We propose a quantum experiment to measure with high precision the Schwarzschild spacetime parameters of the Earth. The scheme can also be applied to measure distances by taking into account the curvature of the Earth's spacetime. As a wave packet of (entangled) light is sent from the Earth to a satellite it is redshifted and deformed due to the curvature of spacetime. Measurements after the propagation enable the estimation of the spacetime parameters. We compare our results with the state of the art, which involves classical measurement methods, and discuss what developments are required in space-based quantum experiments to improve on the current measurement of the Schwarzschild radius of the Earth.
We propose a quantum experiment to measure with high precision the Schwarzschild spacetime parameters of the Earth. The scheme can also be applied to measure distances by taking into account the curvature of the Earth's spacetime. As a wave packet of (entangled) light is sent from the Earth to a satellite it is redshifted and deformed due to the curvature of spacetime. Measurements after the propagation enable the estimation of the spacetime parameters. We compare our results with the state of the art, which involves classical measurement methods, and discuss what developments are required in space-based quantum experiments to improve on the current measurement of the Schwarzschild radius of the Earth.
We study how quantum systems that propagate in the spacetime of a rotating planet are affected by the curved background. Spacetime curvature affects wavepackets of photons propagating from Earth to a satellite, and the changes in the wavepacket encode the parameters of the spacetime. This allows us to evaluate quantitatively how quantum communications are affected by the curved spacetime background of the Earth and to achieve precise measurements of Earth's Schwarzschild radius and equatorial angular velocity. We then provide a comparison with the state of the art in parameter estimation obtained through classical means. Satellite to satellite communications and future directions are also discussed.
We consider quantum communication schemes where quantum optical signals are exchanged between a source on Earth and a satellite. The background curved spacetime affects the quantum state of the propagating photons. We employ quantum-metrology techniques to obtain optimal bounds for the precision of quantum measurements of relevant physical parameters encoded in the final state. We focus on satellites in low Earth orbits and we find that our scheme improves the precision of the measurement of the Schwarzschild radius obtained within previous studies. Therefore, our techniques can provide the theoretical tools for novel developments that can potentially outperform the state-of-the-art obtained through classical means. We also review the impact of the relativistic effects on a simple quantum key distribution protocol within satellite schemes and find that such effects can be greatly damaging if they are not properly accounted for.
In this thesis we study relativistic effects on quantum systems. Quantum physics in curved spacetime is reviewed in a first place, with a focus on continuous variables formalism, quantum metrology techniques, and the relativistic treatment of polarised photons. Then, three topics of interest are studied. The first one is the phononic gravitational wave detector, where resonant mode-mixing and particle creation are triggered in a Bose-Einstein condensate by the passing of a gravitational wave, which can then be measured thanks to quantum metrology techniques. The theory for the phonons’ transformation is developed in details in different resonance scenarios and some sources of noise are considered, like shaking of the cavity where the condensate is trapped and thermal noise. The second topic adressed is quantum communication and metrology in space. In this part, we describe quantum experiments involving communications between Earth and satellites using frequency modes of photons. The propagated and measured photons encode parameters of the spacetime background that can be measured using quantum metrology. Several satellite schemes are discussed, such as satellite to satellite radial communications in Kerr spacetime or Earth to satellite communications in Schwarzschild spacetime. The last topic of this thesis is the evolution of helicity states of photons in a relativistic picture. Two experiments are considered: one where the photons propagate between Earth and satellites through the curved spacetime background surrounding the Earth. The other experiment looks at quantum states of polarised photons as seen by centrifuged observers. For each of these parts, we provide the theory for novel experimental proposals, within the frameworks of either (or both) quantum communications and quantum metrology, that, we believe, would lead to a better understanding in the overlap of quantum mechanics and the relativity theories.
