Abstract
We saw that there are striking similarities between thermodynamics and black hole mechanics as summarized in (Wald, University of Chicago Press, 2010, [8]). These were considered by many to be mere surface similarities, until Hawking showed that semiclassical black holes emit thermal radiation at inverse temperature \(\beta = \frac{2\pi }{\kappa }\) (Hawking, Commun Math Phys, 43:199–220, 1975, [9]). That is, black holes seem to be truly thermodynamic objects which radiate at a well-defined temperature. However, this immediately poses a problem, as thermal radiation is in a mixed quantum state, which means we need a density matrix to describe it. Hence, if a black hole formed out of a pure state evaporates into mixed thermal radiation, we have a pure-to-mixed state transition, which violates the unitarity postulate of quantum mechanics. There thus seems to be a conflict between quantum mechanics and general relativity, which presents perhaps the most important unsolved problem of contemporary theoretical physics. The remaining sections will look at the origin of this problem as well as some partial solutions that have been proposed thus far.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2019 The Author(s), under exclusive license to Springer Nature Switzerland AG
About this chapter
Cite this chapter
Lüst, D., Vleeshouwers, W. (2019). Hawking and Unruh Radiation. In: Black Hole Information and Thermodynamics. SpringerBriefs in Physics. Springer, Cham. https://doi.org/10.1007/978-3-030-10919-6_14
Download citation
DOI: https://doi.org/10.1007/978-3-030-10919-6_14
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-030-10918-9
Online ISBN: 978-3-030-10919-6
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)