Current and Future Constraints on Models of Cosmic Acceleration
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Current and Future Constraints on Models of Cosmic Acceleration Jochen Weller Universitäts-Sternwarte München – LMU Excellence Cluster for “Origin and Structure of the Universe” Max-Planck Institute for Extraterrestrial Physics 1 9th Vienna Central European Seminar on Particle Physics and Quantumn Field Theory
Current and Future Constraints on Models of Cosmic Acceleration
Current and Future Constraints on Models of Cosmic Acceleration. Jochen Weller Universitäts-Sternwarte München – LMU Excellence Cluster for “Origin and Structure of the Universe” Max-Planck Institute for Extraterrestrial Physics. The Cosmic Pie. Baryons. Dark Matter. Dark Energy. - PowerPoint PPT Presentation
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Current and Future Constraints on Models of Cosmic
Acceleration
Current and Future Constraints on Models of Cosmic
AccelerationJochen WellerUniversitts-Sternwarte Mnchen
LMUExcellence Cluster for Origin and Structure of the
UniverseMax-Planck Institute for Extraterrestrial Physics19th
Vienna Central European Seminar on Particle Physics and Quantumn
Field TheoryThe Cosmic Pie
Dark Energy
Dark Matter
Baryons29th Vienna Central European Seminar on Particle Physics
and Quantumn Field TheoryThe Hubble Diagram with Type Ia
Supernovae9th Vienna Central European Seminar on Particle Physics
and Quantumn Field Theory3Physics Nobel Prize 2011Probe Studium -
September 20124
Saul PerlmutterBrian P. SchmidtAdam G. RiessThe Nobel Prize in
Physics 2011 was divided, one half awarded to Saul Perlmutter, the
other half jointly to Brian P. Schmidt and Adam G. Riess "for the
discovery of the accelerating expansion of the Universe through
observations of distant supernovae".Consequences of SNe
Observationfor Friedman-Robertson-Walker metric (homogenous and
isotropic) + data: > 0accelerated expansionfrom Einstein
equations: ~ -(+3p)need: p
