| dc.contributor.author | Rodnianski, Igor | |
| dc.contributor.author | Speck, Jared R. | |
| dc.date.accessioned | 2018-05-30T18:40:54Z | |
| dc.date.available | 2018-05-30T18:40:54Z | |
| dc.date.issued | 2017-12 | |
| dc.date.submitted | 2015-02 | |
| dc.identifier.issn | 0003-486X | |
| dc.identifier.uri | http://hdl.handle.net/1721.1/115990 | |
| dc.description.abstract | We linearize the Einstein-scalar field equations, expressed relative to constant mean curvature (CMC)-transported spatial coordinates gauge, around members of the well-known family of Kasner solutions on (0;∞) × T[superscript 3]. The Kasner solutions model a spatially uniform scalar field evolving in a (typically) spatially anisotropic spacetime that expands towards the future and that has a "Big Bang" singularity at (t = 0). We place initial data for the linearized system along (t = 1) ≃ T[superscript 3] and study the linear solution's behavior in the collapsing direction t ↓ 0. Our first main result is the proof of an approximate L[superscript 2] monotonicity identity for the linear solutions. Using it, we prove a linear stability result that holds when the background Kasner solution is sufficiently close to the Friedmann-Lemaĭtre-Robertson-Walker (FLRW) solution. In particular, we show that as t ↓ 0, various time- rescaled components of the linear solution converge to regular functions defined along (t = 0). In addition, we motivate the preferred direction of the approximate monotonicity by showing that the CMC-transported spatial coordinates gauge can be viewed as a limiting version of a family of parabolic gauges for the lapse variable; an approximate monotonicity identity and corresponding linear stability results also hold in the para-bolic gauges, but the corresponding parabolic PDEs are locally well posed only in the direction t ↓ 0. Finally, based on the linear stability results, we outline a proof of the following result, whose complete proof will appear elsewhere: the FLRW solution is globally nonlinearly stable in the collapsing direction t↓ 0 under small perturbations of its data at (t = 1). Keywords: BKL conjectures, constant mean curvature, FLRW, Kasner solution, monotonicity, parabolic gauge, quiescent cosmology, spatial harmonic coordinates, stable blowup, strong cosmic censorship, transported spatial coordinates | en_US |
| dc.description.sponsorship | National Science Foundation (U.S.) (Grant DMS-1162211) | en_US |
| dc.description.sponsorship | National Science Foundation (U.S.) (CAREER Grant DMS1454419) | en_US |
| dc.description.sponsorship | Alfred P. Sloan Foundation. Fellowship | en_US |
| dc.description.sponsorship | Solomon Buchsbaum AT&T Research Fund | en_US |
| dc.publisher | Princeton University Press | en_US |
| dc.relation.isversionof | http://dx.doi.org/10.4007/ANNALS.2018.187.1.2 | en_US |
| dc.rights | Creative Commons Attribution-Noncommercial-Share Alike | en_US |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | en_US |
| dc.source | arXiv | en_US |
| dc.title | A regime of linear stability for the Einstein-scalar field system with applications to nonlinear Big Bang formation | en_US |
| dc.type | Article | en_US |
| dc.identifier.citation | Rodnianski, Igor, and Jared Speck. “A Regime of Linear Stability for the Einstein-Scalar Field System with Applications to Nonlinear Big Bang Formation.” Annals of Mathematics, vol. 187, no. 1, Jan. 2018, pp. 65–156. | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Mathematics | en_US |
| dc.contributor.mitauthor | Speck, Jared R. | |
| dc.relation.journal | Annals of Mathematics | en_US |
| dc.eprint.version | Author's final manuscript | en_US |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
| eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
| dc.date.updated | 2018-05-30T16:41:57Z | |
| dspace.orderedauthors | Rodnianski, Igor; Speck, Jared | en_US |
| dspace.embargo.terms | N | en_US |
| dc.identifier.orcid | https://orcid.org/0000-0001-5020-3568 | |
| mit.license | OPEN_ACCESS_POLICY | en_US |