TY  - JOUR
AU  - Adrover, M.
AU  - Althueser, L.
AU  - Andrieu, B.
AU  - Angelino, E.
AU  - Angevaare, J. R.
AU  - Antunović, Biljana
AU  - Aprile, E.
AU  - Babicz, M.
AU  - Bajpai, D.
AU  - Barberio, E.
AU  - Baudis, L.
AU  - Bazyk, M.
AU  - Bell, N.
AU  - Bellagamba, L.
AU  - Biondi, R.
AU  - Biondi, Y.
AU  - Bismark, A.
AU  - Boehm, C.
AU  - Breskin, A.
AU  - Brookes, E. J.
AU  - Brown, A.
AU  - Bruno, G.
AU  - Budnik, R.
AU  - Capelli, C.
AU  - Cardoso, J. M. R.
AU  - Chauvin, A.
AU  - Cimental Chavez, A. P.
AU  - Colijn, A. P.
AU  - Conrad, J.
AU  - Cuenca-García, J. J.
AU  - D’Andrea, V.
AU  - Decowski, M. P.
AU  - Deisting, A.
AU  - Di Gangi, P.
AU  - Diglio, S.
AU  - Doerenkamp, M.
AU  - Drexlin, G.
AU  - Eitel, K.
AU  - Elykov, A.
AU  - Engel, R.
AU  - Farrell, S.
AU  - Ferella, A. D.
AU  - Ferrari, C.
AU  - Fischer, H.
AU  - Flierman, M.
AU  - Fulgione, W.
AU  - Gaemers, P.
AU  - Gaior, R.
AU  - Galloway, M.
AU  - Garroum, N.
AU  - Ghosh, S.
AU  - Girard, F.
AU  - Glade-Beucke, R.
AU  - Glück, F.
AU  - Grandi, L.
AU  - Grigat, J.
AU  - Größle, R.
AU  - Guan, H.
AU  - Guida, M.
AU  - Hammann, R.
AU  - Hannen, V.
AU  - Hansmann-Menzemer, S.
AU  - Hargittai, N.
AU  - Hasegawa, T.
AU  - Hils, C.
AU  - Higuera, A.
AU  - Hiraoka, K.
AU  - Hoetzsch, L.
AU  - Iacovacci, M.
AU  - Itow, Y.
AU  - Jakob, J.
AU  - Jörg, F.
AU  - Kara, M.
AU  - Kavrigin, P.
AU  - Kazama, S.
AU  - Keller, M.
AU  - Kilminster, B.
AU  - Kleifges, M.
AU  - Kobayashi, M.
AU  - Kopec, A.
AU  - von Krosigk, B.
AU  - Kuger, F.
AU  - Landsman, H.
AU  - Lang, R. F.
AU  - Li, I.
AU  - Li, S.
AU  - Liang, S.
AU  - Lindemann, S.
AU  - Lindner, M.
AU  - Lombardi, F.
AU  - Loizeau, J.
AU  - Luce, T.
AU  - Ma, Y.
AU  - Macolino, C.
AU  - Mahlstedt, J.
AU  - Mancuso, A.
AU  - Marrodán Undagoitia, T.
AU  - Lopes, J. A. M.
AU  - Marignetti, F.
AU  - Martens, K.
AU  - Masbou, J.
AU  - Mastroianni, S.
AU  - Milutinovic, S.
AU  - Miuchi, K.
AU  - Miyata, R.
AU  - Molinario, A.
AU  - Monteiro, C. M. B.
AU  - Morå, K.
AU  - Morteau, E.
AU  - Mosbacher, Y.
AU  - Müller, J.
AU  - Murra, M.
AU  - Newstead, J. L.
AU  - Ni, K.
AU  - Oberlack, U. G.
AU  - Ostrovskiy, I.
AU  - Paetsch, B.
AU  - Pandurovic, M.
AU  - Pellegrini, Q.
AU  - Peres, R.
AU  - Pienaar, J.
AU  - Pierre, M.
AU  - Piotter, M.
AU  - Plante, G.
AU  - Pollmann, T. R.
AU  - Principe, L.
AU  - Qi, J.
AU  - Qin, J.
AU  - Rajado Silva, M.
AU  - Ramírez García, D.
AU  - Razeto, A.
AU  - Sakamoto, S.
AU  - Sanchez, L.
AU  - Sanchez-Lucas, P.
AU  - dos Santos, J. M. F.
AU  - Sartorelli, G.
AU  - Scaffidi, A.
