Top Qs
Timeline
Chat
Perspective
Hartle–Hawking proposal
Proposal concerning the state of the universe prior to the Planck epoch From Wikipedia, the free encyclopedia
Remove ads
The Hartle–Hawking state, also known as the no-boundary wave function, is a cosmological model that applies quantum mechanics to the Big Bang.[2]: 769 It is named after James Hartle and Stephen Hawking, who first proposed it in 1983.[3][4] The concept can also be considered as an initial condition for models of quantum cosmology.[5]: 14

Remove ads
Ingredients
The Hartle-Hawking proposal includes several ingredients. First it uses Richard Feynman's sum over histories approach to quantum mechanics. In this approach every possible path a particle can take through spacetime contributes to the solution with its own an amplitude and phase. Technical challenges with those sums lead to the second ingredient, a transformation to Euclidean space-time: a geometry which combines 3 space dimensions with an imaginary time dimension.[6]: 172 This is related to the Wick rotation, , and it converts the spacetime metric in to a Euclidean metric, . In Hawking approach this rotation is applied to every path, not to the background space of the paths as in Wick's approach and therefore the sum of histories becomes a quantum superposition of spacetimes.[2]: 769 This curved Euclidean spacetime can be analogous to a sphere in being both finite in extent and yet have no boundary.[6]: 174
Remove ads
History
The original 1983 paper by Hartle and Hawking grew out of a summer visit by Hawking to UC Santa Barbara where Hartle worked. Hawking was exploring the idea that the boundary condition for space time was simply no-boundary at all. With Hartle this idea was converted in to a proposal and published.[6]: 175 In 1998 Hawking worked with Neil Turok to expand the Hartle-Hawking concept to include a hyperbolic or open geometry.[7][2][8][1]
Remove ads
See also
References
Wikiwand - on
Seamless Wikipedia browsing. On steroids.
Remove ads
