Abstract
Here we examined whether the Matsuda–DeFronzo insulin sensitivity index (ISI-M) is more efficient than the homeostasis model assessment of insulin resistance (HOMA-IR) for assessing risk of hypertension. Cross-sectional and longitudinal analyses were conducted using normotensive subjects who were selected among 1399 subjects in the Tanno–Sobetsu cohort. In the cross-sectional analysis (n=740), blood pressure (BP) level was correlated with HOMA-IR and with ISI-M, but correlation coefficients indicate a tighter correlation with ISI-M. Multiple linear regression analysis adjusted by age, sex, body mass index (BMI) and serum triglyceride level (TG) showed contribution of ISI-M and fasting plasma glucose, but not of HOMA-IR. In the longitudinal analysis (n=607), 241 subjects (39.7%) developed hypertension during a 10-year follow-up period, and multiple logistic regression indicated that age, TG, systolic BP and ISI-M, but not HOMA-IR, were associated with development of hypertension. In subjects <60 years old, odds ratio of new-onset hypertension was higher in the low ISI-M group (ISI-M, less than the median) than in the high ISI-M group for any tertile of BMI. In conclusion, ISI-M is a better predictor of hypertension than is HOMA-IR. Non-hepatic IR may be a determinant, which is independent of TG, BP level and BMI, of the development of hypertension.
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Acknowledgements
The present study was supported by a Program for Developing the Supporting System for Upgrading the Education and Research of the Ministry of Education, Culture, Sports, Science and Technology, Tokyo, Japan, a grant for scientific research from the Ministry of Health, Labor and Welfare, Tokyo Japan (H19-cardiovascular-common-021) and Japanese Society for the Promotion of Science Grants-in-Aid for Scientific Research (no. 19590639), Tokyo, Japan.
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Furugen, M., Saitoh, S., Ohnishi, H. et al. Matsuda–DeFronzo insulin sensitivity index is a better predictor than HOMA-IR of hypertension in Japanese: the Tanno–Sobetsu study. J Hum Hypertens 26, 325–333 (2012). https://doi.org/10.1038/jhh.2011.23
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DOI: https://doi.org/10.1038/jhh.2011.23
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