The twenty first century has, thus far, been a period of rapid progress in cosmology. And yet this very success has begun to expose the limits of current methods and forced cosmologists to explore new ways of learning about the universe and its history. At this conference, we will explore three related areas where methodological innovation has been called for, and where it has already begun. One theme will concern the epistemology of inflation. Does inflationary cosmology inexorably lead us to postulate a multiverse where anything that can happen does happen? And if so, what does it mean to test a theory that is compatible with anything we might observe? Or can we treat inflation as a more conventional theory, with unambiguous observational signatures? A second theme will concern dark matter and dark energy. We have inferred the existence of these entities by comparing observational evidence with models of general relativity. But one might just as well infer, from the behavior of the visible matter in the universe, that general relativity breaks down at cosmological (or even galactic) length scales. What are the prospects for alternatives to general relativity at cosmological scales? How might cosmology be used to test general relativity? The final theme will concern the role of simulation in our understanding of the history of the actual universe. Can simulations be used to test theories of the early universe? Do they provide an independent source of information about cosmology, or are they an intermediary between theory and observation?
See the conference webpage for further details.
