. T., Azzolini, O., Banks, T. I., Bari, G., Beeman, J.W., Bellini, F., Bersani, A., Biassoni, M., Branca, A., Brofferio, C., Bucci, C., Camacho, A., Caminata, A., Canonica, L., Cao, X. G., Capelli, S., Cappelli, L., Carbone, L., Cardani, L., Carniti, P., Casali, N., Cassina, L., Chiesa, D., Chott, N., Clemenza, M., Cosmelli, C., Cremonesi, O., Creswick, R. J., Cushman, J. S., D’Addabbo, A., Dafinei, I., Davis, C. J., Dell’Oro, S., Deninno, M. M., Di Domizio, S., Di Vacri, M. L., Drobizhev, A., Fang, D. Q., Faverzani, M., Fernandes, G., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M. A., Freedman, S. J., Fujikawa, B. K., Giachero, A., Gironi, L., Giuliani, A., Gladstone, L., Gorla, P., Gotti, C., Gutierrez, T. D., Haller, E. E., Han, K., Hansen, E., Heeger, K. M., Hennings-Yeomans, R., Hickerson, K. P., Huang, H. Z., Kadel, R., Keppel, G., Kolomensky, Yu. G., Leder, A., Ligi, C., Lim, K. E., Liu, X., Ma, Y. G., Maino, M., Marini, L., Martinez, M., Maruyama, R. H., Mei, Y., Moggi, N., Morganti, S., Mosteiro, P. J., Napolitano, T., Nones, C., Norman, E. B., Nucciotti, A., O’Donnell, T., Orio, F., Ouellet, J. L., Pagliarone, C. E., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pessina, G., Pettinacci, V., Piperno, G., Pira, c C., Pirro, S., Pozzi, S., Previtali, E., Rosenfeld, C., Rusconi, C., Sangiorgio, S., Santone, D., Scielzo, N. D., Singh, V., Sisti, M., Smith, A. R., Taffarello, L., Tenconi, M., Terranova, F., Tomei, C., Trentalange, S., Vignati, M., Wagaarachchi, S. L., Wang, B. S., Wang, H. W., Wilson, J., Winslow, L. A., Wise, T., Woodcraft, A., Zanotti, L., Zhang, G. Q., Zhu, B. X., Zimmermann, S., Zucchelli, S.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: IOP Publishing 2021
Subjects:
Online Access:https://hdl.handle.net/1721.1/137621
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author Copello, S.
Alduino, C.
Alfonso, K.
Artusa, D. R.
Avignone, F. T.
Azzolini, O.
Banks, T. I.
Bari, G.
Beeman, J.W.
Bellini, F.
Bersani, A.
Biassoni, M.
Branca, A.
Brofferio, C.
Bucci, C.
Camacho, A.
Caminata, A.
Canonica, L.
Cao, X. G.
Capelli, S.
Cappelli, L.
Carbone, L.
Cardani, L.
Carniti, P.
Casali, N.
Cassina, L.
Chiesa, D.
Chott, N.
Clemenza, M.
Cosmelli, C.
Cremonesi, O.
Creswick, R. J.
Cushman, J. S.
D’Addabbo, A.
Dafinei, I.
Davis, C. J.
Dell’Oro, S.
Deninno, M. M.
Di Domizio, S.
Di Vacri, M. L.
Drobizhev, A.
Fang, D. Q.
Faverzani, M.
Fernandes, G.
Ferri, E.
Ferroni, F.
Fiorini, E.
Franceschi, M. A.
Freedman, S. J.
Fujikawa, B. K.
Giachero, A.
Gironi, L.
Giuliani, A.
Gladstone, L.
Gorla, P.
Gotti, C.
Gutierrez, T. D.
Haller, E. E.
Han, K.
Hansen, E.
Heeger, K. M.
Hennings-Yeomans, R.
Hickerson, K. P.
Huang, H. Z.
Kadel, R.
Keppel, G.
Kolomensky, Yu. G.
Leder, A.
Ligi, C.
Lim, K. E.
Liu, X.
Ma, Y. G.
Maino, M.
Marini, L.
Martinez, M.
Maruyama, R. H.
Mei, Y.
