The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at...

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The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at Berkeley and LBNL

Transcript of The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at...

Page 1: The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at Berkeley and LBNL.

The Discovery of Dark Energy

Gerson GoldhaberPhysics Department

University of California at Berkeley

and LBNL

Page 2: The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at Berkeley and LBNL.

Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Calibrated Standard Candles

Page 3: The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at Berkeley and LBNL.

Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Why are all the Type Ia SNe of nearly the same brightness?

• When a star of near Solar Mass uses up all of its Hydrogen and Helium it collapses to a White Dwarf. (W.D.)

• If the White Dwarf has a companion star then, for the right conditions, Mass can be Transferred to the W.D.

• Type Ia SNe are due to the explosion of a W.D. This occurs when it reaches a mass of 1.4 M0 (the Chandrasekhar limit) from Mass Transfer

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Positive Image Dec 28, 1989

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Negative Image Jan 23 1990

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Superimposed images

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Supernova Discovery and Measurement Sequence.

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

The Sky in Chile

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By Chris Smith at Cerro Tololo

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

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The Hubble SpaceTelescope

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Expansion History of the Universe

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Discovery of Dark Energy

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A Supernova explodes and the light reaches us some 9 billion years later. The light started out about 4.5 billion years before our solar system was formed.

Page 14: The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at Berkeley and LBNL.

Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Supernova Light Curve and Spectrum

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

SNe Light Curves from the HST and Images

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Type Ia SNe and the Expansion of the UniverseObservation of Time Dilation negates “Tired Light”

1/(1+z)

1/(1+z)s

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Adjusting for Stretch

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Series of Hubble Curves to allow the Measurement of M

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Hubble Curves

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Sullivan et al. 2003Elliptical Galaxies contain less Dust

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Concordance between SNe, CMB and Clusters

M

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

w vs. M (w =p/)

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

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Riess et al. 2004 SNe from the HST. Acceleration and earlier Deceleration

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

Strong Gravitational Lensing

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

NASA/WMAP Science Team

Precision measurements show Temperature fluctuations

Temperature Map

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Nov. 21, 2005

First SN discovered in a cluster in this search

Cluster RCS0221-03

at z = 1.02

preliminary

Page 32: The Discovery of Dark Energy Gerson Goldhaber Physics Department University of California at Berkeley and LBNL.

Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

SNe discovered in ongoing search

z=0.926

z=1.316

preliminary

preliminary

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Nov. 21, 2005 Gerson Goldhaber, SFSU Colloquium

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