Standard

A next-generation liquid xenon observatory for dark matter and neutrino physics. / Aalbers, J.; Abdussalam, S. S.; Abe, K. и др.

в: Journal of Physics G: Nuclear and Particle Physics, Том 50, № 1, 013001, 01.2023.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Aalbers, J, Abdussalam, SS, Abe, K, Aerne, V, Agostini, F, Ahmed Maouloud, S, Akerib, DS, Akimov, DY, Akshat, J, Al Musalhi, AK, Alder, F, Alsum, SK, Althueser, L, Amarasinghe, CS, Amaro, FD, Ames, A, Anderson, TJ, Andrieu, B, Angelides, N, Angelino, E, Angevaare, J, Antochi, VC, Antón Martin, D, Antunovic, B, Aprile, E, Araújo, HM, Armstrong, JE, Arneodo, F, Arthurs, M, Asadi, P, Baek, S, Bai, X, Bajpai, D, Baker, A, Balajthy, J, Balashov, S, Balzer, M, Bandyopadhyay, A, Bang, J, Barberio, E, Bargemann, JW, Baudis, L, Bauer, D, Baur, D, Baxter, A, Baxter, AL, Bazyk, M, Beattie, K, Behrens, J, Bell, NF, Bellagamba, L, Beltrame, P, Benabderrahmane, M, Bernard, EP, Bertone, GF, Bhattacharjee, P, Bhatti, A, Biekert, A, Biesiadzinski, TP, Binau, AR, Biondi, R, Biondi, Y, Birch, HJ, Bishara, F, Bismark, A, Blanco, C, Blockinger, GM, Bodnia, E, Boehm, C, Bolozdynya, AI, Bolton, PD, Bottaro, S, Bourgeois, C, Boxer, B, Brás, P, Breskin, A, Breur, PA, Brew, CAJ, Brod, J, Brookes, E, Brown, A, Brown, E, Bruenner, S, Bruno, G, Budnik, R, Bui, TK, Burdin, S, Buse, S, Busenitz, JK, Buttazzo, D, Buuck, M, Buzulutskov, A, Cabrita, R, Cai, C, Cai, D, Capelli, C, Cardoso, JMR, Carmona-Benitez, MC, Cascella, M, Catena, R, Chakraborty, S, Chan, C, Chang, S, Chauvin, A, Chawla, A, Chen, H, Chepel, V, Chott, NI, Cichon, D, Cimental Chavez, A, Cimmino, B, Clark, M, Co, RT, Colijn, AP, Conrad, J, Converse, MV, Costa, M, Cottle, A, Cox, G, Creaner, O, Cuenca Garcia, JJ, Cussonneau, JP, Cutter, JE, Dahl, CE, D'Andrea, V, David, A, Decowski, MP, Dent, JB, Deppisch, FF, De Viveiros, L, Di Gangi, P, Di Giovanni, A, Di Pede, S, Dierle, J, Diglio, S, Dobson, JEY, Doerenkamp, M, Douillet, D, Drexlin, G, Druszkiewicz, E, Dunsky, D, Eitel, K, Elykov, A, Emken, T, Engel, R, Eriksen, SR, Fairbairn, M, Fan, A, Fan, JJ, Farrell, SJ, Fayer, S, Fearon, NM, Ferella, A, Ferrari, C, Fieguth, A, Fieguth, A, Fiorucci, S, Fischer, H, Flaecher, H, Flierman, M, Florek, T, Foot, R, Fox, PJ, Franceschini, R, Fraser, ED, Frenk, CS, Frohlich, S, Fruth, T, Fulgione, W, Fuselli, C, Gaemers, P, Gaior, R, Gaitskell, RJ, Galloway, M, Gao, F, Garcia Garcia, I, Genovesi, J, Ghag, C, Ghosh, S, Gibson, E, Gil, W, Giovagnoli, D, Girard, F, Glade-Beucke, R, Glück, F, Gokhale, S, De