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The top documents tagged [dark energy slide]
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dark energy slide
Distance Ladder. Pre-class Problem You stand are looking at “famous local landmark” from two positions on either side of the “other famous local place”.
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Observed Features of the Universe Universe is homogeneous and isotropic on lengths > 100 Mpc Universe expanding uniformly ordinary matter is more abundant.
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1 Dark Energy and How to Find It: The SNAP Experiment Stuart Mufson IU Astronomy June 2007.
213 views
Entropic Gravity SISSA, Statistical Physics JC Friday 28, 2011 E. Verlinde, arXiv: 1003.4464v2 [hep-th]
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Seven sisters 20051 How I Stopped Worrying and Learned to Love the Universe Marilena LoVerde Columbia University Hubble Deep Field, NASA.
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DISCOVERING A NEW UNIVERSE AT THE SMALLEST SCALES Jonathan Feng University of California, Irvine Osher Lifelong Learning Institute at UCI 29 February 2008.
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production in p+p and Au+Au collisions at 200 GeV in STAR Rosi Reed UC Davis.
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Cosmology. Observational evidence? “Cosmologists are often in error but never in doubt.” L.D. Landau.
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2 June 05Feng 1 DARK MATTERS Jonathan Feng University of California, Irvine 2 June 2005 UCSC Colloquium Graphic: N. Graf.
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Cosmic Acceleration 1)The evidence 2)What it could be 3)Why each options is interesting/confusing 4)Planning the next steps.
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Original Picture : Sora GWADW2010 (May 20, 2010, Kyoto, Japan) On behalf of DECIGO working group Masaki Ando (Department of Physics, Kyoto University)
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DARK MATTERS Jonathan Feng University of California, Irvine Physics Department Colloquium University of Chicago 2 December 2004.
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