Does cosmological expansion affect local physics?

Research output: Contribution to journalArticleResearchpeer review

Authors

  • Domenico Giulini

Research Organisations

External Research Organisations

  • University of Bremen
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Details

Original languageEnglish
Pages (from-to)24-37
Number of pages14
JournalStudies in History and Philosophy of Science Part B - Studies in History and Philosophy of Modern Physics
Volume46
Issue number1
Early online date28 Oct 2013
Publication statusPublished - May 2014

Abstract

In this contribution I wish to address the question whether, and how, the global cosmological expansion influences local physics, like particle orbits and black hole geometries. Regarding the former I argue that a pseudo Newtonian picture can be quite accurate if "expansion" is taken to be an attribute of the inertial structure rather than of "space" in some substantivalist sense. This contradicts the often-heard suggestion to imagine cosmological expansion as that of "space itself". Regarding isolated objects in full General Relativity, like black holes, I emphasise the need for proper geometric characterisations in order to meaningfully compare them in different spacetimes, like static and expanding ones. Examples are discussed in some detail to clearly map out the problems. A slightly extended version of this contribution may be found at philsci-archive.pitt.edu/10033.

Keywords

    Cosmological expansion, General relativity, Space time

ASJC Scopus subject areas

Cite this

Does cosmological expansion affect local physics? / Giulini, Domenico.
In: Studies in History and Philosophy of Science Part B - Studies in History and Philosophy of Modern Physics, Vol. 46, No. 1, 05.2014, p. 24-37.

Research output: Contribution to journalArticleResearchpeer review

Download
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