| Literature DB >> 35276701 |
Michael A Stone1,2, Emanuele Perugia1, Warren Bakay3, Melanie Lough1, Helen Whiston1, Christopher J Plack1,4.
Abstract
OBJECTIVES: The threshold equalizing noise (TEN(HL)) is a clinically administered test to detect cochlear "dead regions" (i.e., regions of loss of inner hair cell [IHC] connectivity), using a "pass/fail" criterion based on the degree of elevation of a masked threshold in a tone-detection task. With sensorineural hearing loss, some elevation of the masked threshold is commonly observed but usually insufficient to create a "fail" diagnosis. The experiment reported here investigated whether the gray area between pass and fail contained information that correlated with factors such as age or cumulative high-level noise exposure (>100 dBA sound pressure levels), possibly indicative of damage to cochlear structures other than the more commonly implicated outer hair cells.Entities:
Mesh:
Year: 2022 PMID: 35276701 PMCID: PMC9197144 DOI: 10.1097/AUD.0000000000001175
Source DB: PubMed Journal: Ear Hear ISSN: 0196-0202 Impact factor: 3.562
Fig. 1.Histograms of participant measures, grouped by color into either two groups (by hearing status, top panel, or music experience, lower panel), or three groups, noise exposure (NESI score, middle panel).
Fig. 2.The distribution of noise exposures as a function of age, stratified by 2° of hearing (normal or mild loss) and 3° of noise exposure (low, medium, and high).
Fig. 3.The distribution of absolute thresholds (first column) and TEN STRs (second two columns, separated by testing level) as a function of frequency, subgrouped by hearing category (top row), noise exposure (middle row), and music experience (bottom row). See text for further details.
Spearman correlations, ρ, of STRs at individual test frequencies as a function of absolute threshold (all measures obtained by use of pulsed tones)
| dB SL | Frequency (kHz) | n | ρ |
| s |
|---|---|---|---|---|---|
| 12 | 0.75 | 111 | 0.354 | 0.000 |
|
| 1 | 112 | 0.281 | 0.003 |
| |
| 3 | 112 | 0.406 | 0.000 |
| |
| 4 | 111 | 0.347 | 0.000 |
| |
| 3 ≤ 15 dBHL | 74 | 0.258 | 0.027 |
| |
| 4 ≤ 15 dBHL | 73 | 0.120 | 0.311 | ||
| 24 | 0.75 | 112 | 0.289 | 0.002 |
|
| 1 | 112 | 0.308 | 0.001 |
| |
| 3 | 112 | 0.488 | 0.000 |
| |
| 4 | 112 | 0.567 | 0.000 |
| |
| 3 ≤ 15 dBHL | 74 | 0.158 | 0.180 | ||
| 4 ≤ 15 dBHL | 74 | 0.411 | 0.000 |
|
Correlations were calculated either with no partialling, or partialling by NESI, age, or music experience. Since the partialling only slightly modified the significance, these variations are not reported. Each row contains the number of data points, “n,” the correlation “ρ” and the probability, p.
Apart from the correlations across all absolute thresholds at 3 and 4 kHz, the correlations for a data subset where only thresholds ≤ 15 dB HL are included, are shown with labels “3 ≤ 15 dB HL” and “4 ≤ 15 dB HL”.
p < 0.05.
p < 0.01.
p < 0.001.
NESI, Noise Exposure Structured Interview.
Fig. 4.Example scatterplots for the relation between STR and absolute threshold: the weakest, STR at 12 dB SL with a test frequency of 1 kHz is shown in the left panel, while the strongest, STR at 24 dB SL with a test frequency of 4 kHz is shown in the right panel. Data points are shape and color coded as per Fig. 2, and repeated in the figure legend.
