detection

LiquidO: Opaque Scintillator Turned Into a Particle Camera

· 12 min read · Editorial

Conventional liquid scintillators are transparent. LiquidO makes them deliberately opaque, trapping light near its origin so a single detector reads both energy and event topology.

For sixty years the conventional wisdom about liquid scintillator detectors has been the same. Make the scintillator as transparent as possible so that photons travel meters across the volume to photomultiplier tubes mounted on the boundary, where they can be efficiently collected. Optical purity is a virtue; light loss is the enemy. KamLAND, Borexino, Daya Bay, JUNO — every major scintillator-based neutrino experiment has chased the same goal of pushing absorption and scattering lengths into the tens of meters.

LiquidO is a deliberate inversion of that strategy. Its central idea is to make the scintillator opaque, with a scattering length of a few centimeters, and read out the light through a dense lattice of wavelength-shifting fibers running through the volume. Each fiber sees only the photons born in its immediate neighborhood. The collected light pattern is no longer a single integrated energy number but a three-dimensional image of where the light was produced — an actual photograph, voxel by voxel, of the particle shower or track inside the scintillator.

The change makes the same device perform two jobs at once: it measures energy through the total light, and it reconstructs the topology of the event through the spatial pattern. For physics that depends on distinguishing event types from shape — telling an electron from a positron from a gamma from a neutron — this is transformative. This post is about how the technique works, why opacity is the right design choice for certain physics goals, and which detectors are being built to exploit it.

Transparency, opacity, and what each preserves

A charged particle moving through liquid scintillator produces a few thousand optical photons per MeV of energy deposit, isotropically along its path. In a conventional transparent scintillator, those photons propagate freely through the bulk over distances of meters. By the time they reach the boundary photomultipliers, their original spatial information is effectively lost — what arrives is a roughly isotropic light wave whose total intensity measures the deposited energy but whose origin is unresolvable in space.

This is by design. The transparent scintillator is treated as a uniform calorimeter: every event is collapsed to a number. For low-energy neutrino physics where the relevant observable is the prompt-plus-delayed coincidence (inverse beta decay) or the spectrum (solar, geoneutrinos), the energy resolution dominates, and the loss of topology is acceptable.

LiquidO inverts the trade-off. By engineering the scintillator to scatter light strongly — typically through a controlled emulsion of two immiscible components with slightly different refractive indices — the mean scattering length is reduced to a few centimeters. Photons no longer travel far; they random-walk until they are either absorbed or hit a wavelength-shifting fiber. The fiber absorbs the photon and re-emits it at a longer wavelength inside the fiber’s own waveguide, propagating along the fiber to silicon photomultipliers at the end. Because each fiber sees only photons born within its scattering-length-scale neighborhood, the readout of all fibers together gives a three-dimensional, voxelized image of the light density inside the detector.

The detector volume becomes literally a camera that photographs every event from the inside.

Transparent vs opaque scintillator readout of the same event transparent (KamLAND-style) event light spreads to all PMTs → integrated energy only opaque (LiquidO-style) 511 keV 511 keV light trapped near origin → voxelized image of the event
Same positron-stopping event read out two ways. In a conventional transparent scintillator (left), photons reach every boundary photomultiplier and only the integrated total can be reconstructed — an energy number, no shape. In LiquidO (right), the opaque medium traps photons near their origin and the dense lattice of wavelength-shifting fibers reads out a three-dimensional light pattern. The two 511 keV gammas from positron annihilation appear as separate light blobs displaced from the main shower, identifying the positron event by topology rather than energy alone.

The science the camera enables

The reason topology matters is that it carries discriminating information that pure energy does not.

A positron stopping in scintillator deposits its kinetic energy as a tight shower, then annihilates with an electron to produce two back-to-back 511 keV gamma rays. The gammas travel a few centimeters through the scintillator before depositing their energy in separate, displaced light clouds. In LiquidO, the prompt event therefore appears as a central shower plus two satellite blobs at roughly the annihilation-gamma mean free path — a unique topological signature.

