gravitational wave造句

Celestial gravitational wave source and the exploration to low frequency gravitational wave have also been discussed.

We need to boost the resolution of a gravitational wave detector-type of kit. Enter the "Holometer."

There is correspondent relation between the variation of index of low-frequency gravitational wave with the time and development of SW vortex.

If GEO600 really has discovered holographic noise from quantum convulsions of space-time, then it presents a double-edged sword for gravitational wave researchers.

Should GEO600 detect a phase change, it could be indicative of a slight change in distance, thus the passage of a gravitational wave.

Based on the index method of low-frequency gravitational wave, diagnosis and forecast on the development of southwest vortex, intensity and area of heavy rain are discussed in this paper.

The space-time ripples cause the distance measured by a light beam to change as the gravitational wave passes by, and the amount of light falling on the photodetector to vary.

These spacetime distortions travel as gravitational waves.

Gravitational waves are fluctuations in the curvature of space and time which propagate through the universe as gravitational waves — outward from its source.

In their final stages the mergers are expected to be intense sources of gravitational waves.

The story was different, though, for the fifth wager—that gravitational waves would be detected.

Cosmic strings would also create incredible gravitational waves, stronger than any other known source.

GEO600 has not detected any gravitational waves so far, but it might inadvertently have made the most important discovery in physics for half a century.

Back in August 2004, Ladbrokes, a British bookmaker, offered odds of 500 to one against gravitational waves being detected by 2010.

Also, pairs of massive black holes in the process of merging are expected to be the most powerful sources of gravitational waves in the Universe.

These merger events produce ripples in time and space (gravitational waves) that could be detected by instruments from as early as 2015.

One on hand, the noise will handicap their attempts to detect gravitational waves. On the other, it could represent an even more fundamental discovery.

The particles could also reveal their presence in bursts of gravitational waves radiated when their clouds are torn apart around the black hole or when particles move from one axion cloud to another.

But the newfound star pair is unique in that they don't swap matter as they spin, providing a "clean clock" to measure the effects of gravitational waves, Brown said.