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Abstract
Thermal light dark matter (LDM) with particle masses in the 1 MeV–1 GeV range could successfully explain the observed dark matter abundance as a relic from the primordial Universe. In this picture, a new feeble interaction acts as a “portal” between the Standard Model and LDM particles, allowing for the exploration of this paradigm at accelerator experiments. In the last years, the “missing energy” experiment NA64e at CERN SPS (Super Proton Synchrotron) has set world-leading constraints in the vector-mediated LDM parameter space, by exploiting a 100 GeV electron beam impinging on an electromagnetic calorimeter, acting as an active target. In this paper, we report a detailed description of the analysis of a preliminary measurement with a 70 GeV/c positron beam at NA64e, performed during summer 2023 with an accumulated statistics of 1.596 × 1010 positrons on target (hereafter referred to as e+OT). This data set was analyzed with the primary aim of evaluating the performance of the NA64e detector with a lower energy positron beam, towards the realization of the post-LS3 program. The analysis results, other than additionally probing unexplored regions in the LDM parameter space, provide valuable information towards the future NA64e positron campaign.
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Details
1 INFN, Sezione di Genova, Genova, Italia (GRID:grid.470205.4)
2 Universidad Andres Bello, Center for Theoretical and Experimental Particle Physics, Facultad de Ciencias Exactas, Santiago, Chile (GRID:grid.412848.3) (ISNI:0000 0001 2156 804X); Millennium Institute for Subatomic Physics at High-Energy Frontier (SAPHIR), Santiago, Chile (GRID:grid.412848.3)
3 CERN, European Organization for Nuclear Research, Geneva, Switzerland (GRID:grid.9132.9) (ISNI:0000 0001 2156 142X)
4 ETH Zürich, Institute for Particle Physics and Astrophysics, Zürich, Switzerland (GRID:grid.5801.c) (ISNI:0000 0001 2156 2780)
5 INFN, Sezione di Genova, Genova, Italia (GRID:grid.470205.4); Università degli Studi di Genova, Genova, Italia (GRID:grid.5606.5) (ISNI:0000 0001 2151 3065)
6 INFN, Sezione di Catania, Catania, Italia (GRID:grid.470198.3) (ISNI:0000 0004 1755 400X)
7 Universität Bonn, Helmholtz-Institut für Strahlen-und Kernphysik, Bonn, Germany (GRID:grid.10388.32) (ISNI:0000 0001 2240 3300)
8 Millennium Institute for Subatomic Physics at High-Energy Frontier (SAPHIR), Santiago, Chile (GRID:grid.412848.3)
9 Millennium Institute for Subatomic Physics at High-Energy Frontier (SAPHIR), Santiago, Chile (GRID:grid.470205.4)
10 Millennium Institute for Subatomic Physics at High-Energy Frontier (SAPHIR), Santiago, Chile (GRID:grid.470205.4); Universidad Técnica Federico Santa María and CCTVal, Valparaíso, Chile (GRID:grid.12148.3e) (ISNI:0000 0001 1958 645X)
11 Instituto de Fisica Corpuscular (CSIC/UV), Paterna, Spain (GRID:grid.470047.0) (ISNI:0000 0001 2178 9889)
12 York University, Department of Physics and Astronomy, Toronto, Canada (GRID:grid.21100.32) (ISNI:0000 0004 1936 9430)
13 Millennium Institute for Subatomic Physics at High-Energy Frontier (SAPHIR), Santiago, Chile (GRID:grid.5801.c); Universidad de La Serena, Departamento de Fisica, Facultad de Ciencias, La Serena, Chile (GRID:grid.19208.32) (ISNI:0000 0001 0161 9268)