語系:
繁體中文
English
說明(常見問題)
回圖書館首頁
手機版館藏查詢
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
FindBook
Google Book
Amazon
博客來
Gravitational Wave Echoes: Theory and Application.
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Gravitational Wave Echoes: Theory and Application./
作者:
Conklin, Randy S.
出版者:
Ann Arbor : ProQuest Dissertations & Theses, : 2021,
面頁冊數:
165 p.
附註:
Source: Dissertations Abstracts International, Volume: 83-06, Section: B.
Contained By:
Dissertations Abstracts International83-06B.
標題:
Physics. -
電子資源:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=28768040
ISBN:
9798496548274
Gravitational Wave Echoes: Theory and Application.
Conklin, Randy S.
Gravitational Wave Echoes: Theory and Application.
- Ann Arbor : ProQuest Dissertations & Theses, 2021 - 165 p.
Source: Dissertations Abstracts International, Volume: 83-06, Section: B.
Thesis (Ph.D.)--University of Toronto (Canada), 2021.
This item must not be sold to any third party vendors.
Black hole mimickers may compose some of what is assumed as the black hole population, and multiple groups have claimed evidence for this in the form of gravitational wave echoes. This thesis elaborates on work by the author and collaborators, detailing echo theory and discussing hints of echoes in gravitational wave data from the LIGO observatory.Echoes from a variety of exotic compact objects are compared, and the effects of spin are investigated. The most characteristic feature of echoes, a series of spectral resonances, is exploited to look for this structure in LIGO data via windowing methods.These resonances are modulated by an initial-condition-dependent source integral, and it is shown that echo features traditionally assumed to be known may be altered by generic production mechanisms. The complete modulation in all variables is calculated, and the impact on echoes is displayed. An analytical method is constructed to test asymptotic radial perturbations. Quantum quadratic gravity is a theory capable of producing echoes, and it can be made renormalizable with ultraviolet completions. It may also satisfy the optical theorem under certain conditions, and these are reviewed and further explored through two subjects: the physical particle spectrum and the complex prescription of propagators. Required conditions for unitarity are defined along with their consequences, and the consistency of the theory is tested against these.The search for echoes is then continued in a recently detected gravitational wave event, GW190521, by employing the latest developments in echo theory. Combining advancements in physical boundary conditions, numerical relativity, and complex representation of the echo spectrum, a model is built to seek for physically motivated echoes across background parameters of mass, spin, and geometry. The search is done over Monte Carlo chains distributed according to background parameter probabilities, with significance assessed by signal to noise ratios and statistical analysis.Potential echo detections in the LIGO events GW151226, GW170104, GW170608, GW170814, and GW170817 are presented with false alarm rates of 1 in 700 or less using the older windowing methods. The latest model is employed to find a false alarm rate of 1 in 50 in GW190521.
ISBN: 9798496548274Subjects--Topical Terms:
516296
Physics.
Subjects--Index Terms:
Black holes
Gravitational Wave Echoes: Theory and Application.
LDR
:03392nmm a2200373 4500
001
2352512
005
20221128104005.5
008
241004s2021 ||||||||||||||||| ||eng d
020
$a
9798496548274
035
$a
(MiAaPQ)AAI28768040
035
$a
AAI28768040
040
$a
MiAaPQ
$c
MiAaPQ
100
1
$a
Conklin, Randy S.
$3
3692149
245
1 0
$a
Gravitational Wave Echoes: Theory and Application.
260
1
$a
Ann Arbor :
$b
ProQuest Dissertations & Theses,
$c
2021
300
$a
165 p.
500
$a
Source: Dissertations Abstracts International, Volume: 83-06, Section: B.
500
$a
Advisor: Holdom, Bob.
502
$a
Thesis (Ph.D.)--University of Toronto (Canada), 2021.
506
$a
This item must not be sold to any third party vendors.
520
$a
Black hole mimickers may compose some of what is assumed as the black hole population, and multiple groups have claimed evidence for this in the form of gravitational wave echoes. This thesis elaborates on work by the author and collaborators, detailing echo theory and discussing hints of echoes in gravitational wave data from the LIGO observatory.Echoes from a variety of exotic compact objects are compared, and the effects of spin are investigated. The most characteristic feature of echoes, a series of spectral resonances, is exploited to look for this structure in LIGO data via windowing methods.These resonances are modulated by an initial-condition-dependent source integral, and it is shown that echo features traditionally assumed to be known may be altered by generic production mechanisms. The complete modulation in all variables is calculated, and the impact on echoes is displayed. An analytical method is constructed to test asymptotic radial perturbations. Quantum quadratic gravity is a theory capable of producing echoes, and it can be made renormalizable with ultraviolet completions. It may also satisfy the optical theorem under certain conditions, and these are reviewed and further explored through two subjects: the physical particle spectrum and the complex prescription of propagators. Required conditions for unitarity are defined along with their consequences, and the consistency of the theory is tested against these.The search for echoes is then continued in a recently detected gravitational wave event, GW190521, by employing the latest developments in echo theory. Combining advancements in physical boundary conditions, numerical relativity, and complex representation of the echo spectrum, a model is built to seek for physically motivated echoes across background parameters of mass, spin, and geometry. The search is done over Monte Carlo chains distributed according to background parameter probabilities, with significance assessed by signal to noise ratios and statistical analysis.Potential echo detections in the LIGO events GW151226, GW170104, GW170608, GW170814, and GW170817 are presented with false alarm rates of 1 in 700 or less using the older windowing methods. The latest model is employed to find a false alarm rate of 1 in 50 in GW190521.
590
$a
School code: 0779.
650
4
$a
Physics.
$3
516296
650
4
$a
Theoretical physics.
$3
2144760
650
4
$a
Astrophysics.
$3
535904
650
4
$a
Computational physics.
$3
3343998
653
$a
Black holes
653
$a
Echoes
653
$a
Gravity
653
$a
Quantum
690
$a
0605
690
$a
0753
690
$a
0596
690
$a
0216
710
2
$a
University of Toronto (Canada).
$b
Physics.
$3
3171865
773
0
$t
Dissertations Abstracts International
$g
83-06B.
790
$a
0779
791
$a
Ph.D.
792
$a
2021
793
$a
English
856
4 0
$u
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=28768040
筆 0 讀者評論
館藏地:
全部
電子資源
出版年:
卷號:
館藏
1 筆 • 頁數 1 •
1
條碼號
典藏地名稱
館藏流通類別
資料類型
索書號
使用類型
借閱狀態
預約狀態
備註欄
附件
W9474950
電子資源
11.線上閱覽_V
電子書
EB
一般使用(Normal)
在架
0
1 筆 • 頁數 1 •
1
多媒體
評論
新增評論
分享你的心得
Export
取書館
處理中
...
變更密碼
登入