Gouvêa, A, Gráf, L, Grandi, L, Grigat, J, Grinstein, B, Van Der Grinten, MGD, Grössle, R, Guan, H, Guida, M, Gumbsheimer, R, Gwilliam, CB, Hall, CR, Hall, LJ, Hammann, R, Han, K, Hannen, V, Hansmann-Menzemer, S, Harata, R, Hardin, SP, Hardy, E, Hardy, CA, Harigaya, K, Harnik, R, Haselschwardt, SJ, Hernandez, M, Hertel, SA, Higuera, A, Hils, C, Hochrein, S, Hoetzsch, L, Hoferichter, M, Hood, N, Hooper, D, Horn, M, Howlett, J, Huang, DQ, Huang, Y, Hunt, D, Iacovacci, M, Iaquaniello, G, Ide, R, Ignarra, CM, Iloglu, G, Itow, Y, Jacquet, E, Jahangir, O, Jakob, J, James, RS, Jansen, A, Ji, W, Ji, X, Joerg, F, Johnson, J, Joy, A, Kaboth, AC, Kalhor, L, Kamaha, AC, Kanezaki, K, Kar, K, Kara, M, Kato, N, Kavrigin, P, Kazama, S, Keaveney, AW, Kellerer, J, Khaitan, D, Khazov, A, Khundzakishvili, G, Khurana, I, Kilminster, B, Kleifges, M, Ko, P, Kobayashi, M, Kodroff, D, Koltmann, G, Kopec, A, Kopmann, A, Kopp, J, Korley, L, Kornoukhov, VN, Korolkova, EV, Kraus, H, Krauss, LM, Kravitz, S, Kreczko, L, Kudryavtsev, VA, Kuger, F, Kumar, J, López Paredes, B, Lacascio, L, Laha, R, Laine, Q, Landsman, H, Lang, RF, Leason, EA, Lee, J, Leonard, DS, Lesko, KT, Levinson, L, Levy, C, Li, I, Li, SC, Li, T, Liang, S, Liebenthal, CS, Lin, J, Lin, Q, Lindemann, S, Lindner, M, Lindote, A, Linehan, R, Lippincott, WH, Liu, X, Liu, K, Liu, J, Loizeau, J, Lombardi, F, Long, J, Lopes, MI, Lopez Asamar, E, Lorenzon, W, Lu, C, Luitz, S, Ma, Y, Machado, PAN, Macolino, C, Maeda, T, Mahlstedt, J, Majewski, PA, Manalaysay, A, Mancuso, A, Manenti, L, Manfredini, A, Mannino, RL, Marangou, N, March-Russell, J, Marignetti, F, Marrodán Undagoitia, T, Martens, K, Martin, R, Martinez-Soler, I, Masbou, J, Masson, D, Masson, E, Mastroianni, S, Mastronardi, M, Matias-Lopes, JA, McCarthy, ME, McFadden, N, McGinness, E, McKinsey, DN, McLaughlin, J, McMichael, K, Meinhardt, P, Menéndez, J, Meng, Y, Messina, M, Midha, R, Milisavljevic, D, Miller, EH, Milosevic, B, Milutinovic, S, Mitra, SA, Miuchi, K, Mizrachi, E, Mizukoshi, K, Molinario, A, Monte, A, Monteiro, CMB, Monzani, ME, Moore, JS, Morå, K, Morad, JA, Morales Mendoza, JD, Moriyama, S, Morrison, E, Morteau, E, Mosbacher, Y, Mount, BJ, Mueller, J, Murphy, ASJ, Murra, M, Naim, D, Nakamura, S, Nash, E, Navaieelavasani, N, Naylor, A, Nedlik, C, Nelson, HN, Neves, F, Newstead, JL, Ni, K, Nikoleyczik, JA, Niro, V, Oberlack, UG, Obradovic, M, Odgers, K, O'Hare, CAJ, Oikonomou, P, Olcina, I, Oliver-Mallory, K, Oranday, A, Orpwood, J, Ostrovskiy, I, Ozaki, K, Paetsch, B, Pal, S, Palacio, J, Palladino, KJ, Palmer, J, Panci, P, Pandurovic, M, Parlati, A, Parveen, N, Patton, SJ, Pěč, V, Pellegrini, Q, Penning, B, Pereira, G, Peres, R, Perez-Gonzalez, Y, Perry, E, Pershing, T, Petrossian-Byrne, R, Pienaar, J, Piepke, A, Pieramico, G, Pierre, M, Piotter, M, Pizzella, V, Plante, G, Pollmann, T, Porzio, D, Qi, J, Qie, Y, Qin, J, Quevedo, F, Raj, N, Rajado