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he Cosmological Constan he Cosmological Constant Inflation, Inflation, and and Dark Energy Dark Energy * * John D. Barrow John D. Barrow

T he Cosmological Constant, Inflation, and Dark Energy * John D. Barrow

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T he Cosmological Constant, Inflation, and Dark Energy * John D. Barrow. T = 2.7255  0.0006 K. Y(He-4)= 4  He/H = 0.2534  0.0083 D/H = 2.87  0.22  10 -5. New Physics?. N eff = 3.046 is standard 3 light neutrino standard model. - PowerPoint PPT Presentation

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Page 1: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

The Cosmological Constant,The Cosmological Constant, Inflation,Inflation,

andandDark EnergyDark Energy

**John D. BarrowJohn D. Barrow

Page 2: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 3: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

T = 2.7255 T = 2.7255 0.0006 K 0.0006 K

Page 4: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 5: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 6: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Y(He-4)= 4Y(He-4)= 4He/H = 0.2534 He/H = 0.2534 0.0083 0.0083

D/H = 2.87 D/H = 2.87 0.22 0.22 10 10-5-5

Page 7: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 8: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Neff = 3.046 is standard 3 light neutrino standard model

New Physics?New Physics?

Page 9: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Habitable UniversesHabitable UniversesNeedNeed

Close to critical expansionClose to critical expansionIsotropic expansionIsotropic expansion

Graininess level of aboutGraininess level of about 1 part in 10 1 part in 1055

Page 10: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

InflationInflation

Early-time inflation at t Early-time inflation at t 10 10-35-35 s s

Page 11: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Acceleration requires Acceleration requires + 3p/c + 3p/c22 <0 <0

Page 12: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

1992 2003 2013

Page 13: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Planck Mission Microwave Sky MapPlanck Mission Microwave Sky Map

Page 14: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

The Spectrum of Temperature FluctuationsThe Spectrum of Temperature Fluctuations

Page 15: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Scalar Fields and LambdaScalar Fields and Lambda

Pressure: Pressure: p = ½(dp = ½(d/dt)/dt)22 – V( – V() = KE - PE) = KE - PE

Energy density: Energy density: = ½(d = ½(d/dt)/dt)22 + V( + V() = KE + PE) = KE + PE

--cc22 ≤ p ≤ + ≤ p ≤ +cc22

dd22a/dta/dt22 = - 4 = - 4G(G( + 3p/c + 3p/c22)a/3 > 0 )a/3 > 0

+ 3p/c+ 3p/c22 < 0 < 0 Necessary for inflationNecessary for inflation

But kills the singularity theoremsBut kills the singularity theorems

V

dd/dt=0/dt=0 p =-p =-

Page 16: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Pressure: Pressure: p = ½(dp = ½(d/dt)/dt)22 – V( – V() = KE - PE) = KE - PE

Energy density: Energy density: = ½(d = ½(d/dt)/dt)22 + V( + V() = KE + PE) = KE + PE

Eg with non-constant VEg with non-constant V

Page 17: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

ns = -3(V’/V)2 + 2(V’’/V) O(1/N) O(1/50)

dns /dln(k) = 2[4(V’/V)2 (V’’/V) – 3(V’/V)4 –V’V’’’/V2] O(1/N2,1/N3)

Gravitational Potential perts 1/(size)ns kns

Page 18: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 19: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 20: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 21: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Our Universe can have a beginningOur Universe can have a beginningButBut

The Multiverse need have no beginningThe Multiverse need have no beginning

Page 22: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 23: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Was there a beginning?

Eternal cycles Eternal changeBeginning

of timeBeginning

in time

no end In thefuture

will end In thefuture

Creation out of nothing

Creationout of

something

order chaos

order is transient

order ispermanent

no yes

Page 24: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 25: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow
Page 26: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Infinities in PhysicsInfinities in Physics

Are they always saying Are they always saying

“must try harder”“must try harder”

??

Page 27: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

We don’t have any trustworthy theory of what happened at t < 10We don’t have any trustworthy theory of what happened at t < 10-43-43ss

Page 28: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Late-time AccelerationLate-time Acceleration

Page 29: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

Why isn’tWhy isn’t 1010+66+66 cm cm-2-2

We observeWe observeobsobs 10 10-55-55 cm cm-2-2

????????No galaxies if > 10 > 10-54-54 cm cm-2-2

A Big Mystery

Page 30: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

1 = 1 = MM + + kk + + wherewhere

MM = = 88GG/3H/3H22

k k == – k/a – k/a22HH22

= = /3H/3H22

HH22 =8 =8GG/3 – k/a/3 – k/a22 + + /3/3

The Return of The Return of Lambda ?Lambda ?

Page 31: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow

W p/ = wo + wa(1 – a) assumed for an evolving dark energy

Simple cosmological constant model iswo = -1 and wa = 0

Or is dark energy a time-changing version of lambda?Or is dark energy a time-changing version of lambda?

Page 32: T he  Cosmological Constant,  Inflation, and Dark Energy * John D. Barrow