ScintIQ™ Custom Scintillation Detectors  •  Data Sheet

LaBr3(Ce) Lanthanum Bromide Scintillation Detectors

Cerium-doped lanthanum bromide delivers the highest energy resolution of any commercially available scintillator, with a typical 3.0% FWHM at 662 keV. The material is fast, bright, and well-suited to high count-rate gamma spectroscopy. An intrinsic background from La-138 and the Ac-227 decay chain is a known tradeoff and must be accounted for in low-background counting scenarios.

Density 5.07 g/cm³
Resolution 3.0% FWHM @ 662 keV
Emission 370 nm
Decay Time 16-20 ns
Hygroscopic Yes
Last revision: 20-01-2025  |  Rev. 0

1Overview

LaBr3(Ce) sets the benchmark for energy resolution among inorganic scintillators in routine production. At 662 keV (Cs-137), a 51 x 51 mm crystal achieves approximately 3.0% FWHM, well ahead of NaI(Tl) at roughly 7% and CeBr3 at approximately 4%. The photon yield is approximately 66,000 photons per MeV, and the decay time of 16 to 20 ns (size dependent) allows high count rates without excessive pile-up.

The material is hygroscopic and requires a sealed, hermetic housing. Its high refractive index (2.09 at 380 nm) is well matched to standard borosilicate and synthetic silica optical windows with appropriate coupling.

3.0% FWHM
Typical energy resolution at 662 keV (Cs-137)
Best-in-class among production scintillators

When to Choose LaBr3(Ce)

Choose LaBr3(Ce) when gamma energy resolution is the primary selection criterion. Isotope identification in complex or mixed-source fields, medical isotope quality control, and nuclear security screening all benefit from the material's sharp photopeaks and fast response. For applications where the intrinsic La-138 background at approximately 1.4 MeV would interfere with the signal of interest, CeBr3 is a lower-background alternative at the cost of slightly reduced resolution.

Intrinsic background note: LaBr3(Ce) contains natural La-138 (0.09% abundance), which produces a continuous beta spectrum and gamma lines visible in the detector's own background. Alpha lines above 2.5 MeV from the Ac-227 decay chain are also present. Both effects are intrinsic to the material and cannot be eliminated by shielding. Low-background measurements at energies near these features require careful background subtraction or a change of material.

2Specifications

ParameterValueNotes
Density5.07 g/cm³
Ce concentration (typical)0.5 mole percent
Maximum emission wavelength370 nmUV/visible; bialkali PMT or SiPM with UV-extended response
Decay time (typical)16-20 nsSize dependent
Refractive index2.09At 380 nm
Photon yieldApprox. 66,000 / MeVRelative light yield ~150 vs. NaI(Tl) = 100
HygroscopicYesRequires hermetic sealed assembly
Typical energy resolution @ 662 keV3.0% FWHM51 x 51 mm crystal; ~2.7% achievable with optimized coupling (verify)
Maximum dimensions76 mm diameter, 76 mm highLarger custom sizes: verify availability
Intrinsic background (unshielded, 51 x 51 mm)Approx. 2.5 counts/s/cm³Beta/gamma continuum from La-138

All values from the authoritative source datasheet (rev. 20-01-2025). Items marked "verify" are pending confirmation against current production data.

3Energy Resolution & Performance

LaBr3(Ce) resolves gamma lines that other scintillators blend together. The combination of high light yield, good proportionality, and fast decay makes it effective across a wide energy range. The figures below show typical spectra measured with a 51 x 51 mm crystal.

Resolution Comparison at 662 keV

LaBr3(Ce)
~2.7-3.0%
Best in class
CeBr3
~4%
No La-138 bg
NaI(Tl)
~7%
Standard reference
Cs-137 662 keV gamma spectrum measured with 51 x 51 mm LaBr3(Ce) crystal
Cs-137 (662 keV) gamma spectrum acquired with a 51 x 51 mm LaBr3(Ce) crystal. The sharp photopeak and favorable peak-to-Compton ratio illustrate the material's best-in-class energy resolution.
Th-228 2605 keV gamma spectrum measured with 51 x 51 mm LaBr3(Ce) crystal
Th-228 (2605 keV) spectrum with 51 x 51 mm LaBr3(Ce) on a log scale. High-energy gamma lines remain well-resolved, demonstrating the material's performance across a broad energy range.

