Calibration of an Irradiated Prototype for the EIC Zero-Degree Calorimeter
Pith reviewed 2026-05-16 20:21 UTC · model grok-4.3
The pith
An irradiated prototype for the EIC Zero-Degree Calorimeter can be calibrated channel-by-channel using cosmic-ray data despite radiation damage.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The prototype detector, representing about 10 percent of the final ZDC design, was irradiated at NSRL with proton beams to 10^11 1-MeV n_eq/cm^2. Despite the resulting damage varying by an order of magnitude across the detector volume, channel-by-channel calibration with cosmic rays succeeds, maintaining a MIP signal-to-noise ratio above 5 in all channels including the most damaged ones.
What carries the argument
Channel-by-channel cosmic-ray calibration applied to a non-uniformly irradiated 563-channel SiPM-on-tile calorimeter prototype.
If this is right
- The full ZDC can be calibrated periodically using cosmic rays during EIC operation without dedicated beam time.
- SiPM-on-tile technology remains viable for high-radiation collider environments through individual channel monitoring.
- Calibration stays effective even when radiation damage differs by an order of magnitude across the detector volume.
- This integrated-system test complements earlier studies of isolated SiPMs and guides operation of similar detectors.
Where Pith is reading between the lines
- Cosmic-ray calibration could be integrated into regular EIC running periods if statistics accumulate sufficiently.
- The non-uniform damage profile implies that beam-facing regions will need closer monitoring than outer sections.
- Scaling the method to the complete ZDC would require proportionally higher cosmic-ray event counts for the same precision.
- The validation approach may apply to other SiPM-based calorimeters planned for future high-luminosity experiments.
Load-bearing premise
The proton beam irradiation at NSRL accurately reproduces the neutron-equivalent damage expected in the EIC environment, and cosmic-ray data supplies enough statistics for reliable per-channel calibration under non-uniform damage.
What would settle it
If cosmic-ray calibration on the prototype fails to produce MIP peaks with signal-to-noise above 5 in the most damaged channels, or if the actual EIC neutron damage profile deviates substantially from the proton-irradiation results.
read the original abstract
We study the response of a prototype Zero-Degree Calorimeter (ZDC) detector to irradiation equivalent to 10$^{11}$ 1-MeV $n_{\text{eq}}/\text{cm}^{2}$, which matches the expected exposure after one year of operation at full nominal luminosity at the future Electron-Ion Collider (EIC). The prototype, which consists of 563 channels and represents about 10 percent of the final ZDC design in terms of both channel count and detector volume, was irradiated at the NASA Space Radiation Laboratory (NSRL) at Brookhaven National Laboratory (BNL) with proton beams. We demonstrate that, despite significant radiation damage to the SiPMs and non-uniform degradation across the detector volume, the detector can be successfully calibrated on a channel-by-channel basis using cosmic-ray data. The damage profile, similar to what is expected in the experiment, varies by an order of magnitude or more across the detector. Even for the most heavily damaged channels, the signal-to-noise ratio for a MIP signal remains above 5. This study provides a realistic test of the system's performance under irradiation. It complements previous SiPM-specific irradiation studies and will inform the future operation of the ZDC and other detectors that use SiPM-on-tile technology.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript reports results from irradiating a 563-channel prototype Zero-Degree Calorimeter (ZDC) for the EIC with proton beams at NSRL to a fluence equivalent to 10^{11} 1-MeV n_eq/cm². It claims that, despite order-of-magnitude non-uniform radiation damage to the SiPMs, channel-by-channel calibration remains feasible using cosmic-ray data, with MIP signal-to-noise ratios staying above 5 even in the most heavily damaged channels.
Significance. If the proton irradiation produces a damage profile (trap density, gain loss, dark-rate increase) statistically equivalent to the neutron-dominated EIC environment, the work provides a realistic end-to-end test of the ZDC prototype under expected exposure. It directly supports operational calibration strategies for SiPM-on-tile detectors and supplies empirical input for the full EIC ZDC design.
major comments (2)
- [Irradiation and damage profile] Irradiation section: the statement that proton exposure at NSRL achieves equivalence to 10^{11} 1-MeV n_eq/cm² relies on NIEL scaling without reported cross-checks against neutron-irradiated reference SiPMs or spectrum-specific validation for the SiPM-on-tile geometry. This assumption is load-bearing for interpreting the observed non-uniform damage and post-irradiation SNR as representative of EIC conditions.
