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Dark Energy and the Homogeneous Universe. 暗能量及宇宙整體之膨脹. Lam Hui Columbia University. 許林. This is a series of 3 talks. Today: Dark energy and the homogeneous universe July 11: Dark matter and the large scale

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dark energy and the homogeneous universe
Dark Energy and the Homogeneous Universe

暗能量及宇宙整體之膨脹

  • Lam Hui
  • Columbia University

許林

slide2
This is a series of 3 talks.

Today: Dark energy and the homogeneous

universe

July 11: Dark matter and the large scale

structure of the universe

July 18: Inflation and the early universe

slide3
Outline

Basic concepts: a homogeneous,

isotropic and expanding universe.

Measurements: how do we measure

the universe’s expansion history?

Dynamics: what determines the

expansion rate?

Dark energy: a surprising recent finding.

slide4
There is by now much evidence for homogeneity and isotropy.

There is also firm evidence for an expanding universe.

slide10
There is by now much evidence for homogeneity and isotropy. There is also firm evidence for an expanding universe.
slide11
There is by now much evidence for homogeneity and isotropy. There is also firm evidence for an expanding universe.

But how should we think about it?

slide13
Frequently Asked Questions:

1. What is the universe expanding into?

2. Where is the center of expansion?

3. Is our galaxy itself expanding?

slide14
Frequently Asked Questions:

1. What is the universe expanding into?

Nothing.

2. Where is the center of expansion?

Everywhere and nowhere.

3. Is our galaxy itself expanding?

No.

slide15
C

C

A

B

A

B

Therefore:

Hubble law: Velocity

Distance

slide19
Age of Universe

Slope = Distance/Velocity = 10 billion years

slide20
Dynamics: what determines the expansion rate and how it changes with time?

R

Secondary school physics:

slide22
Important equation:

Example 1 - ordinary matter

Example 2 - cosmological constant

Acceleration!

Dark Energy:

slide24
Wood-Vasey et al. 07

70% dark energy, 30% matter

slide26
What is dark energy?

1. Vacuum energy

(Einstein’s cosmological constant)

2. Scalar field (Bose Einstein condensate)

3. Modified gravity (Einstein was wrong!)

slide27
What is dark energy?

1. Vacuum energy

(Einstein’s cosmological constant)

Observed value too small.

2. Scalar field (Bose Einstein condensate)

Required mass too small.

3. Modified gravity (Einstein was wrong!)

No compelling theory.

slide30
Wang, LH, May & Haiman 07

See also Li & Chu, Li, Chan & Chu 06

slide31
Summary

- Basic concepts of a homogeneous,

isotropic and expanding universe.

- Surprisingly, our current expansion

appears to be accelerating. Explaining

it, and measuring it precisely, is a major

goal of cosmology today.

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