The Development of Black Hole Thermodynamics: A Novel Historical Approach

Since the inception of the specific study of Black Hole Thermodynamics by Jacob Bekenstein and Stephen Hawking, said study has taken a central focus in the world of both Experimental and Theoretical Physics. 

This presentation will attempt to illuminate the intellectual and philosophical history of Black Hole Thermodynamics through rigorously observing the shifting Mathematical and Physical landscape that both defined it and that it influenced. Jacob Bekenstein’s initial conjecture along with Stephen Hawking’s confirmation of the namesake ‘Hawking Radiation’ will be discussed in detail as well as subsequent developments by String Theorists and other camps within Theoretical Physics that strove to contribute to the imperative questions put forth by Quantum Gravity and greater Physical Cosmology. Thus, it is hoped that through a historical, yet in depth, overview of the subject, the imperative of history may be expounded to those interested in this fashionable field whilst maintaining succinct relevance to relative research topics. 

This will be achieved via a novel metatheoretical approach dubbed ‘The Weinberg Method’: a meta-theoretical renormalization framework combining axiomatic consistency analysis, information ontology, and historical epistemology to systematize theoretical physics.

 It is hoped that a push towards “cataloguing” the contemporary world of Physics will be insinuated in order to ensure that operational standards of Theoretical Physics (in this example at least) may be at their utmost refined at any given time to ensure that future research lays upon rigorous axioms and may always be consistently updated. 

This presentation then will contextualize Black Hole Thermodynamics within the greater ‘Weinberg Method’ framework.