The Minimum and Maximum Temperature of Black Body Radiation

Abstract

We show, in different ways, that in the ubiquitous phenomenon of black body radiation there exists a minimum and maximum temperature. These limiting values are so small and large respectively, that they are of no practical use, except in an extreme situation of black hole evaporation where they lead to maximum and minimum mass.

7 pages, 1 figure

References in corpus (3)

• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• The Generalized Uncertainty Principle and Black Hole Remnants
• Scales Set by the Cosmological Constant

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