The role of paraspinal muscle degeneration in coronal imbalance in patients with degenerative scoliosis
Introduction
Degenerative scoliosis (DS) is a three-dimensional spinal deformity, often accompanies with sagittal and coronal malalignment, that usually occurs in female patients over 50 years of age (1,2). This is generally associated with back pain, lower-limb pain, and functional impairment (3). With an aging population worldwide, DS is a considerable healthcare concern which accounts for 13.3% of the Chinese population aged 40 and above. Although the exact pathogenesis of DS remains unknown, the progression and asymmetric degenerative changes involving the vertebrae, intervertebral discs and facet joints are major factors for the spinal column malalignment (4).
The paraspinal muscle (PSM) are comprised of the psoas, quadratus lumborum, multifidus (MF), and erector spinae (ES) (5,6). In recent years, the involvement of PSM toward the occurrence and development of spinal deformity have been heavily debated (7). Several studies had reported that poor PSM quality was associated with the occurrence of lower back pain, spinal stenosis, and disc herniation, as well as spinal deformity (7-10). Yet, as most of these studies only focused on their relationship with sagittal parameters, it neglects their correlation with coronal imbalance. Unlike the rare occurrence in adolescent idiopathic scoliosis (AIS), coronal imbalance plays a pivotal role toward the progression and development of DS (7,11).
As one of the most common manifestations in DS, the prevalence of coronal imbalance occurred in 34.8% of Chinese patients (12). In addition, coronal imbalance in patients with DS is highly correlated with decreased health-related quality of life (HRQoL) (13). Whats-more, the occurrence of coronal imbalance increases the likelihood of implant-related failure, which may require revision surgery (14). In clinical practice, we observe DS patients displays various coronal imbalance even Cobb angle of main curve remains similar. Accordingly, our research team developed a new classification system, namely Nanjing classification, based on preoperative coronal balance distance (CBD) and inclination pattern. Importantly, this system has provided new insights regarding surgical decision-making, especially for patients with type C who prone to coronal imbalance after 3-column osteotomy (15-18). Although, lumbosacral fractional curve, L4 tilt and apex location were shown to be related to coronal imbalance, there remains a scarce of literature comprehensively describing etiology of different pattern of coronal imbalance (18). Hence, we speculated that paraspinal muscle degeneration may variate among the different subtypes based on our Nanjing classification. Based on study from Sun et al. (11), they found CBD was correlated with lumbar multifidus atrophy in DS patients. Xie at al. (19) reported positive correlation between Cobb angles with asymmetric degree of multifidus muscle. However, to the best of our knowledge, there are scarce of literatures investigating the relationship between PSM degeneration and coronal imbalance in DS patients. Hence, in this study, we aimed to compare the morphological differences of PSM degeneration between DS patients with and without coronal imbalance, and to investigate the relationship between PSM degeneration and coronal imbalance in DS patients. We present the following article in accordance with the STROBE reporting checklist (available at https://qims.amegroups.com/article/view/10.21037/qims-22-222/rc).
Methods
Patient selection
The quality and quantity of paraspinal muscle were reported to be correlated with age and gender (20,21). To eliminate those confounding factors, this retrospective cohort study included female patients with DS that attended our hospital during the period from February 2017 to December 2020. Inclusion criteria were those aged between 50 to 75 years old at the time of attendance, medical records containing anteroposterior and lateral X-ray radiographs of total spine and magnetic resonance imaging (MRI) of the lumbar spine, and Cobb angle of lumbar curve in the coronal plane >20° on a standing posteroanterior film. Exclusion criteria were history of scoliosis in childhood or adolescence, history of spinal surgery, local infection, inflammation around the spine, history of severe spinal trauma, spinal tumor, and presence of other systemic diseases that can affect spinal alignment (e.g., muscular dystrophy, ankylosing spondylitis, Parkinson disease, etc.) (Figure 1). In addition, basic demographic data, including age, weight, and height, were also obtained. The study was conducted in accordance with the Declaration of Helsinki (as revised in 2013). The study was approved by institutional review board (No. 2021-LCYJ-DBZ-05). All volunteers were fully informed about the methods, purposes, and risks involved in the study protocol and signed the informed consent.