Silva, M, Ramanathan, K, Ramírez García, D, Ravanis, J, Redard-Jacot, L, Redigolo, D, Reichard, S, Reichenbacher, J, Rhyne, CA, Richards, A, Riffard, Q, Rischbieter, GRC, Rocchetti, A, Rosenfeld, SL, Rosero, R, Rupp, N, Rushton, T, Saha, S, Salucci, P, Sanchez, L, Sanchez-Lucas, P, Santone, D, Dos Santos, JMF, Sarnoff, I, Sartorelli, G, Sazzad, ABMR, Scheibelhut, M, Schnee, RW, Schrank, M, Schreiner, J, Schulte, P, Schulte, D, Schulze Eissing, H, Schumann, M, Schwemberger, T, Schwenk, A, Schwetz, T, Scotto Lavina, L, Scovell, PR, Sekiya, H, Selvi, M, Semenov, E, Semeria, F, Shagin, P, Shaw, S, Shi, S, Shockley, E, Shutt, TA, Si-Ahmed, R, Silk, JJ, Silva, C, Silva, MC, Simgen, H, Šimkovic, F, Sinev, G, Singh, R, Skulski, W, Smirnov, J, Smith, R, Solmaz, M, Solovov, VN, Sorensen, P, Soria, J, Sparmann, TJ, Stancu, I, Steidl, M, Stevens, A, Stifter, K, Strigari, LE, Subotic, D, Suerfu, B, Suliga, AM, Sumner, TJ, Szabo, P, Szydagis, M, Takeda, A, Takeuchi, Y, Tan, PL, Taricco, C, Taylor, WC, Temples, DJ, Terliuk, A, Terman, PA, Thers, D, Thieme, K, Thümmler, T, Tiedt, DR, Timalsina, M, To, WH, Toennies, F, Tong, Z, Toschi, F, Tovey, DR, Tranter, J, Trask, M, Trinchero, GC, Tripathi, M, Tronstad, DR, Trotta, R, Tsai, YD, Tunnell, CD, Turner, WG, Ueno, R, Urquijo, P, Utku, U, Vaitkus, A, Valerius, K, Vassilev, E, Vecchi, S, Velan, V, Vetter, S, Vincent, AC, Vittorio, L, Volta, G, Von Krosigk, B, Von Piechowski, M, Vorkapic, D, Wagner, CEM, Wang, AM, Wang, B, Wang, Y, Wang, W, Wang, JJ, Wang, LT, Wang, M, Wang, Y, Watson, JR, Wei, Y, Weinheimer, C, Weisman, E, Weiss, M, Wenz, D, West, SM, Whitis, TJ, Williams, M, Wilson, MJ, Winkler, D, Wittweg, C, Wolf, J, Wolf, T, Wolfs, FLH, Woodford, S, Woodward, D, Wright, CJ, Wu, VHS, Wu, P, Wüstling, S, Wurm, M, Xia, Q, Xiang, X, Xing, Y, Xu, J, Xu, Z, Xu, D, Yamashita, M, Yamazaki, R, Yan, H, Yang, L, Yang, Y, Ye, J, Yeh, M, Young, I, Yu, HB, Yu, TT, Yuan, L, Zavattini, G, Zerbo, S, Zhang, Y, Zhong, M, Zhou, N, Zhou, X, Zhu, T, Zhu, Y, Zhuang, Y, Zopounidis, JP, Zuber, K & Zupan, J 2023, 'A next-generation liquid xenon observatory for dark matter and neutrino physics', Journal of Physics G: Nuclear and Particle Physics, Том. 50, № 1, 013001. https://doi.org/10.1088/1361-6471/ac841a

