Skip to main content Accessibility help
×
Hostname: page-component-76fb5796d-dfsvx Total loading time: 0 Render date: 2024-04-28T21:35:22.643Z Has data issue: false hasContentIssue false

5 - Newtonian Cosmology

from Part II - Newtonian Cosmology

Published online by Cambridge University Press:  04 May 2017

Bernard J. T. Jones
Affiliation:
Rijksuniversiteit Groningen, The Netherlands
Get access

Summary

We will use Newtonian versions of solutions to the Einstein field equations to describe a series of model universes that provide a framework within which we can better understand how our Universe works. Newton's theory of gravitation has been replaced by Einstein's, but in many respects Newton's theory is a pretty good approximation: good enough that we depend on it in our everyday lives. The Newtonian view is certainly easier for us to relate to and exploit, but we must understand the inherent limitations.

Here, we highlight the fundamental differences between the Newtonian and Einsteinian theories: Newton with his absolute space and universal time, and Einstein with his geometrisation of gravity. Fortunately, there are some relevant solutions of the Einstein equations that have direct Newtonian analogues. Those Newtonian analogues are lacking some important features, notably a lack of a description of how light propagates. Fortunately, we can graft the information from some of the Einstein models onto the Newtonian models to produce what we might call Newtonian surrogates of the Einsteinian models.

In this chapter we introduce the simplest of a series of homogeneous and isotropic cosmological models formulated within the limited framework of Newtonian gravity. These models contains only ‘dust’: pressure free matter made up of particles that are neither created nor destroyed, and that do not interact with one another. The Universe evolves under the mutual gravitational interaction of those particles.

While this model is not realistic it nevertheless allows us to develop a full cosmological model that is the template for the more complex models that follow. We develop these models in considerable detail since much of what is done will be repeated for the other, more realistic, models.

It is worth remarking that these models are fundamental to numerical N-body simulations of the Universe in which the constituent particles are ‘dust’. Such dust models can also be used to study the growth of the structure in the Universe.

Why Bother with Newton?

Two Views of Gravity

The expansion of the Universe is dominated by the gravitational force. The best theory we have for the gravitational force is Einstein's Theory of General Relativity (Einstein, 1916a), which relates geometry with the material content of the space-time containing that matter.

Type
Chapter
Information
Precision Cosmology
The First Half Million Years
, pp. 97 - 129
Publisher: Cambridge University Press
Print publication year: 2017

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

  • Newtonian Cosmology
  • Bernard J. T. Jones, Rijksuniversiteit Groningen, The Netherlands
  • Book: Precision Cosmology
  • Online publication: 04 May 2017
  • Chapter DOI: https://doi.org/10.1017/CBO9781139027809.007
Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

  • Newtonian Cosmology
  • Bernard J. T. Jones, Rijksuniversiteit Groningen, The Netherlands
  • Book: Precision Cosmology
  • Online publication: 04 May 2017
  • Chapter DOI: https://doi.org/10.1017/CBO9781139027809.007
Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Newtonian Cosmology
  • Bernard J. T. Jones, Rijksuniversiteit Groningen, The Netherlands
  • Book: Precision Cosmology
  • Online publication: 04 May 2017
  • Chapter DOI: https://doi.org/10.1017/CBO9781139027809.007
Available formats
×