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Transcript of X What is the shape of our universe? By Sandro Berndt.
x
What is the shape of our universe?What is the shape of our universe?
By Sandro BerndtBy Sandro Berndt
22What is the shape of our universe?
x
Historic views
Theory / Topology
CMB data
Introduction Introduction
Historic views on the universeHistoric views on the universe Theory / TopologyTheory / Topology What CMB tells usWhat CMB tells us
33What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
GeocentricGeocentric
Heliocentric Heliocentric
(~1543)(~1543)
KeplerianKeplerian
(~1606)(~1606)
Early modelsEarly models
[2][3]
44What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Steady state modelSteady state model
Based on the Based on the perfect cosmological principleperfect cosmological principle
(Universe looks the same from every place and at every time)(Universe looks the same from every place and at every time)
Expansion of the universe fixed by “creation of mass”Expansion of the universe fixed by “creation of mass”
[2]
55What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Einstein‘s Einstein‘s contributioncontribution
Theory of general relativity Theory of general relativity ↔ shape of the universe↔ shape of the universe
GRT leads to expansion and / or collapseGRT leads to expansion and / or collapse Cosmological constant Cosmological constant ΛΛ introduced as a mathematical fix introduced as a mathematical fix
Different solutions for GRTDifferent solutions for GRT
[2]
66What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
ToposTopos = places = places Defined on a set Defined on a set ConnectionsConnections of subsets / of subsets /
elementselements Topology determines geometryTopology determines geometry Imagination limited to three Imagination limited to three
dimensionsdimensions
TopologiesTopologies
[4]
77What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Flat geometry: Flat geometry: Simple “parallel transport”Simple “parallel transport” Sum of angles in a triangle 180°Sum of angles in a triangle 180°
Connect opposite sides
Connect circles
TopologiesTopologies
88What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Torus represents a flat Torus represents a flat geometrygeometry
Finite volumeFinite volume
Torus constructionTorus construction
[3]
99What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Creatures living in a 1-d worldCreatures living in a 1-d world
22ndnd dimension cannot be realized by inhabitants of the “line” dimension cannot be realized by inhabitants of the “line” No “footsteps” in 1-dNo “footsteps” in 1-d
x x x x x x ???
Low dimensional examples ILow dimensional examples I
1010What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Low dimensional examples IILow dimensional examples II
Creatures in a “plane” worldCreatures in a “plane” world No movement in the 3No movement in the 3rdrd dimension dimension
x x x
x x ???
1111What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
What about us?What about us?
““Shortcut” through 4Shortcut” through 4thth dimension dimension
would not be traceablewould not be traceable
x x
???
1212What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
The edge of our universeThe edge of our universe
Faces are connectedFaces are connected No end / edge detectableNo end / edge detectable
(Like flat earth turned out to be spheric)(Like flat earth turned out to be spheric)
1313What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Our Galaxy
A hall of mirrors?A hall of mirrors?
Similar to Olbers paradoxSimilar to Olbers paradox Solved by Solved by
redshift redshift size of the universesize of the universe lifetime of stars / galaxieslifetime of stars / galaxies
1414What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Astronomers Arno Penzias & Robert Wilson Astronomers Arno Penzias & Robert Wilson (Nobel Prize in 1978)(Nobel Prize in 1978)
Isotropic radiation ~ 2.7 KelvinIsotropic radiation ~ 2.7 Kelvin Leftover from hotter and smaller universeLeftover from hotter and smaller universe Supports Big Bang theory Supports Big Bang theory
Discovery in 1964Discovery in 1964
[1]
1515What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
1989 - 1993 1989 - 1993 Detailed view of CMBDetailed view of CMB Explored age / geometry / composition of the universeExplored age / geometry / composition of the universe Supports flat universeSupports flat universe
Cosmic background explorer (COBE)Cosmic background explorer (COBE)
[1]
1616What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
T = 2.725 KT = 2.725 K Perfect blackbodyPerfect blackbody
Cosmic background explorer (COBE)Cosmic background explorer (COBE)
[1]
1717What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Launched 2001Launched 2001 22 – 90 GHz / 3.3 -13.6 mm22 – 90 GHz / 3.3 -13.6 mm 20 x resolution of COBE20 x resolution of COBE ΔΔT = 20 - 35 µK T = 20 - 35 µK
Wilkinson Microwave Anisotropy ProbeWilkinson Microwave Anisotropy Probe
[1]
1818What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Test for model universeTest for model universe
Angular spectrumAngular spectrum
6000
5000
4000
3000
2000
1000
0
Tem
per
atur
e F
luct
uatio
ns
[µ
K2]
Multipole moment l10 100 500 1000
Angular Size2° 0,5° 0,2°90°
closedflat
open
[1]
1919What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Age: 13.73 Age: 13.73 ± 0.12± 0.12 billion years billion years Flat curvature (within 1 %)Flat curvature (within 1 %) Baryonic matter only ~ 4.6 %Baryonic matter only ~ 4.6 % Dark matter ~ 23.3 %Dark matter ~ 23.3 % Dark energy ~ 72.1 %Dark energy ~ 72.1 %
WMAP resultsWMAP results
[1]
2020What is the shape of our universe?
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Theory / Topology
CMB data
……
WMAP ResultsWMAP Results
[1]
2121What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
PLANCK launched May 14PLANCK launched May 14thth 2009 2009 Temperature resolution up by factor 3Temperature resolution up by factor 3 Higher angular resolution Higher angular resolution 25 – 1000 GHz receiver25 – 1000 GHz receiver
More information about the oldest structures and their formationMore information about the oldest structures and their formation New physics for “non-baryonic” matterNew physics for “non-baryonic” matter Consistent theory for the beginning of time / spaceConsistent theory for the beginning of time / space New insights if gravitational waves can be detectedNew insights if gravitational waves can be detected
Still to come…Still to come…
2222What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
[1][1] WMAP mission page, WMAP mission page, http://map.gsfc.nasa.govhttp://map.gsfc.nasa.gov
[2][2] http://www.pbs.org/wnet/hawking/universes/html/univ.htmlhttp://www.pbs.org/wnet/hawking/universes/html/univ.html
[3][3] Free online enzyclopedia, Free online enzyclopedia, http://www.wikipedia.dehttp://www.wikipedia.de
[4] Andreas Müller – Astrophysik, [4] Andreas Müller – Astrophysik, http://www.wissenschaft-online.de/astrowissen/http://www.wissenschaft-online.de/astrowissen/
[5] Kurze Einführung in die Kosmologie,[5] Kurze Einführung in die Kosmologie,
http://www.astro.uni-bonn.de/~peter/cosmo_short.pdf http://www.astro.uni-bonn.de/~peter/cosmo_short.pdf
[6] Collected papers of Albert Einstein[6] Collected papers of Albert Einstein
http://www.ffn.ub.es/luisnavarro/nuevo_maletin/Einstein_GRelativity_1916.pdfhttp://www.ffn.ub.es/luisnavarro/nuevo_maletin/Einstein_GRelativity_1916.pdf
ReferencesReferences
2323What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
Thank you for your attention!Thank you for your attention!
2424What is the shape of our universe?
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Historic views
Theory / Topology
CMB data
[1]