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89 results on '"Ferreiro Iachellini N"'

1. Characterization of a kg-scale archaeological lead-based PbWO[formula omitted] cryogenic detector for the RES-NOVA experiment

Author

Beeman, J.W., Benato, G., Bucci, C., Canonica, L., Carniti, P., Celi, E., Clemenza, M., D’Addabbo, A., Danevich, F.A., Di Domizio, S., Di Lorenzo, S., Dubovik, O.M., Ferreiro Iachellini, N., Ferroni, F., Fiorini, E., Fu, S., Garai, A., Ghislandi, S., Gironi, L., Gorla, P., Gotti, C., Guillaumon, P.V., Helis, D.L., Kovtun, G.P., Mancuso, M., Marini, L., Olmi, M., Pagnanini, L., Pattavina, L., Pessina, G., Petricca, F., Pirro, S., Pozzi, S., Puiu, A., Quitadamo, S., Rothe, J., Scherban, A.P., Schönert, S., Solopikhin, D.A., Strauss, R., Tarabini, E., Tretyak, V.I., Tupitsyna, I.A., and Wagner, V.

Published
2023
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2. Secular equilibrium assessment in a CaWO4 target crystal from the dark matter experiment CRESST using Bayesian likelihood normalisation

Author

Angloher, G., Banik, S., Benato, G., Bento, A., Bertolini, A., Breier, R., Bucci, C., Burkhart, J., Canonica, L., D’Addabbo, A., Di Lorenzo, S., Einfalt, L., Erb, A., Feilitzsch, F.v., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Garai, A., Ghete, V.M., Gorla, P., Gupta, S., Hauff, D., Ješkovský, M., Jochum, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Marini, L., Mokina, V., Nilima, A., Olmi, M., Ortmann, T., Pagliarone, C., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pröbst, F., Pucci, F., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., Zema, V., Ferella, F., Laubenstein, M., and Nisi, S.

Published
2023
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4. Radiopurity of a kg-scale PbWO4 cryogenic detector produced from archaeological Pb for the RES-NOVA experiment

Author

Beeman, J. W., Benato, G., Bucci, C., Canonica, L., Carniti, P., Celi, E., Clemenza, M., D’Addabbo, A., Danevich, F. A., Di Domizio, S., DiLorenzo, S., Dubovik, O. M., Ferreiro Iachellini, N., Ferroni, F., Fiorini, E., Fu, S., Garai, A., Ghislandi, S., Gironi, L., Gorla, P., Gotti, C., Guillaumon, P. V., Helis, D. L., Kovtun, G. P., Mancuso, M., Marini, L., Olmi, M., Pagnanini, L., Pattavina, L., Pessina, G., Petricca, F., Pirro, S., Pozzi, S., Puiu, A., Quitadamo, S., Rothe, J., Scherban, A. P., Schönert, S., Solopikhin, D. A., Strauss, R., Tarabini, E., Tretyak, V. I., Tupitsyna, I. A., and Wagner, V.

Published
2022
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6. Probing spin-dependent dark matter interactions with 6Li: CRESST Collaboration

Author

Angloher, G., Benato, G., Bento, A., Bertoldo, E., Bertolini, A., Breier, R., Bucci, C., Canonica, L., D’Addabbo, A., Di Lorenzo, S., Einfalt, L., Erb, A., Feilitzsch, F. v., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Garai, A., Ghete, V. M., Gorla, P., Gupta, S., Hauff, D., Ješkovský, M., Jochum, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Marini, L., Mokina, V., Nilima, A., Olmi, M., Ortmann, T., Pagliarone, C., Palušová, V., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pröbst, F., Pucci, F., Reindl , F., Rothe, J., Schäffner, K., Schieck, J., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., and Zema, V.

Published
2022
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7. Characterization of a kg-scale archaeological lead-based PbWO4 cryogenic detector for the RES-NOVA experiment

Author

Beeman, J, Benato, G, Bucci, C, Canonica, L, Carniti, P, Celi, E, Clemenza, M, D'Addabbo, A, Danevich, F, Di Domizio, S, Di Lorenzo, S, Dubovik, O, Ferreiro Iachellini, N, Ferroni, F, Fu, S, Garai, A, Ghislandi, S, Gironi, L, Gorla, P, Gotti, C, Guillaumon, P, Helis, D, Kovtun, G, Mancuso, M, Marini, L, Olmi, M, Pagnanini, L, Pattavina, L, Pessina, G, Petricca, F, Pirro, S, Quitadamo, S, Rothe, J, Scherban, A, Schönert, S, Solopikhin, D, Strauss, R, Tarabini, E, Tretyak, V, Tupitsyna, I, Wagner, V, Puiu, A, Pozzi, S, Fiorini, E, Beeman J. W., Benato G., Bucci C., Canonica L., Carniti P., Celi E., Clemenza M., D'Addabbo A., Danevich F. A., Di Domizio S., Di Lorenzo S., Dubovik O. M., Ferreiro Iachellini N., Ferroni F., Fu S., Garai A., Ghislandi S., Gironi L., Gorla P., Gotti C., Guillaumon P. V., Helis D. L., Kovtun G. P., Mancuso M., Marini L., Olmi M., Pagnanini L., Pattavina L., Pessina G., Petricca F., Pirro S., Quitadamo S., Rothe J., Scherban A. P., Schönert S., Solopikhin D. A., Strauss R., Tarabini E., Tretyak V. I., Tupitsyna I. A., Wagner V., Puiu A., Pozzi S., Fiorini E., Beeman, J, Benato, G, Bucci, C, Canonica, L, Carniti, P, Celi, E, Clemenza, M, D'Addabbo, A, Danevich, F, Di Domizio, S, Di Lorenzo, S, Dubovik, O, Ferreiro Iachellini, N, Ferroni, F, Fu, S, Garai, A, Ghislandi, S, Gironi, L, Gorla, P, Gotti, C, Guillaumon, P, Helis, D, Kovtun, G, Mancuso, M, Marini, L, Olmi, M, Pagnanini, L, Pattavina, L, Pessina, G, Petricca, F, Pirro, S, Quitadamo, S, Rothe, J, Scherban, A, Schönert, S, Solopikhin, D, Strauss, R, Tarabini, E, Tretyak, V, Tupitsyna, I, Wagner, V, Puiu, A, Pozzi, S, Fiorini, E, Beeman J. W., Benato G., Bucci C., Canonica L., Carniti P., Celi E., Clemenza M., D'Addabbo A., Danevich F. A., Di Domizio S., Di Lorenzo S., Dubovik O. M., Ferreiro Iachellini N., Ferroni F., Fu S., Garai A., Ghislandi S., Gironi L., Gorla P., Gotti C., Guillaumon P. V., Helis D. L., Kovtun G. P., Mancuso M., Marini L., Olmi M., Pagnanini L., Pattavina L., Pessina G., Petricca F., Pirro S., Quitadamo S., Rothe J., Scherban A. P., Schönert S., Solopikhin D. A., Strauss R., Tarabini E., Tretyak V. I., Tupitsyna I. A., Wagner V., Puiu A., Pozzi S., and Fiorini E.

Published
2023

8. Results on sub-GeV dark matter from a 10 eV threshold CRESST-III silicon detector

Author

Angloher, G, Banik, S, Benato, G, Bento, A, Bertolini, A, Breier, R, Bucci, C, Burkhart, J, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Einfalt, L, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuchs, D, Fuss, A, Garai, A, Ghete, V, Gerster, S, Gorla, P, Guillaumon, P, Gupta, S, Hauff, D, Jeskovsky, M, Jochum, J, Kaznacheeva, M, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Marini, L, Meyer, L, Mokina, V, Nilima, A, Olmi, M, Ortmann, T, Pagliarone, C, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Pucci, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Wagner, F, Willers, M, Zema, V, Angloher G., Banik S., Benato G., Bento A., Bertolini A., Breier R., Bucci C., Burkhart J., Canonica L., D'Addabbo A., Di Lorenzo S., Einfalt L., Erb A., Feilitzsch F. V., Ferreiro Iachellini N., Fichtinger S., Fuchs D., Fuss A., Garai A., Ghete V. M., Gerster S., Gorla P., Guillaumon P. V., Gupta S., Hauff D., Jeskovsky M., Jochum J., Kaznacheeva M., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Marini L., Meyer L., Mokina V., Nilima A., Olmi M., Ortmann T., Pagliarone C., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Pucci F., Reindl F., Rothe J., Schaffner K., Schieck J., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Wagner F., Willers M., Zema V., Angloher, G, Banik, S, Benato, G, Bento, A, Bertolini, A, Breier, R, Bucci, C, Burkhart, J, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Einfalt, L, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuchs, D, Fuss, A, Garai, A, Ghete, V, Gerster, S, Gorla, P, Guillaumon, P, Gupta, S, Hauff, D, Jeskovsky, M, Jochum, J, Kaznacheeva, M, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Marini, L, Meyer, L, Mokina, V, Nilima, A, Olmi, M, Ortmann, T, Pagliarone, C, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Pucci, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Wagner, F, Willers, M, Zema, V, Angloher G., Banik S., Benato G., Bento A., Bertolini A., Breier R., Bucci C., Burkhart J., Canonica L., D'Addabbo A., Di Lorenzo S., Einfalt L., Erb A., Feilitzsch F. V., Ferreiro Iachellini N., Fichtinger S., Fuchs D., Fuss A., Garai A., Ghete V. M., Gerster S., Gorla P., Guillaumon P. V., Gupta S., Hauff D., Jeskovsky M., Jochum J., Kaznacheeva M., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Marini L., Meyer L., Mokina V., Nilima A., Olmi M., Ortmann T., Pagliarone C., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Pucci F., Reindl F., Rothe J., Schaffner K., Schieck J., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Wagner F., Willers M., and Zema V.

