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

Author:

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,Angelino E,Angevaare J,Antochi V C,Antón Martin D,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,Cimental Chavez A,Cimmino B,Clark M,Co R T,Colijn A P,Conrad J,Converse M V,Costa M,Cottle A,Cox G,Creaner O,Cuenca Garcia J J,Cussonneau J P,Cutter J E,Dahl C E,D’Andrea V,David A,Decowski M P,Dent J B,Deppisch F F,de Viveiros L,Di Gangi P,Di Giovanni A,Di Pede S,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 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 M G D,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,López Paredes B,LaCascio L,Laha R,Laine Q,Landsman H,Lang R FORCID,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,Lopez Asamar E,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,Marrodán Undagoitia T,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,Morales Mendoza J D,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,Rajado Silva M,Ramanathan K,Ramírez García D,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,dos Santos J M F,Sarnoff I,Sartorelli G,Sazzad A B M R,Scheibelhut M,Schnee R W,Schrank M,Schreiner J,Schulte P,Schulte D,Schulze Eissing H,Schumann M,Schwemberger T,Schwenk A,Schwetz T,Scotto Lavina L,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,von Krosigk B,von Piechowski M,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

Abstract

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.

Funder

Division of Physics

Science and Technology Facilities Council

Publisher

IOP Publishing

Subject

Nuclear and High Energy Physics

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