ZnWO$_4$ anisotropic scintillator for Dark Matter investigation with the directionality technique - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Année : 2017

ZnWO$_4$ anisotropic scintillator for Dark Matter investigation with the directionality technique

R. Bernabei
  • Fonction : Auteur
P. Belli
  • Fonction : Auteur
F. Cappella
  • Fonction : Auteur
V. Caracciolo
  • Fonction : Auteur
R. Cerulli
  • Fonction : Auteur
F.A. Danevich
  • Fonction : Auteur
A. d'Angelo
A.Di Marco
  • Fonction : Auteur
A. Incicchitti
  • Fonction : Auteur
V.M. Mokina
  • Fonction : Auteur
O.G. Polischuk
  • Fonction : Auteur
C. Taruggi
  • Fonction : Auteur
V.I. Tretyak
  • Fonction : Auteur

Résumé

The ZnWO4 crystal scintillator has unique features that make it very promising to realize a pioneering experiment to pursue Dark Matter investigation with the directionality technique. In particular in this detector the light output and the scintillation pulse shape for heavy particles (p, α, nuclear recoils) depend on the direction of the impinging particle with respect to the crystal axes, while the response to γ/β radiation is isotropic. The anisotropy of the light output can be considered to point out the presence in the diurnal counting rate of a Dark Matter signal produced by candidate particle inducing just nuclear recoils. In addition this crystal detector has also other important characteristics for a Dark Matter experiment: high light output, high level of radiopurity. In this paper the present performances of the developed ZnWO4 crystal scintillator will be summarized together with the possible future improvements. Some reachable sensitivities – under given assumptions – in the investigation of DM candidate particles with the directionality technique will also be addressed.

Dates et versions

hal-01833786 , version 1 (10-07-2018)

Identifiants

Citer

R. Bernabei, P. Belli, F. Cappella, V. Caracciolo, R. Cerulli, et al.. ZnWO$_4$ anisotropic scintillator for Dark Matter investigation with the directionality technique. 6th Roma International Workshop on Astroparticle Physics, Jun 2016, Rome, Italy. pp.05002, ⟨10.1051/epjconf/201713605002⟩. ⟨hal-01833786⟩
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