Dark energy from cosmic structure

Type of content
Conference Contributions - Other
Publisher's DOI/URI
Thesis discipline
Degree name
Publisher
University of Canterbury. Physics and Astronomy
Journal Title
Journal ISSN
Volume Title
Language
Date
2014
Authors
Wiltshire, D.L.
Abstract

Apparent cosmic acceleration can be understood by treating geometry of universe more realistically understanding fundamental aspects of general relativity which have not been fully explored – quasi–local gravitational energy, of gradients in kinetic energy of expansion etc. “Timescape” model gives good fit to major independent tests of CDM with new perspectives on many puzzles – e.g., ‘local’/global differences in H0; primordial 7Li ? Many tests can be done to distinguish from CDM. Must be careful not to assume Friedmann equation in any data reduction. “Modified Geometry” rather than “Modified Gravity”

Description
Citation
Wiltshire, D.L. (2014) Dark energy from cosmic structure. Auckland, New Zealand: COSPA 2014: 10th International Symposium on Cosmology and Particle Astrophysics, 8-12 Dec 2014.
Keywords
Ngā upoko tukutuku/Māori subject headings
ANZSRC fields of research
Fields of Research::51 - Physical sciences::5101 - Astronomical sciences::510103 - Cosmology and extragalactic astronomy
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