منابع مشابه
Gravitational Wave Detection by Interferometry (Ground and Space)
Significant progress has been made in recent years on the development of gravitational wave detectors. Sources such as coalescing compact binary systems, 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 ...
متن کاملToward gravitational wave detection
An overview of some tools and techniques being developed for data conditioning (regression of instrumental and environmental artifacts from the data channel), detector design evaluation (modeling the science “reach” of alternative detector designs and configurations), noise simulations for mock data challenges and analysis system validation, and analyses for the detection of gravitational radia...
متن کاملGravitational Wave detection through microlensing?
It is shown that accurate photometric observations of a relatively high–magnification microlensing event (A ≫ 1), occurring close to the line of sight of a gravitational wave (GW) source, represented by a binary star, can allow the detection of subtle gravitational effects. After reviewing the physical nature of such effects, it is discussed to what extent these phenomena can actually be due to...
متن کاملGround-based gravitational-wave detection
In the past three years, the first generation of large gravitational-wave interferometers has begun operation near their design sensitivities, taking up the mantle from the bar detectors that pioneered the search for the first direct detection of gravitational waves. Even as the current ground-based interferometers were reaching their design sensitivities, plans were being laid for the future. ...
متن کاملPulsars and Gravitational Wave Detection
The number of known millisecond pulsars has dramatically increased in the last few years. Regular observations of these pulsars may allow gravitational waves with frequencies ∼ 10 Hz to be detected. A “pulsar timing array” is therefore complimentary to other searches for gravitational waves using ground-based or space-based interferometers that are sensitive to much higher frequencies. In this ...
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ژورنال
عنوان ژورنال: International Journal of Modern Physics D
سال: 2016
ISSN: 0218-2718,1793-6594
DOI: 10.1142/s0218271816300019