bob nichol - nobel prize public talk

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The Nobel Prize in Physics 2011 Bob Nichol (ICG Portsmouth) “majority of its surface area is only about 10 feet above sea level”

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Page 1: Bob Nichol - Nobel Prize Public Talk

The Nobel Prize in Physics 2011

Bob Nichol (ICG Portsmouth)

“majority of its surface area is only about 10 feet above sea level”

Page 2: Bob Nichol - Nobel Prize Public Talk

General Relativity Primer

Page 3: Bob Nichol - Nobel Prize Public Talk

Cosmology Primer I   Assumptions

  Cosmological Principle; not special place, time or physics   Homogeneous and isotropic; defines “simple” FRW metric

  Assume GR and FRW metric; solve to get Friedmann’s equations (including Einstein’s Cosmological Constant)

H 2 ≡˙ a a⎛

⎝ ⎜ ⎞

⎠ ⎟

2

=8π3ρ −

kR2 −

Λ3

Page 4: Bob Nichol - Nobel Prize Public Talk

Cosmology Primer II

  Hubble discovered the expansion of the Universe in 1929

  Einstein dropped his cosmological constant

  Next 70 years was the search for two numbers!   “Hubbles’ Constant”   Density of matter

!

"0 #$0$c

=8%G3H0

2 $0

Distance from us

Re

cess

ion

Ve

loci

ty

Ω0 =1 for a flat universe

Page 5: Bob Nichol - Nobel Prize Public Talk

Distances and SNeIa

n

Thermonuclear explosions of White Dwarf stars

White Dwarf accretes mass from or merges with a companion star, growing to a critical mass ~1.4Msun (Chandrasekhar)

A violent explosion is triggered at or near the center, and the star is completely incinerated within seconds. In the core, light elements are burned in fusion reactions to produce ~0.6Msun Nickel. The radioactive decay of Nickel and Cobalt makes it shine for a couple of months

Page 6: Bob Nichol - Nobel Prize Public Talk

Standardizable Candles

A"er  correc(on,  σ~  0.16  mag  (~8%  distance  error)  

Kim et al. 1997

Page 7: Bob Nichol - Nobel Prize Public Talk

Industrial Astronomy

Sciama Building

Only ~1 SNe per ~100 years in our Galaxy

Page 8: Bob Nichol - Nobel Prize Public Talk

SN Hubble Diagram (circa 1999)

Sciama Building

ICG only UK institute in SDSS-III

a=1/(1+z)

W

Ω0 =ΩM +ΩΛ

Ω0 =ΩM +ΩΛ

Page 9: Bob Nichol - Nobel Prize Public Talk
Page 10: Bob Nichol - Nobel Prize Public Talk

Nobel Prize 2011 "for the discovery of the accelerating expansion of the Universe

through observations of distant supernovae"

Page 11: Bob Nichol - Nobel Prize Public Talk

Baryon Acoustic Oscillations

  Initial fluctuation in DM. Sound wave driven out by intense pressure at 0.57c.

Initial fluctuation in DM. Sound wave driven out by intense pressure at 0.57c. Photons free stream, while baryons

remain still as pressure is gone

Today. Baryons and DM in equilibrium. The final configuration is the original peak at the center and an echo (the sound horizon) ~150Mpc in radius

Illustrations by Martin White

Page 12: Bob Nichol - Nobel Prize Public Talk

Standard Rulers in the Sky

WMAP 1st year data

First year WMAP power spectrum

150Mpc

Page 13: Bob Nichol - Nobel Prize Public Talk

Flat Universe

WMAP 1st year data

“Ruler” is 150Mpc and distance to CMB is known to high accuracy (z=1089)

Page 14: Bob Nichol - Nobel Prize Public Talk

Today

Densities known to ~10%

Page 15: Bob Nichol - Nobel Prize Public Talk
Page 16: Bob Nichol - Nobel Prize Public Talk

Energy of Nothingness!

Coincidence problem?

Log[a0/a(t)] €

ρDE ~ a−3(1+w )

wi(z) ≡piρi

Page 17: Bob Nichol - Nobel Prize Public Talk

Cosmological Constant

ρDE ~ a−3(1+w )

(10120 too small)