Moggi, N.
Morganti, S.
Mosteiro, P. J.
Napolitano, T.
Nones, C.
Norman, E. B.
Nucciotti, A.
O’Donnell, T.
Orio, F.
Ouellet, J. L.
Pagliarone, C. E.
Pallavicini, M.
Palmieri, V.
Pattavina, L.
Pavan, M.
Pessina, G.
Pettinacci, V.
Piperno, G.
Pira, c C.
Pirro, S.
Pozzi, S.
Previtali, E.
Rosenfeld, C.
Rusconi, C.
Sangiorgio, S.
Santone, D.
Scielzo, N. D.
Singh, V.
Sisti, M.
Smith, A. R.
Taffarello, L.
Tenconi, M.
Terranova, F.
Tomei, C.
Trentalange, S.
Vignati, M.
Wagaarachchi, S. L.
Wang, B. S.
Wang, H. W.
Wilson, J.
Winslow, L. A.
Wise, T.
Woodcraft, A.
Zanotti, L.
Zhang, G. Q.
Zhu, B. X.
Zimmermann, S.
Zucchelli, S.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Copello, S.
Alduino, C.
Alfonso, K.
Artusa, D. R.
Avignone, F. T.
Azzolini, O.
Banks, T. I.
Bari, G.
Beeman, J.W.
Bellini, F.
Bersani, A.
Biassoni, M.
Branca, A.
Brofferio, C.
Bucci, C.
Camacho, A.
Caminata, A.
Canonica, L.
Cao, X. G.
Capelli, S.
Cappelli, L.
Carbone, L.
Cardani, L.
Carniti, P.
Casali, N.
Cassina, L.
Chiesa, D.
Chott, N.
Clemenza, M.
Cosmelli, C.
Cremonesi, O.
Creswick, R. J.
Cushman, J. S.
D’Addabbo, A.
Dafinei, I.
Davis, C. J.
Dell’Oro, S.
Deninno, M. M.
Di Domizio, S.
Di Vacri, M. L.
Drobizhev, A.
Fang, D. Q.
Faverzani, M.
Fernandes, G.
Ferri, E.
Ferroni, F.
Fiorini, E.
Franceschi, M. A.
Freedman, S. J.
Fujikawa, B. K.
Giachero, A.
Gironi, L.
Giuliani, A.
Gladstone, L.
Gorla, P.
Gotti, C.
Gutierrez, T. D.
Haller, E. E.
Han, K.
Hansen, E.
Heeger, K. M.
Hennings-Yeomans, R.
Hickerson, K. P.
Huang, H. Z.
Kadel, R.
Keppel, G.
Kolomensky, Yu. G.
Leder, A.
Ligi, C.
Lim, K. E.
Liu, X.
Ma, Y. G.
Maino, M.
Marini, L.
Martinez, M.
Maruyama, R. H.
Mei, Y.
Moggi, N.
Morganti, S.
Mosteiro, P. J.
Napolitano, T.
Nones, C.
Norman, E. B.
Nucciotti, A.
O’Donnell, T.
Orio, F.
Ouellet, J. L.
Pagliarone, C. E.
Pallavicini, M.
Palmieri, V.
Pattavina, L.
Pavan, M.
Pessina, G.
Pettinacci, V.
Piperno, G.
Pira, c C.
Pirro, S.
Pozzi, S.
Previtali, E.
Rosenfeld, C.
Rusconi, C.
Sangiorgio, S.
Santone, D.
Scielzo, N. D.
Singh, V.
Sisti, M.
Smith, A. R.
Taffarello, L.
Tenconi, M.
Terranova, F.
Tomei, C.
Trentalange, S.
Vignati, M.
Wagaarachchi, S. L.
Wang, B. S.
Wang, H. W.
Wilson, J.
Winslow, L. A.
Wise, T.
Woodcraft, A.
Zanotti, L.
Zhang, G. Q.
Zhu, B. X.
Zimmermann, S.
