Download presentation
Presentation is loading. Please wait.
Published byMerryl Weaver Modified over 9 years ago
1
By: Tony Strazzara
2
Why might our universe be finite? medieval philosophers gave the first logical arguments supporting a finite universe during the early 20 th century, Einstein proposed a closed, static universe shaped like a hypersphere in 1929, Edwin Hubble discovers constant rate of expansion of universe
3
Galaxy clusters slowly growing farther apart If distance between them is increasing today, then they were closer together in the past Raisin bread analogy Roughly 13.7 billion years ago
5
Discovered accidentally in 1964 by two radio astronomers, the CMB is electromagnetic radiation filling the universe Photons emitted from hydrogen plasma roughly 300,000 years after the big bang occurred Thermal spectrum of ~2.725 K
6
The surface of last scattering (LSS) Observing the CMB means looking back in time Looking every direction at one instant in time produces a sphere
7
COBE – Cosmic Background Explorer launched November 1989 DMR (differential microwave radiometer) used to map cosmic radiation WMAP – Wilkinson Microwave Anisotropy Probe launched June 2001 mission: to determine the content, evolution and geometry of the universe
8
Colors Contrast in clarity Shape of data
9
Temperature fluctuations Large angular scales Small and infinite universe ~ 70 billion light years across Let’s change gears…
10
A manifold is a space that on a local scale resembles Euclidean geometry of a specific dimension while on a global scale may be more complicated What is a 2-manifold? 3-manifolds Cosmologists consider only 3 types of geometries for our universe: hyperbolic (negative curvature), elliptic (positive curvature), and Euclidean (zero curvature)
11
The Hyperbolic Plane
12
What is a 3-torus? To an observer, line of sight straight ahead eventually leads to seeing the back of one’s own head And looking up or the right? We’ll take a look later…
13
No – data of CMB from COBE disproves a cubic 3-torus (T3 space) In fact, cosmologists have ruled out the possibility of any toroidal model T1 and T2 spaces T1 space T2 space T3 space
14
Due to the nature of most other 3-manifolds, our universe is presumably negatively curved Cosmologists can propose a topology for the universe, deduce what the CMB should look like, then observe how well COBE/WMAP data matches up So how does this data “match up”?
15
If observed space (LSS) is larger than physical space, expect correlations in CMB Balloon-cube analogy Correlation is in form of circle pairs 2 identical circles – one from sphere leaving a face of the manifold and one from sphere entering opposite face back into the manifold Seen as 2 circles with identical variations in temperature fluctuations
16
Think about it first in a 2-manifold… Torus
17
Now for a 3-manifold… 3-Torus
18
Distance between points in a circle pair is a path Note – if you choose the same point in both circles, one as a starting point of the path and the other as the ending point, you have constructed a loop! Why? By constructing loops in the fundamental group, we can predict the topology of the universe
19
Distortion due to a negatively curved universe The lines that light follow in hyperbolic space Circles in the sky will be distorted into ovals because of this curvature of space
20
PDS is a possible manifold for topology of universe 12 faced polyhedron Each face is a pentagon Glue opposite faces to each other with a minimal clockwise turn
21
New evidence supporting the possibility Temperature fluctuations around 12 dodecahedrally spaced circles of radius ~11 degrees found in WMAP correspond unusually well dodecahedrally - phase shift of 36 degrees Would mean universe has slightly positive curvature
23
3-Torus Mirrored Dodecahedron Poincare Dodecahedron
24
7-year map released earlier this year Neutrinos Zero curvature
25
Cornish, Neil J., Spergel, David N., and Starkman, Glenn D. “Measuring the Topology of the Universe.”.http://www.pnas.org/content/95/1/82.full.pdf+html Oliveira-Costa, Angelica de, Smoot, George F., and Starobinsky, Alexei A.. “Can the Lack of Symmetry in the COBE/DMR Maps Constrain the Topology of the Universe?”.http://arxiv.org/PS_cache/astro-ph/pdf/9510/9510109v2.pdf Levin, Janna J., Barrow, John D., Bunn, Emory F., and Silk, Joseph. “Flat Spots: Topological Signatures of an Open Universe in COBE Sky Maps.”.http://arxiv.org/PS_cache/astro- ph/pdf/9702/9702242v1.pdf Levin, Janna. “Missing Lorenz-boosted Circles in the Sky.”.http://arxiv.org/PS_cache/astro- ph/pdf/0403/0403036v1.pdf Roukema, Boudewijn F., Lew, Bartosz, Cechowska, Magdalena, Marecki, Andrzej, and Bajtlik, Stanislaw. “A Hint of Poincare Dodecahedral Topology in the WMAP First Year Sky Map.”.http://arxiv.org/PS_cache/astro-ph/pdf/0402/0402608v4.pdf Greason, Michael R. “Cosmic Background Explorer.”.http://lambda.gsfc.nasa.gov/product/cobe/ Greason, Michael R. “Wilkinson Microwave Anisotropy Probe.”.http://lambda.gsfc.nasa.gov/product/map/current/ Muir, Hazel. “Tantalising Evidence Hints Universe is Finite.”.http://www.newscientist.com/article/dn4250-tantalising-evidence-hints-universe-is- finite.html
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.