Quantum simulation of cosmic inflation in two-component Bose-Einstein condensates
Uwe R. Fischer, Ralf Sch\"utzhold

TL;DR
This paper proposes using two-component Bose-Einstein condensates to simulate cosmic inflation, offering a flexible platform to study early universe quantum fluctuations through analogue gravity models.
Contribution
It extends the quantum simulation of cosmic inflation from one-component to two-component Bose-Einstein condensates, highlighting increased flexibility and experimental advantages.
Findings
Demonstrates effective sonic geometries in two-component BECs
Proposes an experiment to simulate inflaton evolution and quantum fluctuations
Shows advantages over one-component setups for analogue gravity
Abstract
Generalizing the one-component case, we demonstrate that the propagation of sound waves in two-component Bose-Einstein condensates can also be described in terms of effective sonic geometries under appropriate conditions. In comparison with the one-component case, the two-component setup offers more flexibility and several advantages. In view of these advantages, we propose an experiment in which the evolution of the inflaton field, and thereby the generation of density quantum fluctuations in the very early stages of our universe during inflation, can be simulated, realizing a {\em quantum simulation via analogue gravity models}.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