APA

Aalbers, J., Abdussalam, S. S., Abe, K., Aerne, V., Agostini, F., Ahmed Maouloud, S., Akerib, D. S., Akimov, D. Y., Akshat, J., Al Musalhi, A. K., Alder, F., Alsum, S. K., Althueser, L., Amarasinghe, C. S., Amaro, F. D., Ames, A., Anderson, T. J., Andrieu, B., Angelides, N., ... Zupan, J. (2023). A next-generation liquid xenon observatory for dark matter and neutrino physics. Journal of Physics G: Nuclear and Particle Physics, 50(1), [013001]. https://doi.org/10.1088/1361-6471/ac841a

Vancouver

Aalbers J, Abdussalam SS, Abe K, Aerne V, Agostini F, Ahmed Maouloud S и др. A next-generation liquid xenon observatory for dark matter and neutrino physics. Journal of Physics G: Nuclear and Particle Physics. 2023 янв.;50(1):013001. doi: 10.1088/1361-6471/ac841a

Author

Aalbers, J. ; Abdussalam, S. S. ; Abe, K. и др. / A next-generation liquid xenon observatory for dark matter and neutrino physics. в: Journal of Physics G: Nuclear and Particle Physics. 2023 ; Том 50, № 1.

BibTeX

@article{c53c42ea784d4ba0aa1ca187e1cc277c,
title = "A next-generation liquid xenon observatory for dark matter and neutrino physics",
abstract = "The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.",
keywords = "astroparticle physics, dark matter, direct detection, neutrinoless double-beta decay, neutrinos, supernova, xenon",
author = "J. Aalbers and Abdussalam, {S. S.} and K. Abe and V. Aerne and F. Agostini and {Ahmed Maouloud}, S. and Akerib, {D. S.} and Akimov, {D. Y.} and J. Akshat and {Al Musalhi}, {A. K.} and F. Alder and Alsum, {S. K.} and L. Althueser and Amarasinghe, {C. S.} and Amaro, {F. D.} and A. Ames and Anderson, {T. J.} and B. Andrieu and N. Angelides and E. Angelino and J. Angevaare and Antochi, {V. C.} and {Ant{\'o}n Martin}, D. and B. Antunovic and E. Aprile and Ara{\'u}jo, {H. M.} and Armstrong, {J. E.} and F. Arneodo and M. Arthurs and P. Asadi and S. Baek and X. Bai and D. Bajpai and A. Baker and J. Balajthy and S. Balashov and M. Balzer and A. Bandyopadhyay and J. Bang and E. Barberio and Bargemann, {J. W.} and L. Baudis and D. Bauer and D. Baur and A. Baxter and Baxter, {A. L.} and M. Bazyk and K. Beattie and J. Behrens and Bell, {N. F.} and L. Bellagamba and P. Beltrame and M. Benabderrahmane and Bernard, {E. P.} and Bertone, {G. F.} and P. Bhattacharjee and A. Bhatti and A. Biekert and Biesiadzinski, {T. P.} and Binau, {A. R.} and R. Biondi and Y. Biondi and Birch, {H. J.} and F. Bishara and A. Bismark and C. Blanco and Blockinger, {G. M.} and E. Bodnia and C. Boehm and Bolozdynya, {A. I.} and Bolton, {P. D.} and S. Bottaro and C. Bourgeois and B. Boxer and P. Br{\'a}s and A. Breskin and Breur, {P. A.} and Brew, {C. A.J.} and J. Brod and E. Brookes and A. Brown and E. Brown and S. Bruenner and G. Bruno and R. Budnik and Bui, {T. K.} and S. Burdin and S. Buse and Busenitz, {J. K.} and D. Buttazzo and M. Buuck and A. Buzulutskov and R. Cabrita and C. Cai and D. Cai and C. Capelli and Cardoso, {J. M.R.} and Carmona-Benitez, {M. C.} and M. Cascella and R. Catena and S. Chakraborty and C. Chan and S. Chang and A. Chauvin and A. Chawla and H. Chen and V. Chepel and Chott, {N. I.} and D. Cichon and {Cimental Chavez}, A. and B. Cimmino and M. Clark and Co, {R. T.} and Colijn, {A. P.} and J. Conrad and Converse, {M. V.} and M. Costa and A. Cottle and G. Cox and O. Creaner and {Cuenca Garcia}, {J. J.} and Cussonneau, {J. P.} and Cutter, {J. E.} and Dahl, {C. E.} and V. D'Andrea and A. David and Decowski, {M. P.} and Dent, {J. B.} and Deppisch, {F. F.