Total shoulder arthroplasty (TSA) and hemiarthroplasty (HA) are used in the management of end-stage glenohumeral arthritis. Improvement in shoulder function and resolution of symptoms are high ...priorities for patients. The aim of this study was to compare patient-reported outcome measures (PROMs) following TSA and HA.
Records from the National Joint Registry of England, Wales, Northern Ireland, and the Isle of Man were linked to the PROMs data set. The study included anatomic shoulder arthroplasties performed for osteoarthritis in patients with an intact rotator cuff. Patients with preoperative and postoperative Oxford Shoulder Scores (OSSs) were included. The improvement in OSS at 6 months and 5 years and the trend in scores over time were analyzed for each prosthesis. A cohort of 2002 patients were matched on 10 variables using propensity scores. OSSs at 6 months following TSA vs. HA were compared in the matched sample.
There was a significant improvement in the OSS in both groups (P < .001). At 6 months, the OSSs were superior following TSA compared with HA (median 42 vs. 36, P < .001). The median score at 5 years was 44 following TSA and 35 following HA. Score distributions were skewed toward the maximum score. The highest possible score (48) was achieved in 28% (134 of 478) of TSAs and 9% (20 of 235) of HAs at 5 years. The improvement in the preoperative to 6-month OSS reached the minimal clinically important difference of 5.5 in 92% (1653 of 1792) of TSAs and in 80% (416 of 523) of HAs. At 5 years, this improvement was maintained in 91% (339 of 374) of TSAs and 78% (136 of 174) of HAs.
TSA resulted in superior OSSs at 6 months in patients with osteoarthritis. The median OSS improved from 6 months to 5 years following TSA; however, there was a small decline in scores following HA. A ceiling effect was shown in the OSS following TSA at 5 years.
Total shoulder arthroplasty (TSA) and hemiarthroplasty (HA) are used in the management of osteoarthritis of the glenohumeral joint. We aimed to determine whether TSA or HA resulted in a lower risk of ...adverse outcomes in patients of all ages with osteoarthritis and an intact rotator cuff and in a subgroup of patients aged 60 years or younger.
Shoulder arthroplasties recorded in the National Joint Registry, UK, between April 1, 2012 and June 30, 2021, were linked to Hospital Episode Statistics in England. Elective TSAs and HAs were matched on propensity scores based on 11 variables. The primary outcome was all-cause revision. Secondary outcomes were combined revision/non-revision reoperations, 30-day inpatient complications, 1-year mortality, and length of stay. 95% confidence intervals (CI) were reported.
11,556 shoulder arthroplasties were included: 7,641 TSAs, 3,915 HAs. At 8 years 95% (CI 94-96) of TSAs and 91% (CI 90-92) of HAs remained unrevised. The hazard ratio (HR) varied across follow-up: 4-year HR 2.7 (CI 1.9-3.5), 8-year HR 2.0 (CI 0.5-3.5). Rotator cuff insufficiency was the most common revision indication. In patients aged 60 years or younger prosthesis survival at 8 years was 92% (CI 89-94) following TSA and 84% (CI 80-87) following HA.
The risk of revision was higher following HA in patients with osteoarthritis and an intact rotator cuff. Patients aged 60 years and younger had a higher risk of revision following HA.
The chameleon gravity model postulates the existence of a scalar field that couples with matter to mediate a fifth force. If it exists, this fifth force would influence the hot X-ray emitting gas ...filling the potential wells of galaxy clusters. However, it would not influence the clusters weak lensing signal. Therefore, by comparing X-ray and weak lensing profiles, one can place upper limits on the strength of a fifth force. This technique has been attempted before using a single, nearby cluster (Coma, z = 0.02). Here we apply the technique to the stacked profiles of 58 clusters at higher redshifts (0.1 < z < 1.2), including 12 new to the literature, using X-ray data from the XMM Cluster Survey and weak lensing data from the Canada–France–Hawaii–Telescope Lensing Survey. Using a multiparameter Markov chain Monte Carlo analysis, we constrain the two chameleon gravity parameters (β and ϕ∞). Our fits are consistent with general relativity, not requiring a fifth force. In the special case of f(R) gravity (where
$\beta = \sqrt{1/6}$
), we set an upper limit on the background field amplitude today of |f
R0| < 6 × 10−5 (95 per cent CL). This is one of the strongest constraints to date on |f
R0| on cosmological scales. We hope to improve this constraint in future by extending the study to hundreds of clusters using data from the Dark Energy Survey.
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