Abstract

We present limits on the spin-independent interaction cross section of dark matter particles with silicon nuclei, derived from data taken with a cryogenic calorimeter with 0.35 g target mass operated in the CRESST-III experiment. A baseline nuclear recoil energy resolution of (1.36±0.05) eVnr, currently the lowest reported for macroscopic particle detectors, and a corresponding energy threshold of (10.0±0.2) eVnr have been achieved, improving the sensitivity to light dark matter particles with masses below 160 MeV/c2 by a factor of up to 20 compared to previous results. We characterize the observed low energy excess, and we exclude noise triggers and radioactive contaminations on the crystal surfaces as dominant contributions.

Published
2023

10. TES-Based Light Detectors for the CRESST Direct Dark Matter Search

Author

Rothe, J., Angloher, G., Bauer, P., Bento, A., Bucci, C., Canonica, L., D’Addabbo, A., Defay, X., Erb, A., Feilitzsch, F. v., Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J.-C., Langenkämper, A., Loebell, J., Mancuso, M., Mondragon, E., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Reindl, F., Schäffner, K., Schieck, J., Schipperges, V., Schönert, S., Seidel, W., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Trinh Thi, H. H., Türkoğlu, C., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., and Wüstrich, M.

Published
2018
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11. A Low Nuclear Recoil Energy Threshold for Dark Matter Search with CRESST-III Detectors

Author

Mancuso, M., Angloher, G., Bauer, P., Bento, A., Bucci, C., Canonica, L., D’Addabbo, A., Defay, X., Erb, A., von Feilitzsch, Franz, Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J. C., Langenkämper, A., Loebell, J., Mondragon, E., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schipperges, V., Schönert, S., Seidel, W., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Thi, H. H. Trinh, Türkoglu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., and Wüstrich, M.

Published
2018
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12. In-situ study of light production and transport in phonon/light detector modules for dark matter search

Author

Kiefer, M., Angloher, G., Bento, A., Bucci, C., Canonica, L., Erb, A., Feilitzsch, F.v., Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kluck, H., Kraus, H., Lanfranchi, J.-C., Loebell, J., Münster, A., Petricca, F., Potzel, W., Pröbst, F., Reindl, F., Roth, S., Rottler, K., Sailer, C., Schäffner, K., Schieck, J., Schönert, S., Seidel, W., Sivers, M.v., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Türkoğlu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, M., and Zöller, A.

Published
2016
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13. Radiopurity of a kg-scale PbWO 4 cryogenic detector produced from archaeological Pb for the RES-NOVA experiment

Author

Beeman, J, Benato, G, Bucci, C, Canonica, L, Carniti, P, Celi, E, Clemenza, M, D'Addabbo, A, Danevich, F, Di Domizio, S, Dilorenzo, S, Dubovik, O, Ferreiro Iachellini, N, Ferroni, F, Fiorini, E, Fu, S, Garai, A, Ghislandi, S, Gironi, L, Gorla, P, Gotti, C, Guillaumon, P, Helis, D, Kovtun, G, Mancuso, M, Marini, L, Olmi, M, Pagnanini, L, Pattavina, L, Pessina, G, Petricca, F, Pirro, S, Pozzi, S, Puiu, A, Quitadamo, S, Rothe, J, Scherban, A, Schonert, S, Solopikhin, D, Strauss, R, Tarabini, E, Tretyak, V, Tupitsyna, I, Wagner, V, Beeman J. W., Benato G., Bucci C., Canonica L., Carniti P., Celi E., Clemenza M., D'Addabbo A., Danevich F. A., Di Domizio S., DiLorenzo S., Dubovik O. M., Ferreiro Iachellini N., Ferroni F., Fiorini E., Fu S., Garai A., Ghislandi S., Gironi L., Gorla P., Gotti C., Guillaumon P. V., Helis D. L., Kovtun G. P., Mancuso M., Marini L., Olmi M., Pagnanini L., Pattavina L., Pessina G., Petricca F., Pirro S., Pozzi S., Puiu A., Quitadamo S., Rothe J., Scherban A. P., Schonert S., Solopikhin D. A., Strauss R., Tarabini E., Tretyak V. I., Tupitsyna I. A., Wagner V., Beeman, J, Benato, G, Bucci, C, Canonica, L, Carniti, P, Celi, E, Clemenza, M, D'Addabbo, A, Danevich, F, Di Domizio, S, Dilorenzo, S, Dubovik, O, Ferreiro Iachellini, N, Ferroni, F, Fiorini, E, Fu, S, Garai, A, Ghislandi, S, Gironi, L, Gorla, P, Gotti, C, Guillaumon, P, Helis, D, Kovtun, G, Mancuso, M, Marini, L, Olmi, M, Pagnanini, L, Pattavina, L, Pessina, G, Petricca, F, Pirro, S, Pozzi, S, Puiu, A, Quitadamo, S, Rothe, J, Scherban, A, Schonert, S, Solopikhin, D, Strauss, R, Tarabini, E, Tretyak, V, Tupitsyna, I, Wagner, V, Beeman J. W., Benato G., Bucci C., Canonica L., Carniti P., Celi E., Clemenza M., D'Addabbo A., Danevich F. A., Di Domizio S., DiLorenzo S., Dubovik O. M., Ferreiro Iachellini N., Ferroni F., Fiorini E., Fu S., Garai A., Ghislandi S., Gironi L., Gorla P., Gotti C., Guillaumon P. V., Helis D. L., Kovtun G. P., Mancuso M., Marini L., Olmi M., Pagnanini L., Pattavina L., Pessina G., Petricca F., Pirro S., Pozzi S., Puiu A., Quitadamo S., Rothe J., Scherban A. P., Schonert S., Solopikhin D. A., Strauss R., Tarabini E., Tretyak V. I., Tupitsyna I. A., and Wagner V.

Published
2022

14. Online triggers for supernova and pre-supernova neutrino detection with cryogenic detectors

Author

Eller, P, Ferreiro Iachellini, N, Pattavina, L, Shtembari, L, Eller P., Ferreiro Iachellini N., Pattavina L., Shtembari L., Eller, P, Ferreiro Iachellini, N, Pattavina, L, Shtembari, L, Eller P., Ferreiro Iachellini N., Pattavina L., and Shtembari L.

Abstract

Supernovae (SNe) are among the most energetic events in the universe still far from being fully understood. An early and prompt detection of neutrinos is a one-time opportunity for the realization of the first multi-messenger observation of these events. In this work, we present the prospects of detecting neutrinos produced before (pre-SN) and during a SN while running an advanced cryogenic detector. Recent advances in the cryogenic detector technique and the discovery of coherent elastic neutrino-nucleus scattering offer a wealth of opportunities in neutrino detection. The combination of the excellent energy resolution of this experimental technique, with the high cross section of this detection channel and its equal sensitivity to all neutrino flavors, enables the realization of highly sensitive neutrino telescopes of the size of a few tens of cm, as the newly proposed RES-NOVA experiment. We present a detailed study on the detection promptness of pre-SN and SN neutrino signals, with direct comparisons among different classes of test statistics. While the well-established Poisson test offers in general best performance under optimal conditions, the nonparametric Recursive Product of Spacing statistical test (RPS) is more robust for triggering astrophysical neutrino signals with no specific prior knowledge. Based on our statistical tests the RES-NOVA experiment is able to identify SN neutrino signals at a 15 kpc distance with 95% of success rate, and pre-SN signal as far as 450 pc with a pre-warn time of the order of 10 s. These results demonstrate the potential of RPS for the identification of neutrino signals and the physics reach of the RES-NOVA experiment.

