Abstract

We report on the results of the search for a new sub-GeV vector boson (A’) mediated production of Dark Matter (χ) in the fixed-target experiment, NA64, at the CERN SPS. The A’, called dark photon, could be generated in the reaction e-Z → e-ZA’ of 100 GeV electrons dumped against an active target which is followed by the prompt invisible decay A’ $ \to \chi \bar{\chi } $. The experimental signature of this process would be an event with an isolated electron and large missing energy in the detector. From the analysis of the data sample collected in 2016 corresponding to 4.3 × 1010 electrons on target no evidence of such a process has been found. The constraints on the A’ mixing strength with photons, 10−5 ≤ ɛ ≤ 10−2, for the A’ mass range mA’ ≤ 1GeV are derived. Significantly more data were taken in 2017 and 2018. The analysis of these data is not yet finished, although the sensitivity is already estimated as about 3 times better than in the previously published result on the 2016 data. For models considering scalar and fermionic thermal Dark Matter interacting with the visible sector through the vector portal the experiment starts to be sensitive to the regions of the dark-matter parameter $ y = \in^{2} \alpha_{D} (\frac{{m_{\chi } }}{{m_{{A^{\prime}}} }})^{4} $ predicted from the cosmological observations of Dark Matter. We also report the improved results on a direct search for a new 16.7 MeV boson (X) which could explain the anomalous excess of e+e- pairs observed in the excited 8Be* nucleus decays. Due to its coupling to electrons, the X could be produced in the bremsstrahlung reaction e-Z → e-ZX by a beam of electrons incident on an active target in the NA64 experiment at the CERN SPS and observed through the subsequent decay into a e+e- pair. With 8.4 × 1010 electrons on target no evidence for such decays was found, allowing to set limits on the X - e- coupling in the range 1 × 10−4 ≤ ɛe ≤ 6 × 10−4 excluding part of the allowed parameter space. We also set new bounds on the mixing strength of photons with dark photons (A’) from non-observation of the decay A’ → e+e- of the bremsstrahlung A’ with a mass ≤ 23MeV. Future plans of the NA64 experiment are presented.

Highlights

  • The NA64 experiment is primarily designed for the search of dark photons A [1,2,3] through the missing energy signature

  • The candidate events were selected with the following criteria chosen to maximize the acceptance of signal events and to minimize the number of background events, using both MC simulation and data: (i) No energy deposition in the V2 counter exceeding about half of the energy deposited by the minimum ionizing particle (MIP); (ii) The signal in the decay counter S4 is consistent with two MIPs; (iii) The sum of energies deposited in the WCAL+electromagnetic calorimeter (ECAL) is equal to the beam energy within the energy resolution of these detectors

  • At least 25% of the total energy should be deposited in the ECAL; (iv) The shower in the WCAL should start to develop within a few first X0, which is ensured by the preshower part energy cut; (v) The cell with maximal energy deposition in the ECAL should be (3,3) (vi) The lateral and longitudinal shape of the shower in the ECAL are consistent with a single e-m one

Read more

Summary

Introduction

The NA64 experiment is primarily designed for the search of dark photons A [1,2,3] through the missing energy signature. The first results of these search were published in [6]. In the runs of 2017 and 2018 a significantly more data were collected. These data correspond in total to about 3 × 1011 EOT. With this statistics the NA64 experiment starts to be sensitive to Dark Matter mixing parameters predicted by some thermal Dark Matter (DM) models [7]

Sensitivity of NA64 to A’ in the invisible mode search
Findings
Conclusion
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call