Zucchelli, S.
author_sort Copello, S.
collection MIT
description © Published under licence by IOP Publishing Ltd. The Cryogenic Underground Observatory for Rare Events (CUORE) is a ton-scale double beta decay experiment based on TeO 2 cryogenic bolometers and is currently in the last construction stage at the Gran Sasso National Laboratory (LNGS). Its primary goal is to observe neutrino-less double beta decay of 130 Te, however thanks to the ultra-low background and large projected exposure it could also be suitable for other rare event searches, as the detection of solar axions, neutrinos from type II supernovae or direct detection of dark matter. The sensitivity for these searches will depend on the performance achieved at the low energy threshold. For this reason a trigger algorithm based on continuous data filtering has been developed which will allow lowering the threshold down to the few keV region. The new trigger has been tested in CUORE-0, a single-tower CUORE prototype consisting of 52 TeO 2 bolometers and recently concluded, and here we present the results in terms of trigger efficiency, data selection and low-energy calibration.
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spelling mit-1721.1/1376212023-12-20T17:49:30Z Lowering the CUORE energy threshold Copello, S. Alduino, C. Alfonso, K. Artusa, D. R. Avignone, F. T. Azzolini, O. Banks, T. I. Bari, G. Beeman, J.W. Bellini, F. Bersani, A. Biassoni, M. Branca, A. Brofferio, C. Bucci, C. Camacho, A. Caminata, A. Canonica, L. Cao, X. G. Capelli, S. Cappelli, L. Carbone, L. Cardani, L. Carniti, P. Casali, N. Cassina, L. Chiesa, D. Chott, N. Clemenza, M. Cosmelli, C. Cremonesi, O. Creswick, R. J. Cushman, J. S. D’Addabbo, A. Dafinei, I. Davis, C. J. Dell’Oro, S. Deninno, M. M. Di Domizio, S. Di Vacri, M. L. Drobizhev, A. Fang, D. Q. Faverzani, M. Fernandes, G. Ferri, E. Ferroni, F. Fiorini, E. Franceschi, M. A. Freedman, S. J. Fujikawa, B. K. Giachero, A. Gironi, L. Giuliani, A. Gladstone, L. Gorla, P. Gotti, C. Gutierrez, T. D. Haller, E. E. Han, K. Hansen, E. Heeger, K. M. Hennings-Yeomans, R. Hickerson, K. P. Huang, H. Z. Kadel, R. Keppel, G. Kolomensky, Yu. G. Leder, A. Ligi, C. Lim, K. E. Liu, X. Ma, Y. G. Maino, M. Marini, L. Martinez, M. Maruyama, R. H. Mei, Y. Moggi, N. Morganti, S. Mosteiro, P. J. Napolitano, T. Nones, C. Norman, E. B. Nucciotti, A. O’Donnell, T. Orio, F. Ouellet, J. L. Pagliarone, C. E. Pallavicini, M. Palmieri, V. Pattavina, L. Pavan, M. Pessina, G. Pettinacci, V. Piperno, G. Pira, c C. Pirro, S. Pozzi, S. Previtali, E. Rosenfeld, C. Rusconi, C. Sangiorgio, S. Santone, D. Scielzo, N. D. Singh, V. Sisti, M. Smith, A. R. Taffarello, L. Tenconi, M. Terranova, F. Tomei, C. Trentalange, S. Vignati, M. Wagaarachchi, S. L. Wang, B. S. Wang, H. W. Wilson, J. Winslow, L. A. Wise, T. Woodcraft, A. Zanotti, L. Zhang, G. Q. Zhu, B. X. Zimmermann, S. Zucchelli, S. Massachusetts Institute of Technology. Department of Physics General Physics and Astronomy © Published under licence by IOP Publishing Ltd. The Cryogenic Underground Observatory for Rare Events (CUORE) is a ton-scale double beta decay experiment based on TeO 2 cryogenic bolometers and is currently in the last construction stage at the Gran Sasso National Laboratory (LNGS). Its primary goal is to observe neutrino-less double beta decay of 130 Te, however thanks to the ultra-low background and large projected exposure it could also be suitable for other rare event searches, as the detection of solar axions, neutrinos from type II supernovae or direct detection of dark matter. The sensitivity for these searches will depend on the performance achieved at the low energy threshold. For this reason a trigger algorithm based on continuous data filtering has been developed which will allow lowering the threshold down to the few keV region. The new trigger has been tested in CUORE-0, a single-tower CUORE prototype consisting of 52 TeO 2 bolometers and recently concluded, and here we present the results in terms of trigger efficiency, data selection and low-energy calibration. 2021-11-05T20:45:22Z 2021-11-05T20:45:22Z 2017-09 2019-06-04T12:14:40Z Article http://purl.org/eprint/type/JournalArticle 1742-6588 1742-6596 https://hdl.handle.net/1721.1/137621 Copello, S., Alduino, C., Alfonso, K., Artusa, D. R., Avignone, F. T. et al. 2017. "Lowering the CUORE energy threshold." 888. en 10.1088/1742-6596/888/1/012047 Creative Commons Attribution 3.0 unported license https://creativecommons.org/licenses/by/3.0/ application/pdf IOP Publishing IOP Publishing
spellingShingle General Physics and Astronomy
Copello, S.