Published
2022

15. Probing spin-dependent dark matter interactions with 6 Li: CRESST Collaboration

Author

Angloher, G, Benato, G, Bento, A, Bertoldo, E, Bertolini, A, Breier, R, Bucci, C, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Einfalt, L, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuchs, D, Fuss, A, Garai, A, Ghete, V, Gorla, P, Gupta, S, Hauff, D, Jeskovsky, M, Jochum, J, Kaznacheeva, M, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Marini, L, Mokina, V, Nilima, A, Olmi, M, Ortmann, T, Pagliarone, C, Palusova, V, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Pucci, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Wagner, F, Willers, M, Zema, V, Angloher G., Benato G., Bento A., Bertoldo E., Bertolini A., Breier R., Bucci C., Canonica L., D'Addabbo A., Di Lorenzo S., Einfalt L., Erb A., Feilitzsch F., Ferreiro Iachellini N., Fichtinger S., Fuchs D., Fuss A., Garai A., Ghete V. M., Gorla P., Gupta S., Hauff D., Jeskovsky M., Jochum J., Kaznacheeva M., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Marini L., Mokina V., Nilima A., Olmi M., Ortmann T., Pagliarone C., Palusova V., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Pucci F., Reindl F., Rothe J., Schaffner K., Schieck J., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Wagner F., Willers M., Zema V., Angloher, G, Benato, G, Bento, A, Bertoldo, E, Bertolini, A, Breier, R, Bucci, C, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Einfalt, L, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuchs, D, Fuss, A, Garai, A, Ghete, V, Gorla, P, Gupta, S, Hauff, D, Jeskovsky, M, Jochum, J, Kaznacheeva, M, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Marini, L, Mokina, V, Nilima, A, Olmi, M, Ortmann, T, Pagliarone, C, Palusova, V, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Pucci, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Wagner, F, Willers, M, Zema, V, Angloher G., Benato G., Bento A., Bertoldo E., Bertolini A., Breier R., Bucci C., Canonica L., D'Addabbo A., Di Lorenzo S., Einfalt L., Erb A., Feilitzsch F., Ferreiro Iachellini N., Fichtinger S., Fuchs D., Fuss A., Garai A., Ghete V. M., Gorla P., Gupta S., Hauff D., Jeskovsky M., Jochum J., Kaznacheeva M., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Marini L., Mokina V., Nilima A., Olmi M., Ortmann T., Pagliarone C., Palusova V., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Pucci F., Reindl F., Rothe J., Schaffner K., Schieck J., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Wagner F., Willers M., and Zema V.

Abstract

CRESST is one of the most prominent direct detection experiments for dark matter particles with sub-GeV/c2 mass. One of the advantages of the CRESST experiment is the possibility to include a large variety of nuclides in the target material used to probe dark matter interactions. In this work, we discuss in particular the interactions of dark matter particles with protons and neutrons of 6Li. This is now possible thanks to new calculations on nuclear matrix elements of this specific isotope of Li. To show the potential of using this particular nuclide for probing dark matter interactions, we used the data collected previously by a CRESST prototype based on LiAlO2 and operated in an above ground test-facility at Max-Planck-Institut für Physik in Munich, Germany. In particular, the inclusion of 6Li in the limit calculation drastically improves the result obtained for spin-dependent interactions with neutrons in the whole mass range. The improvement is significant, greater than two order of magnitude for dark matter masses below 1 GeV/c2, compared to the limit previously published with the same data.

Published
2022

16. Testing spin-dependent dark matter interactions with lithium aluminate targets in CRESST-III

Author

Angloher, G, Banik, S, Benato, G, Bento, A, Bertolini, A, Breier, R, Bucci, C, Burkhart, J, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Einfalt, L, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuchs, D, Fuss, A, Garai, A, Ghete, V, Gerster, S, Gorla, P, Guillaumon, P, Gupta, S, Hauff, D, Jeskovsky, M, Jochum, J, Kaznacheeva, M, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Marini, L, Meyer, L, Mokina, V, Nilima, A, Olmi, M, Ortmann, T, Pagliarone, C, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Pucci, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Wagner, F, Willers, M, Zema, V, Angloher G., Banik S., Benato G., Bento A., Bertolini A., Breier R., Bucci C., Burkhart J., Canonica L., D'Addabbo A., Di Lorenzo S., Einfalt L., Erb A., Feilitzsch F. V., Ferreiro Iachellini N., Fichtinger S., Fuchs D., Fuss A., Garai A., Ghete V. M., Gerster S., Gorla P., Guillaumon P. V., Gupta S., Hauff D., Jeskovsky M., Jochum J., Kaznacheeva M., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Marini L., Meyer L., Mokina V., Nilima A., Olmi M., Ortmann T., Pagliarone C., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Pucci F., Reindl F., Rothe J., Schaffner K., Schieck J., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Wagner F., Willers M., Zema V., Angloher, G, Banik, S, Benato, G, Bento, A, Bertolini, A, Breier, R, Bucci, C, Burkhart, J, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Einfalt, L, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuchs, D, Fuss, A, Garai, A, Ghete, V, Gerster, S, Gorla, P, Guillaumon, P, Gupta, S, Hauff, D, Jeskovsky, M, Jochum, J, Kaznacheeva, M, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Marini, L, Meyer, L, Mokina, V, Nilima, A, Olmi, M, Ortmann, T, Pagliarone, C, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Pucci, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Wagner, F, Willers, M, Zema, V, Angloher G., Banik S., Benato G., Bento A., Bertolini A., Breier R., Bucci C., Burkhart J., Canonica L., D'Addabbo A., Di Lorenzo S., Einfalt L., Erb A., Feilitzsch F. V., Ferreiro Iachellini N., Fichtinger S., Fuchs D., Fuss A., Garai A., Ghete V. M., Gerster S., Gorla P., Guillaumon P. V., Gupta S., Hauff D., Jeskovsky M., Jochum J., Kaznacheeva M., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Marini L., Meyer L., Mokina V., Nilima A., Olmi M., Ortmann T., Pagliarone C., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Pucci F., Reindl F., Rothe J., Schaffner K., Schieck J., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Wagner F., Willers M., and Zema V.

Abstract

In the past decades, numerous experiments have emerged to unveil the nature of dark matter, one of the most discussed open questions in modern particle physics. Among them, the Cryogenic Rare Event Search with Superconducting Thermometers (CRESST) experiment, located at the Laboratori Nazionali del Gran Sasso, operates scintillating crystals as cryogenic phonon detectors. In this work, we present first results from the operation of two detector modules which both have 10.46 g LiAlO2 targets in CRESST-III. The lithium contents in the crystal are Li6, with an odd number of protons and neutrons, and Li7, with an odd number of protons. By considering both isotopes of lithium and Al27, we set the currently strongest cross section upper limits on spin-dependent interaction of dark matter with protons and neutrons for the mass region between 0.25 and 1.5 GeV/c2.

Published
2022

17. Characterization of a kg-scale archaeological lead-based PbWO4 cryogenic detector for the RES-NOVA experiment

Author

Beeman, J.W., primary, Benato, G., additional, Bucci, C., additional, Canonica, L., additional, Carniti, P., additional, Celi, E., additional, Clemenza, M., additional, D’Addabbo, A., additional, Danevich, F.A., additional, Di Domizio, S., additional, Di Lorenzo, S., additional, Dubovik, O.M., additional, Ferreiro Iachellini, N., additional, Ferroni, F., additional, Fiorini, E., additional, Fu, S., additional, Garai, A., additional, Ghislandi, S., additional, Gironi, L., additional, Gorla, P., additional, Gotti, C., additional, Guillaumon, P.V., additional, Helis, D.L., additional, Kovtun, G.P., additional, Mancuso, M., additional, Marini, L., additional, Olmi, M., additional, Pagnanini, L., additional, Pattavina, L., additional, Pessina, G., additional, Petricca, F., additional, Pirro, S., additional, Pozzi, S., additional, Puiu, A., additional, Quitadamo, S., additional, Rothe, J., additional, Scherban, A.P., additional, Schönert, S., additional, Solopikhin, D.A., additional, Strauss, R., additional, Tarabini, E., additional, Tretyak, V.I., additional, Tupitsyna, I.A., additional, and Wagner, V., additional

Published
2023
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18. Impact of coherent neutrino nucleus scattering on direct dark matter searches based on CaWO4 crystals

Author

Gütlein, A., Angloher, G., Bento, A., Bucci, C., Canonica, L., Erb, A., Feilitzsch, F. v., Ferreiro Iachellini, N., Gorla, P., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J.-C., Loebell, J., Münster, A., Petricca, F., Potzel, W., Pröbst, F., Reindl, F., Roth, S., Rottler, K., Sailer, C., Schäffner, K., Schieck, J., Schönert, S., Seidel, W., Sivers, M. v., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, M., and Zöller, A.

Published
2015
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19. Testing spin-dependent dark matter interactions with lithium aluminate targets in CRESST-III

Author

Angloher, G., Banik, S., Benato, G., Bento, A., Bertolini, A., Breier, R., Bucci, C., Burkhart, J., Canonica, L., D Addabbo, A., Di Lorenzo, S., Einfalt, L., Erb, A., Feilitzsch, F. V., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Garai, A., Ghete, V. M., Gerster, S., Gorla, P., Guillaumon, P. V., Gupta, S., Hauff, D., Ješkovský, M., Jochum, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Marini, L., Meyer, L., Mokina, V., Nilima, A., Olmi, M., Ortmann, T., Pagliarone, C., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pröbst, F., Pucci, F., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Felix Wagner, Willers, M., and Zema, V.

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Nuclear Experiment, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

In the past decades, numerous experiments have emerged to unveil the nature of dark matter, one of the most discussed open questions in modern particle physics. Among them, the CRESST experiment, located at the Laboratori Nazionali del Gran Sasso, operates scintillating crystals as cryogenic phonon detectors. In this work, we present first results from the operation of two detector modules which both have 10.46 g LiAlO$_2$ targets in CRESST-III. The lithium contents in the crystal are $^6$Li, with an odd number of protons and neutrons, and $^7$Li, with an odd number of protons. By considering both isotopes of lithium and $^{27}$Al, we set the currently strongest cross section upper limits on spin-dependent interaction of dark matter with protons and neutrons for the mass region between 0.25 and 1.5 GeV/c$^2$., Comment: 9 pages, 8 figures

Published
2023
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20. Exploring Low-Mass Dark Matter with CRESST

Author

Strauss, R., Angloher, G., Bento, A., Bucci, C., Canonica, L., Defay, X., Erb, A., Feilitzsch, F. v., Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J. C., Loebell, J., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Reindl, F., Schäffner, K., Schieck, J., Schönert, S., Seidel, W., Stodolsky, L., Strandhagen, C., Tanzke, A., Trinh Thi, H. H., Türkoglu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, M., and Zöller, A.

