INTEGRAL is an ESA mission in fundamental astrophysics that was launched in October 2002. It has been in orbit for over 18 years, during which it has been observing the high-energy sky with a set of instruments specifically designed to probe the emission from hard X-ray and soft $\gamma$-ray sources. This paper is devoted to the subject of black hole binaries, which are among the most important sources that populate the high-energy sky. We present a review of the scientific literature based on INTEGRAL data, which has significantly advanced our knowledge in the field of relativistic astrophysics. We briefly summarise the state-of-the-art of the study of black hole binaries, with a particular focus on the topics closer to the INTEGRAL science. We then give an overview of the results obtained by INTEGRAL and by other observatories on a number of sources of importance in the field. Finally, we review the main results obtained over the past 18 years on all the black hole binaries that INTEGRAL has observed. We conclude with a summary of the main contributions of INTEGRAL to the field, and on the future perspectives.

INTEGRAL是欧空局于 2002 年 10 月发射的一项基础天体物理学任务。它已在轨道上运行超过 18 年，在此期间，它一直使用一套专门设计用于探测硬 X 发射的仪器来观测高能天空。 - 光线和柔软$\gamma$-射线源。本文专门讨论黑洞双星这一主题，它们是高能天空中最重要的来源之一。我们对基于INTEGRAL数据的科学文献进行了回顾，这极大地提高了我们在相对论天体物理学领域的知识。我们简要总结了黑洞双星研究的最新技术，特别关注更接近INTEGRAL科学的主题。然后，我们概述了INTEGRAL和其他天文台在该领域的许多重要来源上获得的结果。最后，我们回顾上都取得了过去18年的黑洞双星的主要结果INTEGRAL观察到。最后，我们总结了INTEGRAL在该领域的主要贡献以及未来展望。