Searching for Dark Energy with Neutrons
- It does not always take a huge accelerator to do particle physics.
- First results from a low-energy, table-top alternative experiment broaden the scope of validity of Newton's gravitational theory and define more narrowly - by more than a hundred thousand times - the potential properties of the forces and particles that may exist beyond it.
- Gravity Resonance Spectroscopy, a method developed at the Vienna University of Technology, is so sensitive that it can now be used to search for Dark Matter and Dark Energy.
All the particles we know to exist make up only about five per cent of the mass and energy of the universe. The rest – “Dark Matter” and “Dark Energy” – remains mysterious. A European collaboration led by researchers from the Vienna University of Technology has now carried out extremely sensitive measurements of gravitational effects at very small distances at the Institut Laue-Langevin (ILL) in Grenoble. These experiments provide limits for possible new particles or fundamental forces which are a hundred thousand times more restrictive than previous estimations.
Dark matter is invisible, but it acts on matter by its gravitational pull, influencing the rotation of galaxies. Dark energy, on the other hand, is responsible for the accelerated expansion of the universe. It can be described by introducing a new physical quantity - Albert Einstein’s Cosmological Constant. Alternatively, so-called quintessence theories have been put forward: “Perhaps empty space is not completely empty after all, but permeated by an unknown field, similar to the Higgs-field”, says Professor Hartmut Abele (TU Vienna), Director of the Atominstitut and group leader of the research group. These theories are named after Aristotle’s “quintessence” – a hypothetical fifth element, in addition to the four classical elements of ancient Greek philosophy.
If new kinds of particles or additional forces of nature exist, it should be possible to observe them here on earth. Tobias Jenke and Hartmut Abele from the Vienna University of Technology developed an extremely sensitive instrument, which they used together with their colleagues to study gravitational forces. Neutrons are perfectly suited for this kind of research. They do not carry electric charge and they are hardly polarisable. In this experiment they are only influenced by gravity – and possibly by additional, as yet unknown forces. Theoretical calculations analysing the behaviour of the neutrons were performed by Larisa Chizhova, Professor Stefan Rotter and Professor Joachim Burgdörfer (TU Vienna). U. Schmidt from Heidelberg University and T. Lauer from TU Munich contributed with an analytical tool.
Forces at Small Distances
The technique the team developed takes very slow neutrons from the strongest continuous ultracold neutron source in the world, at the ILL in Grenoble, and funnels them between two parallel plates. According to quantum theory, the neutrons can only occupy discrete quantum states with energies which depend on the force that gravity exerts on the particle. By mechanically oscillating the two plates, the quantum state of the neutron can be switched. In this way, the difference between the energy levels can be measured.
“This work is an important step towards modelling gravitational interactions at very short distances. The ultracold neutrons produced at ILL together with the measurement devices from Vienna are the best tool in the world for studying the predicted tiny deviations from pure Newtonian gravity”, says Peter Geltenbort (ILL, Grenoble).
Different parameters determine the level of precision required to find such tiny deviations – for instance, the coupling strength between hypothetical new fields and the matter we know. Certain parameter ranges for the coupling strength of quintessence particles or forces have already been excluded following other high-precision measurements. But all previous experiments still left a large parameter space in which new physical non-Newtonian phenomena could be hidden.
A Hundred Thousand Times Better than Other Methods
The new neutron method can test theories in this parameter range: “We have not yet detected any deviations from the well-established Newtonian law of gravity”, says Hartmut Abele. “Therefore, we can exclude a broad range of parameters.” The measurements determine a new limit for the coupling strength, which is lower than the limits established by other methods by a factor of a hundred thousand.
Even if the existence of certain hypothetical quintessence particles is disproved by these measurements, the search will continue, as it is possible that new physics can still be found below this improved level of accuracy. Therefore, Gravity Resonance Spectroscopy will need to be improved further - and increasing the accuracy by another few orders of magnitude seems feasible to Abele’s team. However, if even that does not yield any evidence of deviations from known forces, Albert Einstein would win yet another victory: his cosmological constant would then appear more and more plausible.
Schematic diagram of the gravity resonance spectroscopy apparatus (not to scale). Copyright T.U. Wien / G Cronenberg and T Jenke
The experiment is mounted on a heavy, polished granite table (1), which serves as a reference for all height adjustments. Ultracold neutrons traverse the setup from left to right (red arrow). Height-aligned, grinded steel baffles (2) restrict their velocity component vx. The neutron mirror setup consists of a flat mirror on the bottom (3a), a second mirror with rough lower surface on top (3b), and mechanical spacers (3c). It is mounted on a nano-positioning device (4), which also serves as source for the mechanical oscillations in height direction.
The neutron transmission is determined using a low-background neutron counter (5).
For all spin-dependent searches, the whole setup was surrounded by coils (6a) producing a homogeneous guide field. Furthermore, a detector with a spin-analyzing entrance foil and detector coils (to polarize this foil) was used (6b).
Contact:Dr Peter Geltenbort, +33 4 76 20 72 42
Notes to editors
About ILL – The Institut Laue-Langevin (ILL) is an international research centre based in Grenoble, France. It has led the world in neutron-scattering science and technology for more than 40 years, since experiments began in 1972. ILL operates one of the most intense neutron sources in the world, feeding beams of neutrons to a suite of 40 high-performance instruments that are constantly upgraded. Each year 1,200 scientists from more than countries worldwide visit ILL (2000 visits), to conduct research into condensed matter physics, (green) chemistry, biology, nuclear physics, and materials science. The UK, along with France and Germany is an associate and major funder of the ILL.