AU  - Schulte, P.
AU  - Schultz-Coulon, H.-C.
AU  - Schulze Eißing, H.
AU  - Schumann, M.
AU  - Scotto Lavina, L.
AU  - Selvi, M.
AU  - Semeria, F.
AU  - Shagin, P.
AU  - Sharma, S.
AU  - Shen, W.
AU  - Silva, M.
AU  - Simgen, H.
AU  - Singh, R.
AU  - Solmaz, M.
AU  - Stanley, O.
AU  - Steidl, M.
AU  - Tan, P.-L.
AU  - Terliuk, A.
AU  - Thers, D.
AU  - Thümmler, T.
AU  - Tönnies, F.
AU  - Toschi, F.
AU  - Trinchero, G.
AU  - Trotta, R.
AU  - Tunnell, C.
AU  - Urquijo, P.
AU  - Valerius, K.
AU  - Vecchi, S.
AU  - Vetter, S.
AU  - Volta, G.
AU  - Vorkapic, D.
AU  - Wang, W.
AU  - Weerman, K. M.
AU  - Weinheimer, C.
AU  - Weiss, M.
AU  - Wenz, D.
AU  - Wittweg, C.
AU  - Wolf, J.
AU  - Wolf, T.
AU  - Wu, V. H. S.
AU  - Wurm, M.
AU  - Xing, Y.
AU  - Yamashita, M.
AU  - Ye, J.
AU  - Zavattini, G.
AU  - Zuber, K.
PY  - 2024
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/12876
AB  - Xenon dual-phase time projections chambers (TPCs) have proven to be a successful technology in studying physical phenomena that require low-background conditions. With 40t of liquid xenon (LXe) in the TPC baseline design, DARWIN will have a high sensitivity for the detection of particle dark matter, neutrinoless double beta decay (0 ν β β), and axion-like particles (ALPs). Although cosmic muons are a source of background that cannot be entirely eliminated, they may be greatly diminished by placing the detector deep underground. In this study, we used Monte Carlo simulations to model the cosmogenic background expected for the DARWIN observatory at four underground laboratories: Laboratori Nazionali del Gran Sasso (LNGS), Sanford Underground Research Facility (SURF), Laboratoire Souterrain de Modane (LSM) and SNOLAB. We present here the results of simulations performed to determine the production rate of 137 Xe, the most crucial isotope in the search for 0 ν β β of 136 Xe. Additionally, we explore the contribution that other muon-induced spallation products, such as other unstable xenon isotopes and tritium, may have on the cosmogenic background.
T2  - The European Physical Journal C
T1  - Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites
VL  - 84
IS  - 1
DO  - 10.1140/epjc/s10052-023-12298-w
ER  - 

@article{
author = "Adrover, M. and Althueser, L. and Andrieu, B. and Angelino, E. and Angevaare, J. R. and Antunović, Biljana and Aprile, E. and Babicz, M. and Bajpai, D. and Barberio, E. and Baudis, L. and Bazyk, M. and Bell, N. and Bellagamba, L. and Biondi, R. and Biondi, Y. and Bismark, A. and Boehm, C. and Breskin, A. and Brookes, E. J. and Brown, A. and Bruno, G. and Budnik, R. and Capelli, C. and Cardoso, J. M. R. and Chauvin, A. and Cimental Chavez, A. P. and Colijn, A. P. and Conrad, J. and Cuenca-García, J. J. and D’Andrea, V. and Decowski, M. P. and Deisting, A. and Di Gangi, P. and Diglio, S. and Doerenkamp, M. and Drexlin, G. and Eitel, K. and Elykov, A. and Engel, R. and Farrell, S. and Ferella, A. D. and Ferrari, C. and Fischer, H. and Flierman, M. and Fulgione, W. and Gaemers, P. and Gaior, R. and Galloway, M. and Garroum, N. and Ghosh, S. and Girard, F. and Glade-Beucke, R. and Glück, F. and Grandi, L. and Grigat, J. and Größle, R. and Guan, H. and Guida, M. and Hammann, R. and Hannen, V. and Hansmann-Menzemer, S. and Hargittai, N. and Hasegawa, T. and Hils, C. and Higuera, A. and Hiraoka, K. and Hoetzsch, L. and Iacovacci, M. and Itow, Y. and Jakob, J. and Jörg, F. and Kara, M. and Kavrigin, P. and Kazama, S. and Keller, M. and Kilminster, B. and