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Graviton

physical science Maturity 7-9 Next article →

The graviton is a hypothetical elementary particle. It is thought to mediate the force of gravitational interaction. In the world of quantum physics, forces are carried by particles called bosons. Other known forces use specific particles to work. Electromagnetism uses the photon. The strong interaction uses gluons. The weak interaction uses W and Z bosons. These particles are all part of the Standard Model. The graviton would be the particle that carries gravity. It would also be a quantum of gravitational wave energy.

Physicists believe the graviton must have very specific properties. If it exists, it is likely a massless particle. We think this because gravity has a very long range. It also appears to travel at the speed of light. Because it is massless, it must be a spin-2 boson. This refers to its intrinsic angular momentum. This specific spin is necessary because gravity comes from the stress-energy tensor. This is a second-order tensor that describes how matter and energy are distributed. In contrast, the photon is a spin-1 particle. A massless spin-2 field would interact with matter in the exact same way gravity does. This means a discovered spin-2 particle would almost certainly be the graviton.

Scientists face major mathematical hurdles when studying gravitons. They use a method called renormalization to handle infinities in equations. In quantum electrodynamics, this method works well. However, quantized general relativity is not perturbatively renormalizable. When physicists use Feynman diagrams to calculate particle interactions, they run into trouble. Diagrams with at least two loops lead to ultraviolet divergences. These are infinite results that cannot be removed. Because of these infinities, the theory loses its predictive power. This suggests we need a more unified theory to describe the Planck scale.

One possible solution to these math problems is string theory. In string theory, the graviton is not a single point. Instead, it is a massless state of a fundamental string. These strings are one-dimensional loops. They avoid mathematical infinities by "smearing out" the gravitational interactions. This prevents the particles from appearing as single, problematic points. While string theory offers a way to include the graviton, it has not made enough progress to be a complete answer. Currently, models have only been worked out for a few weakly interacting strings.

The history of this idea spans many centuries. Pierre-Simon Laplace anticipated particles that carry gravity long ago. However, his ideas predated quantum mechanics and special relativity. He thought these particles traveled faster than light. In 1916, Albert Einstein discussed quantized gravitational radiation. The actual name "graviton" was coined in 1934 by Soviet physicists Dmitry Blokhintsev and others. Later, in 1959, Paul Dirac reintroduced the term in lectures. He noted that the energy of a gravitational field should come in discrete bits called quanta.

Detecting a single graviton is an extreme challenge. The interaction between gravitons and matter is incredibly weak. This is known as a low cross section. For example, imagine a detector with the mass of Jupiter. Even if it were 100% efficient and near a neutron star, it might see only one graviton every 10 years. It would also be impossible to shield the detector from neutrinos. A shield large enough to stop neutrinos would collapse into a black hole. Instead, scientists use gravitational waves to find clues. The LIGO and Virgo collaborations have detected these waves directly.

We can use these observations to set limits on the graviton. If gravitational waves move slower than the speed of light, the graviton must have mass. Currently, observations of gravitational waves set an upper mass bound of 10^-23 eV. Space missions like Cassini and MESSENGER provide a similar bound through planetary measurements. We also know the graviton's Compton wavelength is at least 1.6 light-years. This corresponds to a mass of no more than 10^-23 eV. Scientists also look at how galaxies rotate to see if gravitons have non-zero mass. All these different methods help us understand the limits of gravity.

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