Geometry and Cosmology
Chris Doran
Anthony Lasenby
www.mrao.cam.ac.uk/~clifford
Non-Euclidean Geometry
" Axioms of geometry date back to
Euclid s Elements
" Among these is the parallel postulate:
Given a line l and a point P not on l, there
exists a unique line m in the same plane as
P and l which passes through P and does
not meet l
" Non-Euclidean geometry arises by
removing the uniqueness requirement
Geometry and Cosmology
Non-Euclidean Geometry
" Developed by Lobachevskii (1792-
1856) and Bolyai (1802-1860)
" In modern terminology this defines
hyperbolic geometry
" A homogeneous, isotropic, unbounded
space of constant negative curvature
" An elegant view of this geometry was
constructed by Poincaré (1854-1912)
Geometry and Cosmology
Poincaré Disc
" Points contained in a disc of unit radius
" Boundary of the disk represents set of
points at infinity
" Lines (geodesics) are represented by
circles which intersect the unit circle at
right angles
" All geodesics through the origin are
straight lines (in Euclidean sense)
Geometry and Cosmology
Poincaré Disc
Set of lines
through A
which miss l
Disc
l
Right-angle
intersection
Plot constructed
in Cinderella
Geometry and Cosmology
Distance
" The metric in the disc representation is
" This is a conformal representation
only differs from flat by a single factor
" Distortions get greater as you move
away from the centre
" Can define tesselations
Geometry and Cosmology
Circle Limit 3
M. Escher
Geometry and Cosmology
de Sitter Space
" Now suppose that the underlying
signature is Lorentzian
" Construct a homogeneous, isotropic
space of constant negative curvature
" This is de Sitter space
" 2D version from embedding picture
Geometry and Cosmology
Embedding View
null geodesic
time
straight line in
embedding space
space
Geometry and Cosmology
Lorentzian View
Circle mapped onto a line via a
stereographic projection.
Extend out assuming null
trajectories are at 45o
Geometry and Cosmology
Lorentzian View
Perpendicular
intersection
Timelike geodesic
Boundary
Hyperbolae
Spacelike
geodesic
Null cone
Always at 45o
Geometry and Cosmology
The Cosmological Constant
" Start with FRW equations
" Introduce the dimensionless ratios
Geometry and Cosmology
The Cosmological Constant
" Write
" Evolution equations now
" Define trajectories via
Geometry and Cosmology
Cosmic Trajectories
Dust Radiation
de Sitter phase
Big Bang
Geometry and Cosmology
The de Sitter Phase
" End of the universe enters a de Sitter
phase
" Should really be closed for pure de Sitter
" Only get a natural symmetric embedding
onto entire de Sitter topology if
" Says that a photon gets ź of the way
across the universe
Geometry and Cosmology
A Preferred Model
Current Observations
Dust
Arrive at a model
quite close to
observation
Critical
For dust (·=0) predict
a universe closed at
about the 10% level
Geometry and Cosmology
Summary
" de Sitter geometry is a natural
extension of non-Euclidean geometry
" Has a straightforward construction in a
Lorentzian space
" Can form a background space for a
gauge theory of gravity
" Appears to pick out a preferred
cosmological model
" But is this causal?
Geometry and Cosmology
Wyszukiwarka
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