4Intrinsic Background

The natural abundance of La-138 (approximately 0.09%) produces a characteristic background in the beta/gamma spectrum at a rate of approximately 2.5 counts per second per cubic centimeter in an unshielded 51 x 51 mm crystal. In addition, alpha lines above 2.5 MeV arise from the Ac-227 decay chain associated with trace actinide impurities in the lanthanum feedstock.

For most spectroscopy tasks, these features are predictable and can be subtracted with a measured background file. In extremely low-background counting or in searches for signals near the La-138 gamma at 1.4 MeV, CeBr3 is the preferred alternative. It is free of the La-138 contribution while retaining high light output and fast decay.

Typical intrinsic background spectrum of unshielded 51 x 51 mm LaBr3(Ce) crystal
Typical background spectrum of an unshielded 51 x 51 mm LaBr3(Ce) crystal (log scale). Visible features include the K-40/La-138 beta/gamma region, the Th-227/Ra-223 series, and alpha lines from Bi-211, Rn-219, and Po-215 above 700 channels. Background rate is approximately 2.5 c/s/cm³.

5Typical Applications

  • Isotope identification (RIID / NORM screening): Sharp photopeaks enable confident isotope library matching in complex mixed-source fields.
  • Nuclear security and border monitoring: High resolution and fast counting support rapid threat discrimination at portals and checkpoints.
  • Medical isotope quality control: Resolves closely spaced gamma lines in radiopharmacy production and dose calibration.
  • Environmental gamma spectrometry: Resolves Eu-152, Cs-134/Cs-137, and other environmental radionuclides that NaI blends together (background subtraction required near La-138 features).
  • Nuclear research and physics: Fast decay and high rate capability suit coincidence measurements and time-of-flight experiments.
  • Homeland security and defense: Used in handheld, backpack, and vehicle-mount systems where resolution and portability both matter.
  • Industrial gauging and process control: High count-rate tolerance is an advantage in high-flux industrial environments.

6Available Configurations

ScintIQ LaBr3(Ce) detectors are built to order. Standard configurations cover a range of crystal sizes up to 76 mm diameter by 76 mm high. Larger custom geometries are available; contact us to verify feasibility and lead time.

Configuration OptionDetails
Crystal sizes (standard)Up to 76 mm diameter x 76 mm high; common standard sizes available (verify current stock)
Readout optionsPMT (bialkali, UV-extended) or SiPM; photodiode readout not recommended due to mismatch at 370 nm emission
HousingHermetic sealed assembly required; aluminum or mu-metal housings available (verify)
Window materialBorosilicate glass or synthetic silica (quartz); quartz preferred for improved UV transmission at 370 nm (verify)
Voltage divider / preamplifierMatched dynode chain or integrated preamp options; specify with order (verify)
MCA / electronics pairingCompatible with ScintIQ TOPAZ-HR, bMCA-Ethernet, bMCA-USB, and bPAD readout electronics
Custom assembliesPhoswich, well configurations, large-area arrays: inquire
Ordering note: Because LaBr3(Ce) is hygroscopic, all detectors are shipped as sealed assemblies. Field crystal replacement is not supported. Specify the PMT or SiPM model, housing style, and window material at the time of order.

7Request a Quote

Talk to a BNC Detector Engineer

Configuration, lead time, pricing, and compatibility with your readout electronics can all be discussed directly with the ScintIQ team. Custom geometries and volume orders welcome.

ScintIQ crystals are grown and finished with our long-standing scintillation partner in the Netherlands (Scionix Holland).