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Eduardo Gueron

Publications and source records attributed to Eduardo Gueron.

7 recordsLinked to original sources

Modular Debiasing: A Robust Method for Quantum Randomness Extraction

We propose a novel modular debiasing technique applicable to any discrete random source, addressing the fundamental challenge of reliably extracting high-quality randomness from inherently imperfect physical processes. The method involves summing the outcomes of multiple independent trials from a biased source and reducing the sum modulo the number of possible outcomes, $m$. We provide a rigorous theoretical framework, utilizing probability generating functions and roots of unity, demonstrating that this simple operation guarantees the exponential convergence of the output distribution to the ideal uniform distribution over $\{0, 1, \dots, m-1\}$. A key theoretical result is the method's remarkable robustness: convergence is proven for any initial bias (provided all outcomes have non-zero probability) and, crucially, is maintained even under non-stationary conditions or time-dependent noise, which are common in physical systems. Analytical bounds quantify this exponential rate of convergence, and are empirically validated by numerical simulations. This technique's simplicity, strong theoretical guarantees, robustness, and data efficiency make it particularly well-suited for practical implementation in quantum settings, such as spatial photon-detection-based Quantum Random Number Generators (QRNGs), offering an efficient method for extracting high-quality randomness resilient to experimental imperfections. This work contributes a valuable tool to the field of Quantum Information Science.

physics.data-an↗

The relativistic glider

We present a purely relativistic effect according to which asymmetric oscillations of a quasi-rigid body slow down or accelerate its fall in a gravitational background.

gr-qc↗

"Swimming" versus "swinging" in spacetime

Wisdom has recently unveiled a new relativistic effect, called ``spacetime swimming'', where quasi-rigid free bodies in curved spacetimes can "speed up", "slow down" or "deviate" their falls by performing "local" cyclic shape deformations. We show here that for fast enough cycles this effect dominates over a non-relativistic related one, named here ``space swinging'', where the fall is altered through "nonlocal" cyclic deformations in Newtonian gravitational fields. We expect, therefore, to clarify the distinction between both effects leaving no room to controversy. Moreover, the leading contribution to the swimming effect predicted by Wisdom is enriched with a higher order term and the whole result is generalized to be applicable in cases where the tripod is in large red-shift regions.

gr-qc↗

A semi-relativistic approach to the circular restricted three body problem and a numerical experiment around the 3:2 resonance

A Hamiltonian that approaches the study of the three-body problem in general relativity is obtained. We use it to study the relativistic version of the circular restricted three-body problem in which the first body is the heaviest and the third body is a test-particle. We focus on the orbits around the 3:2 resonance. We show that, in spite of the notable difference between the relativistic and Newtonian orbits, most of the resonant region is preserved. Nevertheless, differently from the Newtonian case, the frequencies between the second and the third body are no longer commensurable.

astro-ph↗

Interacting Geodesics: Binary Systems around a Black Hole

We present a novel method to study interacting orbits in a fixed mean gravitational field associated with a solution of the Einstein field equations. The idea is to consider the Newton gravity among the orbiting particles in a geometry given by the main source. We apply the technique in the of study two and three self-gravitating particles moving around a black hole, i.e., in a Schwarzschild geometry. We also compare with the equivalent Newtonian problem and noted differences in the structural stability, e.g., binary systems were found only in the general relativistic approach.

astro-ph↗

Stability and chaos around multipolar deformed bodies: A general relativistic approach

The exact solution to the Einstein equations that represents a static axially symmetric source deformed by an internal quadrupole is considered. By using the Poincare section method we numerically study the geodesic motion of test particles. For the prolate quadrupolar deformations we found chaotic motions contrary to the oblate case where only regular motion is found. We also study the metric that represents a rotating black hole deformed by a quadrupolar term. This metric is obtained as a two soliton solution in the context of Belinsky--Zakharov inverse scattering method. The stability of geodesics depends strongly on the relative direction of the spin of the center of attraction and the test particle angular momentum. The rotation does not alter the regularity of geodesic motions in the oblate case, i.e., the orbits in this case remain regular. We also employ the method of Lyapounov characteristic numbers to examine the stability of orbits evolving around deformed nonrotating centers of attraction. The typical time to observe instability of orbits is analyzed.

astro-ph↗