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

Aalbers, J and Abdussalam, SS and Abe, K and Aerne, V and Agostini, F and Ahmed Maouloud, S and Akerib, DS and Akimov, DY and Akshat, J and Al Musalhi, AK and Alder, F and Alsum, SK and Althueser, L and Amarasinghe, CS and Amaro, FD and Ames, A and Anderson, TJ and Andrieu, B and Angelides, N and Angelino, E and Angevaare, J and Antochi, VC and Antón Martin, D and Antunovic, B and Aprile, E and Araújo, HM and Armstrong, JE and Arneodo, F and Arthurs, M and Asadi, P and Baek, S and Bai, X and Bajpai, D and Baker, A and Balajthy, J and Balashov, S and Balzer, M and Bandyopadhyay, A and Bang, J and Barberio, E and Bargemann, JW and Baudis, L and Bauer, D and Baur, D and Baxter, A and Baxter, AL and Bazyk, M and Beattie, K and Behrens, J and Bell, NF and Bellagamba, L and Beltrame, P and Benabderrahmane, M and Bernard, EP and Bertone, GF and Bhattacharjee, P and Bhatti, A and Biekert, A and Biesiadzinski, TP and Binau, AR and Biondi, R and Biondi, Y and Birch, HJ and Bishara, F and 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and Schumann, M and Schwemberger, T and Schwenk, A and Schwetz, T and Scotto Lavina, L and Scovell, PR and Sekiya, H and Selvi, M and Semenov, E and Semeria, F and Shagin, P and Shaw, S and Shi, S and Shockley, E and Shutt, TA and Si-Ahmed, R and Silk, JJ and Silva, C and Silva, MC and Simgen, H and Šimkovic, F and Sinev, G and Singh, R and Skulski, W and Smirnov, J and Smith, R and Solmaz, M and Solovov, VN and Sorensen, P and Soria, J and Sparmann, TJ and Stancu, I and Steidl, M and Stevens, A and Stifter, K and Strigari, LE and Subotic, D and Suerfu, B and Suliga, AM and Sumner, TJ and Szabo, P and Szydagis, M and Takeda, A and Takeuchi, Y and Tan, P-L and Taricco, C and Taylor, WC and Temples, DJ and Terliuk, A and Terman, PA and Thers, D and Thieme, K and Thümmler, T and Tiedt, DR and Timalsina, M and To, WH and Toennies, F and Tong, Z and Toschi, F and Tovey, DR and Tranter, J and Trask, M and Trinchero, GC and Tripathi, M and Tronstad, DR and Trotta, R and Tsai, YD and Tunnell, CD and Turner, WG and Ueno, R and Urquijo, P and Utku, U and Vaitkus, A and Valerius, K and Vassilev, E and Vecchi, S and Velan, V and Vetter, S and Vincent, AC and Vittorio, L and Volta, G and Von Krosigk, B and Von Piechowski, M and Vorkapic, D and Wagner, CEM and Wang, AM and Wang, B and Wang, Y and Wang, W and Wang, JJ and Wang, L-T and Wang, M and Wang, Y and Watson, JR and Wei, Y and Weinheimer, C and Weisman, E and Weiss, M and Wenz, D and West, SM and Whitis, TJ and Williams, M and Wilson, MJ and Winkler, D and Wittweg, C and Wolf, J and Wolf, T and Wolfs, FLH and Woodford, S and Woodward, D and Wright, CJ and Wu, VHS and Wu, P and Wüstling, S and Wurm, M and Xia, Q and Xiang, X and Xing, Y and Xu, J and Xu, Z and Xu, D and Yamashita, M and Yamazaki, R and Yan, H and Yang, L and Yang, Y and Ye, J and Yeh, M and Young, I and Yu, HB and Yu, TT and Yuan, L and Zavattini, G and Zerbo, S and Zhang, Y and Zhong, M and Zhou, N and Zhou, X and Zhu, T and Zhu, Y and Zhuang, Y and Zopounidis, JP and Zuber, K and Zupan, J (2023) A next-generation liquid xenon observatory for dark matter and neutrino physics. In: Journal of Physics G: Nuclear and Particle Physics, 50 (1).

Jou_Phy_Gnu_50-1_2023.pdf - Published Version

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Official URL: https://doi.org/10.1088/1361-6471/ac841a


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.

Item Type: Journal Article
Publication: Journal of Physics G: Nuclear and Particle Physics
Publisher: Institute of Physics
Additional Information: The copyright for this article belongs to the Authors.
Keywords: astroparticle physics; dark matter; direct detection; neutrinoless double-beta decay; neutrinos; supernova; xenon
Department/Centre: Division of Physical & Mathematical Sciences > Centre for High Energy Physics
Date Deposited: 31 Jan 2023 07:08
Last Modified: 31 Jan 2023 07:08
URI: https://eprints.iisc.ac.in/id/eprint/79620

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