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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

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 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 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

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

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

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Probing the curvature and dark energy

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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

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NY Times current event in Physics.

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