What is behind dark energy – and what connects it to the cosmological constant introduced by Albert Einstein? Two physicists from the University of Luxembourg point the way to answering these open questions of physics.

The universe has a number of bizarre properties that are difficult to understand with everyday experience. For example, the matter we know, consisting of elementary and composite particles building molecules and materials, apparently makes up only a small part of the energy of the universe. The largest contribution, about two-thirds, comes from “dark energy” – a hypothetical form of energy whose background physicists are still puzzling over. Moreover, the universe is not only expanding steadily, but also doing so at an ever-faster pace. Both characteristics seem to be connected, because dark energy is also considered a driver of accelerated expansion. Moreover, it could reunite two powerful physical schools of thought: quantum field theory and the general theory of relativity developed by Albert Einstein. But there is a catch: calculations and observations have so far been far from matching. Now two researchers from Luxembourg have shown a new way to solve this 100 years old riddle in a paper published by the journal Physical Review Letters.

### The trail of virtual particles in a vacuum

“Vacuum has energy. This is a fundamental result of quantum field theory,” explains Prof. Alexandre Tkatchenko, Professor of Theoretical Physics at the Department of Physics and Materials Science at the University of Luxembourg. This theory was developed to bring together quantum mechanics and special relativity, but quantum field theory seems to be incompatible with general relativity. Its essential feature: in contrast to quantum mechanics, the theory considers not only particles but also matter-free fields as quantum objects. “In this framework, many researchers regard dark energy as an expression of the so-called vacuum energy,” says Tkatchenko: a physical quantity that, in a vivid image, is caused by a constant emergence and interaction of pairs of particles and their antiparticles – such as electrons and positrons – in what is actually empty space.

Physicists speak of this coming and going of virtual particles and their quantum fields as vacuum or zero-point fluctuations. While the particle pairs quickly vanish into nothingness again, their existence leaves behind a certain amount of energy. “This vacuum energy also has a meaning in general relativity,” the Luxembourg scientist notes: “It manifests itself in the cosmological constant Einstein included into his equations for physical reasons.”

### A colossal mismatch

Unlike vacuum energy, which can only be deduced from the formulae of quantum field theory, the cosmological constant can be determined directly by astrophysical experiments. Measurements with the Hubble space telescope and the Planck space mission have yielded close and reliable values for the fundamental physical quantity. Calculations of dark energy on the basis of quantum field theory, on the other hand, yield results that correspond to a value of the cosmological constant that is up to 10^{120} times larger – a colossal discrepancy, although in the world view of physicists prevailing today, both values should be equal. The discrepancy found instead is known as the “cosmological constant enigma”. “It is undoubtedly one of the greatest inconsistencies in modern science,” says Alexandre Tkatchenko.

### Unconventional way of interpretation

Together with his Luxembourg research colleague Dr. Dmitry Fedorov, he has now brought the solution to this puzzle, which has been open for decades, a significant step closer. In a theoretical work, the results of which they recently published in Physical Review Letters, the two Luxembourg researchers propose a new interpretation of dark energy. It assumes that the zero-point fluctuations lead to a polarisability of the vacuum, which can be both measured and calculated. “In pairs of virtual particles with an opposite electric charge, it arises from electrodynamic forces that these particles exert on each other during their extremely short existence,” Tkatchenko explains. The physicists refer to this as a vacuum self-interaction. “It leads to an energy density that can be determined with the help of a new model,” says the Luxembourg scientist.

Together with his research colleague Fedorov, they developed the basic model for atoms a few years ago and presented it for the first time in 2018. The model was originally used to describe atomic properties, in particular the relation between polarisability of atoms and the equilibrium properties of certain non-covalently bonded molecules and solids. Since the geometric characteristics are quite easy to measure experimentally, polarisability can also be determined via their formula. “We transferred this procedure to the processes in the vacuum”, explains Fedorov. To this end, the two researchers looked at the behaviour of quantum fields, in particular representing the “coming and going” of electrons and positrons. The fluctuations of these fields can also be characterised by an equilibrium geometry which is already known from experiments. “We inserted it into the formulas of our model and in this way ultimately obtained the strength of the intrinsic vacuum polarisation,” Fedorov reports. The last step was then to quantum mechanically calculate the energy density of the self-interaction between fluctuations of electrons and positrons. The result obtained in this way agrees well with the measured values for the cosmological constant. This means: “Dark energy can be traced back to the energy density of the self-interaction of quantum fields”, emphasises Alexandre Tkatchenko.

### Consistent values and verifiable forecasts

“Our work thus offers an elegant and unconventional approach to solving the riddle of the cosmological constant,” sums up the physicist. “Moreover, it provides a verifiable prediction: namely, that quantum fields such as those of electrons and positrons do indeed possess a small but ever-present intrinsic polarisation.” This finding points the way for future experiments to detect this polarisation in the laboratory as well, say the two Luxembourg researchers. “Our goal is to derive the cosmological constant from a rigorous quantum theoretical approach”, emphasises Dmitry Fedorov. “And our work contains a recipe on how to realise this.” He sees the new results obtained together with Alexandre Tkatchenko as the first step towards a better understanding of dark energy – and its connection to Albert Einstein’s cosmological constant. Finally, Tkatchenko is convinced: “In the end, this could also shed light on the way in which quantum field theory and general relativity theory are interwoven as two ways of looking at the universe and its components.”

Read the full article in Physical Review Letters: Casimir Self-Interaction Energy Density of Quantum Electrodynamic Fields