Einstein field equations for Bose-Einstein condensates in cosmology
Creators
- 1. Department of Mathematics and Applications, University of Milano-Bicocca, Via Cozzi 55, 20125, Milano (Italy)
Description
In this work we consider the Gross-Pitaevskii equation for Bose-Einstein condensates (BECs) in a general Riemannian metric. Given initial conditions dictated by an external potential, we consider the free expansion of the condensate when the external potential is turned off. Focusing on the forces associated with the geometry of the initial configuration, we show how these are related to the Ricci curvature tensor and the Ricci scalar and we find an Einstein field equation governing the steady flow. Some important correlations between the study of defects in BECs and the appearance of cosmological singularities will be addressed, in particular the emergence of an effective Lorentzian spacetime geometry, which is what is needed to obtain Hawking radiation effects. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/1730/1/012017Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 1730
- Journal Issue
- 1
- Journal Page Range
- [7 p.]
- ISSN
- 1742-6596
Conference
- Title
- 9. International Conference on Mathematical Modeling in Physical Sciences (IC-MSQUARE)
- Dates
- 7-10 Sep 2020
- Place
- Tinos (Greece)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 54005606
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BOSE-EINSTEIN CONDENSATION; CONDENSATES; COSMOLOGY; DEFECTS; EINSTEIN FIELD EQUATIONS; GEOMETRY; METRICS; RADIATION EFFECTS; SCALARS; SINGULARITY; SPACE-TIME; STEADY FLOW; TENSORS
- Descriptors DEC
- EQUATIONS; FIELD EQUATIONS; FLUID FLOW; MATHEMATICS