서브메뉴
검색
Wormholes and Statistics in Quantum Gravity
Wormholes and Statistics in Quantum Gravity
상세정보
- 자료유형
- 학위논문 서양
- 최종처리일시
- 20260202104808
- ISBN
- 9798293824052
- DDC
- 530
- 서명/저자
- Wormholes and Statistics in Quantum Gravity
- 발행사항
- [Sl] : Cornell University, 2025
- 발행사항
- Ann Arbor : ProQuest Dissertations & Theses, 2025
- 형태사항
- 594 p
- 주기사항
- Source: Dissertations Abstracts International, Volume: 87-03, Section: B.
- 주기사항
- Advisor: Hartman, Thomas.
- 학위논문주기
- Thesis (Ph.D.)--Cornell University, 2025.
- 초록/해제
- 요약In this thesis, we present our work on computing signatures of quantum chaos in gravity. More specifically, we show how higher topologies in the gravitational path integral-called Euclidean wormholes- encode statistical properties of the data of strongly coupled Conformal Field Theories (CFTs) thereby establishing how quantum gravity realizes a version of the Eigenstate Thermalization Hypothesis (ETH) based on the randomness of CFT data.First, we propose a novel correspondence between wormhole solutions to Einstein's equations in semiclassical 3D gravity and averages of corresponding observables in 2D CFT and support out proposal using several examples. We then discuss the construction of wormholes in higher dimensions sourced by spherically symmetric thin shells of dust particles and interpret them in individual CFTs in terms of coarse-graining CFT data.Developing this idea further, we establish a correspondence between the statistics of black holes formed from such dust shells in 3D gravity and the dynamics of a non-conformal line defect in 2D CFT. We also construct wormholes using domain wall solutions in AdS/CFT and show how these wormholes capture covariances between observables in different CFTs thereby providing a precision test for the realization of ETH in gravity.As an interesting application, by employing information-theoretic ideas, we construct a quantitative random tensor network model for black holes using CFT data, which exhibits essential features of the black hole interior.
- 일반주제명
- Physics
- 일반주제명
- Theoretical physics
- 일반주제명
- Statistical physics
- 일반주제명
- Astrophysics
- 일반주제명
- Computational physics
- 키워드
- Gravity
- 기타저자
- Cornell University Physics
- 기본자료저록
- Dissertations Abstracts International. 87-03B.
- 전자적 위치 및 접속
- 로그인 후 원문을 볼 수 있습니다.
MARC
008260126s2025 us c eng d■001000017358909
■00520260202104808
■006m o d
■007cr#unu||||||||
■020 ▼a9798293824052
■035 ▼a(MiAaPQ)AAI32166525
■040 ▼aMiAaPQ▼cMiAaPQ
■0820 ▼a530
■1001 ▼aNamburi, Jeevan Chandra.▼0(orcid)0000-0001-9978-5992
■24510▼aWormholes and Statistics in Quantum Gravity
■260 ▼a[Sl]▼bCornell University▼c2025
■260 1▼aAnn Arbor▼bProQuest Dissertations & Theses▼c2025
■300 ▼a594 p
■500 ▼aSource: Dissertations Abstracts International, Volume: 87-03, Section: B.
■500 ▼aAdvisor: Hartman, Thomas.
■5021 ▼aThesis (Ph.D.)--Cornell University, 2025.
■520 ▼aIn this thesis, we present our work on computing signatures of quantum chaos in gravity. More specifically, we show how higher topologies in the gravitational path integral-called Euclidean wormholes- encode statistical properties of the data of strongly coupled Conformal Field Theories (CFTs) thereby establishing how quantum gravity realizes a version of the Eigenstate Thermalization Hypothesis (ETH) based on the randomness of CFT data.First, we propose a novel correspondence between wormhole solutions to Einstein's equations in semiclassical 3D gravity and averages of corresponding observables in 2D CFT and support out proposal using several examples. We then discuss the construction of wormholes in higher dimensions sourced by spherically symmetric thin shells of dust particles and interpret them in individual CFTs in terms of coarse-graining CFT data.Developing this idea further, we establish a correspondence between the statistics of black holes formed from such dust shells in 3D gravity and the dynamics of a non-conformal line defect in 2D CFT. We also construct wormholes using domain wall solutions in AdS/CFT and show how these wormholes capture covariances between observables in different CFTs thereby providing a precision test for the realization of ETH in gravity.As an interesting application, by employing information-theoretic ideas, we construct a quantitative random tensor network model for black holes using CFT data, which exhibits essential features of the black hole interior.
■590 ▼aSchool code: 0058.
■650 4▼aPhysics
■650 4▼aTheoretical physics
■650 4▼aStatistical physics
■650 4▼aAstrophysics
■650 4▼aComputational physics
■653 ▼aEuclidean wormholes
■653 ▼aGravity
■653 ▼aEigenstate Thermalization Hypothesis
■653 ▼aConformal Field Theories
■653 ▼aEinstein's equations
■690 ▼a0605
■690 ▼a0753
■690 ▼a0596
■690 ▼a0217
■690 ▼a0216
■71020▼aCornell University▼bPhysics.
■7730 ▼tDissertations Abstracts International▼g87-03B.
■790 ▼a0058
■791 ▼aPh.D.
■792 ▼a2025
■793 ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17358909▼nKERIS▼z이 자료의 원문은 한국교육학술정보원에서 제공합니다.
