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That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

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Page 1: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

That other pesky 95%Dark Energy and Dark Matter

Prof. Lawrence WienckeDepartment of Physics EngineeringColorado School of MinesNov 9 2011

Page 2: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

The Dark SideThe Dark Side

95% of theUniverse Is Dark!

Page 3: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011
Page 4: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011
Page 5: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011
Page 6: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Energy budget of Universe

• Stars and galaxies are only ~0.5%• Neutrinos are <1%• Rest of ordinary matter (electrons and protons) are ~5%• Dark Matter ~25%• Dark Energy ~70%• Anti-Matter 0%

Page 7: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

THE HIGGS!?#

No Dark MatterNo Dark Energy

Page 8: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

M81Spitzer Space Telescope

Page 9: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

105

100

50

Expected if the mass of the galaxy = the mass we can see

Observed

Some sort of invisible Mass must extend out ~10 times further than the stars!

Ro

tati

on

sp

eed

Distance from the center

Vera Rubin 1980s

Page 10: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Full Court Press!!Produce at an acceleratorDetect them in our haloDetect annihilation products

Page 11: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Dark Matter annihilating in our halo should produce positrons,

neutrinos and gamma rays

Page 12: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Evidence for Dark Matter from Lensing

Einstein: Gravity bends light

Light travels along straight lines unless it passes a massive object.

Light coming from behind a massive object such as a star, a galaxy, a cluster of galaxies or a clump of dark matter will be bent the same way a glass lens works.

The more massive the object, the more gravity it has and the more the light is bent

Page 13: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

giant arcs are galaxies behind the cluster, gravitationally lensed

Zoom in on a galaxy cluster – Gravity from the invisible matter is bending light and we can see the distorted images that result

Page 14: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Michael S Turner

Discovery of Cosmic Microwave Background, 1964

Page 15: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Michael S Turner

The Universe circa 380,000 yrsWMAP

±0.001% Fluctuations

Page 16: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

fraction of a second later

Hot Primordial Soup

380,000 years later

Radiation Last Scattered

13.78 thousand-million years later

Today

DARK MATTERfrom the

Primordial Soup

DARK MATTERfrom the

Primordial Soup

Page 17: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Most of the matter is dark

and

it’s not even “normal” stuff!

Tip of the IcebergTip of the Iceberg

Page 18: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

STRING THEORY - 11 dimensions and more …..

Go to 11???

Page 19: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

19

What is Dark Energy ?What is Dark Energy ?

“ ‘Most embarrassing observation in physics’ – that’s the only quick thing I can say about dark energy that’s also true.”

Edward Witten

Page 20: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Discovery! – 1998

Hi z Supernova TeamSupernova Cosmology Project

Brian P. SchmidtSaul Perlmutter

Adam G. Riess

Nobel Prize in Physics 2011

Page 21: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011
Page 22: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Inquiring into Dark Energy

22

NSTA - Baltimore 2006

A dying star becomes a white dwarf.

1. Create a White Dwarf

Page 23: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Inquiring into Dark Energy

23

NSTA - Baltimore 2006

The white dwarf strips gas from its stellar companion….

2. Dump more mass onto it

Page 24: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Inquiring into Dark Energy

24

NSTA - Baltimore 2006

….and uses it to become a hydrogen bomb. Bang!

3. Until it explodes

Page 25: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Inquiring into Dark Energy

25

NSTA - Baltimore 2006

The explosion is as bright as an entire galaxy of stars….…..and can be seen in galaxies across the universe.

4. Observe it in a distant galaxy

Page 26: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

The Sloan Digital Sky Survey (SDSS) is a telescope Fermilab helped build and operate.

It has a 2.4m mirror and no Dome

Located in New Mexico• First started collecting images in 2000•120 MegaPixel digital camera

SDSShas measured ~ 1 million galaxies and over 500 type 1a Supernova and also found that the expansion of the universe is accelerating

Page 27: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

SDSS-II Supernova Survey

~500 Well studied SNe Ia, suitable for framing

Page 28: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

Our Universe’s Expansion is Accelerating!

time

exp

ansi

on open

closed

accelerating

Now

Page 29: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011
Page 30: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

“The most beautiful thing we can experience is the mysterious. It is the source of all true art and all science. Those to whom this emotion is a stranger, who can no longer pause to wonder and stand rapt in awe, are as good as dead: their eyes are closed.”

Albert Einstein

Page 31: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011

95% of theUniverse Is Dark!

What can we learn about it?

Will!!

Page 32: That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov 9 2011