The top documents tagged [dark energy slide]

Astronomy 100 The Beginning and End of the Universe
Documents Astronomy 100 The Beginning and End of the Universe

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EUCLID : From Dark Energy to Earth mass planets and beyond Jean-Philippe Beaulieu Institut dAstrophysique de Paris Dave Bennett University of Notre Dame
Documents EUCLID : From Dark Energy to Earth mass planets and beyond Jean-Philippe Beaulieu Institut dAstrophysique de Paris Dave Bennett University of Notre Dame

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Lecture 2 Temperature anisotropies cont: what we can learn CMB polarisation: what it is and what we can learn
Documents Lecture 2 Temperature anisotropies cont: what we can learn CMB polarisation: what it is and what we can learn

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Cosmological measurements with Supernovae Ia What is a SNIa? Distance and cosmology Observations Standardisation (x1,c) Hubble diagram Spectra: SNfactory
Documents Cosmological measurements with Supernovae Ia What is a SNIa? Distance and cosmology Observations Standardisation (x1,c) Hubble diagram Spectra: SNfactory

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CHALLENGES OF RELATIVISTIC ASTROPHYSICS Reuven Opher (Univ. of Sao Paulo/Cornell. Univ.)
Documents CHALLENGES OF RELATIVISTIC ASTROPHYSICS Reuven Opher (Univ. of Sao Paulo/Cornell. Univ.)

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Dark Matter, Dark Energy, and the Fate of the Universe
Documents Dark Matter, Dark Energy, and the Fate of the Universe

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Dark Energy. Conclusions from Hubble’s Law The universe is expanding Space itself is expanding Galaxies are held together by gravity on “small” distance
Documents Dark Energy. Conclusions from Hubble’s Law The universe is expanding Space itself is expanding Galaxies are held together by gravity on “small” distance

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Formation of the Universe Review. observed change in the frequency of a wave when the source or observer is moving
Documents Formation of the Universe Review. observed change in the frequency of a wave when the source or observer is moving

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Hiromi Suenaga Cody Tamura Period 1. It affects the Universe’s expansion Other than that it is a total mystery Roughly 70 % of the universe is dark
Documents Hiromi Suenaga Cody Tamura Period 1. It affects the Universe’s expansion Other than that it is a total mystery Roughly 70 % of the universe is dark

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WFMOS: a tool for probing dark energy David Parkinson EDEN in Paris, December 2005
Documents WFMOS: a tool for probing dark energy David Parkinson EDEN in Paris, December 2005

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Large Scale Structure in 2MRS & 6dF Ofer Lahav (University College London) 6dF workshop, AAO/Sydney, 26-27 April 2005
Documents Large Scale Structure in 2MRS & 6dF Ofer Lahav (University College London) 6dF workshop, AAO/Sydney, 26-27 April 2005

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Recent Progress on Dark Energy Study Xinmin Zhang IHEP2007-09-07
Documents Recent Progress on Dark Energy Study Xinmin Zhang IHEP2007-09-07

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