Published
2016
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22. Radiopurity of a kg-scale PbWO $$_4$$ <math> <msub> <mrow></mrow> <mn>4</mn> </msub> </math> cryogenic detector produced from archaeological Pb for the RES-NOVA experiment

Author

Beeman, J., Benato, G., Bucci, C., Canonica, L., Carniti, P., Celi, E., Clemenza, M., D’Addabbo, A., Danevich, F., Di Domizio, S., DiLorenzo, S., Dubovik, O., Ferreiro Iachellini, N., Ferroni, F., Fiorini, E., Fu, S., Garai, A., Ghislandi, S., Gironi, L., Gorla, P., Gotti, C., Guillaumon, P., Helis, D., Kovtun, G., Mancuso, M., Marini, L., Olmi, M., Pagnanini, L., Pattavina, L., Pessina, G., Petricca, F., Pirro, S., Pozzi, S., Puiu, A., Quitadamo, S., Rothe, J., Scherban, A., Schönert, S., Solopikhin, D., Strauss, R., Tarabini, E., Tretyak, V., Tupitsyna, I., and Wagner, V.

Abstract

RES-NOVA is a newly proposed experiment for detecting neutrinos from astrophysical sources, mainly Supernovae, using an array of cryogenic detectors made of PbWO $$_4$$ 4 crystals produced from archaeological Pb. This unconventional material, characterized by intrinsic high radiopurity, enables low-background levels in the region of interest for the neutrino detection via Coherent Elastic neutrino-Nucleus Scattering (CE $$\nu $$ ν NS). This signal lies at the detector energy threshold, O(1 keV), and it is expected to be hidden by naturally occurring radioactive contaminants of the crystal absorber. Here, we present the results of a radiopurity assay on a 0.84 kg PbWO $$_4$$ 4 crystal produced from archaeological Pb operated as a cryogenic detector. The crystal internal radioactive contaminations are: $$^{232}$$ 232 Th μ Bq/kg, $$^{238}$$ 238 U μ Bq/kg, $$^{226}$$ 226 Ra 1.3 mBq/kg and $$^{210}$$ 210 Pb 22.5 mBq/kg. We also present a background projection for the final experiment and possible mitigation strategies for further background suppression. The achieved results demonstrate the feasibility of realizing this new class of detectors.

Published
2022

23. Probing spin-dependent dark matter interactions with $$^6$$ <math> <msup> <mrow></mrow> <mn>6</mn> </msup> </math> Li

Author

Angloher, G., Benato, G., Bento, A., Bertoldo, E., Bertolini, A., Breier, R., Bucci, C., Canonica, L., D’Addabbo, A., Lorenzo, S., Einfalt, L., Erb, A., Feilitzsch, F., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Garai, A., Ghete, V., Gorla, P., Gupta, S., Hauff, D., Ješkovský, M., Jochum, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Marini, L., Mokina, V., Nilima, A., Olmi, M., Ortmann, T., Pagliarone, C., Palušová, V., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pröbst, F., Pucci, F., Reindl , F., Rothe, J., Schäffner, K., Schieck, J., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., and Zema, V.

Abstract

CRESST is one of the most prominent direct detection experiments for dark matter particles with sub-GeV/c $$^2$$ 2 mass. One of the advantages of the CRESST experiment is the possibility to include a large variety of nuclides in the target material used to probe dark matter interactions. In this work, we discuss in particular the interactions of dark matter particles with protons and neutrons of $$^{6}$$ 6 Li. This is now possible thanks to new calculations on nuclear matrix elements of this specific isotope of Li. To show the potential of using this particular nuclide for probing dark matter interactions, we used the data collected previously by a CRESST prototype based on LiAlO $$_2$$ 2 and operated in an above ground test-facility at Max-Planck-Institut für Physik in Munich, Germany. In particular, the inclusion of $$^{6}$$ 6 Li in the limit calculation drastically improves the result obtained for spin-dependent interactions with neutrons in the whole mass range. The improvement is significant, greater than two order of magnitude for dark matter masses below 1 GeV/c $$^2$$ 2 , compared to the limit previously published with the same data.

Published
2022

24. Probing spin-dependent dark matter interactions with $^6$Li

Author

Angloher, G., Benato, G., Bento, A., Bertoldo, E., Bertolini, A., Breier, R., Bucci, C., Canonica, L., D???addabbo, A., Di Lorenzo, S., Einfalt, L., Erb, A., Feilitzsch, F. v., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Garai, A., Ghete, V. M., Gorla, P., Gupta, S., Hauff, D., Je??kovsk??, M., Jochum, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenk??mper, A., Mancuso, M., Marini, L., Mokina, V., Nilima, A., Olmi, M., Ortmann, T., Pagliarone, C., Palu??ov??, V., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pr??bst, F., Pucci, F., Reindl, F., Rothe, J., Sch??ffner, K., Schieck, J., Schmiedmayer, D., Sch??nert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., and Zema, V.

Subjects
Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Nuclear Experiment, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract

CRESST is one of the most prominent direct detection experiments for dark matter particles with sub-GeV/c$^2$ mass. One of the advantages of the CRESST experiment is the possibility to include a large variety of nuclides in the target material used to probe dark matter interactions. In this work, we discuss in particular the interactions of dark matter particles with protons and neutrons of $^{6}$Li. This is now possible thanks to new calculations on nuclear matrix elements of this specific isotope of Li. To show the potential of using this particular nuclide for probing dark matter interactions, we used the data collected previously by a CRESST prototype based on LiAlO$_2$ and operated in an above ground test-facility at Max-Planck-Institut f\"ur Physik in Munich, Germany. In particular, the inclusion of $^{6}$Li in the limit calculation drastically improves the result obtained for spin-dependent interactions with neutrons in the whole mass range. The improvement is significant, greater than two order of magnitude for dark matter masses below 1 GeV/c$^2$, compared to the limit previously published with the same data.

Published
2022

25. Latest observations on the low energy excess in CRESST-III

Author

Angloher, G., Banik, S., Benato, G., Bento, A., Bertolini, A., Breier, R., Bucci, C., Canonica, L., D Addabbo, A., Di Lorenzo, S., Einfalt, L., Erb, A., Feilitzsch, F. V., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Garai, A., Ghete, V. M., Gerster, S., Gorla, P., Guillaumon, P. V., Gupta, S., Hauff, D., Ješkovský, M., Jochum, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Marini, L., Meyer, L., Mokina, V., Athoy Nilima, Olmi, M., Ortmann, T., Pagliarone, C., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pröbst, F., Pucci, F., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., and Zema, V.

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The CRESST experiment observes an unexplained excess of events at low energies. In the current CRESST-III data-taking campaign we are operating detector modules with different designs to narrow down the possible explanations. In this work, we show first observations of the ongoing measurement, focusing on the comparison of time, energy and temperature dependence of the excess in several detectors. These exclude dark matter, radioactive backgrounds and intrinsic sources related to the crystal bulk as a major contribution., Comment: 10 pages, 5 figures; to be published in IDM2022 proceedings; corrected several minor typos

Published
2022
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26. Neutrino observatory based on archaeological lead

Author

Pattavina, L, Ferreiro Iachellini, N, Tamborra, I, Pattavina L., Ferreiro Iachellini N., Tamborra I., Pattavina, L, Ferreiro Iachellini, N, Tamborra, I, Pattavina L., Ferreiro Iachellini N., and Tamborra I.

