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Signal Detection and Analysis for Gravitational Wave Astronomy
Signal Detection and Analysis for Gravitational Wave Astronomy
Signal Detection and Analysis for Gravitational Wave Astronomy

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자료유형  
 학위논문 서양
최종처리일시  
20260202103528
ISBN  
9798288866333
DDC  
530
저자명  
Leslie, Nathaniel Allen.
서명/저자  
Signal Detection and Analysis for Gravitational Wave Astronomy
발행사항  
[Sl] : University of California, Berkeley, 2025
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2025
형태사항  
125 p
주기사항  
Source: Dissertations Abstracts International, Volume: 87-02, Section: B.
주기사항  
Advisor: Dai, Liang.
학위논문주기  
Thesis (Ph.D.Physics.)--University of California, Berkeley, 2025.
초록/해제  
요약I provide an introduction to the field of gravitational wave data analysis, including a summary of the history and future of gravitational wave detection, a derivation of wave solutions to the linearized Einstein equations, a discussion of observable parameters of the sources of gravitational waves, how gravitational waves create strain in Michelson interferometers, and how that strain data is analyzed to extract those observable parameters. I present mode-by-mode relative binning, a new algorithm for fast and accurate likelihood estimation for gravitational waveform models with higher modes and precession effects. This method reduces full parameter estimation runtime from weeks to hours. I also discuss a new analytic gravitational waveform model for binaries undergoing small center-of-mass acceleration, including those in hierarchal triple systems. I present a Fisher analysis quantifying the detectability of this acceleration at various source chirp masses. Finally, I demonstrate how multi-messenger measurements of double white dwarf systems can be used to break the degeneracy between chirp mass and the impact of tides on orbital evolution. This can enable measurements of either tidal locking or moment of inertia of the white dwarfs without prohibitively expensive radial velocity measurements.
일반주제명  
Physics
일반주제명  
Astrophysics
일반주제명  
Computational physics
키워드  
Double white dwarf tides
키워드  
Gravitational wave parameter inference
키워드  
Gravitational waves
키워드  
Mode-by-mode relative binning
키워드  
Multi-messenger astronomy
기타저자  
University of California, Berkeley Physics
기본자료저록  
Dissertations Abstracts International. 87-02B.
전자적 위치 및 접속  
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MARC

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■020    ▼a9798288866333
■035    ▼a(MiAaPQ)AAI32039512
■040    ▼aMiAaPQ▼cMiAaPQ
■0820  ▼a530
■1001  ▼aLeslie,  Nathaniel  Allen.
■24510▼aSignal  Detection  and  Analysis  for  Gravitational  Wave  Astronomy
■260    ▼a[Sl]▼bUniversity  of  California,  Berkeley▼c2025
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2025
■300    ▼a125  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  87-02,  Section:  B.
■500    ▼aAdvisor:  Dai,  Liang.
■5021  ▼aThesis  (Ph.D.Physics.)--University  of  California,  Berkeley,  2025.
■520    ▼aI  provide  an  introduction  to  the  field  of  gravitational  wave  data  analysis,  including  a  summary  of  the  history  and  future  of  gravitational  wave  detection,  a  derivation  of  wave  solutions  to  the  linearized  Einstein  equations,  a  discussion  of  observable  parameters  of  the  sources  of  gravitational  waves,  how  gravitational  waves  create  strain  in  Michelson  interferometers,  and  how  that  strain  data  is  analyzed  to  extract  those  observable  parameters.  I  present  mode-by-mode  relative  binning,  a  new  algorithm  for  fast  and  accurate  likelihood  estimation  for  gravitational  waveform  models  with  higher  modes  and  precession  effects.  This  method  reduces  full  parameter  estimation  runtime  from  weeks  to  hours.  I  also  discuss  a  new  analytic  gravitational  waveform  model  for  binaries  undergoing  small  center-of-mass  acceleration,  including  those  in  hierarchal  triple  systems.  I  present  a  Fisher  analysis  quantifying  the  detectability  of  this  acceleration  at  various  source  chirp  masses.  Finally,  I  demonstrate  how  multi-messenger  measurements  of  double  white  dwarf  systems  can  be  used  to  break  the  degeneracy  between  chirp  mass  and  the  impact  of  tides  on  orbital  evolution.  This  can  enable  measurements  of  either  tidal  locking  or  moment  of  inertia  of  the  white  dwarfs  without  prohibitively  expensive  radial  velocity  measurements.
■590    ▼aSchool  code:  0028.
■650  4▼aPhysics
■650  4▼aAstrophysics
■650  4▼aComputational  physics
■653    ▼aDouble  white  dwarf  tides
■653    ▼aGravitational  wave  parameter  inference
■653    ▼aGravitational  waves
■653    ▼aMode-by-mode  relative  binning
■653    ▼aMulti-messenger  astronomy
■690    ▼a0605
■690    ▼a0596
■690    ▼a0216
■71020▼aUniversity  of  California,  Berkeley▼bPhysics.
■7730  ▼tDissertations  Abstracts  International▼g87-02B.
■790    ▼a0028
■791    ▼aPh.D.Physics.
■792    ▼a2025
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17357550▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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