1. Introduction
The background models for ordinary particles and their contributions in direct detection experiments, which search for dark matter particles interacting with ordinary matter in a terrestrial detector target, are extremely important. These background models are used in various ongoing and future dark matter search experiments (see, for example, [
1,
2,
3,
4,
5,
6,
7,
8,
9]) and are studied, in detail, for their contributions in the signal search region using extensive Monte Carlo simulations. To reduce background contributions from ordinary particles, typically the direct dark matter search experiments are placed deep in underground laboratories, where contributions from ordinary background sources, such as cosmic rays, are greatly reduced. However, the environmental background still exists and needs to be known or measured.
Underground facilities in North America nowadays represent suitable places to perform numerous experiments that are highly sensitive to any source of background radiation. Reviews of the major low-level background underground facilities in North America that are currently available for “state-of-the-art” physics experiments are provided by [
10,
11]. The deep underground facilities are required by the science community due to rigorous radiation background constraints to afford shielding from penetrating cosmic rays and their induced by-products [
12]. Many modern research topics require laboratory environments as free as possible from cosmic radiation and radioactive isotopes. A dedicated effort to determine how to comply with such requirements and, at the same time, to provide a comprehensive list of current and potential underground experiments has been made recently for SNOLAB in [
13,
14] and the Sanford underground research facility at Homestake in [
15,
16].
SNOLAB is located near Sudbury, Ontario, at the operating Creighton nickel mine (owned by Vale Inco, now Vale Canada Limited) and has vertical access [
13,
14]. It is an extension of the existing facilities that were constructed originally for the Sudbury Neutrino Observatory (SNO) solar neutrino experiment [
14]. The entire lab, which hosts many experiments, is operated as a large clean room.
SNOLAB has a rather complicated layout (see
Figure 1). It consists of an “old” part that hosted the original SNO [
17] experiment (now transformed to SNO+; see the latest development in [
18]) and a relatively “new” part that has been excavated to host many experiments, and that shares the same lab infrastructure. It is currently the deepest underground laboratory in North America, with a 2 km overburden (estimated to be equivalent to 6000 m of water). It is surrounded by norite granite rock. SNOLAB currently houses several experiments, including the dark matter experiment using argon pulseshape discrimination (DEAP-3600), currently the world’s largest and most sensitive liquid argon dark matter detector, which is located in Cube Hall (see
Figure 1 and cross-section of Cube Hall with DEAP-3600 experiment in
Figure 2). The Cube Hall clean room space is approximately 18.3 m in length, 15 m in width, and 19.7 m in height and includes the experimental areas hosting MiniCLEAN [
19] and DEAP-3600 [
20] experiments, as well as ancillary spaces. DEAP-3600 and MiniCLEAN are searching for interactions of weakly interacting massive particles (WIMPs) with argon nuclei. WIMPs are currently the best candidates to explain dark matter, which makes up roughly 85% of the mass content of the universe. At the time of the ambient dose measurement with integrating passive detectors, the MiniCLEAN experiment was in the decommissioning state. Currently, the Cube Hall clean room is also occupied by the light dark matter particle candidate search NEWS-G (New Experiments With Spheres-Gas) experiment [
21].
There are various ways to characterize the low-level gamma-ray background at underground laboratory facilities. For example, a low-background high-purity germanium (HPGe) gamma spectrometer has been used to measure environmental radioactivity (i.e., the natural radioactivity) in the underground Callio Lab facility [
22]. Specific to Cube Hall at SNOLAB, some techniques used to characterize the electromagnetic background at the DEAP-3600 detector are discussed in detail in [
6]. DEAP-3600 has exquisite control of radioactive backgrounds from the argon, detector materials, and surrounding rock. The detector (originally designed to host 3600 kg) consists of a 3.2-tonne quantity of liquid argon inside a radiopure acrylic vessel. Attached to the acrylic vessel are 255 photomultiplier tubes (PMTs) 8” in diameter, which are sensitive enough to detect single photons. The PMTs are separated by 50-cm-long 8” diameter acrylic light guides [
20]. The detector is placed inside an 8-m-tall water tank (see
Figure 2) to shield it from radioactivity in the rock and to tag cosmic ray muons.
