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Strong Constraints on Sub-GeV Dark Matter from SLAC Beam Dump E137

Brian Batell, Rouven Essig, Ze'ev Surujon

TL;DR

E137 probes new and significant ranges of parameter space and constrains the well-motivated possibility that dark photons that decay to light dark-sector particles can explain the ∼3.6σ discrepancy between the measured and standard model value of the muon anomalous magnetic moment.

Abstract

We present new constraints on sub-GeV dark matter and dark photons from the electron beam-dump experiment E137 conducted at SLAC in 1980-1982. Dark matter interacting with electrons (e.g., via a dark photon) could have been produced in the electron-target collisions and scattered off electrons in the E137 detector, producing the striking, zero-background signature of a high-energy electromagnetic shower that points back to the beam dump. E137 probes new and significant ranges of parameter space, and constrains the well-motivated possibility that invisibly decaying dark photons can explain the $\sim 3.6 σ$ discrepancy between the measured and SM value of the muon anomalous magnetic moment. It also restricts the parameter space in which the relic density of dark matter in these models is obtained from thermal freeze-out. E137 also convincingly demonstrates that (cosmic) backgrounds can be controlled and thus serves as a powerful proof-of-principle for future beam-dump searches for sub-GeV dark matter scattering off electrons in the detector.

Strong Constraints on Sub-GeV Dark Matter from SLAC Beam Dump E137

TL;DR

E137 probes new and significant ranges of parameter space and constrains the well-motivated possibility that dark photons that decay to light dark-sector particles can explain the ∼3.6σ discrepancy between the measured and standard model value of the muon anomalous magnetic moment.

Abstract

We present new constraints on sub-GeV dark matter and dark photons from the electron beam-dump experiment E137 conducted at SLAC in 1980-1982. Dark matter interacting with electrons (e.g., via a dark photon) could have been produced in the electron-target collisions and scattered off electrons in the E137 detector, producing the striking, zero-background signature of a high-energy electromagnetic shower that points back to the beam dump. E137 probes new and significant ranges of parameter space, and constrains the well-motivated possibility that invisibly decaying dark photons can explain the discrepancy between the measured and SM value of the muon anomalous magnetic moment. It also restricts the parameter space in which the relic density of dark matter in these models is obtained from thermal freeze-out. E137 also convincingly demonstrates that (cosmic) backgrounds can be controlled and thus serves as a powerful proof-of-principle for future beam-dump searches for sub-GeV dark matter scattering off electrons in the detector.

Paper Structure

This paper contains 8 equations, 2 figures.

Figures (2)

  • Figure 1: Top: Layout of the E137 experiment (adapted from Fig. 2 in E137). Middle and Bottom: An electron beam hits an aluminum target, creating DM particles $\chi$ via bremsstrahlung of $A'$(bottom left). The $\chi$ traverse a $\sim 179$ m deep hill and another $\sim 204$ m-long open region before scattering off electrons (bottom right), which are detected in an electromagnetic shower calorimeter.
  • Figure 2: Top left: Constraints (95% C.L.) in the $\epsilon-m_{A'}$ plane for dark photons $A'$ decaying invisibly to light DM $\chi$, with $m_\chi < 0.5$ MeV. The SLAC E137 experiment excludes a Dirac fermion (red shading/red solid line) or complex scalar (red long dashed) DM. We fix $\alpha_D = 0.1$ and assume an electron recoil threshold energy of $E_{\rm th} = 1$ GeV in the E137 detector (for comparison, the red dotted line shows $E_{\rm th} = 3$ GeV for a fermionic $\chi$). Also shown are constraints from the anomalous magnetic moment of the electron ($a_e$, $2\sigma$, blue dashed) and muon ($a_\mu$, $5\sigma$, dark green dashed), and a light-green dashed region in which the $A'$ explains the $a_\mu$ discrepancy. Other model-dependent constraints (see text for details), arise from LSND (yellow solid), SLAC mQ experiment (cyan solid), B A B A R (blue dotted), and BNL E787 and E949 (brown dotted). The inset focuses on $m_{A'} = 100-300$ MeV. Top right and Bottom left: Same as top left but for $m_\chi = 10$ MeV and 50 MeV, respectively. Above the black solid line, the thermal relic abundance of a scalar $\chi$ satisfies $\Omega_\chi \le \Omega_{\rm DM}$; the region above the blue solid line is excluded if $\chi$ can scatter off electrons in the XENON10 experiment, assuming $\chi$ makes up all the DM; the light gray regions/dotted lines are excluded from searches for $A' \to e^+e^-$ (if this mode is available for $m_{A'} < 2 m_\chi$) in E141, E774, Orsay, HADES, or A1. Bottom right: 95% C.L. upper limits on $\alpha_D$ as a function of $m_{A'}$ for a Dirac fermion $\chi$, assuming $\epsilon$ is fixed to the smallest value consistent with explaining the $a_\mu$ anomaly. The E137 constraint is shown for $m_\chi < 0.5$ MeV (red shading/solid line) and for $m_\chi = 10,50$ MeV (dashed red), while the remaining constraints are only shown for $m_\chi < 0.5$ MeV. The solid gray curve is the limit from $A'\to visible$ searches, while the gray dashed represents the transition between $A'\to\chi\bar{\chi}$ and $A'\to visible$ decays dominating.