“Many researchers believe that physics will not be complete until it can explain not just the behavior of space and time, but where these entities come from”

             is a gripping thought at the start of an article on space-time appeared in the Nature magazine last year. I fully enjoyed the article, which indeed conveyed in fine detail the overall progress made in physics in our quest to envision the absolute nature. While brilliant theories (some of them I hope to discuss later on) address sharp ways to see the structure and flow of space-time, figuring out an origin would be an entirely different undertaking, and perhaps the most difficult one.

                In a broad sense, the current state of physics knowledge point to an infinitely curved space-time where matter was infinitely condensed (about a billionth the size of a subatomic particle)—referred to as “gravitational singularity”—to be a beginning point from which the universe expanded. The obvious question ensues. Where from this surpassingly dense material emerge? Whereas, overall, we have a crisp picture of how matter evolved through the physical forces into the enormously expanded universe we see today (the depiction included below), tracing it back our interpretive theories only culminate into this very “point.”

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                    Can the information be interpreted in such a way that there aren’t major lacunae left behind, and we can see a rational picture?