-
81por Weinstein, A“…We will survey the techniques and technologies for detecting gravitational waves for the first time, including bar detectors and broadband interferometers, and give a brief status report on the international search effort, with special emphasis on the LIGO detectors and search results.…”
Publicado 2005
Enlace del recurso
-
82“…Moreover, its amplitude for a GUT scale scenario turns out to be within the range and sensitivity of BBO and marginally detectable by LIGO and LISA. This new gravitational wave background can compete with the one generated during inflation, and distinguishing both may require extra information.…”
Enlace del recurso
Enlace del recurso
-
83“…The LIGO observation of gravitational waves from a binary black hole merger has begun a new era in fundamental physics. …”
Enlace del recurso
Enlace del recurso
-
84“…Using recent experimental results of detection of gravitational waves from the binary black hole signals by Advanced LIGO and Advanced Virgo, we investigate the propagation of gravitational waves in the context of fourth order gravity nonminimally coupled to a massive scalar field. …”
Enlace del recurso
Enlace del recurso
-
85“…Currently, the sub-60 Hz sensitivity of gravitational-wave (GW) detectors like Advanced LIGO (aLIGO) is limited by the control noises from auxiliary degrees of freedom which nonlinearly couple to the main GW readout. …”
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
86por Landry, Michael R“…In this three-part lecture series, we give an overview of the field, including material on gravitional wave sources, detection methods, some details of interferometric detectors, data analysis methods, and current results from observational data-taking runs of the LIGO and GEO projects.…”
Publicado 2006
Enlace del recurso
-
87por Ellis, John, Hütsi, Gert, Kannike, Kristjan, Marzola, Luca, Raidal, Martti, Vaskonen, Ville“…In particular, our calculations indicate that the presence of a DM core with a mass fraction ∼5% could affect significantly the interpretation of these NS data as constraints on the nuclear equation of state (EOS), potentially excluding some EOS models on the basis of the measured mass of PSR J0348+0432, while allowing other EOS models to become consistent with the LIGO/Virgo upper limit on Λ. Specific scenarios for generating such DM cores are explored in an Appendix.…”
Publicado 2018
Enlace del recurso
Enlace del recurso
-
88“…In this case, they produce a stochastic background of gravitational waves that evades current pulsar timing bounds, but features a flat spectrum with amplitude h2ΩGW∼10−8 at interferometer frequencies. Ongoing and future LIGO observations will hence probe the scale of B−L breaking.…”
Enlace del recurso
Enlace del recurso
-
89“…The SGWB produced by cosmic strings with such values of Gμ would be beyond the reach of LIGO, but could be measured by other planned and proposed detectors such as SKA, LISA, TianQin, AION-1 km, AEDGE, Einstein Telescope, and Cosmic Explorer.…”
Enlace del recurso
Enlace del recurso
-
90por Bernitt, Sonja, Bertone, Gianfranco, Cardoso, Vitor, Emparan, Roberto, Galatyuk, Tetyana, Kurkela, Aleksi, Larsen, Ann-Cecilie, Nahrgang, Marlene, Nissanke, Samaya, Pani, Paolo, Porto, Rafael, Riotto, Antonio, Rosswog, Stephan“…Recording a GW […] has never been a big motivation for LIGO, the motivation has always been to open a new window to the Universe.…”
Publicado 2022
Enlace del recurso
Enlace del recurso
-
91por TROVATO, Agata“…<!--HTML-->The LIGO and Virgo collaborations actively pursue an open science program. …”
Publicado 2021
Enlace del recurso
-
92por Palenzuela, Carlos, Pani, Paolo, Bezares, Miguel, Cardoso, Vitor, Lehner, Luis, Liebling, Steven“…Here we extend this study to include an analysis of the gravitational waves radiated during the coalescence of such a binary, which is crucial to distinguish these events from other binaries with LIGO and Virgo observations. Our studies reveal that the remnant’s gravitational wave signature is mainly governed by its fundamental frequency as it settles down to a nonrotating boson star, emitting significant gravitational radiation during this post-merger state. …”
Publicado 2017
Enlace del recurso
Enlace del recurso
-
93“…The detection of gravitational waves originating from a neutron-star merger, GW170817, by the LIGO and Virgo Collaborations has recently provided new stringent limits on the tidal deformabilities of the stars involved in the collision. …”
Enlace del recurso
Enlace del recurso
-
94por Metzger, Brian D.“…I assess the prospects of kilonova detection following future GW detections of NS–NS/BH–NS mergers in light of the recent follow-up campaign of the LIGO binary BH–BH mergers.…”
Publicado 2017
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
95“…Gravitational-wave data (discovered first in 2015 by the Advanced LIGO interferometers and awarded by the Nobel Prize in 2017) are characterized by non-Gaussian and non-stationary noise. …”
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
96por Damour, Thibault“…--HTML-->A network of ground-based interferometric gravitational wave detectors (LIGO/VIRGO/GEO/...) is currently taking data near its planned sensitivity. …”
Publicado 2010
Enlace del recurso
-
97“…Written by outstanding researchers directly involved with the scientific program of the Laser Interferometer Gravitational-Wave Observatory (LIGO), the book begins with a brief review of general relativity before going on to describe the physics of gravitational waves and the astrophysical sources of gravitational radiation. …”
Enlace del recurso
-
98por Allday, Jonathan“…This edition brings the book completely up to date by including advances in particle physics and cosmology, such as the discovery of the Higgs boson, the LIGO gravitational wave discovery and the WMAP and PLANCK results.…”
Publicado 2016
Enlace del recurso
-
99por Holdom, Bob“…Observable consequences might even lurk in present LIGO data.…”
Publicado 2019
Enlace del recurso
-
100“…It highlights recent, exciting experimental findings from LHC, KEK, LIGO and several other facilities, and discusses new ideas for the unified treatment of cosmology and particle physics and in the light of new observations, which could pave the way for a better understanding of the universe we live in. …”
Enlace del recurso
Enlace del recurso