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COSMOLOGY Eduard Massó UAB/IFAE International Meeting of Fundamental Physics (“Winter” meeting) Santiago de Compostela, 2007

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COSMOLOGY. International Meeting of Fundamental Physics (“Winter” meeting) Santiago de Compostela, 2007. Eduard Mas só UAB/IFAE. Program. The standard cosmological model The observed universe Inflation. Neutrinos in cosmology. Emphasis on “Particles”. Science, vol. 315, 2007. - PowerPoint PPT Presentation

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Page 1: COSMOLOGY

COSMOLOGY

Eduard MassóUAB/IFAE

International Meeting of Fundamental Physics(“Winter” meeting)Santiago de Compostela, 2007

Page 2: COSMOLOGY

Program

1. The standard cosmological model

2. The observed universe

3. Inflation. Neutrinos in cosmology

Emphasis on “Particles”

Page 3: COSMOLOGY

Science, vol. 315, 2007

Page 4: COSMOLOGY

Our universe is expanding

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redshift

co-movingdistancescale

lights-yearsago

today

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Co-moving co-ordinates

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On top: peculiar (real) velocities

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Hubble’s law & Cosmological principle

Universe homogenous & isotropicon large scales

Cosmological principle

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Hubble’s discoveryQuickTime™ and aPNG decompressor

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Hubble’s law: QuickTime™ and aPNG decompressor

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(today)

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Expansion (or contraction) is inevitable

RG + CP

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Robertson-Walker metric(homogeneity & isotropy)

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Parameters:

Parametersare relatedby eqs.

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Cosmological equations

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Friedmann eqs.

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1

2a

1+2a -> 2b

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Spatial geometry &Light propagationQuickTime™ and aPNG decompressor

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OpenFLAT Closed

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3D

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Spatial geometry &Light propagationQuickTime™ and aPNG decompressor

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Luminosity distanceQuickTime™ and aPNG decompressor

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Measured flux(E/time/area)

Absolute luminosityE/time in rest frame

Luminosity distance

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Hubble’s law

Exact:

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That was kinematics

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Cosmological constant contribution

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Negativepressure

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+ any other component

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Solution to cosmological eqs.

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Equation of state

Assume i - dominance and

RD universe

MD universe.

CCD universe

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Critical density

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Define also

(Today)

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Not energy-density contribution

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Rewriting Friedmann eqs.QuickTime™ and aPNG decompressor

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Cosmic sum rule

2a today

Notice signs

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The future QuickTime™ and aPNG decompressorare needed to see this picture.

+ Initial conditions taken today

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Diff. eq.

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Eternal Expansion OR Recollapse ?

EE

R

EE

R

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1

2

3

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Distance - RedshiftQuickTime™ and a

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Co-moving distance to source:

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Where:

Can neglect QuickTime™ and aPhoto - JPEG decompressorare needed to see this picture.QuickTime™ and a

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Distance-redshift relation is function of

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Age of the universe

look-back time

lifetime

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Our univ.QuickTime™ and aPNG decompressor

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(Age crisis: Open universe gave too low lifetime)

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Which universe ?

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The past universe

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today

rad

mat

cc

equality

recombination

nucleosynthesis

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next

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The hot universe

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number density

energy density

pressure

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distribution

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g= deg. of freedom

Equilibrium thermodynamics

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Decoupling of speciesExpansion:

Interaction:

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rates

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Phase transitionsSymmetry restoring

2n order

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1st order

Phase transitions

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Conformal timeQuickTime™ and aPNG decompressorare needed to see this picture.

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Particle HorizonIt is the physical distance photons can travel until a time t Defines causal distance at a given time t

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Page 28: COSMOLOGY

Program

1. The standard cosmological model

2. The observed universe

3. Inflation. Neutrinos in cosmology