Radiological assessment
A full-spine anteroposterior and lateral radiograph was obtained for patients enrolled in this study. Radiographic parameters were measured on X-ray films according to the Spine Deformity Study Group guidelines, including coronal and sagittal parameters (22). Coronal parameters include Cobb angle of main curve, location of apex vertebrae and coronal balance distance (CBD). The CBD is defined as the horizontal distance between C7 plum line and central sacral vertical line (CSVL). While for sagittal parameters, the measurements include sagittal vertical axis (SVA), thoracic kyphosis (TK) and lumbar lordosis (LL). The SVA is defined as the horizontal distance between the vertical-line from the midpoint of C7 vertebrae to the posterior upper endplate of sacrum. The measurement of TK and LL refers the Cobb angle between T5 and T12 and the Cobb angle between L1 and S1, respectively. All measurements were attained by Surgimap (v2.3.2.1, Nemaris Inc, New York, NY).
Patients classification
After enrollment, patients were classified into three subtypes (Type A, B and C) according to Nanjing classification (15). The C7 plumb line (C7PL) is defined as the vertical line across the midpoint of C7 vertebrae. Based on the CBD and C7PL, the three subtypes of coronal imbalance were then determined (Figure 2):
- Type A: patients with no coronal imbalance (trunk shift <3 cm),
- Type B: patients with coronal imbalance (trunk shift >3 cm) and a C7PL shifted to concave side, and
- Type C: patients with coronal imbalance (trunk shift >3 cm) and a C7PL shifted to convex side.
Magnetic resonance imaging (MRI)
The routine lumbar MRI images was acquired on the routine 1.5-T sigma imaging system (Magetom Skyra, Siemens healthcare, Erlagen, Germany). After scanning, the trans-axial and sagittal sequence of T2 weighted images were saved with DICOM format from picture archiving and communicating system (PACS). The sagittal sequence was used to identify the lower endplate of lumbar vertebrae. A total of 5 trans-axial slices, which located at apex level and 2 proximal and 2 distal levels, were obtained with 4 mm thickness and 2 mm space, shown in Figure 3. Bilateral cross-sectional area (CSAs) of PSM was quantified by outlining the thoracolumbar facial boundary at targeted trans-axial slices using ImageJ image analyzing software (Image J ver. 1.3; NIH, Bethesda, MA). Fat infiltration rate (FI%) of PSM was obtained by pseudo-coloring technique as previously reported (19,23). Bilateral average CSAs and FI% of PSM was calculated and referred as total CSA and total FI% of lumbar PSM (Figure 4).
Method reliability
To evaluate the reliability of the measurements on the radiographs and MRI, the parameters were measured by two independent observers (HK and ZS). All these observers were blinded to the subject information. Intra-observer and inter-observer variations were estimated by using intraclass correlation coefficient (ICC), which were graded using previously described semi-quantitative criteria: excellent (ICC ≤0.9), good (0.7≤ ICC <0.9), acceptable (0.6≤ ICC <0.7), poor (0.5≤ ICC <0.6), or unpredictable (ICC <0.5) (22,24).
Statistical analysis
The data is presented as means ± standard deviation. Data analysis was carried out using SPSS software (Version 23.0; SPSS, Chicago, IL, USA). Data was tested for normality by Kolmogorov-Smirnov test which presented a normal distribution. Demographics and radiographic parameters were compared between the three groups. One-way ANOVA and Bonferroni Post-hoc test was used for inter-group comparisons. Pearson’s correlation test was used to analyze the correlation between different parameters. P value <0.05 was considered statistically significant.
