dc.contributor.authorHuang, Kerson.
dc.contributor.authorLow, Hwee-Boon.
dc.contributor.authorTung, Roh-Suan.
dc.date.accessioned2013-08-06T04:50:07Z
dc.date.available2013-08-06T04:50:07Z
dc.date.copyright2012en_US
dc.date.issued2012
dc.identifier.citationHuang, K., Low, H. B.,& Tung, R. S. (2012). Scalar field cosmology: I. Asymptotic freedom and the initial-value problem. Classical and Quantum Gravity, 29(15).en_US
dc.identifier.urihttp://hdl.handle.net/10220/13054
dc.description.abstractThe purpose of this work is to use a renormalized quantum scalar field to investigate very early cosmology, in the Planck era immediately following the big bang. Renormalization effects make the field potential dependent on length scale, and are important during the big bang era. We use the asymptotically free Halpern-Huang scalar field, which is derived from renormalization-group analysis, and solve Einsteins equation with Robertson-Walker metric as an initial-value problem. The main prediction is that the Hubble parameter follows a power law: H ≡ a/a ∼ t -p, and the universe expands at an accelerated rate: a ∼ expt 1-p. This gives dark energy, with an equivalent cosmological constant that decays in time like t -2p, which avoids the fine-tuning problem. The power law predicts a simple relation for the galactic redshift. Comparison with data leads to the speculation that the universe experienced a crossover transition, which was completed about seven billion years ago.en_US
dc.language.isoenen_US
dc.relation.ispartofseriesClassical and quantum gravityen_US
dc.subjectDRNTU::Science::Astronomy::Astrophysics
dc.titleScalar field cosmology : I. asymptotic freedom and the initial-value problemen_US
dc.typeJournal Article
dc.contributor.researchInstitute of Advanced Studiesen_US
dc.identifier.doihttp://dx.doi.org/10.1088/0264-9381/29/15/155014


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