Imaging in Space and Time 28/8-1/9 2006 Brijuni The Shape of Space: from Black Holes to the Universe J.-P.Luminet Observatoire de Paris (LUTH) 4 levels of geometry Cosmic topology Cosmology Black holes ? Quantum gravity General Relativity Gij = k Tij geometry = matter-energy ds2 = gij dxixj spacetime metric gravity = spacetime curvature Einstein ring Gravitational lensing If M* > 30 MS BLACK HOLE ! Imaging Black Holes Newtonian spacetime curved spacetime Image of a spherical black hole with thin accretion disk (J.-P. Luminet, 1979) Flight into a black hole (J.A.Marck, 1993) Black hole in front of Milky Way (Riazuelo, 2006) Capella Castor & Pollux Aldebaran Orion Sirius Black hole in front of Constellations Capella 1 Imaging spacetime : light cones Aldebaran 2 Orion 2 Capella 2 Orion 1 Aldebaran 1 Einstein ring Southern Cross Canopus a & b Cen Achernar Black hole in front of Magellanic Clouds Southern Cross 1 Canopus 1 Achernar 2 a & b Cen 2 Southern Cross 2 Canopus 2 Einstein ring Achernar 1 See movie 1 Black hole in front of Magellanic Clouds Imaging spacetime : light cones Curved spacetime Flat (Minskowski) spacetime Gravitational collapse to a Schwarzschild black hole metric: 2GM 2 dr2 2 2 2 2 ds (1 )dt r (d sin d ) 2GM rc 2 1 rc 2 2 Schwarzschild radius: r 2GM rc 2 Event horizon Embedding Step 1: Schwarzschild metric outside mass M (G=c=1) : 2M(r) 2 dr2 ds (1 )dt r 2 (d 2 sin2 d 2 ) 2M(r) r 1 r 2 Step 2: Step 3: Equatorial section /2 Time section t const in 3D Embedding Euclidian space Curved 2-geometry: dr2 ds r 2 d 2 2M(r) 1 r 2 ds2 dz2 dr2 r 2 d 2 Result for ordinary star (R* > 2M) z(r) 8M(r 2M) for r R* Outer solution (asymptotically flat) z(r) 8M(r)(r 2M(r)) for r R* Inner solution (regular) Result for black hole z(r) 8M(r 2M) for r 2M Outer solution only (Flamm paraboloid) Spherical black hole in Kruskal coordinates (r,t) (u,v) coth(t /4 M) if r 2M r v u2 v 2 ( 1)exp(r /2M) ; 1 ifr 2M 2M u th(t /4 M) if r 2M v u Flight into a static black hole Radial photons (A.Riazuelo, 2006) What is seen in C See movie 1 What is seen in E Flight into a static black hole 2 Non-radial photons What is seen in C What is seen in E See movie 2 What is seen further Flight into a Kerr (rotating) black hole no movie yet! Cosmology finite (no edge) Homogeneity => constant space curvature ! espace sphérique espace Euclidien espace hyperbolique finite or infinite finite or infinite Space-time curvature ==> a dynamical universe ! Expansion Big bang models open closed What is the size and shape of space ? G Horizon G T Horizon G Assumption Not testable 1 (only L >> Universe is Rinfinite h) G if L >~ Universe is Rfinite h (without boundary) but greater than the observable one G G T G Assumption 2 • May be testable G Horizon T Infini G G G Assumption 3 Testable Universe is finite (without boundary) and smaller than the observable one • topological lensing Think finite space without edge Sphere = 2D Surface finite area, no edge Lignes droites Hypersphere = 3D space finite volume, no edge A finite flat space without a boundary • Torus QuickTime™ et un décompresseur codec YUV420 sont requis pour visionner cette image. Topological lens effect horizon Hypertorus Physical Space Observed Space Cosmic Microwave Background The universe as a cosmic « drumhead » Cosmic Microwave Background Observed on a 2-sphere T l us a Ylm lm m Spherical harmonics 1 Cl 2l 1 l a 2 lm l Multipole moments The CMB multipoles Quadrupole Power spectrum Tl2 = l(l+1)Cl/2 Doppler peaks (Boomerang, Archeops, etc.) l=180°/ Large scales (COBE, WMAP) WMAP power spectrum (2003- 2006) • Universe seems to be positively curved W = 1.02 ± 0.02 flat infinite universe • Lack of power at large scales (> 60°) Space might be finite with a special shape! Poincaré Dodecahedral Space FP : 12 faces regular dodecahedron S3/I* 120 copies tessellate S3 Poincaré Dodecahedral Spherical space (PDS) • fit low quadrupole • fit low octopole • < Wtot < 1.02 Luminet et al., Nature 425, 593 (2003) Planck Surveyor (2007) The « football Universe » 36° Also compatible … Octahedral space Tetrahedral space (Wtot > 1.015) (Wtot > 1.025) J. Weeks, 2006 Imaging Quantum Gravity Quantum foam (J. Wheeler) Solution 1 : string theory Veneziano, Green, Schwarz, Witten, etc. Price to pay : extra-dimensions Closed string Open string bulk Solution 2 : loop quantum gravity Ashtekhar, Smolin, Rovelli, Bojowald Atoms of space: 10-99 cm3 Spin network Knot theory Atoms of time : 10-43 sec Spin foam If God had consulted me before embarking upon Creation, I should have recommended something simpler. Alfonso X, King of Castile