Published
2020

27. Searches for Light Dark Matter with the CRESST-III Experiment

Author

Mancuso, M, Abdelhameed, A, Angloher, G, Breier, R, Bauer, P, Bento, A, Bertoldo, E, Bucci, C, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Erb, A, von Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuss, A, Gorla, P, Hauff, D, Jeskovsky, M, Jochum, J, Kaizer, J, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mokina, V, Mondragon, E, Olmi, M, Ortmann, T, Pagliarone, C, Palusova, V, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schipperges, V, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Turkoglu, C, Usherov, I, Willers, M, Zema, V, Zeman, J, Mancuso M., Abdelhameed A. H., Angloher G., Breier R., Bauer P., Bento A., Bertoldo E., Bucci C., Canonica L., D'Addabbo A., Di Lorenzo S., Erb A., von Feilitzsch F., Ferreiro Iachellini N., Fichtinger S., Fuss A., Gorla P., Hauff D., Jeskovsky M., Jochum J., Kaizer J., Kinast A., Kluck H., Kraus H., Langenkamper A., Mokina V., Mondragon E., Olmi M., Ortmann T., Pagliarone C., Palusova V., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Reindl F., Rothe J., Schaffner K., Schieck J., Schipperges V., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Turkoglu C., Usherov I., Willers M., Zema V., Zeman J., Mancuso, M, Abdelhameed, A, Angloher, G, Breier, R, Bauer, P, Bento, A, Bertoldo, E, Bucci, C, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Erb, A, von Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuss, A, Gorla, P, Hauff, D, Jeskovsky, M, Jochum, J, Kaizer, J, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mokina, V, Mondragon, E, Olmi, M, Ortmann, T, Pagliarone, C, Palusova, V, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schipperges, V, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Turkoglu, C, Usherov, I, Willers, M, Zema, V, Zeman, J, Mancuso M., Abdelhameed A. H., Angloher G., Breier R., Bauer P., Bento A., Bertoldo E., Bucci C., Canonica L., D'Addabbo A., Di Lorenzo S., Erb A., von Feilitzsch F., Ferreiro Iachellini N., Fichtinger S., Fuss A., Gorla P., Hauff D., Jeskovsky M., Jochum J., Kaizer J., Kinast A., Kluck H., Kraus H., Langenkamper A., Mokina V., Mondragon E., Olmi M., Ortmann T., Pagliarone C., Palusova V., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Reindl F., Rothe J., Schaffner K., Schieck J., Schipperges V., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Turkoglu C., Usherov I., Willers M., Zema V., and Zeman J.

Abstract

Cryogenic Rare Event Search with Superconducting Thermometers (CRESST) is a long-standing direct dark matter detection experiment with cryogenic detectors located at the underground facility Laboratori Nazionali del Gran Sasso in Italy. CRESST-III, the third generation of CRESST, was specifically designed to have a world-leading sensitivity for low-mass dark matter (DM) (less than 2 GeV/c 2) to probe the spin-independent DM-nucleus cross section. At present, a large part of the parameter space for spin-independent scattering off nuclei remains untested for dark matter particles with masses below few GeV/c 2 although many motivated theoretical models having been proposed. The CRESST-III experiment employs scintillating CaWO 4 crystals of ∼ 25 g as target material for dark matter interactions operated as cryogenic scintillating calorimeters at ∼ 10 mK. CRESST-III first data taking was successfully completed in 2018, achieving an unprecedented energy threshold for nuclear recoils. This result extended the present sensitivity to DM particles as light as ∼ 160 MeV/c 2. In this paper, an overview of the CRESST-III detectors and results will be presented.

Published
2020

28. Latest results of CRESST-III's search for sub-GeV/c2 dark matter

Author

Kluck, H, Abdelhameed, A, Angloher, G, Bauer, P, Bento, A, Bertoldo, E, Breier, R, Bucci, C, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuss, A, Gorla, P, Hauff, D, Jeskovsky, M, Jochum, J, Kaizer, J, Kinast, A, Kraus, H, Langenkamper, A, Mancuso, M, Mokina, V, Mondragon, E, Olmi, M, Ortmann, T, Pagliarone, C, Palusova, V, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Reindl, F, Rothe, J, Schaner, K, Schieck, J, Schipperges, V, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Willers, M, Zema, V, Zeman, J, Kluck H., Abdelhameed A. H., Angloher G., Bauer P., Bento A., Bertoldo E., Breier R., Bucci C., Canonica L., D'Addabbo A., Di Lorenzo S., Erb A., Feilitzsch F. V., Ferreiro Iachellini N., Fichtinger S., Fuss A., Gorla P., Hauff D., Jeskovsky M., Jochum J., Kaizer J., Kinast A., Kraus H., Langenkamper A., Mancuso M., Mokina V., Mondragon E., Olmi M., Ortmann T., Pagliarone C., Palusova V., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Reindl F., Rothe J., Schaner K., Schieck J., Schipperges V., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Willers M., Zema V., Zeman J., Kluck, H, Abdelhameed, A, Angloher, G, Bauer, P, Bento, A, Bertoldo, E, Breier, R, Bucci, C, Canonica, L, D'Addabbo, A, Di Lorenzo, S, Erb, A, Feilitzsch, F, Ferreiro Iachellini, N, Fichtinger, S, Fuss, A, Gorla, P, Hauff, D, Jeskovsky, M, Jochum, J, Kaizer, J, Kinast, A, Kraus, H, Langenkamper, A, Mancuso, M, Mokina, V, Mondragon, E, Olmi, M, Ortmann, T, Pagliarone, C, Palusova, V, Pattavina, L, Petricca, F, Potzel, W, Povinec, P, Probst, F, Reindl, F, Rothe, J, Schaner, K, Schieck, J, Schipperges, V, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Usherov, I, Willers, M, Zema, V, Zeman, J, Kluck H., Abdelhameed A. H., Angloher G., Bauer P., Bento A., Bertoldo E., Breier R., Bucci C., Canonica L., D'Addabbo A., Di Lorenzo S., Erb A., Feilitzsch F. V., Ferreiro Iachellini N., Fichtinger S., Fuss A., Gorla P., Hauff D., Jeskovsky M., Jochum J., Kaizer J., Kinast A., Kraus H., Langenkamper A., Mancuso M., Mokina V., Mondragon E., Olmi M., Ortmann T., Pagliarone C., Palusova V., Pattavina L., Petricca F., Potzel W., Povinec P., Probst F., Reindl F., Rothe J., Schaner K., Schieck J., Schipperges V., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Usherov I., Willers M., Zema V., and Zeman J.

Abstract

The CRESST-III experiment searches for direct interactions of dark matter with ordinary matter. The main event signature would be a nuclear recoil inside one of the scintillating CaWO4 crystals. Operating the crystals as cryogenic calorimeters provides a phonon signal as measure of the deposited energy. The simultaneous readout of both signals is used to actively discriminate backgrounds. CRESST-III focuses on the sub-GeV/c2 mass region where the sensitivity is driven by the threshold. In the _rst data taking campaign of CRESST-III from 2016-2018 an unprecedented low threshold of 30.1 eV for nuclear recoils was obtained. In this contribution, we will report the status of the experiment and the latest results.

Published
2020

29. Operation of a Diamond Cryogenic Detector for Low-Mass Dark Matter Searches

Author

Canonica, L, Abdelhameed, A, Bauer, P, Bento, A, Bertoldo, E, Ferreiro Iachellini, N, Fuchs, D, Hauff, D, Mancuso, M, Petricca, F, Pröbst, F, Rothe, J, Canonica L, Abdelhameed A H, Bauer P, Bento A, Bertoldo E, Ferreiro Iachellini N, Fuchs D, Hauff D, Mancuso M, Petricca F, Pröbst F, Rothe J, Canonica, L, Abdelhameed, A, Bauer, P, Bento, A, Bertoldo, E, Ferreiro Iachellini, N, Fuchs, D, Hauff, D, Mancuso, M, Petricca, F, Pröbst, F, Rothe, J, Canonica L, Abdelhameed A H, Bauer P, Bento A, Bertoldo E, Ferreiro Iachellini N, Fuchs D, Hauff D, Mancuso M, Petricca F, Pröbst F, and Rothe J

Abstract

Despite the multiple and convincing evidence of the existence of dark matter (DM) in our Universe, its detection is one of the most pressing questions in particle physics. As of today, there is no unambiguous hint which could clarify the particle nature of DM. For these reasons, a huge experimental effort is ongoing, trying to realize experiments which can probe the particle properties of DM. In particular, direct search experiments are trying to cover the largest possible mass range, from a few MeVs up to TeVs. Particularly suited for the sub-GeV mass region are detectors containing light nuclei, which are sensitive to the scattering of light DM candidates. Among them, we investigate a carbon-based absorber to explore DM masses down to the MeV region. Thanks to their cryogenic properties (high Debye temperature and long-lived phonon modes), carbon-based materials operated as low temperature calorimeters could reach an energy threshold in the eV range and would allow for the exploration of new parameters of the DM–nucleus cross section. Despite several proposals, the possibility of operating a carbon-based cryogenic detector is yet to be demonstrated. In this contribution, the preliminary results obtained with a diamond absorber operated with a TES temperature sensor will be reported. The potential of such a detector in the current landscape of DM searches will also be illustrated.