Kleifges, M. and Kobayashi, M. and Kopec, A. and von Krosigk, B. and Kuger, F. and Landsman, H. and Lang, R. F. and Li, I. and Li, S. and Liang, S. and Lindemann, S. and Lindner, M. and Lombardi, F. and Loizeau, J. and Luce, T. and Ma, Y. and Macolino, C. and Mahlstedt, J. and Mancuso, A. and Marrodán Undagoitia, T. and Lopes, J. A. M. and Marignetti, F. and Martens, K. and Masbou, J. and Mastroianni, S. and Milutinovic, S. and Miuchi, K. and Miyata, R. and Molinario, A. and Monteiro, C. M. B. and Morå, K. and Morteau, E. and Mosbacher, Y. and Müller, J. and Murra, M. and Newstead, J. L. and Ni, K. and Oberlack, U. G. and Ostrovskiy, I. and Paetsch, B. and Pandurovic, M. and Pellegrini, Q. and Peres, R. and Pienaar, J. and Pierre, M. and Piotter, M. and Plante, G. and Pollmann, T. R. and Principe, L. and Qi, J. and Qin, J. and Rajado Silva, M. and Ramírez García, D. and Razeto, A. and Sakamoto, S. and Sanchez, L. and Sanchez-Lucas, P. and dos Santos, J. M. F. and Sartorelli, G. and Scaffidi, A. and Schulte, P. and Schultz-Coulon, H.-C. and Schulze Eißing, H. and Schumann, M. and Scotto Lavina, L. and Selvi, M. and Semeria, F. and Shagin, P. and Sharma, S. and Shen, W. and Silva, M. and Simgen, H. and Singh, R. and Solmaz, M. and Stanley, O. and Steidl, M. and Tan, P.-L. and Terliuk, A. and Thers, D. and Thümmler, T. and Tönnies, F. and Toschi, F. and Trinchero, G. and Trotta, R. and Tunnell, C. and Urquijo, P. and Valerius, K. and Vecchi, S. and Vetter, S. and Volta, G. and Vorkapic, D. and Wang, W. and Weerman, K. M. and Weinheimer, C. and Weiss, M. and Wenz, D. and Wittweg, C. and Wolf, J. and Wolf, T. and Wu, V. H. S. and Wurm, M. and Xing, Y. and Yamashita, M. and Ye, J. and Zavattini, G. and Zuber, K.",
year = "2024",
abstract = "Xenon dual-phase time projections chambers (TPCs) have proven to be a successful technology in studying physical phenomena that require low-background conditions. With 40t of liquid xenon (LXe) in the TPC baseline design, DARWIN will have a high sensitivity for the detection of particle dark matter, neutrinoless double beta decay (0 ν β β), and axion-like particles (ALPs). Although cosmic muons are a source of background that cannot be entirely eliminated, they may be greatly diminished by placing the detector deep underground. In this study, we used Monte Carlo simulations to model the cosmogenic background expected for the DARWIN observatory at four underground laboratories: Laboratori Nazionali del Gran Sasso (LNGS), Sanford Underground Research Facility (SURF), Laboratoire Souterrain de Modane (LSM) and SNOLAB. We present here the results of simulations performed to determine the production rate of 137 Xe, the most crucial isotope in the search for 0 ν β β of 136 Xe. Additionally, we explore the contribution that other muon-induced spallation products, such as other unstable xenon isotopes and tritium, may have on the cosmogenic background.",
journal = "The European Physical Journal C",
title = "Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites",
volume = "84",
number = "1",
doi = "10.1140/epjc/s10052-023-12298-w"
}

