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 . .