An electron does the same minus the annihilation, so the event is a single shower with no satellite blobs. Electron-versus-positron discrimination, impossible in a transparent scintillator, becomes an event-by-event tag in LiquidO. This single capability is the foundation of the technique’s leading physics application: reactor antineutrino monitoring.

A gamma ray Compton-scatters multiple times before being absorbed, producing a chain of small displaced energy depositions rather than a single shower. The topology is again distinct from an electron’s, even when the deposited energy is the same.

A proton recoiling from a neutron-induced event has a much shorter range than an electron of comparable energy, so its shower is tightly concentrated. Neutrons themselves are tagged by the delayed gamma emission from capture, just as in conventional inverse-beta-decay detection.

A muon decay produces a long track plus an electron at the endpoint. The shape distinguishes it from a single electron event.

In each case the topology carries information the energy alone does not, and the opacity-induced spatial resolution makes it accessible.

Reactor antineutrino monitoring

The most concrete near-term application is reactor antineutrino monitoring, where the goal is to count the antineutrinos coming out of a reactor core in real time and infer the reactor’s power level and fuel composition. The technique has applications in nuclear nonproliferation: a clandestine reactor producing weapons-grade plutonium has a distinctive antineutrino signature that could be detected from outside the facility.

In a conventional liquid scintillator the dominant signature of an electron antineutrino is inverse beta decay on a free proton, producing a prompt positron plus a delayed neutron capture. The prompt-delayed coincidence is the standard tag, and it works well when the rate is high enough. But at low rates, accidental coincidences become a problem: any pair of single events that happen to fall in the time and space window can mimic the inverse-beta-decay signature.

LiquidO’s event-by-event positron identification — through the two displaced annihilation gammas — turns the inverse-beta-decay event into a clean positive tag rather than a coincidence requirement. The accidental background drops by orders of magnitude, and a relatively small detector close to a reactor core can detect antineutrinos efficiently in real time. This is the use case the LiquidO collaboration has emphasized in its proposals, and demonstrators are being built specifically to validate the technique for nonproliferation monitoring.

Other physics targets

Beyond reactor monitoring, several other applications motivate scaling LiquidO up.

Geoneutrinos from thorium and uranium decay chains in the Earth’s mantle and crust are an extreme low-rate signal — a few events per kiloton per year — and the inverse-beta-decay signature is similarly buried in backgrounds. The combination of positron tagging and the topology-based rejection of cosmogenic and natural-radioactivity backgrounds could substantially improve the signal-to-noise of geoneutrino measurements at large scale.

The diffuse supernova neutrino background is the canonical example of a barely-detectable inverse-beta-decay signal sitting beneath a sea of atmospheric and solar backgrounds. SK-Gd is the current leading effort to detect it; a kiloton-scale LiquidO complement would attack the same signal with completely different systematics and could provide independent confirmation.

Solar neutrinos from the CNO cycle, recently detected by Borexino, are a sub-MeV-scale spectrum measurement where event topology is less informative than energy resolution. LiquidO’s energy resolution is in principle comparable to a transparent scintillator’s, but achieving it at sub-MeV with the dense fiber readout requires further development.

The engineering reality

Several technical challenges have to be solved at scale.

The first is scintillator opacity stability. The opacity is produced by a controlled microemulsion, and maintaining it over years without phase separation or settling is a chemistry problem the collaboration has been working on at the prototype level. Aging of the scintillator changes the scattering length, and a slow drift would distort event reconstruction.

The second is fiber density. Reaching the spatial resolution needed for event topology demands fibers spaced every few centimeters throughout the volume, far denser than the photodetector array in conventional scintillator. The mechanical engineering of stringing thousands of kilometers of fiber through a multi-ton detector volume, while maintaining optical uniformity, is non-trivial.

The third is light yield. Some photons are absorbed before reaching a fiber, and the overall light collection efficiency is somewhat lower than in transparent scintillator. The energy resolution can match a transparent detector only by paying careful attention to fiber coverage and scintillator yield.

