Browsing by Author "Liu, K."

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    A next-generation liquid xenon observatory for dark matter and neutrino physics
    (IOP Publishing, 2022) Aalbers, J.; AbdusSalam, S.S.; Abe, K.; Aerne, V.; Agostini, F.; Maouloud, S. Ahmed; Akerib, D.S.; Akimov, D.Y.; Akshat, J.; Musalhi, A.K. Al; Alder, F.; Alsum, S.K.; Althueser, L.; Amarasinghe, C.S.; Amaro, F.D.; Ames, A.; Anderson, T.J.; Andrieu, B.; Angelides, N.; Angelino, E.; Angevaare, J.; Antochi, V.C.; Martin, D. Antón; Antunovic, B.; Aprile, E.; Araújo, H.M.; Armstrong, J.E.; 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, J.W.; Baudis, L.; Bauer, D.; Baur, D.; Baxter, A.; Baxter, A.L.; Bazyk, M.; Beattie, K.; Behrens, J.; Bell, N.F.; Bellagamba, L.; Beltrame, P.; Benabderrahmane, M.; Bernard, E.P.; Bertone, G.F.; Bhattacharjee, P.; Bhatti, A.; Biekert, A.; Biesiadzinski, T.P.; Binau, A.R.; Biondi, R.; Biondi, Y.; Birch, H.J.; Bishara, F.; Bismark, A.; Blanco, C.; Blockinger, G.M.; Bodnia, E.; Boehm, C.; Bolozdynya, A.I.; Bolton, P.D.; Bottaro, S.; Bourgeois, C.; Boxer, B.; Brás, P.; Breskin, A.; Breur, P. A.; Brew, C.A.J.; Brod, J.; Brookes, E.; Brown, A.; Brown, E.; Bruenner, S.; Bruno, G.; Budnik, R.; Bui, T.K.; Burdin, S.; Buse, S.; Busenitz, J.K.; Buttazzo, D.; Buuck, M.; Buzulutskov, A.; Cabrita, R.; Cai, C.; Cai, D.; Capelli, C.; Cardoso, J.M.R.; Carmona-Benitez, M.C.; Cascella, M.; Catena, R.; Chakraborty, S.; Chan, C.; Chang, S.; Chauvin, A.; Chawla, A.; Chen, H.; Chepel, V.; Chott, N.I.; Cichon, D.; Chavez, A. Cimental; Cimmino, B.; Clark, M.; Co, R.T.; Colijn, A.P.; Conrad, J.; Converse, M.V.; Costa, M.; Cottle, A.; Cox, G.; Creaner, O.; Garcia, J.J. Cuenca; Cussonneau, J.P.; Cutter, J.E.; Dahl, C.E.; D’Andrea, V.; David, A.; Decowski, M.P.; Dent, J.B.; Deppisch, F.F.; Viveiros, L. de; Gangi, P. Di; Giovanni, A. Di; Pede, S. Di; Dierle, J.; Diglio, S.; Dobson, J.E.Y.; Doerenkamp, M.; Douillet, D.; Drexlin, G.; Druszkiewicz, E.; Dunsky, D.; Eitel, K.; Elykov, A.; Emken, T.; Engel, R.; Eriksen, S.R.; Fairbairn, M.; Fan, A.; Fan, J.J.; Farrell, S.J.; Fayer, S.; Fearon, N.M.; Ferella, A.; Ferrari, C.; Fieguth, A.; Fieguth, A.; Fiorucci, S.; Fischer, H.; Flaecher, H.; Flierman, M.; Florek, T.; Foot, R.; Fox, P.J.; Franceschini, R.; Fraser, E.D.; Frenk, C.S.; Frohlich, S.; Fruth, T.; Fulgione, W.; Fuselli, C.; Gaemers, P.; Gaior, R.; Gaitskell, R.J.; Galloway, M.; Gao, F.; Garcia, I. Garcia; Genovesi, J.; Ghag, C.; Ghosh, S.; Gibson, E.; Gil, W.; Giovagnoli, D.; Girard, F.; Glade-Beucke, R.; Glück, F.; Gokhale, S.; Gouvêa, A. de; Gráf, L.; Grandi, L.; Grigat, J.; Grinstein, B.; Grinten, M.G.D. van der; Grössle, R.; Guan, H.; Guida, M.; Gumbsheimer, R.; Gwilliam, C. B.; Hall, C.R.; Hall, L.J.; Hammann, R.; Han, K.; Hannen, V.; Hansmann-Menzemer, S.; Harata, R.; Hardin, S.P.; Hardy, E.; Hardy, C.A.; Harigaya, K.; Harnik, R.; Haselschwardt, S.J.; Hernandez, M.; Hertel, S.A.; Higuera, A.; Hils, C.; Hochrein, S.; Hoetzsch, L.; Hoferichter, M.; Hood, N.; Hooper, D.; Horn, M.; Howlett, J.; Huang, D.Q.; Huang, Y.; Hunt, D.; Iacovacci, M.; Iaquaniello, G.; Ide, R.; Ignarra, C.M.; Iloglu, G.; Itow, Y.; Jacquet, E.; Jahangir, O.; Jakob, J.; James, R.S.; Jansen, A.; Ji, W.; Ji, X.; Joerg, F.; Johnson, J.; Joy, A.; Kaboth, A.C.; Kalhor, L.; Kamaha, A.C.; Kanezaki, K.; Kar, K.; Kara, M.; Kato, N.; Kavrigin, P.; Kazama, S.; Keaveney, A.W.; 