The Physikalisch-Technische Bundesanstalt established an underground laboratory for dosimetry and spectrometry at the Asse salt mine, near Braunschweig, where a coaxial low-background HPGe detector with extended shielding was exploited [
23]. A detailed investigation of the dose rate within the underground low-level background laboratories at the Unirea salt mine (Slanic-Prahova) has shown a relatively uniform distribution varying between 1.3 ± 0.3 nSv h
−1 outside the Low-Level Background Laboratory (LLBL) and 1.6 ± 0.3 nSv h
−1 inside it [
24,
25]. This measurement was performed by means of a calibrated scintillator rate meter. Two rounds of measurement of ambient dose rate were obtained at a significant number of points situated inside the Praid salt mine, by using the very sensitive Romanian thermoluminescent dosimetry (TLD) system, as reported in [
26]. Authors in [
26] showed a consistency between gamma-ray spectrometry results and results from the TLD-based system.
It is well known that the TLD systems have the advantage of being cheap, compact, easy to manipulate and allow the monitoring of various places in an extended location, such as Cube Hall. The continuous survey of the areas of interest, without disturbing the experiments can be assured by using TLD-based systems. Thus, one registers every variation in the background values that could influence the basic measurement results. Measurements have been performed around the water shielding for the DEAP-3600 experiment [
5,
20]. As can be seen from the report on natural gamma-ray backgrounds in the underground LLBL ([
22,
25] or [
23]), the rate could be quite uniform and stable all over the lab, or it could vary (see, for example, [
26]).
Many factors could contribute to either uniform or non-uniform distributions of natural environmental gamma-ray backgrounds in underground labs. In this paper, we apply a measurement technique using many integrating passive detectors, such as TLDs, that are used successfully at Chalk River Laboratories (CRL) to monitor doses. The methods and approach that we used are subject to a regular annual independent blind test from the Canadian regulator that CRL Dosimetry Services has successfully passed.
The DEAP-3600 detector searches for direct interaction with dark matter particles using noble gas. Using extensive Monte Carlo studies, optimization of the water shielding has been performed for the muon background rejection and the protection against environmental gamma background. These studies assume a uniform distribution of environmental gamma flux background around a large-scale detector, such as DEAP-3600. This approach allows us to get a very conservative upper limit. As we mentioned previously, the natural gamma-ray background around the detector is assumed to be uniform. Integrating passive TLD detectors is the tool of choice for testing this assumption.
Scope of Work
For this project, we have identified the following objectives:
First, would it be possible to use integrating passive detectors, such as TLDs, for ambient dose and dose rate measurements in low-level background underground facilities, in particular at SNOLAB? To the best of our knowledge, SNOLAB is one of the world’s deepest operating underground facilities [
27]. The underground laboratory was created to provide an almost background-free environment for very sensitive experiments, such as the direct observation of potential dark matter particle candidates. One of the current challenges was that SNOLAB hosts an operational DEAP-3600 detector [
28], which, on a regular basis, takes calibration measurements using quite strong external sources; therefore, it was a logistical challenge to find and organize a four-week-long interval for TLD deployment.
Second, in the ongoing experiment, the performance of the detector shielding against various types of background radiations is studied via careful and detailed Monte Carlo simulations. One of the assumptions in these studies is the distribution of background radiation, such as gamma radiation, around the detector shielding. A typical assumption is that at the detector shielding surface, the radiation distribution is uniform. Here, we would like to test this assumption.
For next-generation ultra-sensitive experiments for the direct detection of dark matter using a multi-ton noble liquids technology, such as DarkSide [
8] and DARWIN [
4,
9]; the knowledge of the external sources of backgrounds is ultimately important. Typically, the design of the shielding from external sources of backgrounds for such experiments is made based on conservative and independent estimates for the upper limit of environmental gammas assuming uniform distributions. With this work, we would like to show that integrating passive detectors, such as TLD, are capable of measuring ambient dose and dose rate around dark matter experiments. Proposed next-generation direct-detection dark matter experiments will be located in the ultra-low-level ambient doses surroundings. The deployment of the integrating passive detectors, such as TLDs, is recommended at the beginning and at the end of the operational campaign for the dark matter detector with an exposure period of around three months or more (see
Section 4) to reach a reasonable uncertainty for ambient dose and dose rate measurements.
