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A theorist’s view of dark energy Andreas Albrecht (UC Davis) UCSC Colloquium Jan 19 2012

A theorist’s view of dark energy Andreas Albrecht (UC Davis) UCSC Colloquium Jan 19 2012. CONCLUSIONS Cosmic acceleration has made life really exciting for the theorist Hardly a closed case. CONCLUSIONS Cosmic acceleration has made life really exciting for the theorist

By nathan

(80 views)

Cosmic Inflation Phy 262 2014 Andreas Albrecht

Cosmic Inflation Phy 262 2014 Andreas Albrecht. Cosmic Inflation: Great phenomenology, but O riginal goal of explaining why the cosmos is *likely* to take the form we observe has proven very difficult to realize. . Cosmic Inflation: Great phenomenology, but

By moriah

(121 views)

Cosmic Inflation Phy 262 2013 Andreas Albrecht

Cosmic Inflation Phy 262 2013 Andreas Albrecht. Cosmic Inflation: Great phenomenology, but O riginal goal of explaining why the cosmos is *likely* to take the form we observe has proven very difficult to realize. . Cosmic Inflation: Great phenomenology, but

By alaire

(143 views)

Inflation, infinity, equilibrium and the observable Universe Andreas Albrecht UC Davis

Inflation, infinity, equilibrium and the observable Universe Andreas Albrecht UC Davis UCD Colloquium October 3, 2011. E. Cosmic Inflation: Great phenomenology, but

By zhen

(110 views)

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Probing the curvature and dark energy

Probing the curvature and dark energy. Gong, Yungui 龚云贵 Chongqing University of Posts and Telecommunications 重庆邮电学院. 2005 International Summer School/Institute on Particle Physics, Astrophysics and Cosmology (Section II) ， August 16, 2005. Dark Energy Introduction

By licia (109 views)

Probing the curvature and dark energy

Probing the curvature and dark energy. Gong, Yungui 龚云贵 Chongqing University of Posts and Telecommunications 重庆邮电学院. “ 宇宙暗物质和暗能量”研讨会， 2005 年 7 月 8 日. Dark Energy Introduction Current Status of Parameterizations One-parameter Parameterization Conclusion. Why Dark Energy?.

By amethyst-whitley (95 views)

Dark Energy

Dark Energy. David Spergel Princeton University. Evidence for cosmic acceleration: Supernovae type Ia. Many Form of Evidence. Jimenez. Stellar Ages ISW Effect Baryon Wiggles Cluster Evolution CMB & Growth of Structure Cluster Properties versus Redshift. ISW Effect.

By gwidon (89 views)

Dark Energy

Dark Energy . L. News on CMB and Structure Formation. f. L. Dark Energy Evidence . f. L. Dark Energy Evidence . f. Spergel et al. 2003. WMAP+ACBAR+CBI+2dF+L . L. Cosmological Constant Problem . G  n = 8 p T mn. f. L. Cosmological Constant Problem . Geometry .

By nituna (145 views)

Dark Energy

Dark Energy. J. Frieman: Overview 30 A. Kim: Supernovae 30 B. Jain: Weak Lensing 30 M. White: Baryon Acoustic Oscillations 30 P5, SLAC, Feb. 22, 2008.

By naeva (176 views)

Dark Energy

Dark Energy. L. News on CMB and Structure Formation. f. L. Dark Energy Evidence. f. L. Dark Energy Evidence. f. Spergel et al. 2003. WMAP+ACBAR+CBI+2dF+L . L. Cosmological Constant Problem. G  n = 8 p T mn. f. L. Cosmological Constant Problem. Geometry.

By irene-wade (121 views)

Dark and dark energy

Dark and dark energy. d. What is it?. Dark energy a mysterious, force that is pulling galaxies apart. It makes up about 70 percent of the universe.

By mliss (131 views)

Dark Energy

Dark Energy. Distance. How far away something is gets complicated at high z How far it is now? How far it was then? How far light travelled? How distant it looks? Let’s call r the distance to an object now It used to be closer, because everything was closer, by factor of a / a 0

By harper (92 views)

Dark Energy

Dark Energy. L. The first Surprise in the era of precision cosmology?. Q. L. Dark Energy Evidence. Low redshift cosmic geometry. Q. L. Dark Energy Evidence. Large Scale Structure. Galaxy distribution favours a low matter Universe; CMB acoustic peak locations indicate a

By herlindan (0 views)

Dark Energy

NY Times current event in Physics.

By msultan (78 views)

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