The author discusses the time evolution of quantum entanglement in the presence of non-collapsing interactions, focusing on relativistic systems. The key points are:
In relativistic systems, the correlation between entangled processes is defined by the equality of the corresponding invariant intervals.
As an example, the entanglement between the products of a particle decay is revisited, leading to correlations in precise agreement with the muon g-2 experimental results. The author postulates that the correlation between the invariant intervals of the muon and the emitted neutrinos can explain the observed anomaly in the muon magnetic moment.
The extension of the postulate about the equality of invariant intervals to the curved space-time is used to discuss the survival of entanglement in the presence of horizons. It is argued that if the postulate holds, any entanglement between an observer outside and an observer falling into a black hole would be lost when the latter crosses the horizon.
However, for the case of two observers in free fall, a correlation can be defined between their processes by equating their proper times, allowing for the possibility of quantum action at a distance, even though no classical signal can escape the black hole.
The author concludes that the observation of quantum entanglement in high-energy experiments involving particle decays will challenge the current developments of a relativistic theory for this phenomenon, which is still not fully understood.
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