2. Materials and Methods
To obtain a cumulative environmental dose measurement of the direct gamma radiation, integration dosimeters, such as TLDs, are used. A typical CRL dosimeter system has two thermoluminescent elements to measure radiation exposure, one of which uses an “open” window to minimize attenuation of beta radiation; the second incorporates an aluminum filter to attenuate beta radiation and, at the same time, minimize the attenuation of low-energy photon radiation.
All environmental photon doses in this work were measured using integrating passive detectors, such as Harshaw LiF:Mg,Ti chips, which have natural isotopic abundances of
6Li and
7Li. This material is widely known as TLD-100. The chip dimensions are 3.2 × 3.2 × 0.89 mm. This TLD chip is referred to as a “thick” chip (see
Figure 3).
Figure 3 also shows integrating passive detectors that are used to measure doses from photon and beta radiation. These doses are measured using Harshaw LiF:Mg,Ti chips enriched in the isotope
7Li (i.e., 99.99%
7Li). This material is widely known as TLD-700. The chip dimensions are 3.2 × 3.2 × 0.38 mm. This TLD chip is referred to as a “thin” chip. As we were interested in the environmental photon doses, the dose readings from a “thin” chip were not used in this work.
Before being mounted on dosimeter plaques, all TLD chips undergo a process of sensitization, whereby a very large dose is delivered to the chips in a gamma cell, after which they are annealed at elevated temperatures in the presence of ultraviolet light. This results in a quasi-permanent increase in sensitivity by a factor of nominally three. The TLD chips are mounted on Kapton tape, which is glued onto a stamped aluminum plaque, the chips occupying cavity positions in the plaque.
Dosimeter plaques, when issued for use, are inserted into badges, which consist of a two-piece plastic molding with appropriate recesses and cavities for the dosimeters. The badge casing contains 1.85-mm-thick aluminum filters positioned in the front and back such that the “thick” TLD chip is positioned between them in the assembled dosimeter badge. The badge casing also has two cavities, front and back, such that the “thin” TLD is not filtered by the badge casing. To protect the dosimeters from dust and light, opaque tape with a mass thickness of nominally 7 mg cm−2 (≃60 m) is wrapped around the badge casing to cover the front and back cavities.
The front of the badge casing contains an identification card with a mass thickness of nominally 0.107 g cm
−2, consisting of 80% polyvinyl chloride and 20% polyethylene terephthalate. Cut-outs in this card are positioned such that the plaque identification (ID) is still visible and such that no additional filtration is introduced in front of the “thin” chip.
Figure 3 shows one of the badges used in this work. It has been opened to reveal its internal structure.
The aluminum filter in the front and back of the “thick” TLD chip also provides a fundamental function, whereby the primary radiation field that consists of indirectly ionizing radiation (for example, gamma rays) that passes through the filter medium may generate secondary charged particles. The secondary charged particles reach charge-particle equilibrium (CPE) within the sensitive volume of the TLD chip, assuming that the primary radiation uniformly irradiates the entire assembly (aluminum filter and TLD chip) and is negligibly attenuated in traversing it. The TL mechanism under CPE is described in detail elsewhere [
29].
TLD plaques are read on Harshaw 6600 automatic TLD readers. For simplicity, in the text, we refer to them as “reader(s)”. The TLD monitoring systems for CRL use calibration irradiation facilities that are traceable to Canadian national standards through the free-in-air exposure quantity. The dosimetry services at the CRL site calibrate their “thick” and “thin”-dose TLD monitoring systems to report personal dose equivalent.
Sources for photon irradiation energy and angle type-testing consisted of
60Co gamma-ray sources from the Health Physics Irradiation Facility at CRL. Requirements for energy and angle type-testing for the CRL dosimetry system used in this work are outlined in a regulatory document [
30]. The Health Physics Irradiation Facility photon irradiations are traceable through measurements using ion chambers and electrometers with a calibration that is traceable to national reference standards.
For calibration irradiations, the response by several influencing quantities are expressed relative to those under reference conditions, or else the variability is type-tested without regard to absolute dose. For these type-tests, it is sufficient that the irradiation geometry is reproducible and that the exposure time is accurately known.
In general, integrating passive detectors, such as TLD chips, which are made by the same manufacturing process, have the same amount of TL materials on the elements, but since this amount is a very small quantity, the amount of TL materials on each element can vary slightly. Thus, the element response of the TLD changes with the variation in the amount of TL materials. Furthermore, the element response of the TLD is gradually decreased by physical conditions, such as impact, heat, humidity, etc., due to repeated use. It is, therefore, necessary to check and compensate for the element response periodically to obtain more accurate and reliable TLD readouts for dose assessment.
