Each interaction has its particle
For many years, physics has attempted to unite the different theories that explain the world we live in. The experimental discovery of the graviton and the gravitational wave is a step further in that direction.
There are four fundamental interactions in physics: they are said to be strong, weak, electromagnetic and gravitational. The first covers the cohesion of atomic cores: the strong interaction is therefore of an extreme intensity but it has a very low range. The second is the weak interaction, which is used to explain radioactivity in particular: its range and intensity are very reduced. The third and fourth are the most known by a long way as they can be seen in everyday life, whether as light, radiocommunications, gravity or planetary movement. The intensity of the electromagnetic interaction is quite high and its range is infinite; the gravitation interaction is by a long way the weakest of all (almost 10-35 weaker than the electromagnetic interaction) even though it also has an infinite range.
Each of these interactions is associated with a particle that describes the energy transported by the interaction it represents. These interactions combined with the different material particles (protons, neutrons and electrons) structure matter at the macroscopic scale. These interactions are all the more important because at the atomic scale, matter is essentially composed of a vacuum: if the finger placed on a table does not pass through it, this is partly also due to the effects of these fundamental interactions.
Relativity and the notion of space-time warp
It was the general theory of relativity that highlighted the theoretical possibility that a particle transports the energy associated with the force of gravity.
Restricted relativity, a theory published by Einstein in 1905, showed that the length and duration depend on the observer’s reference. In a moving system, time is dilated and length contracted compared to the observer’s.
The general theory of relativity goes further by hypothesising that weight “warps” space-time. One of the commonly used images to illustrate this notion is that of an elastic, cross ruled and stretched fabric. If a weight is placed on it, the heavier the weight, the more the fabric will bend; and the more the fabric bends, the more time and lengths will be impacted. There is an example in a recent American anticipatory film where one of the vessels gravitating near a black hole approaches it. When it moves away, its occupants are much younger than those in the other vessel which stayed at distance.
Both the restricted and general theories of relativity were verified experimentally in 1971 (published in Science in 1972) by Hafele and Keating using three synchronised atomic clocks and two commercial airliners. Two atomic clocks were placed on board two airliners travelling around the world, one travelling east and the other west, the third clock remained on the ground. According to the restricted theory of relativity, time should have slightly dilated for the airliner travelling east (as the earth rotates from east to west) and on the contrary should have contracted for the airliner travelling west. Furthermore, aircraft flying at a certain altitude are subjected to a weaker gravity field than the clock that remained on the ground: their time should therefore be accelerated compared to the clock on the ground with differences in the order of a hundred nanoseconds. The theory was verified quite accurately, making it possible to conclude that the two theories of relativity were relevant.
The effects of relativity are currently regularly taken into account in satellite navigation systems (GPS or Galileo for example) by correcting the time on atomic clocks on board satellites.
Gravitational waves, associated with a particle called a graviton, propagate the space-time energy transitions. These new waves dilate or contract space-time. If we detect electromagnetic waves using antennas that amplify electron movements, gravitational waves can only be perceived using systems that show length variations. However they are difficult to measure as they are of very weak intensity. It is estimated that the order of the length deformation of an object when crossed by these waves is in the order of 0.0000000000001 mm, or 1e-16m! To detect these new waves, highly sensitive receivers had to be developed based on lasers measuring ultra-accurate distances in tunnels several kilometres long on the one hand, and on the other hand it was necessary to focus on ultra-powerful transmitters resulting from extreme phenomena impacting space-time, such as the merging of two stars.
The existence of gravitational waves is now proven and they can be detected, opening up a new era for astronomical observation. In France, this success was rewarded by the 2017 CNRS Gold Medal to the physicists Alain Brillet and Thibault Damour, and by the 2017 Nobel prize for physics, awarded to the physicists Raider Weiss, Barry C. Barish and Kip S. Thorne.