TY - JOUR
T1 - Mechanical cosmology
T2 - Simulating scalar fluctuations in expanding universes using synthetic mechanical lattices
AU - Rhyno, Brendan
AU - Velkovsky, Ivan
AU - Adshead, Peter
AU - Gadway, Bryce
AU - Vishveshwara, Smitha
N1 - Acknowledgments. We thank Naceur Gaaloul and Zain Mehdi for insightful discussions. We gratefully acknowledge support by the National Aeronautics and Space Administration, Jet Propulsion Laboratory Research Support Agreement No. 1699891 (B.R. and S.V.), by the United States Department of Energy, DE-SC0015655 (P.A.), and the AFOSR MURI program under Agreement No. FA9550-22-1-0339 (I.V. and B.G.).
PY - 2025/4
Y1 - 2025/4
N2 - Inspired by recent advances in observational astrophysics and continued explorations in the field of analog gravity, we discuss the prospect of simulating models of cosmology within the context of synthetic mechanical lattice experiments. We focus on the physics of expanding universe scenarios described by the Friedmann-Lemaître-Robertson-Walker (FLRW) metric. Specifically, quantizing scalar fluctuations in a background FLRW spacetime leads to a quadratic bosonic Hamiltonian with temporally varying pair production terms. Here we present a mapping that provides a one-to-one correspondence between these classes of cosmology models and feedback-coupled mechanical oscillators. As proof of principle, we then perform experiments on a synthetic mechanical lattice composed of such oscillators. We simulate two different FLRW expansion scenarios with universes dominated by vacuum energy and matter and discuss our experimental results.
AB - Inspired by recent advances in observational astrophysics and continued explorations in the field of analog gravity, we discuss the prospect of simulating models of cosmology within the context of synthetic mechanical lattice experiments. We focus on the physics of expanding universe scenarios described by the Friedmann-Lemaître-Robertson-Walker (FLRW) metric. Specifically, quantizing scalar fluctuations in a background FLRW spacetime leads to a quadratic bosonic Hamiltonian with temporally varying pair production terms. Here we present a mapping that provides a one-to-one correspondence between these classes of cosmology models and feedback-coupled mechanical oscillators. As proof of principle, we then perform experiments on a synthetic mechanical lattice composed of such oscillators. We simulate two different FLRW expansion scenarios with universes dominated by vacuum energy and matter and discuss our experimental results.
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U2 - 10.1103/PhysRevResearch.7.L022004
DO - 10.1103/PhysRevResearch.7.L022004
M3 - Article
AN - SCOPUS:105001870253
SN - 2643-1564
VL - 7
JO - Physical Review Research
JF - Physical Review Research
IS - 2
M1 - L022004
ER -