Adrover, M., Althueser, L., Andrieu, B., Angelino, E., Angevaare, J. R., Antunović, B., Aprile, E., Babicz, M., Bajpai, D., Barberio, E., Baudis, L., Bazyk, M., Bell, N., Bellagamba, L., Biondi, R., Biondi, Y., Bismark, A., Boehm, C., Breskin, A., Brookes, E. J., Brown, A., Bruno, G., Budnik, R., Capelli, C., Cardoso, J. M. R., Chauvin, A., Cimental Chavez, A. P., Colijn, A. P., Conrad, J., Cuenca-García, J. J., D’Andrea, V., Decowski, M. P., Deisting, A., Di Gangi, P., Diglio, S., Doerenkamp, M., Drexlin, G., Eitel, K., Elykov, A., Engel, R., Farrell, S., Ferella, A. D., Ferrari, C., Fischer, H., Flierman, M., Fulgione, W., Gaemers, P., Gaior, R., Galloway, M., Garroum, N., Ghosh, S., Girard, F., Glade-Beucke, R., Glück, F., Grandi, L., Grigat, J., Größle, R., Guan, H., Guida, M., Hammann, R., Hannen, V., Hansmann-Menzemer, S., Hargittai, N., Hasegawa, T., Hils, C., Higuera, A., Hiraoka, K., Hoetzsch, L., Iacovacci, M., Itow, Y., Jakob, J., Jörg, F., Kara, M., Kavrigin, P., Kazama, S., Keller, M., Kilminster, B., Kleifges, M., Kobayashi, M., Kopec, A., von Krosigk, B., Kuger, F., Landsman, H., Lang, R. F., Li, I., Li, S., Liang, S., Lindemann, S., Lindner, M., Lombardi, F., Loizeau, J., Luce, T., Ma, Y., Macolino, C., Mahlstedt, J., Mancuso, A., Marrodán Undagoitia, T., Lopes, J. A. M., Marignetti, F., Martens, K., Masbou, J., Mastroianni, S., Milutinovic, S., Miuchi, K., Miyata, R., Molinario, A., Monteiro, C. M. B., Morå, K., Morteau, E., Mosbacher, Y., Müller, J., Murra, M., Newstead, J. L., Ni, K., Oberlack, U. G., Ostrovskiy, I., Paetsch, B., Pandurovic, M., Pellegrini, Q., Peres, R., Pienaar, J., Pierre, M., Piotter, M., Plante, G., Pollmann, T. R., Principe, L., Qi, J., Qin, J., Rajado Silva, M., Ramírez García, D., Razeto, A., Sakamoto, S., Sanchez, L., Sanchez-Lucas, P., dos Santos, J. M. F., Sartorelli, G., Scaffidi, A., Schulte, P., Schultz-Coulon, H.-C., Schulze Eißing, H., Schumann, M., Scotto Lavina, L., Selvi, M., Semeria, F., Shagin, P., Sharma, S., Shen, W., Silva, M., Simgen, H., Singh, R., Solmaz, M., Stanley, O., Steidl, M., Tan, P.-L., Terliuk, A., Thers, D., Thümmler, T., Tönnies, F., Toschi, F., Trinchero, G., Trotta, R., Tunnell, C., Urquijo, P., Valerius, K., Vecchi, S., Vetter, S., Volta, G., Vorkapic, D., Wang, W., Weerman, K. M., Weinheimer, C., Weiss, M., Wenz, D., Wittweg, C., Wolf, J., Wolf, T., Wu, V. H. S., Wurm, M., Xing, Y., Yamashita, M., Ye, J., Zavattini, G.,& Zuber, K.. (2024). Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites. in The European Physical Journal C, 84(1).
https://doi.org/10.1140/epjc/s10052-023-12298-w

Adrover M, Althueser L, Andrieu B, Angelino E, Angevaare JR, Antunović B, Aprile E, Babicz M, Bajpai D, Barberio E, Baudis L, Bazyk M, Bell N, Bellagamba L, Biondi R, Biondi Y, Bismark A, Boehm C, Breskin A, Brookes EJ, Brown A, Bruno G, Budnik R, Capelli C, Cardoso JMR, Chauvin A, Cimental Chavez AP, Colijn AP, Conrad J, Cuenca-García JJ, D’Andrea V, Decowski MP, Deisting A, Di Gangi P, Diglio S, Doerenkamp M, Drexlin G, Eitel K, Elykov A, Engel R, Farrell S, Ferella AD, Ferrari C, Fischer H, Flierman M, Fulgione W, Gaemers P, Gaior R, Galloway M, Garroum N, Ghosh S, Girard F, Glade-Beucke R, Glück F, Grandi L, Grigat J, Größle R, Guan H, Guida M, Hammann R, Hannen V, Hansmann-Menzemer S, Hargittai N, Hasegawa T, Hils C, Higuera A, Hiraoka K, Hoetzsch L, Iacovacci M, Itow Y, Jakob J, Jörg F, Kara M, Kavrigin P, Kazama S, Keller M, Kilminster B, Kleifges M, Kobayashi M, Kopec A, von Krosigk B, Kuger F, Landsman H, Lang RF, Li I, Li S, Liang S, Lindemann S, Lindner M, Lombardi F, Loizeau J, Luce T, Ma Y, Macolino C, Mahlstedt J, Mancuso A, Marrodán Undagoitia T, Lopes JAM, Marignetti F, Martens K, Masbou J, Mastroianni S, Milutinovic S, Miuchi K, Miyata R, Molinario A, Monteiro CMB, Morå K, Morteau E, Mosbacher Y, Müller J, Murra M, Newstead JL, Ni K, Oberlack UG, Ostrovskiy