Abstract
The Einstein-Milne relations for the continuum are generalized to a nondegenerate relativistic gas in thermodynamic equilibrium, using the relativistic ionization equation which has been recently established by us [J. Phys. A 16, 2347 (1983)] and which must replace the Saha equation at temperatures above ${10}^{8}$ K. The macroscopic continuum opacity and emissivity of this gas are also derived.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
