Image de couverture de livre

A new dark matter direct search based on archaeological Pb

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Alloni, D., Benato, G., Carniti, P., Cataldo, M., Chen, L., Clemenza, M., Consonni, M., Croci, G., Dafinei, I., Danevich, F. A., Di Martino, D., Di Stefano, E., Iachellini, N. Ferreiro, Ferroni, F., Filippini, F., Ghislandi, S., Giachero, A., Gironi, L., Gorla, P., Gotti, C., Helis, D. L., Kasperovych, D. V., Kobychev, V. V., Marcucci, G., Melchiorre, A., Menegolli, A., Nisi, S., Musa, M., Pagnanini, L., Pattavina, L., Pessina, G., Pirro, S., Polischuk, O. G., Pozzi, S., Prata, M. C., Puiu, A., Quitadamo, S., Riccardi, M. P., Rossella, M., Rossini, R., Saliu, F., Salvini, A., Scherban, A. P., Solopikhin, D. A., Tretyak, V. I., Trotta, D., Yuan, H.
Format:	Preprint
Publié:	2025
Sujets:	Instrumentation and Detectors Cosmology and Nongalactic Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

_version_	1866908420596039680
author	Alloni, D. Benato, G. Carniti, P. Cataldo, M. Chen, L. Clemenza, M. Consonni, M. Croci, G. Dafinei, I. Danevich, F. A. Di Martino, D. Di Stefano, E. Iachellini, N. Ferreiro Ferroni, F. Filippini, F. Ghislandi, S. Giachero, A. Gironi, L. Gorla, P. Gotti, C. Helis, D. L. Kasperovych, D. V. Kobychev, V. V. Marcucci, G. Melchiorre, A. Menegolli, A. Nisi, S. Musa, M. Pagnanini, L. Pattavina, L. Pessina, G. Pirro, S. Polischuk, O. G. Pozzi, S. Prata, M. C. Puiu, A. Quitadamo, S. Riccardi, M. P. Rossella, M. Rossini, R. Saliu, F. Salvini, A. Scherban, A. P. Solopikhin, D. A. Tretyak, V. I. Trotta, D. Yuan, H.
author_facet	Alloni, D. Benato, G. Carniti, P. Cataldo, M. Chen, L. Clemenza, M. Consonni, M. Croci, G. Dafinei, I. Danevich, F. A. Di Martino, D. Di Stefano, E. Iachellini, N. Ferreiro Ferroni, F. Filippini, F. Ghislandi, S. Giachero, A. Gironi, L. Gorla, P. Gotti, C. Helis, D. L. Kasperovych, D. V. Kobychev, V. V. Marcucci, G. Melchiorre, A. Menegolli, A. Nisi, S. Musa, M. Pagnanini, L. Pattavina, L. Pessina, G. Pirro, S. Polischuk, O. G. Pozzi, S. Prata, M. C. Puiu, A. Quitadamo, S. Riccardi, M. P. Rossella, M. Rossini, R. Saliu, F. Salvini, A. Scherban, A. P. Solopikhin, D. A. Tretyak, V. I. Trotta, D. Yuan, H.
contents	The RES-NOVA project is an experimental initiative aimed at detecting neutrinos from the next galactic supernova using PbWO$_{4}$ cryogenic detectors, operated at low temperatures in a low-background environment. By utilizing archaeological lead (Pb) as the target material, RES-NOVA leverages its high radiopurity, large nuclear mass, and the natural abundance of $^{207}$Pb, making it well-suited for exploring both spin-independent and spin-dependent Dark Matter (DM) interactions via nuclear scattering. This work presents a background model developed for the RES-NOVA technology demonstrator and evaluates its implications for Dark Matter detection. Detailed calculations of nuclear matrix elements, combined with the unique properties of archaeological Pb, demonstrate RES-NOVA's potential as a complementary tool to existing direct detection experiments for studying Dark Matter interactions. The experiment will conduct DM searches over a broad mass range spanning 4 orders of magnitude, from sub-GeV/$c^2$ to TeV/$c^2$. In the most optimistic scenario, RES-NOVA is expected to probe DM-nucleon cross-sections down to 1$\times 10^{-43}$ cm$^2$ and 2$\times 10^{-46}$ cm$^2$ for candidates with masses of 2 GeV/$c^2$ and 20 GeV/$c^2$, respectively.
format	Preprint
id	arxiv_https___arxiv_org_abs_2501_12409
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	A new dark matter direct search based on archaeological Pb Alloni, D. Benato, G. Carniti, P. Cataldo, M. Chen, L. Clemenza, M. Consonni, M. Croci, G. Dafinei, I. Danevich, F. A. Di Martino, D. Di Stefano, E. Iachellini, N. Ferreiro Ferroni, F. Filippini, F. Ghislandi, S. Giachero, A. Gironi, L. Gorla, P. Gotti, C. Helis, D. L. Kasperovych, D. V. Kobychev, V. V. Marcucci, G. Melchiorre, A. Menegolli, A. Nisi, S. Musa, M. Pagnanini, L. Pattavina, L. Pessina, G. Pirro, S. Polischuk, O. G. Pozzi, S. Prata, M. C. Puiu, A. Quitadamo, S. Riccardi, M. P. Rossella, M. Rossini, R. Saliu, F. Salvini, A. Scherban, A. P. Solopikhin, D. A. Tretyak, V. I. Trotta, D. Yuan, H. Instrumentation and Detectors Cosmology and Nongalactic Astrophysics The RES-NOVA project is an experimental initiative aimed at detecting neutrinos from the next galactic supernova using PbWO$_{4}$ cryogenic detectors, operated at low temperatures in a low-background environment. By utilizing archaeological lead (Pb) as the target material, RES-NOVA leverages its high radiopurity, large nuclear mass, and the natural abundance of $^{207}$Pb, making it well-suited for exploring both spin-independent and spin-dependent Dark Matter (DM) interactions via nuclear scattering. This work presents a background model developed for the RES-NOVA technology demonstrator and evaluates its implications for Dark Matter detection. Detailed calculations of nuclear matrix elements, combined with the unique properties of archaeological Pb, demonstrate RES-NOVA's potential as a complementary tool to existing direct detection experiments for studying Dark Matter interactions. The experiment will conduct DM searches over a broad mass range spanning 4 orders of magnitude, from sub-GeV/$c^2$ to TeV/$c^2$. In the most optimistic scenario, RES-NOVA is expected to probe DM-nucleon cross-sections down to 1$\times 10^{-43}$ cm$^2$ and 2$\times 10^{-46}$ cm$^2$ for candidates with masses of 2 GeV/$c^2$ and 20 GeV/$c^2$, respectively.
title	A new dark matter direct search based on archaeological Pb
topic	Instrumentation and Detectors Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2501.12409