The calibration of all the TLD was performed at CRL, where the gamma irradiators are controlled under a rigorous quality assurance program. The photon fields used in this work were gamma rays from
60Co that were produced following the methods of ISO 4037-1 [
31]. Gamma-ray irradiations for TLD calibration were performed using the GC60 Gamma Beam Irradiator from Hopewell Designs located at CRL.
By using a set of calibration dosimeters and a gamma-ray
60Co irradiation source, the reader’s performance can be kept at a constant level in spite of high-voltage changes, repairs, dirt accumulation, or long-term drift. At CRL, typically, a set of six calibration dosimeters are used that are exposed to a known photon dose. The calibration factor for the readers is known as the reader calibration factor or
. This factor converts the raw charge data from the PMTs (in nanocoulombs) to dosimetric units (rems, for example) for input to the following formula:
where
is the measured dose in detector
i,
is the number of counts in detector
i,
is the reader calibration factor, and
is the average of the count of the zero-dose readings (or background readings). Note that the same formula could be used to deduce
for the reader.
The uncertainty of the
could be estimated based on the quality assurance and quality control program at CRL Dosimetry Services, which requires annual independent tests for “thick” TLD chips as outlined in previous [
32] and current [
30] Canadian regulatory documents. For the independent test, 50 “thick” TLD chips were submitted to an external organization where chips were exposed to doses that were not revealed to CNL. The doses were measured afterward, in-house, by the CNL Dosimetry Services personnel following the standard operational practice. The results were submitted to the external organization for validation. For the time when the “thick” TLD chips had been deployed in Cube Hall, one could estimate uncertainty in
as a relative standard deviation of the measurements of 1.6% [
33]. For the time when the “thick” TLD chips had been removed from Cube Hall and analyzed, one could estimate uncertainty in
of 2.0% [
34]. The organization used for the independent test delivers multiple exposures for “thick” TLD chips expressed in milliroentgen with combined uncertainty at the point of measurements of approximately 0.6%, corresponding to one standard deviation. At CNL, the calibration process for “thick” TLD chips used in this work is linked to external doses expressed in milliroentgen. Therefore, we report ambient dose and dose rate measurements for SNOLAB in roentgen. The conversion factor from roentgen to SI unit gray will be provided further on.
The calibration factor for dosimeters is called the element correction factor, or . The is used as a multiplier with the reader output to make the response of each dosimeter comparable to the average response of a designated group of dosimeters maintained as calibration dosimeters. Again, to compensate for the element response of the TLD, an is usually used. The is defined as the light output of one TL element relative to the average light output among similar elements within a group of reference TLDs. A set of calibration dosimeters is used as group reference TLDs. To generate s, a method for normalizing the light output of an element to the actual delivered dose is usually used.
For the determination of
for each “thick” TLD chip used in this work, CRL Dosimetry Services also follow the best industrial practices and requirements outlined in the current [
30] and previous [
32] Canadian regulatory documents. Moreover, it has been shown that for the TLD chips of the same type as TLD-100 [
35], the
is portable to a different dose. In other words, the
obtained for a particular dose could be used for a different dose as well.
To test the reproducibility, a “thick” TLD chip was cleared, exposed to a certain dose, and read. This cycle was repeated a few times. The details on the particular dose used for the
calculation include information owned and developed by CNL that has particular value to CNL’s business interests. The final result is expressed as a relative standard deviation of the measurements and is less than 3%. Typical batch homogeneity (or uniformity) for “thick” chips is expressed as a relative standard deviation of 4% to 5% and represents the variation in examined samples containing a set of TLD-100 chips that are irradiated to a certain dose value. The uniformity and reproducibility of TLD-100 dosimeters are also studied in detail elsewhere [
36] and reported as 4% for both.
Prior to
generation, the TLD reader must be calibrated to obtain the correct light output of the TL element. The
s for the first irradiation of the reference TLDs are calculated by the following equation:
where
is the element correction factor in detector
i,
A is the average of the counts of the set of calibration dosimeters, and
is the count in the detector
i exposed to the same dose as a set of calibration dosimeters. Combining Equations (
1) and (
2), the ambient dose could be obtained.
