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dc.contributor.authorRodnianski, Igor
dc.contributor.authorSpeck, Jared R.
dc.date.accessioned2018-05-30T18:40:54Z
dc.date.available2018-05-30T18:40:54Z
dc.date.issued2017-12
dc.date.submitted2015-02
dc.identifier.issn0003-486X
dc.identifier.urihttp://hdl.handle.net/1721.1/115990
dc.description.abstractWe 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 coordinatesen_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant DMS-1162211)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (CAREER Grant DMS1454419)en_US
dc.description.sponsorshipAlfred P. Sloan Foundation. Fellowshipen_US
dc.description.sponsorshipSolomon Buchsbaum AT&T Research Funden_US
dc.publisherPrinceton University Pressen_US
dc.relation.isversionofhttp://dx.doi.org/10.4007/ANNALS.2018.187.1.2en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleA regime of linear stability for the Einstein-scalar field system with applications to nonlinear Big Bang formationen_US
dc.typeArticleen_US
dc.identifier.citationRodnianski, 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.departmentMassachusetts Institute of Technology. Department of Mathematicsen_US
dc.contributor.mitauthorSpeck, Jared R.
dc.relation.journalAnnals of Mathematicsen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2018-05-30T16:41:57Z
dspace.orderedauthorsRodnianski, Igor; Speck, Jareden_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-5020-3568
mit.licenseOPEN_ACCESS_POLICYen_US


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