Abstract In this paper, we study the phenomenon of quantum interference in the presence of external gravitational fields described by alternative theories of gravity. We analyze both non-relativistic and relativistic effects induced by the underlying curved background on a superposed quantum system. In the non-relativistic regime, it is possible to come across a gravitational counterpart of the Bohm–Aharonov effect, which results in a phase shift proportional to the derivative of the modified Newtonian potential. On the other hand, beyond the Newtonian approximation, the relativistic nature of gravity plays a crucial rôle. Indeed, the existence of a gravitational time dilation between the two arms of the interferometer causes a loss of coherence that is in principle observable in quantum interference patterns. We work in the context of generalized quadratic theories of gravity to compare their physical predictions with the analogous outcomes in general relativity. In so doing, we show that the decoherence rate strongly depends on the gravitational model under investigation, which means that this approach turns out to be a promising test bench to probe and discriminate among all the extensions of Einstein’s theory in future experiments.
Quantum mechanics and general relativity have been extensively and independently confirmed in many experiments. However, the interplay of the two theories has never been tested: all experiments that measured the influence of gravity on quantum systems are consistent with non-relativistic, Newtonian gravity. On the other hand, all tests of general relativity can be described within the framework of classical physics. Here we discuss a quantum interference experiment with single photons that can probe quantum mechanics in curved space-time. We consider a single photon traveling in superposition along two paths in an interferometer, with each arm experiencing a different gravitational time dilation. If the difference in the time dilations is comparable with the photon's coherence time, the visibility of the quantum interference is predicted to drop, while for shorter time dilations the effect of gravity will result only in a relative phase shift between the two arms. We discuss what aspects of the interplay between quantum mechanics and general relativity are probed in such experiments and analyze the experimental feasibility.
Current attempts to probe general relativistic effects in quantum mechanics focus on precision measurements of phase shifts in matter–wave interferometry. Yet, phase shifts can always be explained as arising because of an Aharonov–Bohm effect, where a particle in a flat space–time is subject to an effective potential. Here we propose a quantum effect that cannot be explained without the general relativistic notion of proper time. We consider interference of a 'clock'—a particle with evolving internal degrees of freedom—that will not only display a phase shift, but also reduce the visibility of the interference pattern. According to general relativity, proper time flows at different rates in different regions of space–time. Therefore, because of quantum complementarity, the visibility will drop to the extent to which the path information becomes available from reading out the proper time from the 'clock'. Such a gravitationally induced decoherence would provide the first test of the genuine general relativistic notion of proper time in quantum mechanics. In the theory of general relativity time flows at different rates depending on the space–time geometry. Here, a drop in the visibility of a quantum 'clock' interference in a gravitational potential is predicted, which cannot be explained without the general relativistic notion of time.
The unification of quantum mechanics and general relativity remains elusive due to the lack of experimental signatures. To explore the parameter regimes where both theories are relevant, growing attention is being paid to investigating the general relativistic effects on low-energy quantum systems. Such research offers valuable insights into the connection between the two pillars of modern physics. Entanglement and gravitational time dilation capture key aspects of quantum mechanics and general relativity, respectively. Thus, the dynamical evolution of entangled systems in curved space unambiguously reflects the interplay between quantum mechanics and general relativity. Specifically, we investigate the interference visibility reduction of entangled N00N states and quadrature entanglement in gravitational fields. The interference visibility reduction induced by gravitational time dilation differs significantly between N00N states and quadrature entanglement, owing to their distinct gravitational phase encoding mechanisms. For N00N states, the gravitational phase is encoded as a relative phase between the H and V polarization modes, and the visibility reduction is enhanced by a factor of N compared to the single-photon case, rendering them highly sensitive to observing the gravitational effect. In contrast, quadrature entanglement encodes the gravitational phase across its full Gaussian spectrum, leading to vanishing interference visibility in large-scale interferometers spanning from geostationary orbit to ground level.