A 1-kiloton LiquidO prototype is in detailed design as of 2025, with deployment expected later in the decade. If it meets its performance targets, it would become the prototype for larger detectors aimed at reactor monitoring, geoneutrino measurements, and the DSNB.

Why it represents a new direction

Most innovations in neutrino detection over the past forty years have been incremental: better scintillators, larger volumes, lower thresholds, more sophisticated photomultipliers. LiquidO is a qualitative change of strategy — accepting a worse traditional figure of merit (transparency) in exchange for a previously unavailable capability (topology). It rhymes structurally with the LArTPC’s decision to combine ionization tracking with scintillation timing in a way that conventional Cherenkov or scintillator detectors do not.

Whether LiquidO becomes a workhorse technology like LArTPC has become for accelerator neutrinos depends on whether scaling it up preserves its advantages. The trade-off is real: a multi-kiloton transparent scintillator delivers better energy resolution and is much easier to build; a multi-kiloton LiquidO delivers event topology that no other detector at that scale provides. Different physics targets will pick different sides of that trade-off, and reactor monitoring is the application where LiquidO’s particular advantage is most direct.

Summary

LiquidO is a novel detection technique in which a liquid scintillator is deliberately made opaque on a centimeter scale, so that the photons produced by a charged particle are trapped near their origin and read out by a dense lattice of wavelength-shifting fibers. The resulting three-dimensional light pattern is a voxelized image of the event, combining energy measurement with event topology in a single device. The technique enables event-by-event tagging of positrons, gammas, electrons, neutrons and muons through their distinctive light shapes, dramatically reducing backgrounds in inverse-beta-decay detection. Its near-term application is reactor antineutrino monitoring with nonproliferation goals; longer-term targets include geoneutrinos and the diffuse supernova background. As of 2026 the technology has demonstrated its principle at the kilogram-to-tonne scale and is moving toward a kiloton prototype that would establish whether it becomes a major detector technology of the coming generation.

FAQ

Frequently asked

What is LiquidO?
LiquidO is a novel particle-detection technique in which a liquid scintillator is engineered to be deliberately opaque — its scattering length is shortened to a few centimeters rather than the meters typical of standard scintillators. The light produced by a charged particle is trapped close to where it was made, so each photon is collected by the nearest of a dense lattice of wavelength-shifting fibers strung through the volume. Reading out each fiber individually produces a three-dimensional light image of the event, in which the spatial distribution of the trapped photons traces the original particle path. The result is a detector that simultaneously measures energy and reconstructs topology — a calorimeter and a tracker in the same device.
Why deliberately make the scintillator opaque?
Transparency in conventional liquid scintillator is treated as a virtue because it lets photons travel meters to photomultiplier tubes mounted on the detector boundary, giving the largest possible light yield. The cost is that all directional and topological information about where the light came from is washed out — a single energy number is recovered but the shape of the event is lost. By making the scintillator opaque on a centimeter scale, LiquidO preserves the topology at the cost of needing a much denser readout system: thousands of wavelength-shifting fibers strung through the volume rather than a few hundred phototubes on the boundary. The trade-off pays off when distinguishing particle types from event shape matters — for example separating electrons from positrons by detecting the two 511 keV annihilation gammas around the positron stopping point.
What experiments are using LiquidO?
LiquidO is in active research and development by a collaboration centered at IJCLab in France, with prototype detectors demonstrating the technique at the kilogram scale. Its first major physics target is reactor antineutrino monitoring, where the ability to identify individual particles event-by-event would dramatically reduce backgrounds and enable nonproliferation applications. Larger-scale plans include geoneutrino measurements and contributions to the diffuse supernova background search alongside SK-Gd. None of these is yet a multi-ton physics experiment, but the technique has progressed from concept to demonstrator over the past five years and is being evaluated for inclusion in future ton- and kiloton-scale detectors.