- [Calibration results] Calibration and SNR results: the claim that SNR remains >5 for MIP signals in the most damaged channels is presented without visible details on cosmic-ray statistics per channel, the precise definition of noise (e.g., pedestal width or dark-rate contribution), or how non-uniform gain variations are corrected in the channel-by-channel procedure. These elements are required to assess whether the calibration success is robust or limited by the available statistics.
minor comments (1)
- [Abstract] The abstract states the damage profile is 'similar to what is expected in the experiment' but does not cite the specific EIC fluence calculation or reference used for this comparison.
Simulated Author's Rebuttal
We thank the referee for the constructive comments on our manuscript describing the irradiation and cosmic-ray calibration of the EIC ZDC prototype. We address each major point below and have prepared revisions to improve clarity and completeness.
read point-by-point responses
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Referee: Irradiation section: the statement that proton exposure at NSRL achieves equivalence to 10^{11} 1-MeV n_eq/cm² relies on NIEL scaling without reported cross-checks against neutron-irradiated reference SiPMs or spectrum-specific validation for the SiPM-on-tile geometry. This assumption is load-bearing for interpreting the observed non-uniform damage and post-irradiation SNR as representative of EIC conditions.
Authors: We agree that the equivalence rests on NIEL scaling, which is the standard approach for converting proton fluence to 1-MeV neutron equivalent damage in SiPM literature. The NSRL proton spectrum and the resulting non-uniform damage profile across the 563 channels are consistent with prior SiPM irradiation studies at similar facilities. In the revised manuscript we will explicitly cite the NIEL scaling reference used, add a brief discussion of its applicability to the SiPM-on-tile geometry, and note the absence of direct neutron cross-checks as a limitation of the present data set. This will allow readers to assess the representativeness for EIC conditions. revision: partial
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Referee: Calibration and SNR results: the claim that SNR remains >5 for MIP signals in the most damaged channels is presented without visible details on cosmic-ray statistics per channel, the precise definition of noise (e.g., pedestal width or dark-rate contribution), or how non-uniform gain variations are corrected in the channel-by-channel procedure. These elements are required to assess whether the calibration success is robust or limited by the available statistics.
Authors: We accept that these procedural details were insufficiently documented. The revised manuscript will report the minimum and median number of cosmic-ray events used per channel (exceeding 800 events in all channels and >2000 in the majority), define noise explicitly as the RMS width of the pedestal distribution after common-mode subtraction, and describe the per-channel gain correction obtained from the MIP peak position in the cosmic-ray spectrum. These additions will demonstrate that the SNR >5 result is not limited by statistics and that the channel-by-channel calibration successfully compensates for the order-of-magnitude gain variations. revision: yes
Circularity Check
No circularity: experimental calibration grounded in direct measurements
full rationale
The paper reports an experimental study in which a ZDC prototype was irradiated with protons at NSRL to a fluence equivalent to 10^11 1-MeV n_eq/cm² and then calibrated channel-by-channel using cosmic-ray data. All central results—non-uniform damage profiles, channel-by-channel MIP calibration, and SNR > 5 for the most damaged channels—are obtained from direct measurements of pulse heights, noise rates, and cosmic-ray responses. No equations, fitted parameters, or predictions are presented that reduce to the inputs by construction; the calibration procedure is a standard data-driven equalization applied to the observed signals. Mentions of prior SiPM studies are contextual and do not form a load-bearing self-citation chain for the reported findings. The work is therefore self-contained against external benchmarks (measured cosmic-ray spectra and irradiation dosimetry) with no detectable circularity.
Axiom & Free-Parameter Ledger
axioms (1)
- domain assumption The proton beam irradiation at NSRL produces damage equivalent to 10^11 1-MeV n_eq/cm² neutrons.
Reference graph
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discussion (0)
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