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, V.N.; Korolkova, E.V.; Kraus, H.; Krauss, L.M.; Kravitz, S.; Kreczko, L.; Kudryavtsev, V.A.; Kuger, F.; Kumar, J.; Paredes, B. López; LaCascio, L.; Laha, R.; Laine, Q.; Landsman, H.; Lang, R.F.; Leason, E.A.; Lee, J.; Leonard, D.S.; Lesko, K.T.; Levinson, L.; Levy, C.; Li, I.; Li, S.C.; Li, T.; Liang, S.; Liebenthal, C.S.; Lin, J.; Lin, Q.; Lindemann, S.; Lindner, M.; Lindote, A.; Linehan, R.; Lippincott, W.H.; Liu, X.; Liu, K.; Liu, J.; Loizeau, J.; Lombardi, F.; Long, J.; Lopes, M.I.; Asamar, E. Lopez; Lorenzon, W.; Lu, C.; Luitz, S.; Ma, Y.; Machado, P.A.N.; Macolino, C.; Maeda, T.; Mahlstedt, J.; Majewski, P.A.; Manalaysay, A.; Mancuso, A.; Manenti, L.; Manfredini, A.; Mannino, R.L.; Marangou, N.; March-Russell, J.; Marignetti, F.; Undagoitia, T. Marrodán; Martens, K.; Martin, R.; Martinez-Soler, I.; Masbou, J.; Masson, D.; Masson, E.; Mastroianni, S.; Mastronardi, M.; Matias-Lopes, J.A.; McCarthy, M.E.; McFadden, N.; McGinness, E.; McKinsey, D.N.; McLaughlin, J.; McMichael, K.; Meinhardt, P.; Menéndez, J.; Meng, Y.; Messina, M.; Midha, R.; Milisavljevic, D.; Miller, E.H.; Milosevic, B.; Milutinovic, S.; Mitra, S.A.; Miuchi, K.; Mizrachi, E.; Mizukoshi, K.; Molinario, A.; Monte, A.; Monteiro, C.M.B.; Monzani, M.E.; Moore, J.S.; Morå, K.; Morad, J.A.; Mendoza, J.D. Morales; Moriyama, S.; Morrison, E.; Morteau, E.; Mosbacher, Y.; Mount, B.J.; Mueller, J.; Murphy, A. St J.; Murra, M.; Naim, D.; Nakamura, S.; Nash, E.; Navaieelavasani, N.; Naylor, A.; Nedlik, C.; Nelson, H.N.; Neves, F.; Newstead, J.L.; Ni, K.; Nikoleyczik, J.A.; Niro, V.; Oberlack, U.G.; Obradovic, M.; Odgers, K.; O’Hare, C.A.J.; Oikonomou, P.; Olcina, I.; Oliver-Mallory, K.; Oranday, A.; Orpwood, J.; Ostrovskiy, I.; Ozaki, K.; Paetsch, B.; Pal, S.; Palacio, J.; Palladino, K.J.; Palmer, J.; Panci, P.; Pandurovic, M.; Parlati, A.; Parveen, N.; Patton, S.J.; 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.; Silva, M. Rajado; Ramanathan, K.; García, D. Ramírez; Ravanis, J.; Redard-Jacot, L.; Redigolo, D.; Reichard, S.; Reichenbacher, J.; Rhyne, C.A.; Richards, A.; Riffard, Q.; Rischbieter, G.R.C.; Rocchetti, A.; Rosenfeld, S. L.; Rosero, R.; Rupp, N.; Rushton, T.; Saha, S.; Salucci, P.; Sanchez, L.; Sanchez-Lucas, P.; Santone, D.; Santos, J.M.F. dos; Sarnoff, I.; Sartorelli, G.; Sazzad, A.B.M.R.; Scheibelhut, M.; Schnee, R.W.; Schrank, M.; Schreiner, J.; Schulte, P.; Schulte, D.; Eissing, H. Schulze; Schumann, M.; Schwemberger, T.; Schwenk, A.; Schwetz, T.; Lavina, L. Scotto; Scovell, P.R.; Sekiya, H.; Selvi, M.; Semenov, E.; Semeria, F.; Shagin, P.; Shaw, S.; Shi, S.; Shockley, E.; Shutt, T.A.; Si-Ahmed, R.; Silk, J.J.; Silva, C.; Silva, M.C.; Simgen, H.; Šimkovic, F.; Sinev, G.; Singh, R.; Skulski, W.; Smirnov, J.; Smith, R.; Solmaz, M.; Solovov, V.N.; Sorensen, P.; Soria, J.; Sparmann, T.J.; Stancu, I.; Steidl, M.; Stevens, A.; Stifter, K.; Strigari, L.E.; Subotic, D.; Suerfu, B.; Suliga, A.M.; Sumner, T.J.; Szabo, P.; Szydagis, M.; Takeda, A.; Takeuchi, Y.; Tan, P.