In addition to the dosimeters deployed at the water shielding of the DEAP-3600 detector, a set of representative control dosimeters of the same type was kept close to the DEAP-3600 detector in a well-shielded location during the measuring period. We used a tungsten cube box (with sides approximately 10 cm long and around 12 mm thick) as shielding to store control dosimeters. The control dosimeters are used to monitor dose that does not belong to the test exposure of the environmental gamma radiation, that is, the dose to which dosimeters are also exposed while they are not in use (during storage and transport when control dosimeters have been taken out of the shielding). This includes doses from background radiation and other sources that are not related to testing exposure.
When processed, the average dose determined using the set of control dosimeters is subtracted from the doses determined using deployed dosimeters so that the net ambient dose can be accurately determined. As we mentioned previously, control dosimeters were shipped with deployed dosimeters during transport in order to identify potential exposure to radiation during transportation and storage. Precautions were taken to protect deployed and control dosimeters from being contaminated with radioactive material. In order to obtain reliable and valid dose results from the measurement at SNOLAB, a rigorous quality assurance and quality control program in accordance with Canadian regulatory requirements [
30,
32] was followed by the CRL Dosimetry Services licensed provider. The precision, accuracy, and reliability of dose estimates by the CRL Dosimetry Services are successfully checked annually via an independent blind test by an external organization, which is mandated by the Canadian Nuclear Safety Commission [
30].
It had been anticipated that ethe nvironmental gamma background at Cube Hall in SNOLAB would be low and that the ambient dose measurements with integrating passive detectors would be close to the minimum detectable level of the TLD technology (in other words, the signal level would be comparable to the background level) [
37]. Therefore, special attention was applied to improving the quality of the measurements. In practice, we used two TLD-100 chips in the same badge casing when they were deployed for ambient dose measurements. This option allowed us to check the quality of the ambient dose measurements. If the ambient dose values at one deployed location were different by more than one standard deviation, these values were not used in the analysis. Dose response linearity and practical factors influencing minimum detectable dose for various thermoluminescent detector types are discussed elsewhere [
38].
3. Results
Detectors were deployed in the Cube Hall at SNOLAB. The majority of the TLDs were located around the DEAP-3600 water shield (see
Figure 4).
Table 1 provides ambient dose results for all detectors that pass the selection rule. Both “rear” and “front” TLD chips (see
Figure 3) results are provided as well as the average value and standard deviation. Detectors were placed in Cube Hall at SNOLAB on Thursday, 27 November 2018 around 2 p.m. and were taken out on Tuesday, 22 January 2019 around noon.
The total duration of the ultra-low-level ambient dose measurements in Cube Hall was 55 days and 22 h, or 1342 h. The deployment and removal of the TLDs took 2 h in total, and we took this time as an uncertainty in the time interval measurements; in other words, the deployment time interval of the passive integrating detectors was 1342 ± 2 h.
We applied the direct comparison method to calibrate the timer used for time records. For this, we followed the recommended practical guide “Stopwatch and Timer Calibrations” [
39] from the National Institute of Standards and Technology (NIST). We verified, following the guidance in [
39], that the timer was within the 0.02% tolerance and calibrated to better than 0.02%. Nevertheless, the accuracy of the time interval and tolerance of the timer used in the measurements of the ambient dose rate were neglected as they were much less than the standard deviation of the ambient dose measurements (see
Table 1).
The roentgen (R) is actually a legacy unit defined operationally as the charge produced by X-rays or gamma rays in one kilogram of air at standard temperature and pressure conditions (1 R =
C/kg). The unit is, therefore, still routinely employed in environments where X-rays and gamma rays are found [
40], such as in the Cube Hall cavity at SNOLAB. Values are often given in milliroentgen (mR). Historically, the roentgen was a convenient unit because early work with radiation was concerned primarily with X-rays, and radiation was commonly detected with instruments that measured the amount of ionization produced in air. The units of dose are the gray (Gy) and the sievert (Sv) in the SI system. In this work, we would recommend the use of roentgen for measured ambient dose in Cube Hall. The situation for dose units is similar to that for other SI units competing with older units. The older units nonetheless remain in common usage in Canada. If the SI dose unit Gy is required, the conversion factor is 8.8
Gy/mR [
41,
42].