The focus of this work is discussing the realization of space based experiments testing quantum mechanics, specifically quantum optics. The main experimental work is the practical realization of the earthbound part of a possible interferometric experiment that can be realized with a delayed-choice operational mode. The full Earth-satellite realization of this experimental scheme could set a new record on the distance to which delayed-choice schemes have been experimentally realized. General relativistic effects on Earth-satellite experiments is also discussed, in the case of two different setups. One of those is essentially the ground-space implementation of the interferometer realized in the laboratory, while the other represents a different possibility that could in principle measure gravitational redshift to single photons to greater extent. Which-path behavior and interference were observed to a very good degree on the interferometer realized in the lab. Specifically, the assessment of interference visibility, which was done after careful alignement of the setup, yields a value of approximately 95%, and a comparable value of approx 93% was obtained with an alternative setup which was also experimentally realized in the laboratory.
As far as theoretical computations are concerned, a good formalism to deal with space-based interferometric measurements was pointed out, which allows to take into account both special relativistic contributes and general relativistic corrections to the amplitude describing the photons involved with this kind of experiments. Two different setups, which are candidates for the measurement of single photon gravitational redshift, were analyzed with this formalism. The setup with one interferometer on the ground and the other on the satellite, in principle, constitutes a good way to observe this effect by means of a phase measurement, to the first order in the gravitational potentials.
Physical theories are developed to describe phenomena in particular regimes, and generally are valid only within a limited range of scales. For example, general relativity provides an effective description of the Universe at large length scales, and has been tested from the cosmic scale down to distances as small as 10 meters. In contrast, quantum theory provides an effective description of physics at small length scales. Direct tests of quantum theory have been performed at the smallest probeable scales at the Large Hadron Collider, ∼10−20 meters, up to that of hundreds of kilometers. Yet, such tests fall short of the scales required to investigate potentially significant physics that arises at the intersection of quantum and relativistic regimes. We propose to push direct tests of quantum theory to larger and larger length scales, approaching that of the radius of curvature of spacetime, where we begin to probe the interaction between gravity and quantum phenomena. In particular, we review a wide variety of potential tests of fundamental physics that are conceivable with artificial satellites in Earth orbit and elsewhere in the solar system, and attempt to sketch the magnitudes of potentially observable effects. The tests have the potential to determine the applicability of quantum theory at larger length scales, eliminate various alternative physical theories, and place bounds on phenomenological models motivated by ideas about spacetime microstructure from quantum gravity. From a more pragmatic perspective, as quantum communication technologies such as quantum key distribution advance into Space towards large distances, some of the fundamental physical effects discussed here may need to be taken into account to make such schemes viable.
n n n The precision of physical parameters is fundamentally limited by irreducible levelsof noise set by quantum mechanics. Quantum metrology is the study of reaching theselimits of noise by employing optimal schemes for parameter estimation. Techniquesin quantum metrology can assist in developing devices to measure the fundamentalinterplay between quantum mechanics and general relativity at state-of-the-artprecision. An example of this is the recent detection of gravitational waves bythe LIGO interferometer. In this thesis, we focus on using quantum metrologyfor estimating space-time parameters. We show the optimal quantum resourcesthat are needed for estimating the gravitational redshift of light propagating in theSchwarzschild space-time of Earth including the inevitable losses due to atmosphericdistortion. We also propose a quantum interferometer using higher order Kerrnon-linearities to improve the sensitivity of estimating gravitational time dilation.In principle, we would be able to downsize interferometers and probe gravity over asmall scale potentially making it practical for measuring gravitational gradients. Wethen study the interesting features of the metric around a rotating massive bodyknown as the Kerr metric and propose implementing a stationary interferometer tomeasure the effect of frame dragging. Finally, we consider loss in the visibility ofquantum interference of single photons in rotating reference frames, and analogouslyin the Kerr metric. In essence, the quantum interference of photons will be affectedby the relativistic effect of rotation. We find experimentally feasible parametersrequiring long optical fibre for long coherence lengths of photons. Our results willhopefully contribute to the efforts of building future quantum technologies that willenter a new regime where general relativistic effects can be measured.