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https://doi.org/10.1007/978-1-4757-1562-0s change as the universe settles into its vacuum state. The discovery of the Higgs [., .], and measurement of its mass suggests that our vacuum may not be entirely stable, and that a further phase transition could take place. This article is based on a talk in the Oldenberg Series, and reviews how w
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Shadows and Accretion Disk Images of Compact Objectsfeasible and opened a major experimental channel for probing the gravitational interaction in the strong field regime. Although considered historically as a property of the black hole spacetimes, the shadow is not exclusively a black hole effect and does not require the presence of an event horizon.
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