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arxiv: 1707.08145 · v1 · submitted 2017-07-25 · ⚛️ physics.ins-det

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DarkSide-20k: A 20 Tonne Two-Phase LAr TPC for Direct Dark Matter Detection at LNGS

C. E. Aalseth , F. Acerbi , P. Agnes , I. F. M. Albuquerque , T. Alexander , A. Alici , A. K. Alton , P. Antonioli
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S. Arcelli R. Ardito I. J. Arnquist D. M. Asner M. Ave H. O. Back A. I. Barrado Olmedo G. Batignani E. Bertoldo S. Bettarini M. G. Bisogni V. Bocci A. Bondar G. Bonfini W. Bonivento M. Bossa B. Bottino M. Boulay R. Bunker S. Bussino A. Buzulutskov M. Cadeddu M. Cadoni A. Caminata N. Canci A. Candela C. Cantini M. Caravati M. Cariello M. Carlini M. Carpinelli A. Castellani S. Catalanotti V. Cataudella P. Cavalcante S. Cavuoti R. Cereseto A. Chepurnov C. Cical\`o L. Cifarelli M. Citterio A. G. Cocco M. Colocci S. Corgiolu G. Covone P. Crivelli I. D'Antone M. D'Incecco D. D'Urso M. D. Da Rocha Rolo M. Daniel S. Davini A. De Candia S. De Cecco M. De Deo G. De Filippis G. De Guido G. De Rosa G. Dellacasa M. Della Valle P. Demontis A. Derbin A. Devoto F. Di Eusanio G. Di Pietro C. Dionisi A. Dolgov I. Dormia S. Dussoni A. Empl M. Fernandez Diaz A. Ferri C. Filip G. Fiorillo K. Fomenko D. Franco G. E. Froudakis F. Gabriele A. Gabrieli C. Galbiati P. Garcia Abia A. Gendotti A. Ghisi S. Giagu P. Giampa G. Gibertoni C. Giganti M. A. Giorgi G. K. Giovanetti M. L. Gligan A. Gola O. Gorchakov A. M. Goretti F. Granato M. Grassi J. W. Grate G. Y. Grigoriev M. Gromov M. Guan M. B. B. Guerra M. Guerzoni M. Gulino R. K. Haaland A. Hallin B. Harrop E. W. Hoppe S. Horikawa B. Hosseini D. Hughes P. Humble E. V. Hungerford An. Ianni C. Jillings T. N. Johnson K. Keeter C. L. Kendziora S. Kim G. Koh D. Korablev G. Korga A. Kubankin M. Kuss M. Ku\'zniak B. Lehnert X. Li M. Lissia G. U. Lodi B. Loer G. Longo P. Loverre R. Lussana L. Luzzi Y. Ma A. A. Machado I. N. Machulin A. Mandarano L. Mapelli M. Marcante A. Margotti S. M. Mari M. Mariani J. Maricic C. J. Martoff M. Mascia M. Mayer A. B. McDonald A. Messina P. D. Meyers R. Milincic A. Moggi S. Moioli J. Monroe A. Monte M. Morrocchi B. J. Mount W. Mu V. N. Muratova S. Murphy P. Musico R. Nania A. Navrer Agasson I. Nikulin V. Nosov A. O. Nozdrina N. N. Nurakhov A. Oleinik V. Oleynikov M. Orsini F. Ortica L. Pagani M. Pallavicini S. Palmas L. Pandola E. Pantic E. Paoloni G. Paternoster V. Pavletcov F. Pazzona S. Peeters K. Pelczar L. A. Pellegrini N. Pelliccia F. Perotti R. Perruzza V. Pesudo Fortes C. Piemonte F. Pilo A. Pocar T. Pollmann D. Portaluppi D. A. Pugachev H. Qian B. Radics F. Raffaelli F. Ragusa M. Razeti A. Razeto V. Regazzoni C. Regenfus B. Reinhold A. L. Renshaw M. Rescigno F. Reti\`ere Q. Riffard A. Rivetti S. Rizzardini A. Romani L. Romero B. Rossi N. Rossi A. Rubbia D. Sablone P. Salatino O. Samoylov E. S\'anchez Garc\'ia W. Sands M. Sant R. Santorelli C. Savarese E. Scapparone B. Schlitzer G. Scioli E. Segreto A. Seifert D. A. Semenov A. Shchagin L. Shekhtman E. Shemyakina A. Sheshukov M. Simeone P. N. Singh P. Skensved M. D. Skorokhvatov O. Smirnov G. Sobrero A. Sokolov A. Sotnikov F. Speziale R. Stainforth C. Stanford G. B. Suffritti Y. Suvorov R. Tartaglia G. Testera A. Tonazzo A. Tosi P. Trinchese E. V. Unzhakov A. Vacca E. V\'azquez-J\'auregui M. Verducci T. Viant F. Villa A. Vishneva B. Vogelaar M. Wada J. Wahl J. Walding S. Walker H. Wang Y. Wang A. W. Watson S. Westerdale R. Williams M. M. Wojcik S. Wu X. Xiang X. Xiao C. Yang Z. Ye A. Yllera de Llano F. Zappa G. Zappal\`a C. Zhu A. Zichichi M. Zullo A. Zullo
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classification ⚛️ physics.ins-det
keywords darkside-20ktimes10vetodarkside-50detectorexposurelartpcmass
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Building on the successful experience in operating the DarkSide-50 detector, the DarkSide Collaboration is going to construct DarkSide-20k, a direct WIMP search detector using a two-phase Liquid Argon Time Projection Chamber (LArTPC) with an active (fiducial) mass of 23 t (20 t). The DarkSide-20k LArTPC will be deployed within a shield/veto with a spherical Liquid Scintillator Veto (LSV) inside a cylindrical Water Cherenkov Veto (WCV). Operation of DarkSide-50 demonstrated a major reduction in the dominant $^{39}$Ar background when using argon extracted from an underground source, before applying pulse shape analysis. Data from DarkSide-50, in combination with MC simulation and analytical modeling, shows that a rejection factor for discrimination between electron and nuclear recoils of $\gt3\times10^9$ is achievable. This, along with the use of the veto system, is the key to unlocking the path to large LArTPC detector masses, while maintaining an "instrumental background-free" experiment, an experiment in which less than 0.1 events (other than $\nu$-induced nuclear recoils) is expected to occur within the WIMP search region during the planned exposure. DarkSide-20k will have ultra-low backgrounds than can be measured in situ. This will give sensitivity to WIMP-nucleon cross sections of $1.2\times10^{-47}$ cm$^2$ ($1.1\times10^{-46}$ cm$^2$) for WIMPs of $1$ TeV$/c^2$ ($10$ TeV$/c^2$) mass, to be achieved during a 5 yr run producing an exposure of 100 t yr free from any instrumental background. DarkSide-20k could then extend its operation to a decade, increasing the exposure to 200 t yr, reaching a sensitivity of $7.4\times10^{-48}$ cm$^2$ ($6.9\times10^{-47}$ cm$^2$) for WIMPs of $1$ TeV$/c^2$ ($10$ TeV$/c^2$) mass.

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