} and {De Viveiros}, L. and {Di Gangi}, P. and {Di Giovanni}, A. and {Di Pede}, S. and J. Dierle and S. Diglio and Dobson, {J. E.Y.} and M. Doerenkamp and D. Douillet and G. Drexlin and E. Druszkiewicz and D. Dunsky and K. Eitel and A. Elykov and T. Emken and R. Engel and Eriksen, {S. R.} and M. Fairbairn and A. Fan and Fan, {J. J.} and Farrell, {S. J.} and S. Fayer and Fearon, {N. M.} and A. Ferella and C. Ferrari and A. Fieguth and A. Fieguth and S. Fiorucci and H. Fischer and H. Flaecher and M. Flierman and T. Florek and R. Foot and Fox, {P. J.} and R. Franceschini and Fraser, {E. D.} and Frenk, {C. S.} and S. Frohlich and T. Fruth and W. Fulgione and C. Fuselli and P. Gaemers and R. Gaior and Gaitskell, {R. J.} and M. Galloway and F. Gao and {Garcia Garcia}, I. and J. Genovesi and C. Ghag and S. Ghosh and E. Gibson and W. Gil and D. Giovagnoli and F. Girard and R. Glade-Beucke and F. Gl{\"u}ck and S. Gokhale and {De Gouv{\^e}a}, A. and L. Gr{\'a}f and L. Grandi and J. Grigat and B. Grinstein and {Van Der Grinten}, {M. G.D.} and R. Gr{\"o}ssle and H. Guan and M. Guida and R. Gumbsheimer and Gwilliam, {C. B.} and Hall, {C. R.} and Hall, {L. J.} and R. Hammann and K. Han and V. Hannen and S. Hansmann-Menzemer and R. Harata and Hardin, {S. P.} and E. Hardy and Hardy, {C. A.} and K. Harigaya and R. Harnik and Haselschwardt, {S. J.} and M. Hernandez and Hertel, {S. A.} and A. Higuera and C. Hils and S. Hochrein and L. Hoetzsch and M. Hoferichter and N. Hood and D. Hooper and M. Horn and J. Howlett and Huang, {D. Q.} and Y. Huang and D. Hunt and M. Iacovacci and G. Iaquaniello and R. Ide and Ignarra, {C. M.} and G. Iloglu and Y. Itow and E. Jacquet and O. Jahangir and J. Jakob and James, {R. S.} and A. Jansen and W. Ji and X. Ji and F. Joerg and J. Johnson and A. Joy and Kaboth, {A. C.} and L. Kalhor and Kamaha, {A. C.} and K. Kanezaki and K. Kar and M. Kara and N. Kato and P. Kavrigin and S. Kazama and Keaveney, {A. W.} and J. Kellerer and D. Khaitan and A. Khazov and G. Khundzakishvili and I. Khurana and B. Kilminster and M. Kleifges and P. Ko and M. Kobayashi and D. Kodroff and G. Koltmann and A. Kopec and A. Kopmann and J. Kopp and L. Korley and Kornoukhov, {V. N.} and Korolkova, {E. V.} and H. Kraus and Krauss, {L. M.} and S. Kravitz and L. Kreczko and Kudryavtsev, {V. A.} and F. Kuger and J. Kumar and {L{\'o}pez Paredes}, B. and L. Lacascio and R. Laha and Q. Laine and H. Landsman and Lang, {R. F.} and Leason, {E. A.} and J. Lee and Leonard, {D. S.} and Lesko, {K. T.} and L. Levinson and C. Levy and I. Li and Li, {S. C.} and T. Li and S. Liang and Liebenthal, {C. S.} and J. Lin and Q. Lin and S. Lindemann and M. Lindner and A. Lindote and R. Linehan and Lippincott, {W. H.} and X. Liu and K. Liu and J. Liu and J. Loizeau and F. Lombardi and J. Long and Lopes, {M. I.} and {Lopez Asamar}, E. and W. Lorenzon and C. Lu and S. Luitz and Y. Ma and Machado, {P. A.N.} and C. Macolino and T. Maeda and J. Mahlstedt and Majewski, {P. A.} and A. Manalaysay and A. Mancuso and L. Manenti and A. Manfredini and Mannino, {R. L.} and N. Marangou and J. March-Russell and F. Marignetti and {Marrod{\'a}n Undagoitia}, T. and K. Martens and R. Martin and I. Martinez-Soler and J. Masbou and D. Masson and E. Masson and S. Mastroianni and M. Mastronardi and Matias-Lopes, {J. A.} and McCarthy, {M. E.} and N. McFadden and E. McGinness and McKinsey, {D. N.} and J. McLaughlin and K. McMichael and P. Meinhardt and J. Men{\'e}ndez and Y. Meng and M. Messina and R. Midha and D. Milisavljevic and Miller, {E. H.} and B. Milosevic and S. Milutinovic and Mitra, {S. A.