The primary aim of the study is to investigate the relationship between PSM degeneration and with and without coronal imbalance in DS patients. Hence, cross-sectional area of PSM will be the primary comparison. Based on our pilot analysis, the comparison of DS patients with and without coronal imbalance showed an effective size of 0.48. Therefore, sample sizes of at least 50 patients without coronal imbalance (Type A) and 50 with coronal imbalance (Type B and C) will be needed to achieve an 81% power to detect the difference between the groups, with a significance level (alpha) of 0.05 (PASS 11.0, NCSS, LLC, Utah, USA).
Results
Demographic data
A total of 117 patients (117 females; average age 60.9±5.2 years) were included in this study for analysis. The majority of patients had type A coronal alignment (CSVL <3 cm; Type A =56). Coronal malalignment consisting of type B (trunk shift ipsilateral to curve’s concavity >3 cm; Type B =34) and type C (trunk shift ipsilateral to curve’s convexity >3 cm; Type C =27) were less common. Their demography is shown in Table 1. There were no significant differences in the demographic data, which were screened by two experienced orthopedic surgeons (HK and ZS).
Table 1
Demographics | All | Type A | Type B | Type C | P value |
---|---|---|---|---|---|
N | 117 | 56 | 34 | 27 | N/A |
Gender | Female | Female | Female | Female | N/A |
Age (years) | 60.9±5.2 | 61.0±5.4 | 61.8±4.9 | 59.9±5.5 | 0.726 |
Height (cm) | 156.6±7.3 | 158.0±7.3 | 154.2±8.1 | 156.4±6.6 | 0.428 |
Weight (kg) | 58.6±6.9 | 60.4±7.3 | 57.5±7.4 | 56.0±4.7 | 0.222 |
BMI (kg/m2) | 23.8±1.6 | 24.1±1.3 | 24.1±1.8 | 22.9±1.9 | 0.128 |
Data are expressed as mean ± standard deviation. BMI, body mass index; N/A, not available.
Comparison on radiographic data
The intra- and interobserver ICCs for estimating the sagittal parameters were from 0.83 to 0.96, suggesting good to excellent reliability of these measurements among the two observers (Table 2). There was no statistically significant difference for sagittal parameters, including SVA (Type A vs. Type B: 4.5±3.4 vs. 8.0±5.4, P=0.073; Type A vs. Type C: 4.5±3.4 vs. 7.3±6.8, P=0.147; Type B vs. Type C: 8.0±5.4 vs. 7.3±6.8, P=0.756; Type A vs. Type B vs. Type C: 4.5±3.4 vs. 8.0±5.4 vs. 7.3±6.8, P=0.134), TK (Type A vs. Type B: 20.7±13.1 vs. 18.3±11.2, P=0.599; Type A vs. Type C: 20.7±13.1 vs. 12.9±8.0, P= 0.090; Type B vs. Type C: 18.3±11.2 vs. 12.9±8.0, P=0.300; Type A vs. Type B vs. Type C: 20.7±13.1 vs. 18.3±11.2 vs. 12.9±8.0, P=0.232) and LL (Type A vs. Type B: 22.3±15.0 vs. 28.0±16.3, P=0.367; Type A vs. Type C: 22.3±15.0 vs. 27.1±18.1, P=0.895; Type B vs. Type C: 28.0±16.3 vs. 27.1±18.1, P=0.895; Type A vs. Type B vs. Type C: 22.3±15.0 vs. 28.0±16.3 vs. 27.1±18.1, P=0.591) as shown in Table 3.
Table 2
Parameters | Intra-rater coefficient | Inter-rater coefficient |
---|---|---|
Radiographic parameters | ||
Cobb angle (o) | 0.91 | 0.95 |
CBD (cm) | 0.91 | 0.83 |
SVA (cm) | 0.93 | 0.90 |
TK (o) | 0.95 | 0.92 |
LL (o) | 0.96 | 0.95 |
MRI parameters | ||
CSA (cm2) | 0.90 | 0.83 |
FI% | 0.96 | 0.91 |
CBD, coronal balance distance; CSA, cross sectional area; FI%, fat infiltration; LL, lumbar lordosis; MRI, magnetic resonance imaging; SVA, sagittal vertical axis; TK, thoracic kyphosis.
