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Gravitational Waves
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abstract
This article reviews current efforts and plans for gravitational-wave detection, the gravitational-wave sources that might be detected, and the information that the detectors might extract from the observed waves. Special attention is paid to (i) the LIGO/VIRGO network of earth-based, kilometer-scale laser interferometers, which is now under construction and will operate in the high-frequency band ($1$ to $10^4$ Hz), and (ii) a proposed 5-million-kilometer-long Laser Interferometer Space Antenna (LISA), which would fly in heliocentric orbit and operate in the low-frequency band ($10^{-4}$ to $1$ Hz). LISA would extend the LIGO/VIRGO studies of stellar-mass ($M\sim2$ to $300 M_\odot$) black holes into the domain of the massive black holes ($M\sim1000$ to $10^8M_\odot$) that inhabit galactic nuclei and quasars.
Forward citations
Cited by 4 Pith papers
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Synergies Between Pulsar Timing Array and Astrometry
Joint SKA PTA and astrometry analysis improves gravitational wave background detection sensitivity by 10-50%.
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False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE
Simulations of unlensed binary black hole mergers show that ~0.01% of event pairs are falsely classified as lensed by GLANCE at SNR threshold 1.5 with time delays of ~1000 days or more.
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Cylindrical gravitational impulse wave
A two-soliton solution in Jordan-Ehlers spacetime is recast with the Piran et al. decomposition to produce explosion and implosion gravitational wave profiles, then tuned visually to mimic LIGO chirps.
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A White Paper on The Multi-Messenger Science Landscape in India
No new scientific result is presented; the document reviews multi-messenger science and recommends a national coordination center linking Indian gravitational wave, electromagnetic, cosmic ray, and neutrino facilities.
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