Current models of quantum interference experiments in external gravitational fields lack a common framework: while matter-wave interferometers are commonly described using the Schrödinger equation with a Newtonian potential, gravitational effects in quantum optics are modeled using either post-Newtonian metrics or highly symmetric exact solutions to Einstein's field equations such as those of Schwarzschild and Kerr. To coherently describe both kinds of experiments, this paper develops a unified framework for modeling quantum interferometers in general stationary space-times. This model provides a rigorous description and coherent interpretation of the effects of classical gravity on quantum probes.
The gravitational decoherence field studies the suppression of coherence in quantum systems caused by effects rooted in the gravitational interaction. This models are not just important to yield interesting ideas about the search, in regimes others than the Planck scale, for the interplay between quantum mechanics and general relativity, but also from a theoretical point of view. The fact that the gravitational field can not be shielded opens the question of how strong will the gravitational ‘environment’ decohere a quantum system? and if this decoherence can somehow explain the absence of macroscopical super- positions? This thesis studies in depth the ‘Classical Channel Gravity’ (CCG) model, a recent proposal of gravitational decoherence that assumes that the gravitational interac- tion is always accompanied with an intrinsic decoherence mechanism which ensures that there is no transmission of quantum information between the parties involved. This model can be understood a series of weak continuous quantum measurements accompanied with a feedback term produced by some underlying hidden gravitational degrees of freedom. We first study all the possible emergent dynamics from collisional Markovian dynamics; these ones range from exact unitary to arbitrary fast decoherence (Zeno effect). The second part of the thesis is devoted to study the Newtonian and post Newtonian limits of the CCG model, with particular focus on the testability features of CCG. In particular, we apply this model to coupled clocks and find that the amount of decoherence predicted by CCG is the same as the decoherence that an ‘environment of clocks’ will imprint in a single clock in the context of unitary evolution. On the other hand, we find that this effect is far from being detectable with the current achieved time accuracy. However, CCG as a model for multi partite systems and two systems with very different masses seems to yield an amount of decoherence that is not only able to be detectable with current experiments but also seems to indicate that this model is ruled out. Nevertheless, we also mention potential caveats with our assumptions and discuss other physically motivated directions to further study this result. Finally, we also explore the extension of CCG for the cosmological scenario. In this context the scale factor is being decohered by test particles ‘sitting’ on spacetime. We find that this decoherence will be seen by an observer unaware of the CCG fundamental mechanism as an emergent form of dark energy filling the universe.
We analyse the gravitational Aharonov-Bohm (AB) phase within the semiclassical framework. We first review the traditional non-relativistic approximation, where a particle of rest mass
m couples to the Newtonian potential via
Hint=mΦ, yielding a gauge-invariant phase analogous to the electromagnetic AB effect. We then show that this approximation fails when the particle's total energy varies between interferometer branches. A rigorous derivation from linearised general relativity reveals that in the weak-field, non-relativistic limit, gravity couples to the local energy density, not merely the rest mass. In a laser-driven atom interferometer, the two branches of the superposition differ by the location of an excitation energy
δE: either stored in the laser apparatus at
xL or carried by the atom at
xA(t). Under a gauge transformation
δhμν=−∂μξν−∂νξμ, the gravitational AB phase acquires a residual
δ(Δϕgrav)=−ℏc2δE[ξ0(xL,tf)−ξ0(xA(tf),tf)] for a purely temporal generator, which is generically nonzero. Since experiments such as Overstreet et al. (2022) measure a stable, reproducible gravitational AB phase, we are compelled to choose between two mutually exclusive possibilities. If gauge invariance (diffeomorphism invariance) is a fundamental principle, then the semiclassical framework is incomplete and a quantum theory of gravity is necessary. If, on the other hand, gauge invariance fails, then semiclassical gravity can be a complete theory. In this case, the gravitational potentials must be understood as real physical fields, and the gauge-dependent phase is a genuine observable, consistent with experiment. These two resolutions are mutually exclusive, and their implications for the nature of gravity and gauge symmetry are profound.