Living Reviews in Relativity最新文献

筛选
英文 中文
Coalescence of Black Hole-Neutron Star Binaries 黑洞-中子星双星的合并
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2011-08-29 DOI: 10.12942/lrr-2011-6
Masaru Shibata, Keisuke Taniguchi
{"title":"Coalescence of Black Hole-Neutron Star Binaries","authors":"Masaru Shibata,&nbsp;Keisuke Taniguchi","doi":"10.12942/lrr-2011-6","DOIUrl":"https://doi.org/10.12942/lrr-2011-6","url":null,"abstract":"<p>We review the current status of general relativistic studies for the coalescence of black hole-neutron star (BH-NS) binaries. First, procedures for a solution of BH-NS binaries in quasi-equilibrium circular orbits and the numerical results, such as quasi-equilibrium sequence and mass-shedding limit, of the high-precision computation, are summarized. Then, the current status of numerical-relativity simulations for the merger of BH-NS binaries is described. We summarize our understanding for the merger and/or tidal disruption processes, the criterion for tidal disruption, the properties of the remnant formed after the tidal disruption, gravitational waveform, and gravitational-wave spectrum.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"14 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2011-08-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2011-6","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"5106035","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 291
Gravitational Wave Detection by Interferometry (Ground and Space) 干涉测量引力波探测(地面和空间)
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2011-07-11 DOI: 10.12942/lrr-2011-5
Matthew Pitkin, Stuart Reid, Sheila Rowan, Jim Hough
{"title":"Gravitational Wave Detection by Interferometry (Ground and Space)","authors":"Matthew Pitkin,&nbsp;Stuart Reid,&nbsp;Sheila Rowan,&nbsp;Jim Hough","doi":"10.12942/lrr-2011-5","DOIUrl":"https://doi.org/10.12942/lrr-2011-5","url":null,"abstract":"<p>Significant progress has been made in recent years on the development of gravitational-wave detectors. Sources such as coalescing compact binary systems, neutron stars in low-mass X-ray binaries, stellar collapses and pulsars are all possible candidates for detection. The most promising design of gravitational-wave detector uses test masses a long distance apart and freely suspended as pendulums on Earth or in drag-free spacecraft. The main theme of this review is a discussion of the mechanical and optical principles used in the various long baseline systems in operation around the world — LIGO (USA), Virgo (Italy/France), TAMA300 and LCGT (Japan), and GEO600 (Germany/U.K.) — and in LISA, a proposed space-borne interferometer. A review of recent science runs from the current generation of ground-based detectors will be discussed, in addition to highlighting the astrophysical results gained thus far. Looking to the future, the major upgrades to LIGO (Advanced LIGO), Virgo (Advanced Virgo), LCGT and GEO600 (GEO-HF) will be completed over the coming years, which will create a network of detectors with the significantly improved sensitivity required to detect gravitational waves. Beyond this, the concept and design of possible future “third generation” gravitational-wave detectors, such as the Einstein Telescope (ET), will be discussed.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"14 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2011-07-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2011-5","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4460558","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 152
The Einstein-Vlasov System/Kinetic Theory 爱因斯坦-弗拉索夫系统/动力学理论
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2011-05-27 DOI: 10.12942/lrr-2011-4
Håkan Andréasson
{"title":"The Einstein-Vlasov System/Kinetic Theory","authors":"Håkan Andréasson","doi":"10.12942/lrr-2011-4","DOIUrl":"https://doi.org/10.12942/lrr-2011-4","url":null,"abstract":"<p>The main purpose of this article is to provide a guide to theorems on global properties of solutions to the Einstein-Vlasov system. This system couples Einstein’s equations to a kinetic matter model. Kinetic theory has been an important field of research during several decades in which the main focus has been on non-relativistic and special relativistic physics, i.e., to model the dynamics of neutral gases, plasmas, and Newtonian self-gravitating systems. In 1990, Rendall and Rein initiated a mathematical study of the Einstein-Vlasov system. Since then many theorems on global properties of solutions to this system have been established. This paper gives introductions to kinetic theory in non-curved spacetimes and then the Einstein-Vlasov system is introduced. We believe that a good understanding of kinetic theory in non-curved spacetimes is fundamental to a good comprehension of kinetic theory in general relativity.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"14 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2011-05-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2011-4","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"5050437","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 114
Analogue Gravity 模拟重力
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2011-05-11 DOI: 10.12942/lrr-2011-3
Carlos Barceló, Stefano Liberati, Matt Visser
