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Correlation Tensor for Magnetic Fields in Cosmological Models: Flat, Lobachevsky, and Spherical Spaces

This study explores the correlation tensor for magnetic fields within the framework of cosmological models. Focusing on flat, Lobachevsky, and spherical spaces, the research by A.S. Rubashny and D.D. Sokoloff delves into the intricate relationships between magnetic field behavior and the underlying geometry of space. By examining these correlations, the authors aim to enhance our understanding of magnetic phenomena in cosmological contexts, contributing to the broader field of astrophysics and cosmology.

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Correlation Tensor for Magnetic Fields in Cosmological Models: Flat, Lobachevsky, and Spherical Spaces

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  1. Correlation Tensor for Magnetic Fields in Cosmological Models Flat space Lobachevsky space Spherical space A.S. Rubashny and D.D. Sokoloff Moscow State University

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