When do you think gravity particles will be detected rather than waves?
Freeman Dyson has suggested that they might never be detectable.
A problem is that gravitons are (at best) most likely extremely weakly interacting so a detector would end up being impractically massive - many hundreds of times the mass of the Earth for any probability of single particle detection over many years of observing (the LIGO mirrors, to detect individual gravitons, would have to be so big that they would collapse under their own gravity and form black holes). At worse gravitons may be hard to tempt out into the open (if at all) in this universe as they may well be intimately wrapped up with higher dimensions.
So they may only ever be observable indirectly, which is in some senses what this experiment has done. A more empirical approach (proposed by Krauss) might be through observing polarisations in the cosmic microwave background, which calculations show would arise from quantum mechanical effects, demonstrating that gravity is quantised and thus inferring the existence of gravitons.
This ^^Freeman Dyson has suggested that they might never be detectable.
A problem is that gravitons are (at best) most likely extremely weakly interacting so a detector would end up being impractically massive - many hundreds of times the mass of the Earth for any probability of single particle detection over many years of observing (the LIGO mirrors, to detect individual gravitons, would have to be so big that they would collapse under their own gravity and form black holes). At worse gravitons may be hard to tempt out into the open (if at all) in this universe as they may well be intimately wrapped up with higher dimensions.
So they may only ever be observable indirectly, which is in some senses what this experiment has done. A more empirical approach (proposed by Krauss) might be through observing polarisations in the cosmic microwave background, which calculations show would arise from quantum mechanical effects, demonstrating that gravity is quantised and thus inferring the existence of gravitons.
I take offence at the suggestion that I might in some way be responsible for the output of D:Ream.

How brief is brief?Indeed, Rainer Weiss (MIT) has been explaining just a few of the engineering challenges in dealing with the noise environment in order to measure at 10^-21. Not just local geological, man made vibrations. Not just thermal noise. But quantum noise too. The measurement they have made is equivalent to measuring the distance from the Earth to the nearest star within an accuracy of the width of a human hair.
This black hole collision was observed on September 14th last year, but it occurred about 1.3 billion years ago. The event was brief but for a moment equivalent to fifty times the power output of the entire observable universe.
How brief is brief?
How brief is brief?
Many thanks
I now have this image of 2hat's avatar reading out his posts in an annoyingly smug tone, while trying to look dishy yet deep.

well it can only get better...I take offence at the suggestion that I might in some way be responsible for the output of D:Ream.
Now further analysis of the LIGO signals received thus far may be hinting that there might be evidence of echoes in the waves, contrary to predictions arising from general relativity (which essentially would not allow for such information leakage from a black hole's event horizon).Amazing achievement - these experiments are very *very* hard to do. Einstein's work continues to hold up incredibly well![]()
"A simultaneous detection of gamma rays and gravitational waves from the same place in the sky is a major milestone in our understanding of the universe," said Davide Lazzati, a theoretical astrophysicist in the OSU College of Science
On July 6, Lazzati's team of theorists had published a paper predicting that, contrary to earlier estimates by the astrophysics community, short gamma-ray bursts associated with the gravitational emission of binary neutron star coalescence could be detected -- whether or not the gamma-ray burst was pointing at Earth
IGO, and the European Gravitational Observatory's Virgo team on Aug. 17, 2017, detected gravitational waves -- ripples in the fabric of space-time -- produced by the coalescence of two neutron stars.

The all-pervading ultra-low frequency background noise of gravitational waves revealed by the NANOGrav collaboration through analysing 15 years worth of pulsar timing data (a very different approach to that used by LIGO and related gravity wave observatories).
News conference shortly:![]()
15 Years of Radio Data Reveals Evidence of Space-Time Murmur
Scientists have found evidence of a universal background of gravitational waves, or ripples in the fabric of space-time.www.jpl.nasa.gov
Note: This has relied on determining the position of the solar system barycentre (centre of mass) to better than 100 metres (a prerequisite for achieving the degree of accuracy necessary in the underlying pulsar timing). The largest contribution to error in this is Jupiter, though refining it might hint towards additional planets in the solar system. One should also be aware that this result is only good to 4σ (physicists are usually only satisfied at 5+σ).
Scientific commentary with links to published papers.