Since experimental data on ambient dose in Cube Hall come from many locations (most of them around the DEAP-3600 water shielding), with each having its own characteristic variability, the problem centers on the appropriate selection of the data to obtain the “true” ambient dose value(s) for TLDs occupying the same badge. In order to achieve this, the statistical analysis should recognize the existence of variability both within the group (i.e., the ambient dose data from TLD badges with the same ID) and between groups (i.e., the ambient dose data from TLD badges with different IDs). Both types of variability are considered here to be random effects and are described by their associated components of variance. In reality, for a TLD badge with a unique ID, only two TLD chips located at the same place were deployed at Cube Hall. Therefore, we have checked via a calibration process (i.e., exposure of a TLD badge with a unique ID to a known dose) that, indeed, the measured dose values coming from the same badge TLD chips are the same within their variance (i.e., this is a “selection criterion” for ambient dose).
Table 1 shows solely the results for the TLDs that passed the selection criterion that was based on the comparison of the ambient dose results for the rear and front TLD chips located in the same badge. As mentioned previously, it was anticipated and verified during the calibration process that ambient dose values were within one standard deviation for the two TLD chips from the same badge. The subtracted control dosimeters dose that identified exposure to radiation during transportation and storage was 9.5 ± 1.1 milliroentgen.
The TLD detectors that were inside badges with IDs, from 4 to 24 (see
Table 1) were placed on the water shielding of the DEAP-3600 detector (see
Figure 4). Badge IDs 25 and 26 were placed next to the fire door (see
Figure 2). Badge ID 28 was placed on the deck of Cube Hall. Badge ID 29 was placed on the top of the water shield of the DEAP-3600 detector. The exact locations (i.e., within centimeter accuracy) of TLD badges with various IDs on the water shielding of the DEAP-3600 detector and around Cube Hall are not provided in this paper as such a determination was outside the scope of work for these studies (see
Section 1).
4. Discussion
As we mentioned in
Section 1, the first goal for this research was to identify if it is possible to use integrating passive detectors, such as TLDs, for ambient dose measurements at the SNOLAB low-level background laboratory. As one can see from
Table 1, it is indeed possible. The second goal was to check the uniformity of the background gamma radiation around the water shielding for DEAP-3600. The background radiation around the detector shielding was found to be not uniform.
Table 1 shows that within one standard deviation of the results from TLD dosimeters placed on the water shielding of the DEAP-3600 detector, there is significant non-uniformity in the results (by at least a factor of two). One of the reasons for the measured non-uniformity of environmental gammas around the DEAP-3600 water tank is the existence of the MiniCLEAN water tank in the Cube Hall next to the DEAP-3600 detector (see
Figure 4). This result has high importance in the assessment of background for the DEAP-3600 detector using Monte Carlo simulations.
On the other hand, the ambient dose and dose rate data presented in
Table 1 could be used as conservative and independent estimates for the upper limit of environmental gammas around the DEAP-3600 water shield. In other words, one could use the upper limit ambient dose value to estimate the thickness of the shield required for a detector, such as DEAP-3600, to become insensitive to the environmental gamma background. For that, one should use the ambient dose data only from the integrating passive detectors placed around the DEAP-3600 water shielding. In other words, the dose data from
Table 1 for badge IDs from 4 to 24 and badge ID 29 result in the ambient dose for the DEAP-3600 water shielding (
) and, taking into account the exposure period of 1342 h, the ambient dose rate (
) as follows:
Using a similar approach, one could estimate the upper limit of environmental gammas in the Cube Hall for any existing or potential large-scale detector. For that, one should use all data from
Table 1, which results in Cube Hall ambient dose (
) and ambient dose rate (
) as follows:
The results shown in Equations (
3) and (
4) are essentially average values and their statistical uncertainties. This approach should be enough for estimates of a conservative upper limit for environmental gammas. An alternative method that takes into account weighting factors or algorithms for the most frequent value could also be applied (see details in [
43] and [
44,
45], respectively) but are not discussed in this paper. As we mentioned previously, Equations (
3) and (
4) show conservative estimates for the upper limit of environmental gammas around the DEAP-3600 water shield and in the Cube Hall, respectively. Those values are useful for the estimation of the appropriate shielding that would significantly reduce the contribution from ambient dose in the signal search regions. It is obvious from the ambient dose and ambient dose rate results shown in
Table 1 that the distribution of environmental gammas around the DEAP-3600 water shielding is non-uniform. Consequently, due to the limited time of measurements (exposure period was 1342 h), the observed statistical uncertainty for some “thick” TLD chips presented in
Table 1 is large (relative statistical uncertainty of 17% for badge ID 20). The statistical uncertainty for ultra-low-level ambient dose and dose rate measurements observed in SNOLAB with “thick” TLD chips could be improved if the exposure period was extended to roughly six months. However, for practical operational reasons, the opportunities for such an exposure period are limited but potentially could be available at the end of the DEAP-3600 operation.
