On relativistic cosmology and on the definition of distance in general relativity
dc.contributor.author
Etherington, I. M. H.
en
dc.date.accessioned
2018-09-13T15:52:37Z
dc.date.available
2018-09-13T15:52:37Z
dc.date.issued
1932
dc.description.abstract
en
dc.description.abstract
I have applied my formulae for astronomical distance
to the de Sitter world to show how they work. In view of
the probability (see page 19) that the real universe
approximates to the de Sitter world as regards the future
and the recent past, but not as regards the remote past,
the numerical results on page 83 are not reliable. But
the formula (85) should give a reliable approximation
when the more accurate form of (84) is established. So far
as I am aware, the formula (86) has not been given before.
en
dc.description.abstract
As I have already indicated, I hope in a future
investigation to apply my formulae for distance to the Expanding Universe, and see whether any corrections are
needed on the numerical results which have been established.
en
dc.identifier.uri
http://hdl.handle.net/1842/32130
dc.publisher
The University of Edinburgh
en
dc.relation.ispartof
Annexe Thesis Digitisation Project 2018 Block 20
en
dc.relation.isreferencedby
en
dc.title
On relativistic cosmology and on the definition of distance in general relativity
en
dc.type
Thesis or Dissertation
en
dc.type.qualificationlevel
Doctoral
en
dc.type.qualificationname
PhD Doctor of Philosophy
en
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