I, Paetsch B, Pandurovic M, Pellegrini Q, Peres R, Pienaar J, Pierre M, Piotter M, Plante G, Pollmann TR, Principe L, Qi J, Qin J, Rajado Silva M, Ramírez García D, Razeto A, Sakamoto S, Sanchez L, Sanchez-Lucas P, dos Santos JMF, Sartorelli G, Scaffidi A, Schulte P, Schultz-Coulon H, Schulze Eißing H, Schumann M, Scotto Lavina L, Selvi M, Semeria F, Shagin P, Sharma S, Shen W, Silva M, Simgen H, Singh R, Solmaz M, Stanley O, Steidl M, Tan P, Terliuk A, Thers D, Thümmler T, Tönnies F, Toschi F, Trinchero G, Trotta R, Tunnell C, Urquijo P, Valerius K, Vecchi S, Vetter S, Volta G, Vorkapic D, Wang W, Weerman KM, Weinheimer C, Weiss M, Wenz D, Wittweg C, Wolf J, Wolf T, Wu VHS, Wurm M, Xing Y, Yamashita M, Ye J, Zavattini G, Zuber K. Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites. in The European Physical Journal C. 2024;84(1).
doi:10.1140/epjc/s10052-023-12298-w .

Adrover, M., Althueser, L., Andrieu, B., Angelino, E., Angevaare, J. R., Antunović, Biljana, Aprile, E., Babicz, M., Bajpai, D., Barberio, E., Baudis, L., Bazyk, M., Bell, N., Bellagamba, L., Biondi, R., Biondi, Y., Bismark, A., Boehm, C., Breskin, A., Brookes, E. J., Brown, A., Bruno, G., Budnik, R., Capelli, C., Cardoso, J. M. R., Chauvin, A., Cimental Chavez, A. P., Colijn, A. P., Conrad, J., Cuenca-García, J. J., D’Andrea, V., Decowski, M. P., Deisting, A., Di Gangi, P., Diglio, S., Doerenkamp, M., Drexlin, G., Eitel, K., Elykov, A., Engel, R., Farrell, S., Ferella, A. D., Ferrari, C., Fischer, H., Flierman, M., Fulgione, W., Gaemers, P., Gaior, R., Galloway, M., Garroum, N., Ghosh, S., Girard, F., Glade-Beucke, R., Glück, F., Grandi, L., Grigat, J., Größle, R., Guan, H., Guida, M., Hammann, R., Hannen, V., Hansmann-Menzemer, S., Hargittai, N., Hasegawa, T., Hils, C., Higuera, A., Hiraoka, K., Hoetzsch, L., Iacovacci, M., Itow, Y., Jakob, J., Jörg, F., Kara, M., Kavrigin, P., Kazama, S., Keller, M., Kilminster, B., Kleifges, M., Kobayashi, M., Kopec, A., von Krosigk, B., Kuger, F., Landsman, H., Lang, R. F., Li, I., Li, S., Liang, S., Lindemann, S., Lindner, M., Lombardi, F., Loizeau, J., Luce, T., Ma, Y., Macolino, C., Mahlstedt, J., Mancuso, A., Marrodán Undagoitia, T., Lopes, J. A. M., Marignetti, F., Martens, K., Masbou, J., Mastroianni, S., Milutinovic, S., Miuchi, K., Miyata, R., Molinario, A., Monteiro, C. M. B., Morå, K., Morteau, E., Mosbacher, Y., Müller, J., Murra, M., Newstead, J. L., Ni, K., Oberlack, U. G., Ostrovskiy, I., Paetsch, B., Pandurovic, M., Pellegrini, Q., Peres, R., Pienaar, J., Pierre, M., Piotter, M., Plante, G., Pollmann, T. R., Principe, L., Qi, J., Qin, J., Rajado Silva, M., Ramírez García, D., Razeto, A., Sakamoto, S., Sanchez, L., Sanchez-Lucas, P., dos Santos, J. M. F., Sartorelli, G., Scaffidi, A., Schulte, P., Schultz-Coulon, H.-C., Schulze Eißing, H., Schumann, M., Scotto Lavina, L., Selvi, M., Semeria, F., Shagin, P., Sharma, S., Shen, W., Silva, M., Simgen, H., Singh, R., Solmaz, M., Stanley, O., Steidl, M., Tan, P.-L., Terliuk, A., Thers, D., Thümmler, T., Tönnies, F., Toschi, F., Trinchero, G., Trotta, R., Tunnell, C., Urquijo, P., Valerius, K., Vecchi, S., Vetter, S., Volta, G., Vorkapic, D., Wang, W., Weerman, K. M., Weinheimer, C., Weiss, M., Wenz, D., Wittweg, C., Wolf, J., Wolf, T., Wu, V. H. S., Wurm, M., Xing, Y., Yamashita, M., Ye, J., Zavattini, G., Zuber, K., "Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites" in The European Physical Journal C, 84, no. 1 (2024),
https://doi.org/10.1140/epjc/s10052-023-12298-w . .