-L.; Taricco, C.; Taylor, W.C.; Temples, D.J.; Terliuk, A.; Terman, P.A.; Thers, D.; Thieme, K.; Thümmler, T.; Tiedt, D.R.; Timalsina, M.; To, W.H.; Toennies, F.; Tong, Z.; Toschi, F.; Tovey, D.R.; Tranter, J.; Trask, M.; Trinchero, G.C.; Tripathi, M.; Tronstad, D.R.; Trotta, R.; Tsai, Y.D.; Tunnell, C.D.; Turner, W.G.; Ueno, R.; Urquijo, P.; Utku, U.; Vaitkus, A.; Valerius, K.; Vassilev, E.; Vecchi, S.; Velan, V.; Vetter, S.; Vincent, A.C.; Vittorio, L.; Volta, G.; Krosigk, B. von; Piechowski, M. von; Vorkapic, D.; Wagner, C.E.M.; Wang, A.M.; Wang, B.; Wang, Y.; Wang, W.; Wang, J.J.; Wang, L.-T.; Wang, M.; Wang, Y.; Watson, J.R.; Wei, Y.; Weinheimer, C.; Weisman, E.; Weiss, M.; Wenz, D.; West, S.M.; Whitis, T.J.; Williams, M.; Wilson, M.J.; Winkler, D.; Wittweg, C.; Wolf, J.; Wolf, T.; Wolfs, F.L.H.; Woodford, S.; Woodward, D.; Wright, C.J.; Wu, V.H.S.; 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, H.B.; Yu, T.T.; Yuan, L.; Zavattini, G.; Zerbo, S.; Zhang, Y.; Zhong, M.; Zhou, N.; Zhou, X.; Zhu, T.; Zhu, Y.; Zhuang, Y.; Zopounidis, J.P.; Zuber, K.; Zupan, J.
    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.
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    Finite-frequency Rayleigh wave tomography of the western Mediterranean: Mapping its lithospheric structure
    (American Geophysical Union, 2014) Palomeras, I.; Thurner, S.; Levander, A.; Liu, K.; Villasenor, A.; Carbonell, R.; Harnafi, M.
    [1] We present a 3-D P wave velocity model of the crust and shallowest mantle under the Italian region, that includes a revised Moho depth map, obtained by regional seismic travel time tomography. We invert 191,850 Pn and Pg wave arrival times from 6850 earthquakes that occurred within the region from 1988 to 2007, recorded by 264 permanent seismic stations. We adopt a high-resolution linear B-spline model representation, with 0.1° horizontal and 2 km vertical grid spacing, and an accurate finite-difference forward calculation scheme. Our nonlinear iterative inversion process uses the recent European reference 3-D crustal model EPcrust as a priori information. Our resulting model shows two arcs of relatively low velocity in the crust running along both the Alps and the Apennines, underlying the collision belts between plates. Beneath the Western Alps we detect the presence of the Ivrea body, denoted by a strong high P wave velocity anomaly. We also map the Moho discontinuity resulting from the inversion, imaged as the relatively sharp transition between crust and mantle, where P wave velocity steps up to values larger than 8 km/s. This simple condition yields an image quite in agreement with previous studies that use explicit representations for the discontinuity. We find a complex lithospheric structure characterized by shallower Moho close by the Tyrrhenian Sea, intermediate depth along the Adriatic coast, and deepest Moho under the two mountain belts.