http://arxiv.org/abs/1901.10963
A recent paper [arXiv:1901.05477] claims that the CSL model of spontaneous wave function collapse is ruled out by observations on heat flow from neutron stars. This type of system-a degenerate Fermi gas-is relevant as it represents the densest form of matter, potentially maximising CSL effects. As it turns out, this is not the case: to leading order, the CSL induced heating is the same as for ordinary matter, and neutron stars do not bound the CSL parameters significantly.
S. Adler, A. Bassi, M. Carlesso, et. al.
Thu, 31 Jan 19
27/59
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