} and K. Miuchi and E. Mizrachi and K. Mizukoshi and A. Molinario and A. Monte and Monteiro, {C. M.B.} and Monzani, {M. E.} and Moore, {J. S.} and K. Mor{\aa} and Morad, {J. A.} and {Morales Mendoza}, {J. D.} and S. Moriyama and E. Morrison and E. Morteau and Y. Mosbacher and Mount, {B. J.} and J. Mueller and Murphy, {A. St J.} and M. Murra and D. Naim and S. Nakamura and E. Nash and N. Navaieelavasani and A. Naylor and C. Nedlik and Nelson, {H. N.} and F. Neves and Newstead, {J. L.} and K. Ni and Nikoleyczik, {J. A.} and V. Niro and Oberlack, {U. G.} and M. Obradovic and K. Odgers and O'Hare, {C. A.J.} and P. Oikonomou and I. Olcina and K. Oliver-Mallory and A. Oranday and J. Orpwood and I. Ostrovskiy and K. Ozaki and B. Paetsch and S. Pal and J. Palacio and Palladino, {K. J.} and J. Palmer and P. Panci and M. Pandurovic and A. Parlati and N. Parveen and Patton, {S. J.} and V. P{\v e}{\v c} and Q. Pellegrini and B. Penning and G. Pereira and R. Peres and Y. Perez-Gonzalez and E. Perry and T. Pershing and R. Petrossian-Byrne and J. Pienaar and A. Piepke and G. Pieramico and M. Pierre and M. Piotter and V. Pizzella and G. Plante and T. Pollmann and D. Porzio and J. Qi and Y. Qie and J. Qin and F. Quevedo and N. Raj and {Rajado Silva}, M. and K. Ramanathan and {Ram{\'i}rez Garc{\'i}a}, D. and J. Ravanis and L. Redard-Jacot and D. Redigolo and S. Reichard and J. Reichenbacher and Rhyne, {C. A.} and A. Richards and Q. Riffard and Rischbieter, {G. R.C.} and A. Rocchetti and Rosenfeld, {S. L.} and R. Rosero and N. Rupp and T. Rushton and S. Saha and P. Salucci and L. Sanchez and P. Sanchez-Lucas and D. Santone and {Dos Santos}, {J. M.F.} and I. Sarnoff and G. Sartorelli and Sazzad, {A. B.M.R.} and M. Scheibelhut and Schnee, {R. W.} and M. Schrank and J. Schreiner and P. Schulte and D. Schulte and {Schulze Eissing}, H. and M. Schumann and T. Schwemberger and A. Schwenk and T. Schwetz and {Scotto Lavina}, L. and Scovell, {P. R.} and H. Sekiya and M. Selvi and E. Semenov and F. Semeria and P. Shagin and S. Shaw and S. Shi and E. Shockley and Shutt, {T. A.} and R. Si-Ahmed and Silk, {J. J.} and C. Silva and Silva, {M. C.} and H. Simgen and F. {\v S}imkovic and G. Sinev and R. Singh and W. Skulski and J. Smirnov and R. Smith and M. Solmaz and Solovov, {V. N.} and P. Sorensen and J. Soria and Sparmann, {T. J.} and I. Stancu and M. Steidl and A. Stevens and K. Stifter and Strigari, {L. E.} and D. Subotic and B. Suerfu and Suliga, {A. M.} and Sumner, {T. J.} and P. Szabo and M. Szydagis and A. Takeda and Y. Takeuchi and Tan, {P. L.} and C. Taricco and Taylor, {W. C.} and Temples, {D. J.} and A. Terliuk and Terman, {P. A.} and D. Thers and K. Thieme and T. Th{\"u}mmler and Tiedt, {D. R.} and M. Timalsina and To, {W. H.} and F. Toennies and Z. Tong and F. Toschi and Tovey, {D. R.} and J. Tranter and M. Trask and Trinchero, {G. C.} and M. Tripathi and Tronstad, {D. R.} and R. Trotta and Tsai, {Y. D.} and Tunnell, {C. D.} and Turner, {W. G.} and R. Ueno and P. Urquijo and U. Utku and A. Vaitkus and K. Valerius and E. Vassilev and S. Vecchi and V. Velan and S. Vetter and Vincent, {A. C.} and L. Vittorio and G. Volta and {Von Krosigk}, B. and {Von Piechowski}, M. and D. Vorkapic and Wagner, {C. E.M.} and Wang, {A. M.} and B. Wang and Y. Wang and W. Wang and Wang, {J. J.} and Wang, {L. T.} and M. Wang and Y. Wang and Watson, {J. R.} and Y. Wei and C. Weinheimer and E. Weisman and M. Weiss and D. Wenz and West, {S. M.} and Whitis, {T. J.} and M. Williams and Wilson, {M. J.