Isaak Markovich Khalatnikov. 17 October 1919—9 January 2021

A. V. Byalko
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Abstract

Isaak Khalatnikov made major contributions to two different branches of theoretical physics: quantum liquids, particularly liquid helium, and general relativity and cosmology. He made outstanding contributions to our theoretical understanding of superfluidity in liquid 4He and in 3He–4He mixtures. He developed the formulation of the two-fluid hydrodynamic equations, including the proper description of very complex dissipative and nonlinear effects. He also developed the idea, originally due to Landau, that the normal fluid can be described in terms of a gas of weakly-interacting excitations. His work on general relativity and cosmology began with the paper written with E. M. Lifshitz (ForMemRS 1982) in 1963. They extended Lifshitz's pioneering paper of 1946, showing how small departures from homogeneity and isotropy in the early Universe would have grown as the Universe expanded. They also tackled the problem of whether or not the equations of general relativity predict that space-time contains singularities, either in the past or in the future. They initially concluded that more general solutions would not contain singularities, but later work with Belinskiĭ not only showed that general solutions could contain singularities, but also indicated how the Universe would behave near a singularity. Later, Khalatnikov showed that nearly all cosmological solutions with a massive scalar field have a period of exponential or inflationary expansion. He became the founding director of the Landau Institute for Theoretical Physics of the USSR Academy of Sciences in 1964. He brought together a powerful group of theoreticians, creating a scientific centre that has played a major role in the development of theoretical physics.
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伊萨克·马尔科维奇·哈拉特尼科夫,1919年10月17日- 2021年1月9日
伊萨克·哈拉特尼科夫对理论物理学的两个不同分支做出了重大贡献:量子液体,特别是液氦,以及广义相对论和宇宙学。他对我们对液态4He和3He-4He混合物超流动性的理论认识作出了杰出贡献。他发展了双流体流体动力学方程的公式,包括对非常复杂的耗散和非线性效应的适当描述。他还提出了一个想法,最初是由朗道提出的,即正常的流体可以用弱相互作用激发的气体来描述。他对广义相对论和宇宙学的研究始于1963年与e.m. Lifshitz (ForMemRS 1982)合著的论文。他们扩展了利夫希茨1946年的开创性论文,展示了早期宇宙中对同质性和各向同性的微小偏离会随着宇宙的膨胀而增长。他们还解决了广义相对论方程是否预测时空包含奇点的问题,无论是在过去还是在未来。他们最初得出的结论是,更一般的解不包含奇点,但后来与belinsky的合作不仅表明了一般解可以包含奇点,而且还指出了宇宙在奇点附近的行为。后来,Khalatnikov证明了几乎所有具有大质量标量场的宇宙学解都有一个指数或暴胀膨胀的周期。他于1964年成为苏联科学院朗道理论物理研究所的创始主任。他召集了一群强大的理论家,创建了一个科学中心,在理论物理学的发展中发挥了重要作用。
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