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Phonon-based quantum testing schemes using BECs for gravity modifications in light of dark matter exploration

Phonon-based quantum testing schemes using BECs for gravity modifications in light of dark matter exploration
Phonon-based quantum testing schemes using BECs for gravity modifications in light of dark matter exploration
The nature of dark matter and dark energy remains an open question in modern physics. While dark matter is inferred from astrophysical observations and dark energy accounts for the accelerated expansion of the universe, their fundamental origins remain unknown. This motivates alternative approaches to explain the observed behaviour of the universe by modifying our current theory of gravity. This thesis proposes a novel method for testing such modified theories of gravity by exploiting the dynamics of quantum phononic excitations present in Bose-Einstein Condensates (BECs), which can be realized in tabletop experiments with current technology. Our proposal implements quantum metrology within the physics of the BEC and its phononic excitations, taking advantage of Gaussian states and the tritter operation to prepare highly sensitive phonon states for estimating gravitational parameters. Specifically, we aim to measure the gravitational potential of an oscillating massive sphere by estimating the exerted acceleration on a BEC, inferred through phonon dynamics. We predict an acceleration precision of approximately $10^{-17}$ m/s$^{2}$, allowing us to test deviations from Newtonian gravity. We examine two modified-gravity models: Modified Newtonian Dynamics (MOND) and Lambda-gravity. The precision of our method enables the distinction between MOND and Newtonian gravity under experimentally feasible conditions. For Lambda-gravity, our setup allows us to measure Newton’s gravitational constant $G$ with a relative precision of 10$^{-7}$, improving current measurements by two orders of magnitude. Additionally, it provides an upper bound on the cosmological constant of $\Lambda < 10^{-31}$ m$^{-2}$, representing the first laboratory-based experimental constraint on $\Lambda$. In conclusion, this thesis presents a novel, high-precision method for probing Newtonian gravity while paving the road for future research focused on probing relativistic effects.
University of Southampton
Fernandez Melendez, Hector Antonio
82124cb1-f255-48a2-a386-81a8c83a1270
Fernandez Melendez, Hector Antonio
82124cb1-f255-48a2-a386-81a8c83a1270
Fuentes-Guridi, Ivette
c6d65a4c-feac-44c1-9097-e0f6a9e0cf44
Belyaev, Alexander
6bdb9638-5ff9-4b65-a8f2-34bae3ac34b3

Fernandez Melendez, Hector Antonio (2025) Phonon-based quantum testing schemes using BECs for gravity modifications in light of dark matter exploration. University of Southampton, Doctoral Thesis.

Record type: Thesis (Doctoral)

Abstract

The nature of dark matter and dark energy remains an open question in modern physics. While dark matter is inferred from astrophysical observations and dark energy accounts for the accelerated expansion of the universe, their fundamental origins remain unknown. This motivates alternative approaches to explain the observed behaviour of the universe by modifying our current theory of gravity. This thesis proposes a novel method for testing such modified theories of gravity by exploiting the dynamics of quantum phononic excitations present in Bose-Einstein Condensates (BECs), which can be realized in tabletop experiments with current technology. Our proposal implements quantum metrology within the physics of the BEC and its phononic excitations, taking advantage of Gaussian states and the tritter operation to prepare highly sensitive phonon states for estimating gravitational parameters. Specifically, we aim to measure the gravitational potential of an oscillating massive sphere by estimating the exerted acceleration on a BEC, inferred through phonon dynamics. We predict an acceleration precision of approximately $10^{-17}$ m/s$^{2}$, allowing us to test deviations from Newtonian gravity. We examine two modified-gravity models: Modified Newtonian Dynamics (MOND) and Lambda-gravity. The precision of our method enables the distinction between MOND and Newtonian gravity under experimentally feasible conditions. For Lambda-gravity, our setup allows us to measure Newton’s gravitational constant $G$ with a relative precision of 10$^{-7}$, improving current measurements by two orders of magnitude. Additionally, it provides an upper bound on the cosmological constant of $\Lambda < 10^{-31}$ m$^{-2}$, representing the first laboratory-based experimental constraint on $\Lambda$. In conclusion, this thesis presents a novel, high-precision method for probing Newtonian gravity while paving the road for future research focused on probing relativistic effects.

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Published date: June 2025

Identifiers

Local EPrints ID: 502334
URI: http://eprints.soton.ac.uk/id/eprint/502334
PURE UUID: f18bef82-ecf1-4f6e-afec-f5a00ba50e33
ORCID for Hector Antonio Fernandez Melendez: ORCID iD orcid.org/0000-0003-3224-1282
ORCID for Alexander Belyaev: ORCID iD orcid.org/0000-0002-1733-4408

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Date deposited: 23 Jun 2025 16:46
Last modified: 11 Sep 2025 03:19

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