Published
2020

30. RES-NOVA sensitivity to core-collapse and failed core-collapse supernova neutrinos

Author

Pattavina, L., primary, Ferreiro Iachellini, N., additional, Pagnanini, L., additional, Canonica, L., additional, Celi, E., additional, Clemenza, M., additional, Ferroni, F., additional, Fiorini, E., additional, Garai, A., additional, Gironi, L., additional, Mancuso, M., additional, Nisi, S., additional, Petricca, F., additional, Pirro, S., additional, Pozzi, S., additional, Puiu, A., additional, Rothe, J., additional, Schönert, S., additional, Shtembari, L., additional, Strauss, R., additional, and Wagner, V., additional

Published
2021
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31. First results from the CRESST-III low-mass dark matter program

Author

Abdelhameed, A, Angloher, G, Bauer, P, Bento, A, Bertoldo, E, Bucci, C, Canonica, L, D'Addabbo, A, Defay, X, Di Lorenzo, S, Erb, A, Feilitzsch, F, Fichtinger, S, Ferreiro Iachellini, N, Fuss, A, Gorla, P, Hauff, D, Jochum, J, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Mokina, V, Mondragon, E, Munster, A, Olmi, M, Ortmann, T, Pagliarone, C, Pattavina, L, Petricca, F, Potzel, W, Probst, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schipperges, V, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Turkolu, C, Usherov, I, Willers, M, Zema, V, Abdelhameed A. H., Angloher G., Bauer P., Bento A., Bertoldo E., Bucci C., Canonica L., D'Addabbo A., Defay X., Di Lorenzo S., Erb A., Feilitzsch F. V., Fichtinger S., Ferreiro Iachellini N., Fuss A., Gorla P., Hauff D., Jochum J., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Mokina V., Mondragon E., Munster A., Olmi M., Ortmann T., Pagliarone C., Pattavina L., Petricca F., Potzel W., Probst F., Reindl F., Rothe J., Schaffner K., Schieck J., Schipperges V., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Turkolu C., Usherov I., Willers M., Zema V., Abdelhameed, A, Angloher, G, Bauer, P, Bento, A, Bertoldo, E, Bucci, C, Canonica, L, D'Addabbo, A, Defay, X, Di Lorenzo, S, Erb, A, Feilitzsch, F, Fichtinger, S, Ferreiro Iachellini, N, Fuss, A, Gorla, P, Hauff, D, Jochum, J, Kinast, A, Kluck, H, Kraus, H, Langenkamper, A, Mancuso, M, Mokina, V, Mondragon, E, Munster, A, Olmi, M, Ortmann, T, Pagliarone, C, Pattavina, L, Petricca, F, Potzel, W, Probst, F, Reindl, F, Rothe, J, Schaffner, K, Schieck, J, Schipperges, V, Schmiedmayer, D, Schonert, S, Schwertner, C, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Turkolu, C, Usherov, I, Willers, M, Zema, V, Abdelhameed A. H., Angloher G., Bauer P., Bento A., Bertoldo E., Bucci C., Canonica L., D'Addabbo A., Defay X., Di Lorenzo S., Erb A., Feilitzsch F. V., Fichtinger S., Ferreiro Iachellini N., Fuss A., Gorla P., Hauff D., Jochum J., Kinast A., Kluck H., Kraus H., Langenkamper A., Mancuso M., Mokina V., Mondragon E., Munster A., Olmi M., Ortmann T., Pagliarone C., Pattavina L., Petricca F., Potzel W., Probst F., Reindl F., Rothe J., Schaffner K., Schieck J., Schipperges V., Schmiedmayer D., Schonert S., Schwertner C., Stahlberg M., Stodolsky L., Strandhagen C., Strauss R., Turkolu C., Usherov I., Willers M., and Zema V.

Abstract

The CRESST experiment is a direct dark matter search which aims to measure interactions of potential dark matter particles in an Earth-bound detector. With the current stage, CRESST-III, we focus on a low energy threshold for increased sensitivity towards light dark matter particles. In this paper we describe the analysis of one detector operated in the first run of CRESST-III (05/2016-02/2018) achieving a nuclear recoil threshold of 30.1 eV. This result was obtained with a 23.6 g CaWO4 crystal operated as a cryogenic scintillating calorimeter in the CRESST setup at the Laboratori Nazionali del Gran Sasso (LNGS). Both the primary phonon (heat) signal and the simultaneously emitted scintillation light, which is absorbed in a separate silicon-on-sapphire light absorber, are measured with highly sensitive transition edge sensors operated at ∼15 mK. The unique combination of these sensors with the light element oxygen present in our target yields sensitivity to dark matter particle masses as low as 160 MeV/c2.

Published
2019

32. Cosmic activation of Cresst’s CaWO4 crystals

Author

Kluck, H., Angloher, G., Benato, G., Bento, A., Bertolini, A., Breier, R., Bucci, C., Canonica, L., D' Addabbo, A., Di Lorenzo, S., Einfalt, L., Erb, A., Feilitzsch, F. v., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Garai, A., Ghete, V. M., Gorla, P., Gupta, S., Hauff, D., Ješkovský, M., Jochum, J., Kaznacheeva, M., Kinast, A., Kraus, H., Langenkamper, A., Mancuso, M., Marini, L., Mokina, V., Nilima, A., Olmi, M., Ortmann, T, Pagliarone, C. E., Palušová, V., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pröbst, F., Pucci, F., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., and Zema, V.

Subjects
background spectrum, History, calcium, calorimeter cryogenics, ddc, Computer Science Applications, Education, calorimeter crystal, cosmic radiation, CRESST, GEANT, tungsten oxygen, background spectrum, nucleus recoil, calorimeter cryogenics, calorimeter crystal, cosmic radiation, CRESST, calcium, tungsten oxygen, numerical calculations, GEANT, nucleus recoil, numerical calculations
Abstract

The CRESST experiment searches for dark matter induced nuclear recoils inside CaWO4 based cryogenic calorimeters at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy. To identify reliably a potential signal, a precise understanding of its background budget is crucial. An important background category could be “cosmogenics”: radionuclides produced via interactions with cosmic rays, mainly during the crystal production at surface facilities. Albeit CaWO4 is a well-established calorimetric material, no systematic study of its susceptibility for cosmic activation existed so far. In this contribution, we will first report the exposure profile of CRESST’s in-house grown TUM93 crystal to cosmic rays. Then we will identify the most prominent cosmogenics via AcTIVIA calculations. Afterwards we discuss the expected background spectrum based on Geant4 simulations and compare it to measurements.

Published
2021
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33. Cryogenic characterization of a $$\hbox {LiAlO}_{2}$$ crystal and new results on spin-dependent dark matter interactions with ordinary matter

Author

Abdelhameed, A. H., Angloher, G., Bauer, P., Bento, A., Bertoldo, E., Breier, R., Bucci, C., Canonica, L., D???addabbo, A., Di Lorenzo, S., Erb, A., Feilitzsch, F. V., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Ghete, V. M., Garai, A., Gorla, P., Hauff, D., Je??kovsk??, M., Jochum, J., Kaizer, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenk??mper, A., Mancuso, M., Mokina, V., Mondragon, E., Olmi, M., Ortmann, T., Pagliarone, C., Palu??ov??, V., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pr??bst, F., Reindl, F., Rothe, J., Sch??ffner, K., Schieck, J., Schipperges, V., Schmiedmayer, D., Sch??nert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., Zema, V., Zeman, J., Br??tzam, M., and Ganschow, S.

Subjects
Dark matter · Cryogenics · Spin-Dependent · Lithium · Neutrons
Published
2020

34. Cryogenic characterization of a LiAlO2 crystal and new results on spin-dependent dark matter interactions with ordinary matter

Author

Abdelhameed, A., Angloher, G., Bauer, P., Bento, A., Bertoldo, E., Breier, R., Bucci, C., Canonica, L., D’Addabbo, A., Di Lorenzo, S., Erb, A., Feilitzsch, F., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Ghete, V., Garai, A., Gorla, P., Hauff, D., Ješkovský, M., Jochum, J., Kaizer, J., Kaznacheeva, M., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Mokina, V., Mondragon, E., Olmi, M., Ortmann, T., Pagliarone, C., Palušová, V., Pattavina, L., Petricca, F., Potzel, W., Povinec, P., Pröbst, F., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schipperges, V., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Usherov, I., Wagner, F., Willers, M., Zema, V., Zeman, J., and Ganschow, M.

Subjects
Physics::Instrumentation and Detectors, Nuclear Experiment
Abstract

In this work, a first cryogenic characterization of a scintillating LiAlO2 single crystal is presented. The results achieved show that this material holds great potential as a target for direct dark matter search experiments. Three different detector modules obtained from one crystal grown at the Leibniz-Institut für Kristallzüchtung (IKZ) have been tested to study different properties at cryogenic temperatures. Firstly, two 2.8 g twin crystals were used to build different detector modules which were operated in an above-ground laboratory at the Max Planck Institute for Physics (MPP) in Munich, Germany. The first detector module was used to study the scintillation properties of LiAlO2 at cryogenic temperatures. The second achieved an energy threshold of (213.02±1.48) eV which allows setting a competitive limit on the spin-dependent dark matter particle-proton scattering cross section for dark matter particle masses between 350 MeV/c^2 and 1.50 GeV/c^2. Secondly, a detector module with a 373 g LiAlO2 crystal as the main absorber was tested in an underground facility at the Laboratori Nazionali del Gran Sasso (LNGS): from this measurement it was possible to determine the radiopurity of the crystal and study the feasibility of using this material as a neutron flux monitor for low-background experiments.

