TL;DR
This paper discusses Schwarzschild black holes as radiometric standards by analyzing their Hawking radiation through the squeezing perspective, building on prior work by Grischuk and Sidorov.
Contribution
It introduces a novel perspective on black hole radiation using squeezing formalism, connecting it to radiometric standards and expanding theoretical understanding.
Findings
Black holes can be modeled as radiometric standards.
Hawking radiation can be described using squeezing formalism.
The approach offers new insights into black hole thermodynamics.
Abstract
Following Grischuk and Sidorov [Phys. Rev. D 42 (1990) 3413] in putting the Bogolubov-Hawking coefficient of Schwarzschild black-holes in the squeezing perspective, we provide a short discussion of Schwarzschild black holes as radiometric standards
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