Nuclear Detection

We have developed a superior resin for use in nuclear particle track detection.  Most of the CR-39 that is sold commercially today is not optimized for use in particle track detection.  Our material has excellent polymer cross linkage, so the disruption caused by a charge particle is readily apparent.  We have also developed automated feature identification and counting, and very simple etching and polishing procedures to detect more complex particle signatures deeper into the resin, such as the characteristic ‘triple tracks’ from high-energy neutron induced carbon disintegration into three alpha particles.  Our CR-39 particle tracks provide an immediate quantitative solution to your radiation detection needs.

We also offer new aerogel technologies for the containment and positioning of nuclear reactants, and for other nuclear applications.  Our silicon oxide and graphene aerogels may be manufactured over a wide range of densities and thicknesses to meet the needs of your custom applications.  Please contact us to discuss your planned applications in detail.

If you need temporal analysis of incoming radiation levels, or if you are interested in doing neutron or charged particle spectroscopy, then we offer solutions centered on new Silicon Photomultiplier (SiPM) detection of fast light flashes as charged particles strike an optimized scintillator material that has been custom-tailored to your application.  These new approaches offer highly integrated and compact design over conventional devices that used large and delicate photomultiplier tubes (PMTs). When coupled with our imbedded microcontroller and programmable gate array technologies on a I2C digital bus, this approach can improve and drastically minimize applications such as positron emission tomography (PET) for brain and cardiac imaging, and a wide range of other ultra-fast nuclear particle detection applications.

CR39

CR-39 for Nuclear Particle Track Detection

The thermoset polymer, CR-39, is used in nuclear particle tracing and calorimetry as a solid state nuclear track detector (SSNTD). When a high energy particle impacts the polymer it breaks bonds and allows for preferential etching during post-exposure processing. These etched tracks can then be observed and characterized under a microscope.

CR-39 is sensitive to many particles such as energetic protons, alpha-particles and heavier ions, and fast neutrons. Thermal/epithermal neutrons can be detected by doping CR-39 with boron to produce the 10B(n,a)7Li reaction and subsequent alpha-particle detection.

This SSNTD has a wide variety of applications of radiation measurement, including home radon detection, dosimetry, and is a less visceral display of radiation damage for educators.

Click here for more information for best practice for the use of CR-39.

Varied energy alpha particles in CR-39

5.5 MeV alpha particles striking the CR-39 from various angles.

5.5 MeV alpha particles with energies moderated by passing through aerogel.

Alpha particles striking CR-39 through large aperture
CR-39 overexposure to alpha particles

Alpha particles striking CR-39 through a large aperture.

Overexposure of CR-39 to alpha particles.

CR39 Recommended Best Practice

CR-39 Recommended Best Practice

All CR-39 squares should be stored well away from radiation sources in a cool-dry environment, and temperatures not to exceed 86°F (30°C). 

CR-39 may be used to measure the particle tracks and accumulated radiation exposure history from alpha particles, other charged particles of adequate mass, and from the recoil of protons in the CR-39 that are struck by energetic neutrons.  In addition, for the detection of thermal neutrons, a thin boron layer coating may be requested on one side of the CR-39 to produce charged lithium-7 and alpha particles when the boron captures the thermal neutron.  The comparison of the boron-coated side of the CR-39 to its opposite bare side provides an accurate estimate of the thermal neutron flux in most radiation measurement environments. 

CR-39 squares are delivered in a hermetically-sealed thin plastic package with a secondary protective film on both sides that will block all alpha particles, and that will keep all alpha emitting gasses from accessing the CR-39.  We recommend that you apply two squares to each measurement.  Keep one sealed as delivered in close-proximity (the control square) to the square that you strip out of its hermetic seal to use to make your measurements (the experimental square). Once your measurement are complete, place both the control and the experimental square into the pouch provided, and ship both back to BSI for processing and analysis.  Only the experimental square will detect alpha particles (and possibly other charged particles) from your experiment, while the control will detect the energetic neutron flux from your experiment (if any), and possibly the high-energy neutrons generated by solar geomagnetic storms and other sources of neutron radiation from the environment surrounding your apparatus.  It will also detect neutrons from these environmental sources during shipping from / to your site, and while in storage. 

If you plan to detect fusion neutrons from DT reactions, or neutrons from any other source that are expected to exceed 8 MeV in kinetic energy, then we encourage you request a more advanced analysis that will image and count tracks at the surface to detect alpha particles and epithermal neutrons as usual, followed by a deep etch (to at least 300 microns below the surface) to detect ‘triple-track’ alpha particles that are produced by these high energy neutrons as they disintegrate carbon atoms in the CR-39.  These deep interactions are produced only by highly energetic neutrons, and they occur with equal probability throughout the bulk of the CR-39 squares.  We recommend that you contact BSI for a brief consultation to assure that we prepare and analyze your CR-39 squares in the most appropriate way to accurately support your planned measurement protocols.

Varied energy alpha particles in CR-39

5.5 MeV alpha particles striking the CR-39 from various angles.

5.5 MeV alpha particles with energies moderated by passing through aerogel.

Alpha particles striking CR-39 through large aperture
CR-39 overexposure to alpha particles

Alpha particles striking CR-39 through a large aperture.

Overexposure of CR-39 to alpha particles.