Published
2020

35. Latest results of CRESST-III’s search for sub-GeV/c2 dark matter

Author

Kluck, H., primary, Abdelhameed, A.H., additional, Angloher, G., additional, Bauer, P., additional, Bento, A., additional, Bertoldo, E., additional, Breier, R., additional, Bucci, C., additional, Canonica, L., additional, D’Addabbo, A., additional, Di Lorenzo, S., additional, Erb, A., additional, Feilitzsch, F. v., additional, Ferreiro Iachellini, N., additional, Fichtinger, S., additional, Fuss, A., additional, Gorla, P., additional, Hauff, D., additional, Ješkovský, M., additional, Jochum, J., additional, Kaizer, J., additional, Kinast, A., additional, Kraus, H., additional, Langenkämper, A., additional, Mancuso, M., additional, Mokina, V., additional, Mondragón, E., additional, Olmi, M., additional, Ortmann, T., additional, Pagliarone, C., additional, Palušová, V., additional, Pattavina, L., additional, Petricca, F., additional, Potzel, W., additional, Povinec, P., additional, Pröbst, F., additional, Reindl, F., additional, Rothe, J., additional, Schäffner, K., additional, Schieck, J., additional, Schipperges, V., additional, Schmiedmayer, D., additional, Schönert, S., additional, Schwertner, C., additional, Stahlberg, M., additional, Stodolsky, L., additional, Strandhagen, C., additional, Strauss, R., additional, Usherov, I., additional, Willers, M., additional, Zema, V., additional, and Zeman, J., additional

Published
2020
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36. Searches for Light Dark Matter with the CRESST-III Experiment.

Author

Mancuso, M., Abdelhameed, A. H., Angloher, G., Breier, R., Bauer, P., Bento, A., Bertoldo, E., Bucci, C., Canonica, L., D'Addabbo, A., Di Lorenzo, S., Erb, A., von Feilitzsch, F., Ferreiro Iachellini, N., Fichtinger, S., Fuss, A., Gorla, P., Hauff, D., Jes̆kovský, M., and Jochum, J.

Subjects
DARK matter, NUCLEAR energy, THRESHOLD energy, DETECTORS
Abstract

Cryogenic Rare Event Search with Superconducting Thermometers (CRESST) is a long-standing direct dark matter detection experiment with cryogenic detectors located at the underground facility Laboratori Nazionali del Gran Sasso in Italy. CRESST-III, the third generation of CRESST, was specifically designed to have a world-leading sensitivity for low-mass dark matter (DM) (less than 2 GeV/ c 2 ) to probe the spin-independent DM-nucleus cross section. At present, a large part of the parameter space for spin-independent scattering off nuclei remains untested for dark matter particles with masses below few GeV/ c 2 although many motivated theoretical models having been proposed. The CRESST-III experiment employs scintillating CaWO 4 crystals of ∼ 25 g as target material for dark matter interactions operated as cryogenic scintillating calorimeters at ∼ 10 mK. CRESST-III first data taking was successfully completed in 2018, achieving an unprecedented energy threshold for nuclear recoils. This result extended the present sensitivity to DM particles as light as ∼ 160 MeV/ c 2 . In this paper, an overview of the CRESST-III detectors and results will be presented. [ABSTRACT FROM AUTHOR]

Published
2020
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37. Lithium-Containing Crystals for Light Dark Matter Search Experiments.

Author

Bertoldo, E., Abdelhameed, A. H., Angloher, G., Bauer, P., Bento, A., Breier, R., Bucci, C., Canonica, L., D'Addabbo, A., Di Lorenzo, S., Erb, A., Feilitzsch, F. V., Ferreiro Iachellini, N., Fichtinger, S., Fuchs, D., Fuss, A., Gorla, P., Hauff, D., Ješkovský, M., and Jochum, J.

Subjects
DARK matter, NEUTRON flux, DIRECT currents, CRYSTALS, NEUTRONS
Abstract

In the current direct dark matter search landscape, the leading experiments in the sub-GeV mass region mostly rely on cryogenic techniques which employ crystalline targets. One attractive type of crystals for these experiments is those containing lithium, due to the fact that 7 Li is an ideal candidate to study spin-dependent dark matter interactions in the low mass region. Furthermore, 6 Li can absorb neutrons, a challenging background for dark matter experiments, through a distinctive signature which allows the monitoring of the neutron flux directly on site. In this work, we show the results obtained with three different detectors based on LiAlO 2 , a target crystal never used before in cryogenic experiments. [ABSTRACT FROM AUTHOR]

Published
2020
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38. TES-Based Light Detectors for the CRESST Direct Dark Matter Search

Author

Massachusetts Institute of Technology. Laboratory for Nuclear Science, Canonica, Lucia, Rothe, J., Angloher, G., Bauer, P., Bento, A., Bucci, C., D’Addabbo, A., Defay, X., Erb, A., Feilitzsch, F. v, Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J.-C., Langenkämper, A., Loebell, J., Mancuso, M., Mondragon, E., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Reindl, F., Schäffner, K., Schieck, J., Schipperges, V., Schönert, S., Seidel, W., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Trinh Thi, H. H, Türkoğlu, C., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, M., Massachusetts Institute of Technology. Laboratory for Nuclear Science, Canonica, Lucia, Rothe, J., Angloher, G., Bauer, P., Bento, A., Bucci, C., D’Addabbo, A., Defay, X., Erb, A., Feilitzsch, F. v, Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J.-C., Langenkämper, A., Loebell, J., Mancuso, M., Mondragon, E., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Reindl, F., Schäffner, K., Schieck, J., Schipperges, V., Schönert, S., Seidel, W., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Trinh Thi, H. H, Türkoğlu, C., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., and Wüstrich, M.

Published
2018

39. A Low Nuclear Recoil Energy Threshold for Dark Matter Search with CRESST-III Detectors

Author

Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Laboratory for Nuclear Science, Canonica, Lucia, Mancuso, M., Angloher, G., Bauer, P., Bento, A., Bucci, C., D’Addabbo, A., Defay, X., Erb, A., von Feilitzsch, Franz, Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J. C, Langenkämper, A., Loebell, J., Mondragon, E., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schipperges, V., Schönert, S., Seidel, W., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Thi, H. H T, Türkoglu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, M., Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Laboratory for Nuclear Science, Canonica, Lucia, Mancuso, M., Angloher, G., Bauer, P., Bento, A., Bucci, C., D’Addabbo, A., Defay, X., Erb, A., von Feilitzsch, Franz, Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J. C, Langenkämper, A., Loebell, J., Mondragon, E., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schipperges, V., Schönert, S., Seidel, W., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Thi, H. H T, Türkoglu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., and Wüstrich, M.

Abstract

The CRESST-III experiment (Cryogenic Rare Events Search with Superconducting Thermometers), located at the underground facility Laboratori Nazionali del Gran Sasso in Italy, uses scintillating CaWO₄ crystals as cryogenic calorimeters to search for direct dark matter interactions in detectors. A large part of the parameter space for spin-independent scattering off nuclei remains untested for dark matter particles with masses below a few GeV/c², despite many naturally motivated theoretical models for light dark matter particles. The CRESST-III detectors are designed to achieve the performance required to probe the low-mass region of the parameter space with a sensitivity never reached before. In this paper, new results on the performance and an overview of the CRESST-III detectors will be presented, emphasizing the results about the low-energy threshold for nuclear recoil of CRESST-III Phase 1 which started collecting data in August 2016. Keywords: Cryogenic detectors; Dark matter; Rare-event searches

Published
2018

40. Search for Low Mass Dark Matter Particles with the CRESST Experiment

Author

Turkoglu, Cenk, primary, Angloher, G., additional, Bauer, P., additional, Bento, A., additional, Bucci, C., additional, Canonica, L., additional, Defay, X., additional, Erb, A., additional, V. Feilitzsch, F, additional, Ferreiro Iachellini, N, additional, Gorla, P., additional, Gütlein, A., additional, Hauff, D., additional, Jochum, J., additional, Kiefer, M., additional, Kluck, H., additional, Kraus, H., additional, C. Lanfranchi, J, additional, Langenkämper, A., additional, Loebell, J., additional, Mancuso, M., additional, Mondragon, E., additional, Münster, A., additional, Pagliarone, C. E., additional, Petricca, F., additional, Potzel, W., additional, Pröbst, F., additional, Puig, R., additional, Reindl, Florian, additional, Rothe, J., additional, Schäffner, K., additional, Schieck, J., additional, Schönert, S., additional, Seidel, W., additional, Stahlberg, M., additional, Stodolsky, L., additional, Strandhagen, C., additional, Strauss, R., additional, Tanzke, A., additional, H. Trinh Thi, H, additional, Uffinger, M., additional, Ulrich, A., additional, Usherov, I., additional, Wawoczny, S., additional, Willers, M., additional, and Wüstrich, M., additional

Published
2017
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41. Limits on Momentum-Dependent Asymmetric Dark Matter with CRESST-II

Author

Angloher, G., primary, Bento, A., additional, Bucci, C., additional, Canonica, L., additional, Defay, X., additional, Erb, A., additional, Feilitzsch, F. v., additional, Ferreiro Iachellini, N., additional, Gorla, P., additional, Gütlein, A., additional, Hauff, D., additional, Jochum, J., additional, Kiefer, M., additional, Kluck, H., additional, Kraus, H., additional, Lanfranchi, J.-C., additional, Loebell, J., additional, Münster, A., additional, Pagliarone, C., additional, Petricca, F., additional, Potzel, W., additional, Pröbst, F., additional, Reindl, F., additional, Schäffner, K., additional, Schieck, J., additional, Schönert, S., additional, Seidel, W., additional, Stodolsky, L., additional, Strandhagen, C., additional, Strauss, R., additional, Tanzke, A., additional, Trinh Thi, H. H., additional, Türkoğlu, C., additional, Uffinger, M., additional, Ulrich, A., additional, Usherov, I., additional, Wawoczny, S., additional, Willers, M., additional, Wüstrich, M., additional, and Zöller, A., additional