{"title":"Analogue Gravity","authors":"Carlos Barceló,&nbsp;Stefano Liberati,&nbsp;Matt Visser","doi":"10.12942/lrr-2011-3","DOIUrl":"https://doi.org/10.12942/lrr-2011-3","url":null,"abstract":"<p>Analogue gravity is a research programme which investigates analogues of general relativistic gravitational fields within other physical systems, typically but not exclusively condensed matter systems, with the aim of gaining new insights into their corresponding problems. Analogue models of (and for) gravity have a long and distinguished history dating back to the earliest years of general relativity. In this review article we will discuss the history, aims, results, and future prospects for the various analogue models. We start the discussion by presenting a particularly simple example of an analogue model, before exploring the rich history and complex tapestry of models discussed in the literature. The last decade in particular has seen a remarkable and sustained development of analogue gravity ideas, leading to some hundreds of published articles, a workshop, two books, and this review article. Future prospects for the analogue gravity programme also look promising, both on the experimental front (where technology is rapidly advancing) and on the theoretical front (where variants of analogue models can be used as a springboard for radical attacks on the problem of quantum gravity).</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"14 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2011-05-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2011-3","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4469055","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 23
Varying Constants, Gravitation and Cosmology 变常数,万有引力和宇宙学
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2011-03-29 DOI: 10.12942/lrr-2011-2
Jean-Philippe Uzan
{"title":"Varying Constants, Gravitation and Cosmology","authors":"Jean-Philippe Uzan","doi":"10.12942/lrr-2011-2","DOIUrl":"https://doi.org/10.12942/lrr-2011-2","url":null,"abstract":"<p>Fundamental constants are a cornerstone of our physical laws. Any constant varying in space and/or time would reflect the existence of an almost massless field that couples to matter. This will induce a violation of the universality of free fall. Thus, it is of utmost importance for our understanding of gravity and of the domain of validity of general relativity to test for their constancy. We detail the relations between the constants, the tests of the local position invariance and of the universality of free fall. We then review the main experimental and observational constraints that have been obtained from atomic clocks, the Oklo phenomenon, solar system observations, meteorite dating, quasar absorption spectra, stellar physics, pulsar timing, the cosmic microwave background and big bang nucleosynthesis. At each step we describe the basics of each system, its dependence with respect to the constants, the known systematic effects and the most recent constraints that have been obtained. We then describe the main theoretical frameworks in which the low-energy constants may actually be varying and we focus on the unification mechanisms and the relations between the variation of different constants. To finish, we discuss the more speculative possibility of understanding their numerical values and the apparent fine-tuning that they confront us with.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"14 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2011-03-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2011-2","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"5623897","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 582
Gravitational Waves from Gravitational Collapse 来自引力坍缩的引力波
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2011-01-20 DOI: 10.12942/lrr-2011-1
Chris L. Fryer, Kimberly C. B. New
{"title":"Gravitational Waves from Gravitational Collapse","authors":"Chris L. Fryer,&nbsp;Kimberly C. B. New","doi":"10.12942/lrr-2011-1","DOIUrl":"https://doi.org/10.12942/lrr-2011-1","url":null,"abstract":"<p>Gravitational-wave emission from stellar collapse has been studied for nearly four decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non-axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with ground-based and space-based interferometric observatories. This review covers the entire range of stellar collapse sources of gravitational waves: from the accretion-induced collapse of a white dwarf through the collapse down to neutron stars or black holes of massive stars to the collapse of supermassive stars.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"14 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2011-01-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2011-1","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4788137","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 91
Tests of Gravity Using Lunar Laser Ranging 用月球激光测距测试重力
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2010-11-02 DOI: 10.12942/lrr-2010-7
Stephen M. Merkowitz
{"title":"Tests of Gravity Using Lunar Laser Ranging","authors":"Stephen M. Merkowitz","doi":"10.12942/lrr-2010-7","DOIUrl":"https://doi.org/10.12942/lrr-2010-7","url":null,"abstract":"<p>Lunar laser ranging (LLR) has been a workhorse for testing general relativity over the past four decades. The three retroreflector arrays put on the Moon by the Apollo astronauts and the French built arrays on the Soviet Lunokhod rovers continue to be useful targets, and have provided the most stringent tests of the Strong Equivalence Principle and the time variation of Newton’s gravitational constant. The relatively new ranging system at the Apache Point 3.5 meter telescope now routinely makes millimeter level range measurements. Incredibly, it has taken 40 years for ground station technology to advance to the point where characteristics of the lunar retroreflectors are limiting the precision of the range measurements. In this article, we review the gravitational science and technology of lunar laser ranging and discuss prospects for the future.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"13 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2010-11-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2010-7","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4098460","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 70
Quantization of Midisuperspace Models 中超空间模型的量化
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2010-10-14 DOI: 10.12942/lrr-2010-6
J. Fernando Barbero G., Eduardo J. S. Villaseñor