TY  - JOUR
AU  - Agostini, F.
AU  - Maouloud, S. E. M. Ahmed
AU  - Althueser, L.
AU  - Amaro, F.
AU  - Antunović, Biljana
AU  - Aprile, E.
AU  - Baudis, L.
AU  - Baur, D.
AU  - Biondi, Y.
AU  - Bismark, A.
AU  - Breur, P. A.
AU  - Brown, A.
AU  - Bruno, G.
AU  - Budnik, R.
AU  - Capelli, C.
AU  - Cardoso, J.
AU  - Cichon, D.
AU  - Clark, M.
AU  - Colijn, A. P.
AU  - Cuenca-García, J. J.
AU  - Cussonneau, J. P.
AU  - Decowski, M. P.
AU  - Depoian, A.
AU  - Dierle, J.
AU  - Gangi, P. Di
AU  - Giovanni, A. Di
AU  - Diglio, S.
AU  - Santos, J. M. F. dos
AU  - Drexlin, G.
AU  - Eitel, K.
AU  - Engel, R.
AU  - Ferella, A. D.
AU  - Fischer, H.
AU  - Galloway, M.
AU  - Gao, F.
AU  - Girard, F.
AU  - Glück, F.
AU  - Grandi, L.
AU  - Größle, R.
AU  - Gumbsheimer, R.
AU  - Hansmann-Menzemer, S.
AU  - Jörg, F.
AU  - Khundzakishvili, G.
AU  - Kopec, A.
AU  - Kuger, F.
AU  - Krauss, L. M.
AU  - Landsman, H.
AU  - Lang, R. F.
AU  - Lindemann, S.
AU  - Lindner, M.
AU  - Lopes, J. a. M.
AU  - Villalpando, A. Loya
AU  - Macolino, C.
AU  - Manfredini, A.
AU  - Undagoitia, T. Marrodán
AU  - Masbou, J.
AU  - Masson, E.
AU  - Meinhardt, P.
AU  - Milutinović, Slobodan
AU  - Molinario, A.
AU  - Monteiro, C. M. B.
AU  - Murra, M.
AU  - Oberlack, U. G.
AU  - Pandurović, Mila
AU  - Peres, R.
AU  - Pienaar, J.
AU  - Pierre, M.
AU  - Pizzella, V.
AU  - Qin, J.
AU  - García, D. Ramírez
AU  - Reichard, S.
AU  - Rupp, N.
AU  - Sanchez-Lucas, P.
AU  - Sartorelli, G.
AU  - Schulte, D.
AU  - Schumann, M.
AU  - Lavina, L. Scotto
AU  - Selvi, M.
AU  - Silva, M.
AU  - Simgen, H.
AU  - Steidl, M.
AU  - Terliuk, A.
AU  - Therreau, C.
AU  - Thers, D.
AU  - Thieme, K.
AU  - Trotta, R.
AU  - Tunnell, C. D.
AU  - Valerius, K.
AU  - Volta, G.
AU  - Vorkapić, D.
AU  - Weinheimer, C.
AU  - Wittweg, C.
AU  - Wolf, J.
AU  - Zopounidis, J. P.
AU  - Zuber, K.
PY  - 2020
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/9633
AB  - The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains about 3.6 t of $$^{136}$$ 136 Xe. Here, we show that its projected half-life sensitivity is $$2.4\times {10}^{27}\,{\hbox {year}}$$ 2.4 × 10 27 year , using a fiducial volume of 5 t of natural xenon and 10 year of operation with a background rate of less than 0.2 events/(t $$\cdot $$ · year) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in $$^{136}$$ 136 Xe.
