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Quantum gravitational spectroscopy with ultracold systems is an emerging field of particle physics based on recent major advances in related experimental and theoretical developments. The gravitational spectroscopy is profiting from its exceptional sensitivity due to extreme weakness of the gravitational interaction compared to other fundamental interactions; thus it provides us with access to the precision frontier in particle physics and other domains. Quantum gravitational spectroscopy is the ultimate limit of gravitational spectroscopy, which studies/measures fragile and thus sensitive quantum states of ultracold particles and systems. To provide observable phenomena with ultracold systems, like neutrons, atoms, or antiatoms, in gravitational quantum states, one has to produce them with sufficiently high phase-space density. Some of such studies in a gravitational field, like those with ultracold neutrons, have become reality; others with ultracold atoms and antiatoms are in preparation.

This subject is traditionally covered in a series of GRANIT Workshops (

The topics include the following: (i) the GRANIT facility, measurements of gravitational quantum states of neutrons, including experimental results and theoretical developments, and also neutron interferometry in broad sense; (ii) novel instruments and methods for gravitational spectroscopy and interferometry, including those capable of improving the performance of GRANIT facility; (iii) fundamental interactions in near-surface quantum systems, including shortrange forces, chameleon-like forces, noncommutative quantum mechanics, emerging gravity, and antimatter and gravity; (iv) precision fundamental measurements with ultracold systems, including gravity with atoms, molecules, neutrons, and antimatter, quantum reflection, and dissipation; (v) surface studies with the GRANIT facility, including materials with predefined properties, levitating nanoparticles, and whispering gallery effect.

Bound states of a system could be formed by interactions of different kind. Detailed studies of such states do not only serve to explore the system itself, but also are a good tool to better understand the interaction responsible for the binding force. The problem is that a gravitational force is very weak to form easily a quantum bound system. One could cite Brian Hatfield in “Feynman Lectures on Gravitation” published in 1995 by Addison-Wesley Publishing Company: “Let us consider another possibility, an atom held together by gravity alone. For example, we might have two neutrons in a bound state. When we calculate the Bohr radius of such an atom, we find that it would be 10^{8} light years, and that the atomic binding energy would be 10^{−70} Rydbergs.

For this observation, one used the fact that ultracold neutrons (UCNs) experience a neutron-optical potential (sometimes called Fermi potential) in matter of a size big enough that matter can totally reflect UCNs if their energy is sufficiently low. In fact, the term “ultracold neutron” is loosely defined as the neutrons which are totally reflected at all incidence angles by the matter used for the confining bottle for them. Here, we focus on UCNs with even lower energy, for which we can approximate the potential in matter as infinite. These neutrons bounce on a horizontal table essentially like ping-pong balls on a table. They are confined in a box formed by the infinite potential of the table and the linear gravitational potential. In order to detect effects of the quantization, one has to focus on neutrons in one of the lowest possible states in such a system.

General solutions of the corresponding one-dimensional Schrödinger equation are given in all major textbooks on quantum mechanics, for instance, in [

The aim of previous experiments performed in the last decade was to discover these quantum states. For the discovery, a method was used that is essentially a measurement of the height and shape of wave functions [^{−1}. In order to improve it, efforts are currently undertaken by qBounce and Tokyo collaborations; the methods used are resonant transitions between quantum states induced by mechanical vibrations of the bottom mirror [

One of the main goals for improving the accuracy of quantum gravitational spectroscopy with neutrons is searches for extra short-range fundamental forces [

Over 50 participants from 12 countries in 4 continents attended the previous GRANIT-2014 Workshop. The organizers would like to thank ILL, IN2P3/CNRS, and UJF/Grenoble for financial support of the Workshop as well as for their help in preparation of the Workshop.