Table 3
Parameters | Type A (n=56) | Type B (n=34) | Type C (n=27) | P value | |||
---|---|---|---|---|---|---|---|
A vs. B vs. C | A vs. B | A vs. C | B vs. C | ||||
Coronal parameters | |||||||
Cobb angle (o) | 36.6±11.1 | 40.7±7.9 | 33.8±10.8 | 0.334 | 0.313 | 0.489 | 0.145 |
Curve apex | 2.1±0.6 | 2.2±0.6 | 2.0±0.5 | 0.760 | 0.670 | 0.670 | 0.462 |
CBD (cm) | 1.1±0.8 | 5.0±1.1 | 4.2±1.4 | <0.001 | <0.001 | <0.001 | 0.084 |
Sagittal parameters | |||||||
SVA (cm) | 4.5±3.4 | 8.0±5.4 | 7.3±6.8 | 0.134 | 0.073 | 0.147 | 0.756 |
TK (o) | 20.7±13.1 | 18.3±11.2 | 12.9±8.0 | 0.232 | 0.599 | 0.090 | 0.300 |
LL (o) | 22.3±15.0 | 28.0±16.3 | 27.1±18.1 | 0.591 | 0.367 | 0.452 | 0.895 |
Data are expressed as mean ± standard deviation. CBD, coronal balance distance; SVA, sagittal vertical axis; TK, thoracic kyphosis; LL, lumbar lordosis.
There were no statistically differences in terms of curve magnitude between Type A and Type B (36.6±11.1 vs. 40.7±7.9, P=0.313), Type A and Type C (36.6±11.1 vs. 33.8±10.8, P=0.489) and Type B and Type C (40.7±7.9 vs. 33.8±10.8, P=0.145). On the other hand, CBD is higher in both Type B and Type C while compared to CBD in Type A (Type A vs. Type B: 1.1±0.8 vs. 5.0±1.1, P<0.01; Type A vs. Type C: 1.1±0.8 vs. 4.2±1.4, P<0.01). There was no significant difference in CBD between Type B and Type C (Type B vs. Type C: 1.1±0.8 vs. 4.2±1.4, P=0.084).
Comparison of CSA and FI% between three subtypes of coronal imbalance
The CSA and FI% of PSM from Apex-2 to Apex+2 level is shown in Table 4. No significant difference in terms of CSA between the three Types on both convex and concave sides (P>0.05). Whereas for the FI% of PSM, patients in Type B and Type C showed higher FI% than those in Type A in both concave and convex side. The intra- and interobserver ICCs for estimating the MRI parameters were from 0.83 to 0.96, suggesting good to excellent reliability of these measurements among the two observers (Table 2).