} and D. Winkler and C. Wittweg and J. Wolf and T. Wolf and Wolfs, {F. L.H.} and S. Woodford and D. Woodward and Wright, {C. J.} and Wu, {V. H.S.} and P. Wu and S. W{\"u}stling and M. Wurm and Q. Xia and X. Xiang and Y. Xing and J. Xu and Z. Xu and D. Xu and M. Yamashita and R. Yamazaki and H. Yan and L. Yang and Y. Yang and J. Ye and M. Yeh and I. Young and Yu, {H. B.} and Yu, {T. T.} and L. Yuan and G. Zavattini and S. Zerbo and Y. Zhang and M. Zhong and N. Zhou and X. Zhou and T. Zhu and Y. Zhu and Y. Zhuang and Zopounidis, {J. P.} and K. Zuber and J. Zupan",
note = "This work has been supported by the US National Science Foundation (NSF, Grants PHYS-1719271, PHYS-2112796, PHYS-2112801, PHYS-2112802, PHYS-2112803, PHYS-2112851, PHYS-2137911); by the Department of Energy (DOE), Office of Science (Grants DE-AC02-05CH11231, DE-AC02-07CH11359, DE-AC02-76SF00515, DE-AC52-07NA27344, DE-FG02-00ER41132, DE-FG02-10ER46709, DE-NA0003180, DE-SC0006605, DE-SC0008475, DE-SC0009999, DE-SC0010010, DE-SC0010072, DE-SC0010813, DE-SC0011640, DE-SC0011702, DE-SC0012161, DOE-SC0012447, DE-SC0012704, DE-SC0013542, DE-SC0014223, DE-SC0015535, DE-SC0015708, DE-SC0018982, DE-SC0019066, DE-SC0020216, UW PRJ82AJ); by the UK Science & Technology Facilities Council (Grants ST/M003655/1, ST/M003981/1, ST/M003744/1, ST/M003639/1, ST/M003604/1, ST/R003181/1, ST/M003469/1); by the German Research Foundation (DFG) [Grants KO 4820/4-1, EXC-2118, 279384907 (SFB 1245)]; by the Max Planck Gesellschaft; by the Dutch Research Council (NWO); by the Swiss National Science Foundation (Grants PCEFP2_181117, 200020-188716); by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Grants 742789, 101020842); by the Portuguese Foundation for Science and Technology (FCT) (Grants PTDC/FIS-PAR/28567/2017); by the Institute for Basic Science, Korea (Grant IBS-R016-D1); by the Australian Research Council through the ARC Center of Excellence for Dark Matter Particle Physics, CE200100008; and by the Marie Skodowska-Curie Grant Agreement No. 860881. BvK acknowledges support from Emmy Noether Grant No. 420484612; AM et al acknowledge additional support from the STFC Boulby Underground Laboratory in the UK, the GridPP [1317, 1318] and IRIS Collaborations, in particular at Imperial College London and additional support by the University College London (UCL) Cosmoparticle Initiative. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. The University of Edinburgh is a charitable body, registered in Scotland, with the registration number SC005336. PK and SB from the National Research Foundation of Korea (NRF) Grants NRF-2018R1A2A3075605 and NRF-2019R1A2C3005009 and by KIAS Individual Grant No. PG021403; RC from an individual research grant from the Swedish Research Council (Dnr 2018-05029); RC and TE from the Knut and Alice Wallenberg project Light Dark Matter (Dnr KAW 2019.0080 and 2019.0080); PB and SS from the Dr Raja Ramanna Fellowship program of the Department of Atomic Energy (DAE), Government of India. RB acknowledges ISF and the Pazy foundation. Finally, RFL acknowledges support from the Purdue University Department of Physics and Astronomy and from the Purdue Research Foundation without which this paper could not have been realized.",
year = "2023",
month = jan,
doi = "10.1088/1361-6471/ac841a",
language = "English",
volume = "50",
journal = "Journal of Physics G: Nuclear and Particle Physics",
issn = "0954-3899",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - A next-generation liquid xenon observatory for dark matter and neutrino physics