T2  - European Physical Journal C. Particles and Fields
T1  - Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe
VL  - 80
IS  - 9
SP  - 1
EP  - 11
DO  - 10.1140/epjc/s10052-020-8196-z
ER  - 

@article{
author = "Agostini, F. and Maouloud, S. E. M. Ahmed and Althueser, L. and Amaro, F. and Antunović, Biljana and Aprile, E. and Baudis, L. and Baur, D. and Biondi, Y. and Bismark, A. and Breur, P. A. and Brown, A. and Bruno, G. and Budnik, R. and Capelli, C. and Cardoso, J. and Cichon, D. and Clark, M. and Colijn, A. P. and Cuenca-García, J. J. and Cussonneau, J. P. and Decowski, M. P. and Depoian, A. and Dierle, J. and Gangi, P. Di and Giovanni, A. Di and Diglio, S. and Santos, J. M. F. dos and Drexlin, G. and Eitel, K. and Engel, R. and Ferella, A. D. and Fischer, H. and Galloway, M. and Gao, F. and Girard, F. and Glück, F. and Grandi, L. and Größle, R. and Gumbsheimer, R. and Hansmann-Menzemer, S. and Jörg, F. and Khundzakishvili, G. and Kopec, A. and Kuger, F. and Krauss, L. M. and Landsman, H. and Lang, R. F. and Lindemann, S. and Lindner, M. and Lopes, J. a. M. and Villalpando, A. Loya and Macolino, C. and Manfredini, A. and Undagoitia, T. Marrodán and Masbou, J. and Masson, E. and Meinhardt, P. and Milutinović, Slobodan and Molinario, A. and Monteiro, C. M. B. and Murra, M. and Oberlack, U. G. and Pandurović, Mila and Peres, R. and Pienaar, J. and Pierre, M. and Pizzella, V. and Qin, J. and García, D. Ramírez and Reichard, S. and Rupp, N. and Sanchez-Lucas, P. and Sartorelli, G. and Schulte, D. and Schumann, M. and Lavina, L. Scotto and Selvi, M. and Silva, M. and Simgen, H. and Steidl, M. and Terliuk, A. and Therreau, C. and Thers, D. and Thieme, K. and Trotta, R. and Tunnell, C. D. and Valerius, K. and Volta, G. and Vorkapić, D. and Weinheimer, C. and Wittweg, C. and Wolf, J. and Zopounidis, J. P. and Zuber, K.",
year = "2020",
abstract = "The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains about 3.6 t of $$^{136}$$ 136 Xe. Here, we show that its projected half-life sensitivity is $$2.4\times {10}^{27}\,{\hbox {year}}$$ 2.4 × 10 27 year , using a fiducial volume of 5 t of natural xenon and 10 year of operation with a background rate of less than 0.2 events/(t $$\cdot $$ · year) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in $$^{136}$$ 136 Xe.",
journal = "European Physical Journal C. Particles and Fields",
title = "Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe",
volume = "80",
number = "9",
pages = "1-11",
doi = "10.1140/epjc/s10052-020-8196-z"
}

Agostini, F., Maouloud, S. E. M. A., Althueser, L., Amaro, F., Antunović, B., Aprile, E., Baudis, L., Baur, D., Biondi, Y., Bismark, A., Breur, P. A., Brown, A., Bruno, G., Budnik, R., Capelli, C., Cardoso, J., Cichon, D., Clark, M., Colijn, A. P., Cuenca-García, J. J., Cussonneau, J. P., Decowski, M. P., Depoian, A., Dierle, J., Gangi, P. D., Giovanni, A. D., Diglio, S., Santos, J. M. F. d., Drexlin, G., Eitel, K., Engel, R., Ferella, A. D., Fischer, H., Galloway, M., Gao, F., Girard, F., Glück, F., Grandi, L., Größle, R., Gumbsheimer, R., Hansmann-Menzemer, S., Jörg, F., Khundzakishvili, G., Kopec, A., Kuger, F., Krauss, L. M., Landsman, H., Lang, R. F., Lindemann, S., Lindner, M., Lopes, J. a. M., Villalpando, A. L., Macolino, C., Manfredini, A., Undagoitia, T. M., Masbou, J., Masson, E., Meinhardt, P., Milutinović, S., Molinario, A., Monteiro, C. M. B., Murra, M., Oberlack, U. G., Pandurović, M., Peres, R., Pienaar, J., Pierre, M., Pizzella, V., Qin, J., García, D. R., Reichard, S., Rupp, N., Sanchez-Lucas, P., Sartorelli, G., Schulte, D., Schumann, M., Lavina, L. S., Selvi, M., Silva, M., Simgen, H., Steidl, M., Terliuk, A., Therreau, C., Thers, D., Thieme, K., Trotta, R., Tunnell, C. D., Valerius, K., Volta, G., Vorkapić, D., Weinheimer, C., Wittweg, C., Wolf, J., Zopounidis, J. P.,& Zuber, K.. (2020). Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe. in European Physical Journal C. Particles and Fields, 80(9), 1-11.