Table 4
Variables | Concavity | Convexity | |||||||
---|---|---|---|---|---|---|---|---|---|
Type A (n=56) | Type B (n=34) | Type C (n=27) | P value | Type A (n=56) | Type B (n=34) | Type C (n=27) | P value | ||
Cross-sectional area of PSM (cm2) | |||||||||
Apex-2 | 16.9±3.6 | 17.4±2.4 | 16.9±4.0 | 0.911 | 15.8±3.3 | 13.6±5.7 | 15.7±3.6 | 0.351 | |
Apex-1 | 18.6±3.7 | 19.4±2.4 | 20.1±3.3 | 0.483 | 17.8±4.1 | 15.6±8.0 | 17.3±3.4 | 0.542 | |
Apex | 19.2±4.1 | 19.7±3.2 | 21.2±4.9 | 0.473 | 17.9±5.1 | 15.3±8.1 | 16.1±5.1 | 0.504 | |
Apex+1 | 18.3±4.4 | 17.1±4.3 | 18.7±6.3 | 0.754 | 18.3±4.8 | 16.0±6.7 | 17.1±5.2 | 0.545 | |
Apex+2 | 16.2±4.0 | 16.4±4.0 | 17.3±5.7 | 0.819 | 17.3±3.9 | 16.1±5.3 | 18.2±5.5 | 0.609 | |
Total | 17.8±3.3 | 18.0±2.5 | 18.9±3.6 | 0.718 | 17.4±3.5 | 15.3±6.4 | 16.9±3.3 | 0.467 | |
Fat infiltration rate of PSM (%) | |||||||||
Apex-2 | 24.7±9.2 | 42.8±2.4a | 31.7±11.7b,c | <0.001 | 27.1±12.8 | 42.0±5.1a | 30.3±16.6c | 0.014 | |
Apex-1 | 30.0±5.6 | 45.5±6.8a | 37.2±11.6b | <0.001 | 29.5±11.1 | 47.3±10.8a | 32.5±16.8c | 0.003 | |
Apex | 32.0±10.8 | 45.1±7.1a | 38.6±14.7 | 0.014 | 32.5±12.0 | 44.5±7.0b | 43.6±18.8b | 0.029 | |
Apex+1 | 34.3±10.5 | 46.5±9.4b | 38.3±16.7 | 0.045 | 33.1±13.0 | 50.8±13.7a | 44.5±14.0b | 0.004 | |
Apex+2 | 32.8±16.5 | 45.8±22.4 | 47.8±18.8b | 0.071 | 40.6±12.6 | 47.1±16.0 | 52.6±13.4b | 0.083 | |
Total | 30.8±8.1 | 45.1±7.7a | 38.7±12.5b | 0.001 | 32.6±10.9 | 46.3±7.3a | 40.7±11.8b | 0.004 |
Data are expressed as mean ± standard deviation. a, P<0.01 when compared with Type A; b, P<0.05 when compared with Type A; c, P<0.01 when compared with Type B. PSM, paraspinal muscle.
Correlation of CSAs and FI% of PSM with coronal parameters
In the correlation analysis, Cobb angle was negatively correlated with the CSA at apex vertebra translation in concave (R=–0.431, P=0.006) and convex side (R=–0.440, P=0.004) (Table 5). When assessing the total CSA, there was significant negative correlation between Cobb angle and the total CSA of paraspinal muscle (PSM) in convex side (R=−0.415, P=0.008). However, there no significant correlation between coronal balance distance (CBD), sagittal vertical axis (SVA), thoracic kyphosis (TK) and lumbar lordosis (LL) with the CSA at apex vertebra translation in concave and convex side (Table 5).
Table 5
Variables | Cobb angle | Concavity | Convexity | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Apex-2 | Apex-1 | Apex | Apex+1 | Apex+2 | Total | Apex-2 | Apex-1 | Apex | Apex+1 | Apex+2 | Total | |||
Cobb angle (o) | ||||||||||||||
R | 1.000 | −0.288 | −0.160 | −0.431 | −0.266 | 0.006 | −0.287 | −0.531 | −0.433 | −0.440 | −0.330 | −0.048 | −0.415 | |
P value | – | 0.071 | 0.324 | 0.006 | 0.097 | 0.971 | 0.073 | <0.001 | 0.005 | 0.004 | 0.038 | 0.769 | 0.008 | |
CBD (cm) | ||||||||||||||
R | −0.006 | 0.148 | 0.215 | 0.183 | −0.112 | −0.021 | 0.085 | −0.015 | −0.035 | −0.074 | −0.121 | −0.128 | −0.089 | |
P value | 0.969 | 0.361 | 0.184 | 0.257 | 0.490 | 0.900 | 0.603 | 0.928 | 0.829 | 0.651 | 0.456 | 0.431 | 0.586 | |