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AU - Zuber, K.

AU - Zupan, J.

N1 - This work has been supported by the US National Science Foundation (NSF, Grants PHYS-1719271, PHYS-2112796, PHYS-2112801, PHYS-2112802, PHYS-2112803, PHYS-2112851, PHYS-2137911); by the Department of Energy (DOE), Office of Science (Grants DE-AC02-05CH11231, DE-AC02-07CH11359, DE-AC02-76SF00515, DE-AC52-07NA27344, DE-FG02-00ER41132, DE-FG02-10ER46709, DE-NA0003180, DE-SC0006605, DE-SC0008475, DE-SC0009999, DE-SC0010010, DE-SC0010072, DE-SC0010813, DE-SC0011640, DE-SC0011702, DE-SC0012161, DOE-SC0012447, DE-SC0012704, DE-SC0013542, DE-SC0014223, DE-SC0015535, DE-SC0015708, DE-SC0018982, DE-SC0019066, DE-SC0020216, UW PRJ82AJ); by the UK Science & Technology Facilities Council (Grants ST/M003655/1, ST/M003981/1, ST/M003744/1, ST/M003639/1, ST/M003604/1, ST/R003181/1, ST/M003469/1); by the German Research Foundation (DFG) [Grants KO 4820/4-1, EXC-2118, 279384907 (SFB 1245)]; by the Max Planck Gesellschaft; by the Dutch Research Council (NWO); by the Swiss National Science Foundation (Grants PCEFP2_181117, 200020-188716); by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Grants 742789, 101020842); by the Portuguese Foundation for Science and Technology (FCT) (Grants PTDC/FIS-PAR/28567/2017); by the Institute for Basic Science, Korea (Grant IBS-R016-D1); by the Australian Research Council through the ARC Center of Excellence for Dark Matter Particle Physics, CE200100008; and by the Marie Skodowska-Curie Grant Agreement No. 860881. BvK acknowledges support from Emmy Noether Grant No. 420484612; AM et al acknowledge additional support from the STFC Boulby Underground Laboratory in the UK, the GridPP [1317, 1318] and IRIS Collaborations, in particular at Imperial College London and additional support by the University College London (UCL) Cosmoparticle Initiative. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. The University of Edinburgh is a charitable body, registered in Scotland, with the registration number SC005336. PK and SB from the National Research Foundation of Korea (NRF) Grants NRF-2018R1A2A3075605 and NRF-2019R1A2C3005009 and by KIAS Individual Grant No. PG021403; RC from an individual research grant from the Swedish Research Council (Dnr 2018-05029); RC and TE from the Knut and Alice Wallenberg project Light Dark Matter (Dnr KAW 2019.0080 and 2019.0080); PB and SS from the Dr Raja Ramanna Fellowship program of the Department of Atomic Energy (DAE), Government of India. RB acknowledges ISF and the Pazy foundation. Finally, RFL acknowledges support from the Purdue University Department of Physics and Astronomy and from the Purdue Research Foundation without which this paper could not have been realized.

PY - 2023/1

Y1 - 2023/1

N2 - The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.

AB - The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.

KW - astroparticle physics

KW - dark matter

KW - direct detection

KW - neutrinoless double-beta decay

KW - neutrinos

KW - supernova

KW - xenon

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85145605367&origin=inward&txGid=cda74f6d527a297395f04691f83e8e67

UR - https://www.mendeley.com/catalogue/f5910c8e-d870-3562-bd88-05f222315d35/

U2 - 10.1088/1361-6471/ac841a

DO - 10.1088/1361-6471/ac841a

M3 - Article

VL - 50

JO - Journal of Physics G: Nuclear and Particle Physics

JF - Journal of Physics G: Nuclear and Particle Physics

SN - 0954-3899

IS - 1

M1 - 013001

ER -

ID: 56497912