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Fifth force

physical science Maturity 11-13 Next article →

In physics, a fifth force is a hypothetical fundamental interaction. Scientists currently recognize four known forces in nature. These are gravity, electromagnetism, the strong nuclear force, and the weak nuclear force. A fifth force would be an entirely new way that objects affect one another. Some speculative theories propose this force to explain observations that do not fit existing models. Currently, no definitive evidence has been found to support these models. The characteristics of such a force depend on the specific hypothesis being tested.

Theoretical proposals for a fifth force are driven by several scientific inconsistencies. One major issue is the gap between general relativity and quantum field theory. Another is the conflict between the hierarchy problem and the cosmological constant problem. These problems suggest there might be corrections to the gravitational potential at very small scales, around 100 micrometers. Additionally, the accelerating expansion of the universe is linked to dark energy. Some physicists speculate that a form of dark energy called quintessence could actually be a fifth force.

One way to search for this force is by testing the strong equivalence principle. This principle is a central part of Einstein's theory of gravity, or general relativity. Some alternative theories, like Brans–Dicke theory, suggest a fifth force might have an infinite range. In these theories, gravity has extra degrees of freedom beyond the metric, which is the mathematical description of space curvature. For example, a scalar field cannot cause the bending of light rays. A fifth force might show up as the Nordtvedt effect, which influences solar system orbits. Scientists test this using Lunar Laser Ranging and very-long-baseline interferometry.

Another approach involves searching for a Yukawa force. This force might arise from Kaluza–Klein theory, supergravity, or string theory. These theories suggest the universe may have extra dimensions. The Yukawa force is transmitted by a light scalar field. The range of this field is determined by its Compton wavelength. Because of this, researchers are testing gravity on very small scales to see if it deviates from the inverse-square law. They are looking for signs that a Yukawa interaction begins to act at specific lengths.

History shows how the term "fifth force" became part of scientific discussion. In 1971, Fujii proposed a model that changed how gravity depends on distance. This model used a Yukawa potential-like term to describe the interaction. Later, in 1986, Ephraim Fischbach and his colleagues reanalyzed data from the Eötvös experiment. They found a distance dependence in gravity that seemed to deviate from the inverse-square law. Fischbach's analysis suggested a force with a strength around 1% of gravity and a range of a few hundred meters. However, many later attempts to reproduce these specific deviations have failed.

Many experiments have attempted to find these discrepancies in different environments. Australian researchers measured the gravitational constant deep in a mine shaft. They found a value that was 2% smaller than predicted. They concluded a repulsive fifth force with a range of centimeters to a kilometer might explain this. Similar experiments were conducted on the submarine USS Dolphin while it was deeply submerged. Scientists also measured gravity in a deep borehole in the Greenland ice sheet. They found discrepancies of a few percent, though they could not rule out geological causes.

In 2015, a team in Hungary led by Attila Krasznahorkay reported a potential discovery. They studied the decay of beryllium-8 nuclei created by firing protons at lithium-7 targets. They observed an excess of decays at a specific opening angle and energy of 17 MeV. This suggested the existence of a new, light boson called the X17 particle. This particle is only 34 times heavier than an electron. In 2019, the team found similar anomalies in the decay of stable helium atoms. Some researchers propose this X17 is a "protophobic" boson, meaning it has suppressed couplings to protons. This particle could potentially explain the muon anomaly or serve as a candidate for dark matter.

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