- Article
16 Pages
Accelerator capabilities beyond those of conventional drivers for compact accelerator-driven neutron sources (CANSs) are needed to serve applications that require high neutron flux, while remaining compact. These applications include—among others—fusion reactor materials testing, medical isotope production, tritium breeding, and nuclear waste transmutation. The deuteron cyclotron auto-resonance accelerator (dCARA) has been proposed as a compact CANS driver that would replace the conventional radiofrequency quadrupole and superconducting radio frequency linac chain with a single rotating-mode transverse electromagnetic cavity operating in a multi-tesla magnetic field. This paper provides an overview of the current readiness and feasibility of dCARA for this role by synthesizing the theory, simulation, and conceptual design studies, while employing specifications of available subsystem technologies. These include high-current deuteron ion sources, large bore multi-tesla superconducting magnets, and high-power radiofrequency systems. The simulations of ion acceleration in dCARA are consistent with analytical predictions. Furthermore, hardware for each major subsystem has already reached a high level of performance and technology readiness in developments for related systems. Integrated engineering design and experimental validation are ongoing, with the aim of extending CANS technology into high-flux application regimes based on use of the dCARA driver.
Instruments
29 October 2026



![Calibration field: (a) static mount for system levelling, (b) laser scanning system, (c) computer connected to the IMU, (d) mobile plate, (e) trapezoidal control targets, (f) displacement of mobile plate, (g) position of the GNSS antenna (adapted from [19]).](https://mdpi-res.com/instruments/instruments-10-00049/article_deploy/html/images/instruments-10-00049-g001-550.jpg)


![A 5 MeV electron beam is incident on a 2 mm thick tungsten target in a Geant4 [2] simulation to generate radiation. (a) shows the radiation spectrum, and (b) shows the photon energy profile. The energy profile indicates that pair production occurs [3], with the energy balance given by
E
γ
=
T
+
+
m
e
c
2
+
T
−
+
m
e
c
2
, where
T
+
and
T
−
are the kinetic energies of the positron and electron, respectively;
m
e
is the electron rest mass; and c is the speed of light. Above the pair-production threshold
2
m
e
c
2
=
1.022
MeV, a peak appears at 511 keV, corresponding to positron–electron annihilation radiation.](https://mdpi-res.com/instruments/instruments-10-00045/article_deploy/html/images/instruments-10-00045-g001-550.jpg)


![A diagram of the beam loss detection mechanism of the oBLM. The large blue arrows represent the beam loss shower, and the small green arrows represent captured Cherenkov photons. Reproduced from [1] with permission.](https://mdpi-res.com/instruments/instruments-10-00040/article_deploy/html/images/instruments-10-00040-ag-550.jpg)