{"title":"Quantization of Midisuperspace Models","authors":"J. Fernando Barbero G.,&nbsp;Eduardo J. S. Villaseñor","doi":"10.12942/lrr-2010-6","DOIUrl":"https://doi.org/10.12942/lrr-2010-6","url":null,"abstract":"<p>We give a comprehensive review of the quantization of midisuperspace models. Though the main focus of the paper is on quantum aspects, we also provide an introduction to several classical points related to the definition of these models. We cover some important issues, in particular, the use of the principle of symmetric criticality as a very useful tool to obtain the required Hamiltonian formulations. Two main types of reductions are discussed: those involving metrics with two Killing vector fields and spherically-symmetric models. We also review the more general models obtained by coupling matter fields to these systems. Throughout the paper we give separate discussions for standard quantizations using geometrodynamical variables and those relying on loop-quantum-gravity-inspired methods.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"13 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2010-10-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2010-6","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4586290","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 33
Brane-World Gravity Brane-World重力
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2010-09-14 DOI: 10.12942/lrr-2010-5
Roy Maartens, Kazuya Koyama
{"title":"Brane-World Gravity","authors":"Roy Maartens,&nbsp;Kazuya Koyama","doi":"10.12942/lrr-2010-5","DOIUrl":"https://doi.org/10.12942/lrr-2010-5","url":null,"abstract":"<p>The observable universe could be a 1+3-surface (the “brane”) embedded in a 1+3+<i>d</i>-dimensional spacetime (the “bulk”), with Standard Model particles and fields trapped on the brane while gravity is free to access the bulk. At least one of the <i>d</i> extra spatial dimensions could be very large relative to the Planck scale, which lowers the fundamental gravity scale, possibly even down to the electroweak (~ TeV) level. This revolutionary picture arises in the framework of recent developments in M theory. The 1+10-dimensional M theory encompasses the known 1+9-dimensional superstring theories, and is widely considered to be a promising potential route to quantum gravity. At low energies, gravity is localized at the brane and general relativity is recovered, but at high energies gravity “leaks” into the bulk, behaving in a truly higher-dimensional way. This introduces significant changes to gravitational dynamics and perturbations, with interesting and potentially testable implications for high-energy astrophysics, black holes, and cosmology. Brane-world models offer a phenomenological way to test some of the novel predictions and corrections to general relativity that are implied by M theory. This review analyzes the geometry, dynamics and perturbations of simple brane-world models for cosmology and astrophysics, mainly focusing on warped 5-dimensional brane-worlds based on the Randall-Sundrum models. We also cover the simplest brane-world models in which 4-dimensional gravity on the brane is modified at <i>low</i> energies — the 5-dimensional Dvali-Gabadadze-Porrati models. Then we discuss co-dimension two branes in 6-dimensional models.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"13 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2010-09-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2010-5","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4587823","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 965
The Pioneer Anomaly 先锋号异常
IF 40.6 2区 物理与天体物理
Living Reviews in Relativity Pub Date : 2010-09-01 DOI: 10.12942/lrr-2010-4
Slava G. Turyshev, Viktor T. Toth
{"title":"The Pioneer Anomaly","authors":"Slava G. Turyshev,&nbsp;Viktor T. Toth","doi":"10.12942/lrr-2010-4","DOIUrl":"https://doi.org/10.12942/lrr-2010-4","url":null,"abstract":"<p>Radio-metric Doppler tracking data received from the Pioneer 10 and 11 spacecraft from heliocentric distances of 20–70 AU has consistently indicated the presence of a small, anomalous, blue-shifted frequency drift uniformly changing with a rate of ~ 6 × 10<sup>?9</sup> Hz/s. Ultimately, the drift was interpreted as a constant sunward deceleration of each particular spacecraft at the level of <i>a</i><sub><i>P</i></sub> = (8.74 ± 1.33) × 10<sup>?10</sup> m/s<sup>2</sup>. This apparent violation of the Newton’s gravitational inverse-square law has become known as the Pioneer anomaly; the nature of this anomaly remains unexplained. In this review, we summarize the current knowledge of the physical properties of the anomaly and the conditions that led to its detection and characterization. We review various mechanisms proposed to explain the anomaly and discuss the current state of efforts to determine its nature. A comprehensive new investigation of the anomalous behavior of the two Pioneers has begun recently. The new efforts rely on the much-extended set of radio-metric Doppler data for both spacecraft in conjunction with the newly available complete record of their telemetry files and a large archive of original project documentation. As the new study is yet to report its findings, this review provides the necessary background for the new results to appear in the near future. In particular, we provide a significant amount of information on the design, operations and behavior of the two Pioneers during their entire missions, including descriptions of various data formats and techniques used for their navigation and radio-science data analysis. As most of this information was recovered relatively recently, it was not used in the previous studies of the Pioneer anomaly, but it is critical for the new investigation.</p>","PeriodicalId":686,"journal":{"name":"Living Reviews in Relativity","volume":"13 1","pages":""},"PeriodicalIF":40.6,"publicationDate":"2010-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrr-2010-4","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4412422","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 148
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
相关产品
×
本文献相关产品
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信