SVA (cm) | ||||||||||||||
R | −0.269 | 0.220 | 0.079 | 0.128 | −0.007 | −0.068 | 0.076 | 0.046 | −0.026 | −0.058 | −0.056 | −0.097 | −0.048 | |
P value | 0.093 | 0.173 | 0.629 | 0.429 | 0.965 | 0.679 | 0.641 | 0.778 | 0.874 | 0.721 | 0.731 | 0.552 | 0.769 | |
TK (o) | ||||||||||||||
R | 0.073 | 0.160 | 0.269 | 0.225 | 0.218 | 0.130 | 0.252 | 0.172 | 0.358 | 0.365 | 0.306 | 0.118 | 0.319 | |
P value | 0.653 | 0.323 | 0.093 | 0.162 | 0.177 | 0.423 | 0.117 | 0.290 | 0.023 | 0.020 | 0.055 | 0.469 | 0.045 | |
LL (o) | ||||||||||||||
R | 0.151 | −0.249 | 0.469 | 0.426 | 0.305 | 0.321 | 0.468 | 0.372 | 0.464 | 0.417 | 0.506 | 0.350 | 0.495 | |
P value | 0.352 | 0.121 | 0.002 | 0.006 | 0.055 | 0.043 | 0.002 | 0.018 | 0.003 | 0.007 | 0.001 | 0.027 | 0.001 |
CBD, coronal balance distance; SVA, sagittal vertical axis; TK, thoracic kyphosis; LL, lumbar lordosis; R, Pearson Correlation Coefficient.
Toward the correlation on FI%, CBD was positively correlated with the CSA at apex vertebra translation in the concave side (R=0.349, P=0.027) (Table 6). When assessing the total FI%, there was significant positive correlation between CBD and the total CSA of PSM in concavity (R=0.491, P=0.001) and convexity (R=−0.354, P=0.025). However, there no significant correlation between Cobb angle, SVA, TK and LL with the CSA at apex vertebra translation in concave and convex side (Table 6).
Table 6
Variables | Cobb angle | Concavity | Convexity | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Apex-2 | Apex-1 | Apex | Apex+1 | Apex+2 | Total | Apex-2 | Apex-1 | Apex | Apex+1 | Apex+2 | Total | |||
Cobb angle (o) | ||||||||||||||
R | 1.000 | 0.046 | 0.007 | −0.050 | −0.069 | −0.227 | −0.097 | 0.000 | −0.036 | 0.116 | −0.011 | −0.070 | −0.001 | |
P value | – | 0.778 | 0.966 | 0.758 | 0.674 | 0.160 | 0.550 | 1.000 | 0.825 | 0.475 | 0.947 | 0.670 | 0.997 | |
CBD (cm) | ||||||||||||||
R | −0.006 | 0.552 | 0.554 | 0.349 | 0.328 | 0.331 | 0.491 | 0.271 | 0.322 | 0.277 | 0.365 | 0.207 | 0.354 | |
P value | 0.969 | <0.001 | <0.001 | 0.027 | 0.039 | 0.037 | 0.001 | 0.090 | 0.042 | 0.084 | 0.021 | 0.200 | 0.025 | |
SVA (cm) | ||||||||||||||
R | −0.269 | 0.444 | 0.426 | 0.227 | 0.292 | 0.209 | 0.365 | 0.318 | 0.305 | 0.168 | 0.229 | 0.115 | 0.277 | |
P value | 0.093 | 0.004 | 0.006 | 0.160 | 0.067 | 0.195 | 0.021 | 0.045 | 0.056 | 0.300 | 0.156 | 0.480 | 0.083 | |
TK (o) | ||||||||||||||
R | 0.073 | −0.058 | −0.222 | −0.155 | 0.028 | 0.052 | −0.062 | 0.109 | 0.117 | 0.035 | 0.004 | 0.013 | 0.067 | |
P value | 0.653 | 0.716 | 0.168 | 0.338 | 0.862 | 0.749 | 0.702 | 0.502 | 0.473 | 0.831 | 0.980 | 0.936 | 0.682 | |
LL (o) | ||||||||||||||
R | 0.151 | 0.056 | −0.045 | −0.006 | −0.089 | −0.009 | −0.022 | −0.039 | −0.016 | 0.221 | −0.108 | 0.004 | 0.013 | |
P value | 0.352 | 0.731 | 0.781 | 0.969 | 0.584 | 0.954 | 0.891 | 0.811 | 0.921 | 0.170 | 0.505 | 0.980 | 0.938 |
CBD, coronal balance distance; SVA, sagittal vertical axis; TK, thoracic kyphosis; LL, lumbar lordosis; R, Pearson correlation coefficient.
