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Gravitational Instantons With Conformally Kahler Geometry
Gravitational Instantons With Conformally Kahler Geometry
Gravitational Instantons With Conformally Kahler Geometry

상세정보

자료유형  
 학위논문 서양
최종처리일시  
20260202103556
ISBN  
9798288862427
DDC  
510
저자명  
Li, Mingyang.
서명/저자  
Gravitational Instantons With Conformally Kahler Geometry
발행사항  
[Sl] : University of California, Berkeley, 2025
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2025
형태사항  
140 p
주기사항  
Source: Dissertations Abstracts International, Volume: 87-01, Section: B.
주기사항  
Advisor: Sun, Song.
학위논문주기  
Thesis (Ph.D.)--University of California, Berkeley, 2025.
초록/해제  
요약We investigate the asymptotic geometry of Hermitian non-Kahler Ricci-flat metrics with finite ∫ |Rm|2 at infinity. Specifically, we prove:• Any such metric is asymptotic to an ALE, ALF-A, AF, skewed special Kasner, ALH∗ model, or their finite quotients at infinity.• Any Hermitian non-Kahler gravitational instanton with non-Euclidean volume growth is one of the following: the Kerr family, the Chen-Teo family, the Taub-bolt space, the reversed Taub-NUT space. This particularly confirms a conjecture by Aksteiner-Andersson. It includes the well-known Kerr family from general relativity. • Hermitian non-Kahler ALE gravitational instantons are in one-to-one correspondence with a special kind of Bach-flat Kahler orbifolds. The scalar curvature of the Bach-flat Kahler orbifolds is non-negative, vanishing at the orbifold point while being positive elsewhere. There is no Hermitian non-Kahler ALE gravitational instanton with structure group contained in SU(2), except for the Eguchi-Hanson metric with reversed orientation.• All Hermitian non-Kahler gravitational instantons can be compactified to log del Pezzo surfaces. This explains a curious relation to compact Hermitian non-Kahler Einstein 4-manifolds. For a 4-dimensional Ricci-flat metric, being Hermitian non-Kahler is equivalent to being non-trivially conformally Kahler.
일반주제명  
Mathematics
일반주제명  
Theoretical mathematics
일반주제명  
Applied mathematics
일반주제명  
Theoretical physics
키워드  
Finite quotients
키워드  
Asymptotic geometry
키워드  
Gravitational instanton
키워드  
Pezzo surfaces
기타저자  
University of California, Berkeley Mathematics
기본자료저록  
Dissertations Abstracts International. 87-01B.
전자적 위치 및 접속  
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MARC

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■020    ▼a9798288862427
■035    ▼a(MiAaPQ)AAI32042084
■040    ▼aMiAaPQ▼cMiAaPQ
■0820  ▼a510
■1001  ▼aLi,  Mingyang.
■24510▼aGravitational  Instantons  With  Conformally  Kahler  Geometry
■260    ▼a[Sl]▼bUniversity  of  California,  Berkeley▼c2025
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2025
■300    ▼a140  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  87-01,  Section:  B.
■500    ▼aAdvisor:  Sun,  Song.
■5021  ▼aThesis  (Ph.D.)--University  of  California,  Berkeley,  2025.
■520    ▼aWe  investigate  the  asymptotic  geometry  of  Hermitian  non-Kahler  Ricci-flat  metrics  with  finite  ∫  |Rm|2  at  infinity.  Specifically,  we  prove:•  Any  such  metric  is  asymptotic  to  an  ALE,  ALF-A,  AF,  skewed  special  Kasner,  ALH∗  model,  or  their  finite  quotients  at  infinity.•  Any  Hermitian  non-Kahler  gravitational  instanton  with  non-Euclidean  volume  growth  is  one  of  the  following:  the  Kerr  family,  the  Chen-Teo  family,  the  Taub-bolt  space,  the  reversed  Taub-NUT  space.  This  particularly  confirms  a  conjecture  by  Aksteiner-Andersson.  It  includes  the  well-known  Kerr  family  from  general  relativity. •  Hermitian  non-Kahler  ALE  gravitational  instantons  are  in  one-to-one  correspondence  with  a  special  kind  of  Bach-flat  Kahler  orbifolds.  The  scalar  curvature  of  the  Bach-flat  Kahler  orbifolds  is  non-negative,  vanishing  at  the  orbifold  point  while  being  positive  elsewhere.  There  is  no  Hermitian  non-Kahler  ALE  gravitational  instanton  with  structure  group  contained  in  SU(2),  except  for  the  Eguchi-Hanson  metric  with  reversed  orientation.•  All  Hermitian  non-Kahler  gravitational  instantons  can  be  compactified  to  log  del  Pezzo  surfaces.  This  explains  a  curious  relation  to  compact  Hermitian  non-Kahler  Einstein  4-manifolds. For  a  4-dimensional  Ricci-flat  metric,  being  Hermitian  non-Kahler  is  equivalent  to  being  non-trivially  conformally  Kahler.
■590    ▼aSchool  code:  0028.
■650  4▼aMathematics
■650  4▼aTheoretical  mathematics
■650  4▼aApplied  mathematics
■650  4▼aTheoretical  physics
■653    ▼aFinite  quotients
■653    ▼aAsymptotic  geometry
■653    ▼aGravitational  instanton
■653    ▼aPezzo  surfaces
■690    ▼a0405
■690    ▼a0642
■690    ▼a0753
■690    ▼a0364
■71020▼aUniversity  of  California,  Berkeley▼bMathematics.
■7730  ▼tDissertations  Abstracts  International▼g87-01B.
■790    ▼a0028
■791    ▼aPh.D.
■792    ▼a2025
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17357760▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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