Search Results - "Dierle, J"

Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$Xe by Agostini, F, Maouloud, S. E. M. Ahmed, Althueser, L, Amaro, F, Antunovic, B, Aprile, E, Baudis, L

“…Abstract The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of…”
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Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136Xe by Agostini, F., Maouloud, S. E. M. Ahmed, Althueser, L., Amaro, F., Antunovic, 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. 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., Milutinovic, S., Molinario, A., Monteiro, C. M. B., Murra, M., Oberlack, U. G., Pandurovic, M., 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., Vorkapic, D., Weinheimer, C., Wittweg, C., Wolf, J., Zopounidis, J. P., Zuber, K.

“…We correct an overestimation of the production rate of 137 Xe in the DARWIN detector operated at LNGS. This formerly dominant intrinsic background source is…”
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Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe by F. Agostini, S. E. M. Ahmed Maouloud, L. Althueser, F. Amaro, B. Antunovic, E. Aprile, L. Baudis, D. Baur, Y. Biondi, A. Bismark, P. A. Breur, A. Brown, G. Bruno, R. Budnik, C. Capelli, J. Cardoso, D. Cichon, M. Clark, A. P. Colijn, J. J. Cuenca-García, J. P. Cussonneau, M. P. Decowski, A. Depoian, J. Dierle, P. Di Gangi, A. Di Giovanni, S. Diglio, J. M. F. dos Santos, G. Drexlin, K. Eitel, R. Engel, A. D. Ferella, H. Fischer, M. Galloway, F. Gao, F. Girard, F. Glück, L. Grandi, R. Größle, R. Gumbsheimer, S. Hansmann-Menzemer, F. Jörg, G. Khundzakishvili, A. Kopec, F. Kuger, L. M. Krauss, H. Landsman, R. F. Lang, S. Lindemann, M. Lindner, J. A. M. Lopes, A. Loya Villalpando, C. Macolino, A. Manfredini, T. Marrodán Undagoitia, J. Masbou, E. Masson, P. Meinhardt, S. Milutinovic, A. Molinario, C. M. B. Monteiro, M. Murra, U. G. Oberlack, M. Pandurovic, R. Peres, J. Pienaar, M. Pierre, V. Pizzella, J. Qin, D. Ramírez García, S. Reichard, N. Rupp, P. Sanchez-Lucas, G. Sartorelli, D. Schulte, M. Schumann, L. Scotto Lavina, M. Selvi, M. Silva, H. Simgen, M. Steidl, A. Terliuk, C. Therreau, D. Thers, K. Thieme, R. Trotta, C. D. Tunnell, K. Valerius, G. Volta, D. Vorkapic, C. Weinheimer, C. Wittweg, J. Wolf, J. P. Zopounidis, K. Zuber, DARWIN Collaboration

“…Abstract The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of…”
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Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe by F. Agostini, S. E. M. Ahmed Maouloud, L. Althueser, F. Amaro, B. Antunovic, E. Aprile, L. Baudis, D. Baur, Y. Biondi, A. Bismark, P. A. Breur, A. Brown, G. Bruno, R. Budnik, C. Capelli, J. Cardoso, D. Cichon, M. Clark, A. P. Colijn, J. J. Cuenca-García, J. P. Cussonneau, M. P. Decowski, A. Depoian, J. Dierle, P. Di Gangi, A. Di Giovanni, S. Diglio, J. M. F. dos Santos, G. Drexlin, K. Eitel, R. Engel, A. D. Ferella, H. Fischer, M. Galloway, F. Gao, F. Girard, F. Glück, L. Grandi, R. Größle, R. Gumbsheimer, S. Hansmann-Menzemer, F. Jörg, G. Khundzakishvili, A. Kopec, F. Kuger, L. M. Krauss, H. Landsman, R. F. Lang, S. Lindemann, M. Lindner, J. A. M. Lopes, A. Loya Villalpando, C. Macolino, A. Manfredini, T. Marrodán Undagoitia, J. Masbou, E. Masson, P. Meinhardt, S. Milutinovic, A. Molinario, C. M. B. Monteiro, M. Murra, U. G. Oberlack, M. Pandurovic, R. Peres, J. Pienaar, M. Pierre, V. Pizzella, J. Qin, D. Ramírez García, S. Reichard, N. Rupp, P. Sanchez-Lucas, G. Sartorelli, D. Schulte, M. Schumann, L. Scotto Lavina, M. Selvi, M. Silva, H. Simgen, M. Steidl, A. Terliuk, C. Therreau, D. Thers, K. Thieme, R. Trotta, C. D. Tunnell, K. Valerius, G. Volta, D. Vorkapic, C. Weinheimer, C. Wittweg, J. Wolf, J. P. Zopounidis, K. Zuber, DARWIN Collaboration