Alduino, C.
Alfonso, K.
Artusa, D. R.
Avignone, F. T.
Azzolini, O.
Banks, T. I.
Bari, G.
Beeman, J.W.
Bellini, F.
Bersani, A.
Biassoni, M.
Branca, A.
Brofferio, C.
Bucci, C.
Camacho, A.
Caminata, A.
Canonica, L.
Cao, X. G.
Capelli, S.
Cappelli, L.
Carbone, L.
Cardani, L.
Carniti, P.
Casali, N.
Cassina, L.
Chiesa, D.
Chott, N.
Clemenza, M.
Cosmelli, C.
Cremonesi, O.
Creswick, R. J.
Cushman, J. S.
D’Addabbo, A.
Dafinei, I.
Davis, C. J.
Dell’Oro, S.
Deninno, M. M.
Di Domizio, S.
Di Vacri, M. L.
Drobizhev, A.
Fang, D. Q.
Faverzani, M.
Fernandes, G.
Ferri, E.
Ferroni, F.
Fiorini, E.
Franceschi, M. A.
Freedman, S. J.
Fujikawa, B. K.
Giachero, A.
Gironi, L.
Giuliani, A.
Gladstone, L.
Gorla, P.
Gotti, C.
Gutierrez, T. D.
Haller, E. E.
Han, K.
Hansen, E.
Heeger, K. M.
Hennings-Yeomans, R.
Hickerson, K. P.
Huang, H. Z.
Kadel, R.
Keppel, G.
Kolomensky, Yu. G.
Leder, A.
Ligi, C.
Lim, K. E.
Liu, X.
Ma, Y. G.
Maino, M.
Marini, L.
Martinez, M.
Maruyama, R. H.
Mei, Y.
Moggi, N.
Morganti, S.
Mosteiro, P. J.
Napolitano, T.
Nones, C.
Norman, E. B.
Nucciotti, A.
O’Donnell, T.
Orio, F.
Ouellet, J. L.
Pagliarone, C. E.
Pallavicini, M.
Palmieri, V.
Pattavina, L.
Pavan, M.
Pessina, G.
Pettinacci, V.
Piperno, G.
Pira, c C.
Pirro, S.
Pozzi, S.
Previtali, E.
Rosenfeld, C.
Rusconi, C.
Sangiorgio, S.
Santone, D.
Scielzo, N. D.
Singh, V.
Sisti, M.
Smith, A. R.
Taffarello, L.
Tenconi, M.
Terranova, F.
Tomei, C.
Trentalange, S.
Vignati, M.
Wagaarachchi, S. L.
Wang, B. S.
Wang, H. W.
Wilson, J.
Winslow, L. A.
Wise, T.
Woodcraft, A.
Zanotti, L.
Zhang, G. Q.
Zhu, B. X.
Zimmermann, S.
Zucchelli, S.
Lowering the CUORE energy threshold
title Lowering the CUORE energy threshold
title_full Lowering the CUORE energy threshold
title_fullStr Lowering the CUORE energy threshold
title_full_unstemmed Lowering the CUORE energy threshold
title_short Lowering the CUORE energy threshold
title_sort lowering the cuore energy threshold
topic General Physics and Astronomy
url https://hdl.handle.net/1721.1/137621
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