{"title":"Decay Estimates for q (Theorem M1)","authors":"S. Klainerman, J. Szeftel","doi":"10.23943/PRINCETON/9780691212425.003.0005","DOIUrl":null,"url":null,"abstract":"This chapter examines the proof for Theorem M1, deriving decay estimates for the quantity q for k ≤ k\n small + 20 derivatives. To this end, it uses the wave equation satisfied by q. The spacetime M is decomposed as M = (int)M u (ext)M and that u is an outgoing optical function on (ext)M while u is an ingoing optical function. The chapter relies on the global frame defined in section 3.5, and r and m denote the corresponding scalar functions associated to it. It also proves two theorems on improved weighted estimates, as well as flux decay estimates for q.","PeriodicalId":371134,"journal":{"name":"Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations","volume":"2003 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.23943/PRINCETON/9780691212425.003.0005","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
This chapter examines the proof for Theorem M1, deriving decay estimates for the quantity q for k ≤ k
small + 20 derivatives. To this end, it uses the wave equation satisfied by q. The spacetime M is decomposed as M = (int)M u (ext)M and that u is an outgoing optical function on (ext)M while u is an ingoing optical function. The chapter relies on the global frame defined in section 3.5, and r and m denote the corresponding scalar functions associated to it. It also proves two theorems on improved weighted estimates, as well as flux decay estimates for q.