Scintillating Bubble Chamber (SBC): The SBC collaboration is working on developing liquid-noble bubble chambers for a large exposure, quasi-background-free detection of low energy nuclear recoils. SBC addresses a current lack of scalable, low-threshold nuclear recoil detection technology, enabling searches for low mass (1 GeV/c^2) dark matter to the neutrino fog and for high-statistic measurements of low-energy neutrino coherent scattering. SBC combines the electron-recoil background discrimination of a bubble chamber with the event-by-event energy resolution of a liquid scintillator detectors. This, along with the lack of bubble-nucleating energy-loss mechanisms available to recoiling electrons in liquid nobles, allows for much stronger electron-recoil discrimination that existing bubble chamber dark matter detectors. In turn, this allows for background=free sensitivity to nuclear recoils at lower energies that can be achieves in any current working detection technique, reaching thresholds low as 100 eV while remaining blind to electron-recoiling backgrounds. The SBC collaboration's first physics-scale device, the 10kg liquid argon bubble chamber SBC-LAr10, is now commissioned and will undergo a series of source calibrations at Fermilab to measure both the discrimination power and low energy nuclear recoil sensitivity of the device, calibrating the detection threshold at 10 eV. Future SBC efforts will include a ton-year dark matter search targeting the solar neutrino fog at 1GeV/c^2 particle mass along with the deployment of a SBC device to measure neutrino cross sections at 1MeV neutrino energy.
[Scintillating Bubble Chambers: Liquid-noble Bubble Chambers for Dark Matter and CEvNS Detection https://arxiv.org/abs/2207.12400]
Top: Stereo image of a candidate nuclear recoil event from a prototype 30-gram xenon bubble chamber from a 252Cf calibration source, with visible xenon vapor bubbles circled in red.
Top: Acoustic record of bubble formation
Bottom: PMT waveforms showing xenon scintillation. The bubble-coincident pulse shown in red; electron recoils in the same bubble time window generate scintillation pulses without bubble nucleation (gray)
SBC Operation: The liquid-noble SBC is an extension of the Freon-based chamber technique used by COUPP and PICO for dark matter searches. The advantage of the SBC for DM searches is the intrinsic insensitivity to electron-recoil (ER) backgrounds, due to the thermodynamics of bubble nucleation. Nucleation requires the formation of a proto-bubble to overcome the free energy barrier arising from the surface tension of the bubble before growing to a visible size. Through the Seitz Hot Spike Model, a particle interaction can create this proto-bubble. In Freon detectors, the electron nuclear recoil insensitivity diminishes significantly below 1 KeV, resulting in γ -induced nucleation indistinguishable from nuclear recoils. Bubble chambers are threshold detectors, where a bubble is nucleated by any energy deposition above the Seitz threshold. If energy deposited is unknown, there will be an inability to differentiate between high and low energy nuclear recoils. Liquid-noble SBC chambers address both of these issues, using LAr (liquid argon) as a target fluid. LAr scintillates in the vacuum-UV under ionization radiation, allowing for the measurement of the total energy deposited and discrimination between low and high energy nuclear recoils.
Unlike Pico , whose acoustic signal accompanying bubble nucleation gives MeV energy resolution, this energy reconstruction in LAr has a resolution in KeV. SBC is driven by a fundamental additional suppression of electron-recoil-induced bubble nucleation in superheated noble liquids, allowing for background free operation at nuclear recoil detection thresholds at magnitudes lower than those achievable in Freon-based detectors. The absence of bubble nucleation by electron recoils in superheated noble liquids is a consequence of the lack of molecular degrees of freedom for recoiling electrons to excite. Lacking energy loss due to molecular vibrational modes, particle interactions can locally heat the fluid only through center of mass motion of individual atoms. Although this is achieved through the Lindhard effect, the kinematics of elastic electron-atom collisions make this an extremely inefficient means of energy loss for electrons, so electron recoil energy is almost entirely carried away by scintillation light, IR radiation, and recombining ionization.
[Scintillating Bubble Chambers for Rare Event Searches https://www.mdpi.com/2218-1997/9/8/346]
Left: Schematic and annotated solid model of the SBC-LAr10 detector
Middle: Test of the SBC-LAr10 inner assembly consisting of the inner and outer fused silica vessels, bellows guides and support structure, stainless steel bellows, and spring-energiezed PTFE silicia-to-metal seals.
Right: Partially assembled HDPE castle isolating the warm target region from the cold, stable region, enclosing the copper SIPM support structure that surrounds the target volume. 3 of 8 piezoelectric acoustic sensors are visible at the bottom of the castle.
SBC-LAr10 Design: The SBC-LAR10 consists of an active LAr volume of 10kg, along with 10-100 ppm of xenon shifting the scintillation wavelength to 175nm. the 175 nm light can passed through the silica vessel where it will be detected by an array of 32 inward facing SiPMs mounted on copper panels to minimizes the vertical thermal gradient across the active volume. Hamamatsu VuV4 SIPMs will be used for the SBC-LAr10 while SBC-SNOWLAB, a parallel detector with a focus on radiopure construction, will use SiPMs with lower uranium and thorium content. The inner components are housed in a stainless steel pressure vessel with LCF4 to act as hydraulic fluid. Resistive temperature detectors are placed throughout the pressure vessel for thermodynamic regulation, and to monitor the temperature. The pressure in the LAR volume is controlled by an external hydraulic piston that connects through a bellow to the pressure vessel, which is housed in a vacuum jet and cold with liquid nitrogen. SBC-LAR10 will operate 100m underground at Fermilab to reduce cosmic-ray muon rate by an amount sufficient to allow low-energy calibration without additional shielding. External shielding will be required to minimize the environmental neutron rate.
[Scintillating Bubble Chambers for Rare Event Searches https://www.mdpi.com/2218-1997/9/8/346]
Top: Solid model base design of SBC-LAr10 with main components annotated
Left: Electron recoil sensitivity of the prototype xenon bubble chamber as a function of superheat (Seitz threshold). There is no evidence seen for bubble nucleation by gamma sources. Dashed lines show the sensitives of measurements based on source strengths, background rates, and exposures. Square points are 90% confidence intervals with background subtraction and round points are the same but without background subtraction. The blue curves show the gamma sensitivity expected for a molecular fluid with the same thermodynamic physical properties as xenon, following the electron recoil bubble nucleation models for delta rays and auger cascades following xenon K-shell capture.
[Scintillating Bubble Chambers: Liquid-noble Bubble Chambers for Dark Matter and CEvNS Detection https://arxiv.org/abs/2207.12400]
Nuclear recoil sensitivity of the prototype xenon bubble chamber. Both plots illustrate a factor of around 2 between the calculated Seitz threshold and the nuclear recoiled detection threshold, matching the threshold behavior in Freon bubble chambers.
Left: chamber response to 152-keV neutron from a 88Y-Be photo-neutron source. The green line illustrates the average sensitivity of 88Y-Al (gammas only). The extrapolated onset of sensitive is at Q = 2.4 keV for the 4.8-keV maximum recoil energy.
Right: The probability of bubble nucleation as a function of nuclear recoil energy at a fixed Seitz threshold of 1.48 keV. The efficiency curve is constrained by the observed bubble rates when exposed to 207BiBe, 88YBe, and 252Cf sources. The solid blue line and shaded region indicate the best fit efficiency curve with the red line indicating the calculated Seitz threshold.
[Scintillating Bubble Chambers: Liquid-noble Bubble Chambers for Dark Matter and CEvNS Detection https://arxiv.org/abs/2207.12400]