Emergence of cosmic space a unified approach
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Abstract
The general theory of relativity is a highly successful theory. It has excelled
newlinein explaining astronomical phenomena and making precise predictions, many of
newlinewhich have been observationally verified. However, the theory also faces challenges
newlinewhen dealing with extreme scenarios, like the collapse of massive stars or the
newlineearly moments of the Universe. Singularities emerge in these conditions where
newlinethe theory breaks down, revealing its incompleteness. Efforts to address these
newlinesingularities have included formulating a quantum theory of gravity, but a successful
newlinequantum theory corresponding to general relativity has yet to be achieved. These
newlineproblems, rooted in the unique structure of Einstein s gravity. These intricacies
newlinepresent formidable challenges in the quest for quantum gravity. This situation
newlineunderscores the incompleteness of general relativity and prompts the exploration of
newlinealternative paradigms for understanding gravity. What sets gravity apart from other
newlinefundamental forces is its profound connection to the thermodynamics of spacetime,
newlinea characteristic that lacks a natural explanation within the framework of general
newlinerelativity.
newlineThe connection between gravity and thermodynamics first emerged in the study
newlineof black hole physics. In 1973, Bekenstein proposed that black holes possess entropy
newlineproportional to their horizon area. Subsequently, Bardeen and others formulated
newlinelaws of black hole dynamics analogous to the laws of thermodynamics, and Hawking
newlineshowed that black holes also possess temperature and can emit radiation. All these
newlineled to the association of temperature and entropy with black holes, raising questions
newlineabout why solutions of general relativity, like black holes, exhibit thermodynamic
newlineproperties. Subsequently, Unruh s work revealed that the phenomenon of black
newlinebody radiation and the associated temperature characteristics of spacetime are not
newlineexclusive to black holes.