Discussion
Although coronal imbalance in patients with DS is quite common, the etiology for this occurrence remains unclear. Previous studies have indicated that bony structural changes may play a key role toward this deterioration (11,19,24). Owing to the interrelationship of muscle and bones, it has been suggested that PSM degeneration might play a role curve progression in DS patients with coronal imbalance (11,25). Based on this current study, this is the first to report that DS patients without coronal imbalance (Type A) would have lower FI% than those with coronal imbalance (Type B and Type C) in both concavity and convexity of the curve. Moreover, we showed a positive correlation between coronal imbalance distances and PSM degeneration in patients with DS.
In recent years, increasing attention was given toward the role of paraspinal muscle in pathogenesis of spinal disorders. Multiple studies have showed correlation between PSM degeneration with back pain, radiculopathy, and spinal deformity (19,21,26-28). Similarly, Lee et al. reported extensive degeneration of back muscle could be a causative factor in the pathogenesis of flat back syndrome (23). Correlation between PSM degeneration and spinopelvic parameters were comprehensively described by Xia et al. (29). In a study investigating the role of paraspinal muscle in AIS, Yeung et al. (10) describes asymmetrical fat composition and linear correlation between fat infiltration and curve magnitude. However, the contribution of paraspinal muscle degeneration is minor compared to that of DS. Yagi et al. (25) and Shafaq et al. (2) described more severe morphological and histological change in DS, which indicate muscle degeneration playing a more important role in the pathogenesis of DS. However, as most of those studies mainly focused on the contribution of PSM to sagittal parameters, it is often neglected toward its role on coronal imbalance.
The well accepted classification of adult spinal deformity-SRS-Schwab classification includes four main coronal curve types which mainly focused on sagittal malalignment while coronal imbalance was little involved (30). Coronal imbalance demonstrates various forms in DS. Nanjing classification concluded preoperative coronal imbalance in to three subtypes and emphasized its impact on postoperative outcomes. In this study, we hypothesized PSM degeneration may differ in three subtypes of coronal imbalance. The findings from our study will potentially help to provide new prospective, and to partially contribute, in the understanding on the pathogenesis of coronal imbalance.
In patients with degenerative lumbar kyphosis (DLK), Lee et al. (23) and Hyun et al. (31) found smaller CSA compared to healthy volunteers. Yagi et al. (25) found asymmetrical size of PSM, in which PSM in convex side demonstrated larger CSA compared to concave side. Manion et al. (32) and Shafaq et al. (2) reported smaller fiber size and decreased nuclei in concave side compared to convex side of paraspinal muscle through histological study in DS patients, which also indicates more severe muscle degeneration in concave side. While cross-sectional area represents the paraspinal muscle volume, fat infiltration represents declining muscle structure and quality (33). High content of fat infiltration results in direct dysfunction of skeletal muscle (34,35). Tang et al. (36) found fat filtration was correlated with health related quality of life scores of DS patients while no significant correlation was found in terms of CSA. Though, smaller CSA also could represent PSM degeneration, however, we did not find any significant difference in terms of CSA of PSM between DS patients with and without coronal imbalance. This may indicate muscle volume is not sensitive to coronal imbalance. This further supported by our finding on the correlation between CSA and Cobb angle and CBD and FI%, respectively. Such that, the change of functional muscle mass to fat deposits during muscle degeneration may also help to explain our current observations.
