Averaging conjecture for non-vacuum LRS Bianchi III solutions
Averaging conjecture for non-vacuum LRS Bianchi III solutions
Let be the solution of the quasi-standard system with arbitrary non-vacuum initial data satisfying , the Hamiltonian constraint, and . Let solve the corresponding averaged equation
where is the averaged vector field. Let and be the two-vectors formed from the and components of and , respectively. Averaging conjecture. There exists such that
This conjecture would provide the error estimate needed to justify the averaged description of the future behaviour, since the system has only quasi-standard rather than standard form. The source does not state a resolution.
Sources & referencesView supporting material
Primary source
David Fajman, Gernot Heißel and Maciej Maliborski, “On the oscillations and future asymptotics of locally rotationally symmetric Bianchi type III cosmologies with a massive scalar field”, arXiv:2001.00252 (2020).
Progress summary
Nothing recorded yet. Refresh searches the literature and the public web for attempts on this problem, and writes the first summary here.
Solutions 0
Sign in to submit a solution.
No solutions have been posted yet.