“…Abstract We correct an overestimation of the production rate of $$^{137}$$ 137 Xe in the DARWIN detector operated at LNGS. This formerly dominant intrinsic…”
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GPU-based optical simulation of the DARWIN detector by Althueser, L, Antunović, B, Aprile, E, Bajpai, D, Baudis, L, Baur, D, Baxter, A. L, Bellagamba, L, Biondi, R, Biondi, Y, Bismark, A, Brown, A, Budnik, R, Chauvin, A, Colijn, A. P, Cuenca-García, J. J, D'Andrea, V, Di Gangi, P, Dierle, J, Diglio, S, Doerenkamp, M, Eitel, K, Farrell, S, Ferella, A. D, Ferrari, C, Findley, C, Fischer, H, Galloway, M, Girard, F, Glade-Beucke, R, Grandi, L, Guida, M, Hansmann-Menzemer, S, Jörg, F, Jones, L, Kavrigin, P, Krauss, L. M, von Krosigk, B, Kuger, F, Landsman, H, Lang, R. F, Li, S, Liang, S, Lindner, M, Loizeau, J, Lombardi, F, Undagoitia, T. Marrodán, Masbou, J, Masson, E, Matias-Lopes, J, Milutinovic, S, Monteiro, C. M. B, Murra, M, Ni, K, Oberlack, U, Ostrovskiy, I, Pandurovic, M, Peres, R, Qin, J, Silva, M. Rajado, García, D. Ramírez, Sanchez-Lucas, P, Santos, J. M. F. dos, Schumann, M, Selvi, M, Semeria, F, Simgen, H, Steidl, M, Tan, P. -L, Terliuk, A, Thieme, K, Trotta, R, Tunnell, C. D, Tönnies, F, Valerius, K, Vetter, S, Volta, G, Wang, W, Wittweg, C, Xing, Y

“…JINST 17 (2022) P07018 Understanding propagation of scintillation light is critical for maximizing the discovery potential of next-generation liquid xenon…”
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Solar Neutrino Detection Sensitivity in DARWIN via Electron Scattering by Aalbers, J, Alfonsi, M, Althueser, L, Amaro, F, Angevaare, J, Antochi, V. C, Antunovic, B, Aprile, E, Baur, D, Biondi, Y, Bismark, A, Breur, P. A, Brown, A, Brown, E, Colijn, A. P, Conrad, J, Cuenca-García, J. J, Cussonneau, J. P, Decowski, M. P, Depoian, A, Dierle, J, Di Gangi, P, Di Giovanni, A, Engel, R, Erdal, E, Ferella, A. D, Fischer, H, Fischer, P, Fulgione, W, Gaemers, P, Galloway, M, Glade-Beucke, R, Glück, F, Grandi, L, Grohmann, S, Größle, R, Gumbsheimer, R, Hannen, V, Hils, C, Howlett, J, Jörg, F, Kellerer, J, Khundzakishvili, G, Kilminster, B, Kleiner, T. K, Kopec, A, Kopmann, A, Krauss, L. M, Kuger, F, LaCascio, L, Landsman, H, Lindner, M, Lombardi, F, Lopes, J. A. M, Villalpando, A. Loya, Macolino, C, Mahlstedt, J, Undagoitia, T. Marrodán, Masbou, J, Masson, D, McFadden, N, Meinhardt, P, Milosevic, B, Milutinovic, S, Molinario, A, Morteau, E, Murra, M, Newstead, J. L, Ni, K, Ostrovskiy, I, Pandurovic, M, Pelssers, B, Peres, R, Pierre, M, Pizzella, V, Qi, J, Qin, J, Rupp, N, Sanchez-Lucas, P, Santos, J, Sartorelli, G, Schumann, M, Shagin, P, Sharma, S, Shen, W, Stern, S, Subotic, D, Szabo, P, Thers, D, Thieme, K, Tunnell, C. D, Valerius, K, Vorkapic, D, Weber, M, Wenz, D, Wittweg, C, Wolf, J, Wuestling, S, Zopounidis, J. P, Zuber, K

“…We detail the sensitivity of the liquid xenon (LXe) DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the…”
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Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $^{136}$Xe by Agostini, F, Maouloud, S. E. M. Ahmed, Althueser, L, Amaro, F, Antunovic, 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, Di Gangi, P, Di Giovanni, A, 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, Milutinovic, S, Molinario, A, Monteiro, C. M. B, Murra, M, Oberlack, U. G, Pandurovic, M, 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, Vorkapic, D, Weinheimer, C, Wittweg, C, Wolf, J, Zopounidis, J. P, Zuber, K

“…Eur. Phys. J. C 80, 808 (2020) The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless…”
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