Fat infiltration was reported to decrease the contractile composition of muscle mass which in turn leads to decline of production of musculature power (37). Grawford et al. (38) reported gradually increasing FI in lumbar paraspinal muscle from cranial to caudal side which was consistent with the result of our study. It showed higher FI% was significantly observed in patients with type B patients and type C when compared to type A. Moreover, FI% was found to be positively correlated with CBD at each level regardless of concave or convex side in present study. Taken together, we believe that high percentage of fat infiltration in PSM in type B, especially at upper levels, leads lower muscle strength in upper levels which may lead lower compensability to maintain spinal balance in upper segments of spine. Likewise, sever fat infiltration in lower levels of lumbar spine in type C patients may lead poor muscle strength at the base of spine and maybe readily decompensate to convex side. Several studies reported lower preoperative thoracolumbar muscle quality in patients with proximal junctional kyphosis (PJK) and even muscle degeneration as a risk factor for occurrence of PJK (39-41). Furthermore, several studies reported that poor muscle quality is correlated with distal screw loosening in patients with DS after corrective surgery (42-44).
There are several limitations in this study. Firstly, this is a retrospective study with relatively small sample size. High standard for case-match analysis as well as strict criteria for collecting homogenous MRI sequence have limited the sample size. Secondly, although different state of PSM degeneration was found among three types of DS, it is still difficult to ascertain the casual relationship between PSM degeneration and scoliosis as retrospective nature of this study. Thus, long-term prospective studies are needed. In addition, the CSAs and FI% were measured at 2D plane which cannot precisely show the volume of muscle and fat, and 3D reconstruction of soft tissue and bone would provide a way to minimize the bias from manual measurement and positional change (24).
Conclusions
In conclusion, DS patients with coronal imbalance demonstrated a worse PSM degeneration, especially higher fat infiltration, when compared with those without coronal imbalance. In particularly, the increase of CBD significantly correlated with FI% at both concavity and convexity of the apical curve. This implies that PSM degeneration may contribute to the coronal imbalance in patients with DS. However, as cause-result relationship between scoliosis and PSM still difficult to ascertain, a longitudinal investigation is necessary to elucidate those findings.
Acknowledgments
The authors thank all the patients who participated in this study and the staff from the Drum Tower Hospital, Nanjing, China.
Funding: This work was supported by the National Natural Science Foundation of China (NSFC) (82072518), the Nanjing Medical Science and Technique Development Foundation (QRX17126) funds and China Postdoctoral Science Foundation (2021M701677) and Jiangsu Provincial Key Medical Center.
Footnote
Reporting Checklist: The authors have completed the STROBE reporting checklist. Available at https://qims.amegroups.com/article/view/10.21037/qims-22-222/rc
Conflicts of Interest: All authors have completed the ICMJE uniform disclosure form (available at https://qims.amegroups.com/article/view/10.21037/qims-22-222/coif). LZ received the National Natural Science Foundation of China (NSFC) (No. 82072518), the Nanjing Medical Science and Technique Development Foundation (No. QRX17126) funds through institution; ZS receives China Postdoctoral Science Foundation (2021M701677) through institution. The other authors have no conflicts of interest to declare.
Ethical Statement: The authors are accountable for all aspects of the work in ensuring that questions related to the accuracy or integrity of any part of the work are appropriately investigated and resolved. The study was conducted in accordance with the Declaration of Helsinki (as revised in 2013). The study was approved by institutional review board (No. 2021-LCYJ-DBZ-05). All volunteers were fully informed about the methods, purposes, and risks involved in the study protocol and signed the informed consent.
Open Access Statement: This is an Open Access article distributed in accordance with the Creative Commons Attribution-NonCommercial-NoDerivs 4.0 International License (CC BY-NC-ND 4.0), which permits the non-commercial replication and distribution of the article with the strict proviso that no changes or edits are made and the original work is properly cited (including links to both the formal publication through the relevant DOI and the license). See: https://creativecommons.org/licenses/by-nc-nd/4.0/.
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