Table of regression coefficients derived from the multiple regression modeling of the STRs as a function of the predictors AbsThr, age, NESI100, music experience, and the interaction term, age × NESI100
| Data to be modeled | Predictor | Standardized beta | CI | SE |
|
| Sig | VIF |
|---|---|---|---|---|---|---|---|---|
| STR @ 12 dB SL0.75 Hz | (Intercept) | –0.029 | –0.215, 0.156 | 0.094 | –0.313 | 0.755 | ||
| AbsThr | 0.367 | 0.183, 0.552 | 0.093 | 3.944 | <0.001 | ‡ | 1.1 | |
| Age | 0.024 | –0.168, 0.217 | 0.097 | 0.249 | 0.804 | 1.2 | ||
| STR @ 12 dB SL3 kHz | (Intercept) | –0.001 | –0.167, 0.165 | 0.084 | –0.012 | 0.991 | ||
| AbsThr | 0.592 | 0.412, 0.771 | 0.091 | 6.535 | <0.001 | ‡ | 1.3 | |
| Age | –0.207 | –0.393, –0.021 | 0.094 | –2.202 | 0.030 | * | 1.3 | |
| STR @ 12 dB SL4 kHz | (Intercept) | –0.008 | –0.191, 0.176 | 0.093 | –0.082 | 0.935 | ||
| AbsThr | 0.397 | 0.194, 0.6 | 0.102 | 3.882 | <0.001 | ‡ | 1.3 | |
| Age | –0.006 | –0.218, 0.206 | 0.107 | –0.055 | 0.956 | 1.4 | ||
| STR @ 24 dB SL3 kHz | (Intercept) | –0.030 | –0.171, 0.11 | 0.071 | –0.431 | 0.668 | ||
| AbsThr | 0.746 | 0.594, 0.898 | 0.077 | 9.727 | <0.001 | ‡ | 1.3 | |
| Age | –0.316 | –0.474, –0.158 | 0.080 | –3.972 | <0.001 | ‡ | 1.3 | |
| STR @ 24 dB SL4 kHz | (Intercept) | –0.032 | –0.182, 0.118 | 0.076 | –0.423 | 0.673 | ||
| AbsThr | 0.699 | 0.53, 0.867 | 0.085 | 8.236 | <0.001 | ‡ | 1.3 | |
| Age | –0.139 | –0.314, 0.036 | 0.088 | –1.570 | 0.119 | 1.4 |
The only significant relationships depended on AbsThr and age, hence only these are detailed. The number of stars in the column “Sig” denotes the probability range of a significant effect, as detailed in the caption to Table 1.
AbsThr, absolute threshold; CI, confidence intervals; STR, signal-to-TEN ratio; VIF, variance inflation factor.
Multiple regression modeling of the STRs as a function of the predictors AbsThr, age, NESI, MExp and the interaction term, age × NESI
| Dependent Variable | R2 | Adjusted R2 | F(df) |
| Sig | Durbin-Watson”s D |
|---|---|---|---|---|---|---|
| STR @ 12 dB SL 0.75 kHz | 0.145 | 0.104 | 3.566 (5,105) | 0.005 |
| 2.14 |
| STR @ 12 dB SL 1 kHz | 0.130 | 0.089 | 3.173 (5,106) | 0.010 | 2.01 | |
| STR @ 12 dB SL 3 kHz | 0.306 | 0.273 | 9.357 (5,106) | 0.000 |
| 2.03 |
| STR @ 12 dB SL 4 kHz | 0.163 | 0.124 | 4.100 (5,105) | 0.002 |
| 2.06 |
| STR @ 24 dB SL, 0.75 kHz | 0.113 | 0.071 | 2.701 (5,106) | 0.024 | 1.89 | |
| STR @ 24 dB SL 1 kHz | 0.103 | 0.060 | 2.422 (5,106) | 0.040 | 2.12 | |
| STR @ 24 dB SL 3 kHz | 0.503 | 0.479 | 21.429 (5,106) | 0.000 |
| 1.78 |
| STR @ 24 dB SL 4 kHz | 0.428 | 0.401 | 15.873 (5,106) | 0.000 |
| 1.67 |
“p” denotes the probability.
Sig” column denotes a significant result.
AbsThr, absolute threshold; MExp, music experience; NESI, Noise Exposure Structured Interview; STR, signal-to-TEN ratio.