Numerical Simulation of Axion Quintessence
Author
Source
Advances in Mathematical Physics
Issue
Vol. 2012, Issue 2012 (31 Dec. 2012), pp.1-11, 11 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2012-07-29
Country of Publication
Egypt
No. of Pages
11
Main Subjects
Abstract EN
Robust, scaled cosmological equations are derived for simulating the evolution of the scalar field, the scale factor, and the Hubble parameter during both expanding and contracting phases of the universe.
These scaled equations are applied to both stable (always expanding universe) and unstable axion quintessence (expanding and then collapsing universe).
When applied to unstable axion quintessence, these scaled equations allow the simulations presented here to proceed much closer to the singularity at the end of a collapsing universe than any previous simulations.
American Psychological Association (APA)
Gardner, Carl L.. 2012. Numerical Simulation of Axion Quintessence. Advances in Mathematical Physics،Vol. 2012, no. 2012, pp.1-11.
https://search.emarefa.net/detail/BIM-466422
Modern Language Association (MLA)
Gardner, Carl L.. Numerical Simulation of Axion Quintessence. Advances in Mathematical Physics No. 2012 (2012), pp.1-11.
https://search.emarefa.net/detail/BIM-466422
American Medical Association (AMA)
Gardner, Carl L.. Numerical Simulation of Axion Quintessence. Advances in Mathematical Physics. 2012. Vol. 2012, no. 2012, pp.1-11.
https://search.emarefa.net/detail/BIM-466422
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-466422