On the other hand, the deployment of multiple integrating passive detectors at the same time reduces the total exposure time that otherwise would be needed with a single active detector sequentially deployed at multiple locations. For example, for the ambient dose data presented in
Table 1, 1342 × 14 × 2 = 37,576 h (i.e., ≃1566 days, or ≃4 years) would be required with a single detector placed sequentially at the same locations in Cube Hall.
Direct dark matter search experiments, such as DEAP-3600, are very sensitive to the background in the observation area of the experiment. Typically, estimates of the background contributions from environmental gamma sources are based on measurements with thallium-activated sodium iodine (NaI(Tl)) or HPGe detectors that are exposed for a long time at various locations in the underground lab. Examples are, for the SNO experiment, a 15.6 kg NaI(Tl) crystal with an exposure of 1490 h (approximately 62 days and 2 h) and a 2.1 kg HPGe detector with an exposure of 20.65 h in the SNO cavern. A NaI(Tl) detector, also located at SNOLAB (see
Figure 1), was used to measure the gamma flux [
46] up to 10 MeV, while an HPGe detector was used previously to measure the gamma flux up to 6 MeV. Active detectors, such as NaI(Tl) and HPGe, for environmental gammas, have been used outside the Cube Hall at SNOLAB [
46], but those results cannot be compared with ours. However, the NaI(Tl) active detector was measuring ultra-low-level Cube Hall background at the time that “thick” TLD chips were deployed at Cube Hall, and the results will be available soon.
The use of a scintillator or semiconductor detector technologies to detect high-energy environmental gammas has a major disadvantage as their efficiency decreases with the increasing energy of the gamma radiation. By contrast, the use of integrating passive detectors, such as TLD, provides less energy-dependent exposure measurement results for gammas with higher energy [
47,
48]. Moreover, because of their size and weight, the integrating passive detectors, such as TLDs, could be deployed directly at the location where one would like to find the ambient dose from environmental gamma flux. Further, because those detectors are passive, they could be exposed for a much longer time to improve the accuracy of the ambient dose results. For example, some environmental TLDs used for measuring ambient dose and ambient dose rates at CRL locations are exposed for 6 or 12 months in the field.
On the other hand, one of the disadvantages of the use of integrating passive detectors, such as TLDs, in measuring ambient dose around an operational dark matter detector, such as DEAP-3600, is their inability to measure a time evolution. In other words, for measuring environmental ambient dose from gamma flux, one should not bring any strong external gamma sources that would be used, for example, to calibrate the gamma response of a large dark matter detector. Therefore, one of the best times to characterize the environmental ambient dose rate from gamma flux would be a long period before the deployment of a large-scale experiment in the underground location. That would allow the use of the measured ambient dose data for environmental gamma flux as input for Monte Carlo simulations in order to assess the performance of a particular large-scale detector at a certain underground location.
In principle, the use of integrating passive detectors, such as TLDs, to measure the ambient dose and dose rate could be complementary to the use of active detector technology, such as a scintillator or semiconductor. The deployment of inexpensive passive technology that provides ambient dose data for the same exposure interval from many locations and that is not dependent on the photon energy up to 10 MeV could be complementary to active detector technology that provides spectral photon information through a single long measurement [
46].
Moreover, the recent successful development of integrating passive technology, such as the optically stimulated luminescence (OSL) technique, provides access to lower-level detection limits [
49] for detectable activity compared with the TLD technique [
50]. OSL is a functionally straightforward but, at the same time, accurate and flexible detector technique, providing significant performance and operational advantages in comparison to the related TL technique with its major re-read capability [
50]. Potential applications of the OSL technique for ambient dose and dose rate measurements at a low-level background laboratory, such as SNOLAB, could reduce exposure time while reaching the same level of sensitivity as the TLD technique presented in this paper.