Gravitational blueshift from a collapsing object
arXiv:1310.1320 · doi:10.1016/j.physletb.2014.12.022
Abstract
We discuss a counterintuitive phenomenon of classical general relativity, in which a significant fraction of the radiation emitted by a collapsing object and detected by a distant observer may be blueshifted rather than redshifted. The key-point is that when the radiation propagates inside the collapsing body it is blueshifted, and this time interval may be sufficiently long for the effect to be larger than the later redshift due to the propagation in the vacuum exterior, from the surface of the body to the distant observer. Unfortunately, the phenomenon can unlikely have direct observational implications, but it is interesting by itself as a pure relativistic effect.
6 pages, 3 figures. v2: refereed version
References in corpus (2)
Cited by in corpus (7)
- Calculating black hole shadows: Review of analytical studies
- Photon sphere and shadow of a time-dependent black hole described by a Vaidya metric
- Observational distinction between black holes and naked singularities: the role of the redshift function
- The gravitational redshift of photons traversing a collapsing dust cloud and observable consequences
- The shadow of a collapsing dark star
- Cauchy horizon stability in a collapsing spherical dust cloud I: geometric optic approximation and spherically symmetric test fields
- Shadow of higher dimensional collapsing dark star and blackhole