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Expansion, geometry, and gravity

Caldwell, Robert R. and Kamionkowski, Marc (2004) Expansion, geometry, and gravity. Journal of Cosmology and Astroparticle Physics, 2004 (9). Art no 9. ISSN 1475-7516. http://resolver.caltech.edu/CaltechAUTHORS:CALjcap04

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Abstract

In general-relativistic cosmological models, the expansion history, matter content, and geometry are closely intertwined. In this brief paper, we clarify the distinction between the effects of geometry and expansion history on the luminosity distance. We show that the cubic correction to the Hubble law, measured recently with high-redshift supernovae, is the first cosmological measurement, apart from the cosmic microwave background, that probes directly the effects of spatial curvature. We illustrate the distinction between geometry and expansion with a toy model for which the supernova results already indicate a curvature radius larger than the Hubble distance.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/astro-ph/0403003arXivDiscussion Paper
ORCID:
AuthorORCID
Kamionkowski, Marc0000-0001-7018-2055
Additional Information:© 2004 IOP Publishing Ltd Received 20 May 2004, accepted for publication 6 September 2004, Published 17 September 2004 This work was supported at Caltech by NASA NAG5-11985 and DoE DE-FG03-92-ER40701, and at Dartmouth by NSF grant PHY-0099543. http://arxiv.org/abs/astro-ph/0403003
Funders:
Funding AgencyGrant Number
NASANAG5-11985
Department of Energy (DOE)DE-FG03-92-ER40701
NSFPHY-0099543
Subject Keywords:supernova type Ia, classical test of cosmology, gravity
Record Number:CaltechAUTHORS:CALjcap04
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:CALjcap04
Alternative URL:http://dx.doi.org/10.1088/1475-7516/2004/09/009
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:1071
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:15 Dec 2005
Last Modified:11 Dec 2016 00:25

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