Does cosmological expansion affect local physics?

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autoren

  • Domenico Giulini

Organisationseinheiten

Externe Organisationen

  • Universität Bremen
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Seiten (von - bis)24-37
Seitenumfang14
FachzeitschriftStudies in History and Philosophy of Science Part B - Studies in History and Philosophy of Modern Physics
Jahrgang46
Ausgabenummer1
Frühes Online-Datum28 Okt. 2013
PublikationsstatusVeröffentlicht - Mai 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.

ASJC Scopus Sachgebiete

Zitieren

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, Jahrgang 46, Nr. 1, 05.2014, S. 24-37.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Download
@article{1592191d756d46f49d0e91c1f533ea1e,
title = "Does cosmological expansion affect local physics?",
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",
author = "Domenico Giulini",
year = "2014",
month = may,
doi = "10.1016/j.shpsb.2013.09.009",
language = "English",
volume = "46",
pages = "24--37",
journal = "Studies in History and Philosophy of Science Part B - Studies in History and Philosophy of Modern Physics",
issn = "1355-2198",
publisher = "Elsevier Ltd.",
number = "1",

}

Download

TY - JOUR

T1 - Does cosmological expansion affect local physics?

AU - Giulini, Domenico

PY - 2014/5

Y1 - 2014/5

N2 - 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.

AB - 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.

KW - Cosmological expansion

KW - General relativity

KW - Space time

UR - http://www.scopus.com/inward/record.url?scp=84886140717&partnerID=8YFLogxK

U2 - 10.1016/j.shpsb.2013.09.009

DO - 10.1016/j.shpsb.2013.09.009

M3 - Article

AN - SCOPUS:84886140717

VL - 46

SP - 24

EP - 37

JO - Studies in History and Philosophy of Science Part B - Studies in History and Philosophy of Modern Physics

JF - Studies in History and Philosophy of Science Part B - Studies in History and Philosophy of Modern Physics

SN - 1355-2198

IS - 1

ER -