Published
2016
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42. The CRESST-III low-mass WIMP detector

Author

Strauss, R, primary, Angloher, G, additional, Bento, A, additional, Bucci, C, additional, Canonica, L, additional, Defay, X, additional, Erb, A, additional, von Feilitzsch, F, additional, Ferreiro Iachellini, N, additional, Gorla, P, additional, Gütlein, A, additional, Hauff, D, additional, Jochum, J, additional, Kiefer, M, additional, Kluck, H, additional, Kraus, H, additional, Lanfranchi, J C, additional, Loebell, J, additional, Münster, A, additional, Pagliarone, C, additional, Petricca, F, additional, Potzel, W, additional, Pröbst, F, additional, Reindl, F, additional, Schäffner, K, additional, Schieck, J, additional, Schönert, S, additional, Seidel, W, additional, Stodolsky, L, additional, Strandhagen, C, additional, Tanzke, A, additional, Trinh Thi, H H, additional, Türkoglu, C, additional, Ufflnger, M, additional, Ulrich, A, additional, Usherov, I, additional, Wawoczny, S, additional, Willers, M, additional, Wüstrich, M, additional, and Zöller, A, additional

Published
2016
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43. New results on low-mass dark matter from the CRESST-II experiment

Author

Petricca, F, primary, Angloher, G, additional, Bento, A, additional, Bucci, C, additional, Canonica, L, additional, Defay, X, additional, Erb, A, additional, v Feilitzsch, F, additional, Ferreiro Iachellini, N, additional, Gorla, P, additional, Gütlein, A, additional, Hauff, D, additional, Jochum, J, additional, Kiefer, M, additional, Kluck, H, additional, Kraus, H, additional, Lanfranchi, J C, additional, Loebell, J, additional, Münster, A, additional, Pagliarone, C, additional, Potzel, W, additional, Pröbst, F, additional, Reindl, F, additional, Schäffner, K, additional, Schieck, J, additional, Schönert, S, additional, Seidel, W, additional, Stodolsky, L, additional, Strandhagen, C, additional, Strauss, R, additional, Tanzke, A, additional, Trinh Thi, H H, additional, Türkoğlu, C, additional, Uffinger, M, additional, Ulrich, A, additional, Usherov, I, additional, Wawoczny, S, additional, Willers, M, additional, Wüstrich, M, additional, and Zoller, A, additional

Published
2016
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44. Impact of coherent neutrino nucleus scattering on direct dark matter searches based on CaWO 4 crystals

Author

Gütlein, A., primary, Angloher, G., additional, Bento, A., additional, Bucci, C., additional, Canonica, L., additional, Erb, A., additional, Feilitzsch, F. v., additional, Ferreiro Iachellini, N., additional, Gorla, P., additional, Hauff, D., additional, Jochum, J., additional, Kiefer, M., additional, Kluck, H., additional, Kraus, H., additional, Lanfranchi, J.-C., additional, Loebell, J., additional, Münster, A., additional, Petricca, F., additional, Potzel, W., additional, Pröbst, F., additional, Reindl, F., additional, Roth, S., additional, Rottler, K., additional, Sailer, C., additional, Schäffner, K., additional, Schieck, J., additional, Schönert, S., additional, Seidel, W., additional, Sivers, M. v., additional, Stodolsky, L., additional, Strandhagen, C., additional, Strauss, R., additional, Tanzke, A., additional, Uffinger, M., additional, Ulrich, A., additional, Usherov, I., additional, Wawoczny, S., additional, Willers, M., additional, Wüstrich, M., additional, and Zöller, A., additional

Published
2015
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45. Beta/gamma and alpha backgrounds in CRESST-II Phase 2

Author

Strauss, R., primary, Angloher, G., additional, Bento, A., additional, Bucci, C., additional, Canonica, L., additional, Erb, A., additional, Feilitzsch, F.v., additional, Ferreiro Iachellini, N., additional, Gorla, P., additional, Gütlein, A., additional, Hauff, D., additional, Jochum, J., additional, Kiefer, M., additional, Kluck, H., additional, Kraus, H., additional, Lanfranchi, J.-C., additional, Loebell, J., additional, Münster, A., additional, Petricca, F., additional, Potzel, W., additional, Pröbst, F., additional, Reindl, F., additional, Roth, S., additional, Rottler, K., additional, Sailer, C., additional, Schäffner, K., additional, Schieck, J., additional, Scholl, S., additional, Schönert, S., additional, Seidel, W., additional, Sivers, M.v., additional, Stodolsky, L., additional, Strandhagen, C., additional, Tanzke, A., additional, Uffinger, M., additional, Ulrich, A., additional, Usherov, I., additional, Wawoczny, S., additional, Willers, M., additional, Wüstrich, M., additional, and Zöller, A., additional

Published
2015
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46. Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground.

Author

Angloher, G., Bauer, P., Bento, A., Bucci, C., Canonica, L., Defay, X., Erb, A., Feilitzsch, F. V., Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J.-C., Langenkämper, A., Loebell, J., and Mancuso, M.

Subjects
CRYOGENICS, DARK matter, MISSING mass problem (Astronomy), WEAKLY interacting massive particles, PHYSICAL cosmology
Abstract

Models for light dark matter particles with masses below 1GeV/c² are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the ν-cleus experiment has achieved an energy threshold of Eth = (19.7±0.9)eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessiable by direct searches. We report the first limit on the spinindependent dark matter particle-nucleon cross section for masses between 140 and 500MeV/c². [ABSTRACT FROM AUTHOR]

Published
2017
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47. Direct dark matter search with the CRESST II experiment

Author

Schieck, J., Angloher, G., Bento, A., Bucci, C., Canonica, L., Defay, X., Erb, A., V Feilitzsch, F., Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Holger Kluck, Kraus, H., Lanfranchi, J. -C, Loebell, J., Mancuso, M., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Reindl, F., Schäffner, K., Schönert, S., Seidel, W., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Thi, H. H. Trinh, Türkoglu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, M., and Zöller, A.

Subjects
Physics - Instrumentation and Detectors, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, High Energy Physics::Experiment, Astrophysics::Cosmology and Extragalactic Astrophysics, Instrumentation and Detectors (physics.ins-det), Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The quest for the particle nature of dark matter is one of the big open questions of modern physics. A well motivated candidate for dark matter is the so-called WIMP - a weakly interacting massive particle. Recently several theoretically well-motivated models with dark matter candidates in a mass region below the WIMP mass-scale gained also a lot of interest, theoretically and experimentally. The CRESST II experiment located at the Gran Sasso laboratory in Italy is optimised for the detection of the elastic scattering of these low-mass dark matter particles with ordinary matter. We show the results obtained with an improved detector setup with increased radio purity and enhanced background rejection and the results obtained with a dedicated low-threshold analysis of a single conventional detector module. The limit achieved is the most stringent limit achieved for direct dark matter experiments in the mass region below 1.8 GeV/$c^{2}$. We will discuss the expected performance for new small CRESST-type detectors to be used during the next data taking phase. We conclude with an outlook of the future potential for direct dark matter detection using further improved CRESST CaWO$_{4}$ cryogenic detectors., Comment: Proceedings, contribution to ICHEP 2016, Chigaco

48. Performance of a CRESST-II Detector Module with True $4\pi$-veto

Author

Angloher, G., Bauer, P., Bento, A., Bucci, C., Canonica, L., Defay, X., Erb, A., Feilitzsch, F. V., Ferreiro-Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J. -C, Langenkämper, A., Loebell, J., Mancuso, M., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schipperges, V., Schönert, S., Seidel, W., Martin Stahlberg, Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Trinh Thi, H. H., Türkoglu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, Marc, and Zöller, A.

49. Description of CRESST-III Data

Author

Abdelhameed, A. H., Angloher, G., Bauer, P., Bento, A., Bertoldo, E., Bucci, C., Canonica, L., D Addabbo, A., Defay, X., Di Lorenzo, S., Erb, A., Feilitzsch, F. V., Fichtinger, S., Ferreiro Iachellini, N., Fuss, A., Gorla, P., Hauff, D., Jochum, J., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Mokina, V., Mondragon, E., Münster, A., Olmi, M., Ortmann, T., Pagliarone, C., Pattavina, L., Petricca, F., Potzel, W., Pröbst, F., Florian Reindl, Rothe, J., Schäffner, K., Schieck, J., Schipperges, V., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Türkoglu, C., Usherov, I., Willers, M., and Zema, V.

50. Description of CRESST-II data

Author

Angloher, G., Bauer, P., Bento, A., Bucci, C., Canonica, L., Defay, X., Erb, A., Feilitzsch, F. V., Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J. -C, Loebell, J., Mancuso, M., Münster, A., Pagliarone, C., Petricca, F., Potzel, W., Pröbst, F., Puig, R., Florian Reindl, Schäffner, K., Schieck, J., Schönert, S., Seidel, W., Stodolsky, L., Strandhagen, C., Strauss, R., Tanzke, A., Trinh Thi, H. H., Türkoğlu, C., Uffinger, M., Ulrich, A., Usherov, I., Wawoczny, S., Willers, M., Wüstrich, M., and Zöller, A.

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