https://doi.org/10.1140/epjc/s10052-020-8196-z

Agostini F, Maouloud SEMA, Althueser L, Amaro F, Antunović B, Aprile E, Baudis L, Baur D, Biondi Y, Bismark A, Breur PA, Brown A, Bruno G, Budnik R, Capelli C, Cardoso J, Cichon D, Clark M, Colijn AP, Cuenca-García JJ, Cussonneau JP, Decowski MP, Depoian A, Dierle J, Gangi PD, Giovanni AD, Diglio S, Santos JMFD, Drexlin G, Eitel K, Engel R, Ferella AD, Fischer H, Galloway M, Gao F, Girard F, Glück F, Grandi L, Größle R, Gumbsheimer R, Hansmann-Menzemer S, Jörg F, Khundzakishvili G, Kopec A, Kuger F, Krauss LM, Landsman H, Lang RF, Lindemann S, Lindner M, Lopes JAM, Villalpando AL, Macolino C, Manfredini A, Undagoitia TM, Masbou J, Masson E, Meinhardt P, Milutinović S, Molinario A, Monteiro CMB, Murra M, Oberlack UG, Pandurović M, Peres R, Pienaar J, Pierre M, Pizzella V, Qin J, García DR, Reichard S, Rupp N, Sanchez-Lucas P, Sartorelli G, Schulte D, Schumann M, Lavina LS, Selvi M, Silva M, Simgen H, Steidl M, Terliuk A, Therreau C, Thers D, Thieme K, Trotta R, Tunnell CD, Valerius K, Volta G, Vorkapić D, Weinheimer C, Wittweg C, Wolf J, Zopounidis JP, Zuber K. Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe. in European Physical Journal C. Particles and Fields. 2020;80(9):1-11.
doi:10.1140/epjc/s10052-020-8196-z .

Agostini, F., Maouloud, S. E. M. Ahmed, Althueser, L., Amaro, F., Antunović, Biljana, Aprile, E., Baudis, L., Baur, D., Biondi, Y., Bismark, A., Breur, P. A., Brown, A., Bruno, G., Budnik, R., Capelli, C., Cardoso, J., Cichon, D., Clark, M., Colijn, A. P., Cuenca-García, J. J., Cussonneau, J. P., Decowski, M. P., Depoian, A., Dierle, J., Gangi, P. Di, Giovanni, A. Di, Diglio, S., Santos, J. M. F. dos, Drexlin, G., Eitel, K., Engel, R., Ferella, A. D., Fischer, H., Galloway, M., Gao, F., Girard, F., Glück, F., Grandi, L., Größle, R., Gumbsheimer, R., Hansmann-Menzemer, S., Jörg, F., Khundzakishvili, G., Kopec, A., Kuger, F., Krauss, L. M., Landsman, H., Lang, R. F., Lindemann, S., Lindner, M., Lopes, J. a. M., Villalpando, A. Loya, Macolino, C., Manfredini, A., Undagoitia, T. Marrodán, Masbou, J., Masson, E., Meinhardt, P., Milutinović, Slobodan, Molinario, A., Monteiro, C. M. B., Murra, M., Oberlack, U. G., Pandurović, Mila, Peres, R., Pienaar, J., Pierre, M., Pizzella, V., Qin, J., García, D. Ramírez, Reichard, S., Rupp, N., Sanchez-Lucas, P., Sartorelli, G., Schulte, D., Schumann, M., Lavina, L. Scotto, Selvi, M., Silva, M., Simgen, H., Steidl, M., Terliuk, A., Therreau, C., Thers, D., Thieme, K., Trotta, R., Tunnell, C. D., Valerius, K., Volta, G., Vorkapić, D., Weinheimer, C., Wittweg, C., Wolf, J., Zopounidis, J. P., Zuber, K., "Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe" in European Physical Journal C. Particles and Fields, 80, no. 9 (2020):1-11,
https://doi.org/10.1140/epjc/s10052-020-8196-z . .