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Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE CMB

Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

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Page 1: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max Tegmark

University of Pennsylvania

Max Tegmark

University of Pennsylvania

NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD

DARK MATTER FROM THE CMB

Page 2: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

exp9911

CMB

Page 3: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

pipeline

CMB

Page 4: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

Budget

PARAMETERS OF THE “MINIMAL COSMOLOGICAL STANDARD MODEL”

PhotonsHeliumHydrogenCDMNeutrinosLambdaCurvature

•Matter budget

•Input fluctuationsQ Scalar normalizationn Scalar tilt Running of tiltT/S Tensor normalizationnT Tensor tilt

Extensions:B-fieldsGeneralized dark matter, e.g. quintessence

Extensions:IsocurvatureTopological defects Other non-Gaussian

Extensions:Stochastic biasNon-linear biasScale-dependent biasGalaxy type dependent biasCMB foreground parameters

•Gastrophysics Reionization optical depthb Galaxy bias

Sum: 14 parameters

Redundant parameters (determined by those above):Hubble constant, age of Universe, galaxy normalization 8, etc

Page 5: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

Boom Box

CMB

Page 6: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

ob

CMB

Page 7: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

ob

MOVIE: Baryon 5Starring: Capt. John Sheridan

CMB

Page 8: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

om

CMB

Page 9: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

on

CMB

Page 10: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

n

CMB

Page 11: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

tau

CMB

MOVIE: The tau of physicsStarring: Fritiof Capra

Page 12: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

nt

CMB

Page 13: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

Ok

CMB

Page 14: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

Ol

CMB

Page 15: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

exp9911

CMB

Page 16: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

mega

CMB

Page 17: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 0

CMB

Page 18: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

noclosed

CMB

Page 19: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 1

CMB

Page 20: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 2

CMB

Page 21: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 3

CMB

Page 22: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 5

CMB

Page 23: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 6

CMB

Page 24: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 7

CMB

Page 25: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 8

CMB

Page 26: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

all65 5

CMB

ALL DATA:

Page 27: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

lyman

CMB

COBE + SASKATOON + QMAP + TOCO:

Page 28: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

boom

CMB

COBE + BOOMERANG:

Page 29: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

snake

CMB

COBE + PYTHON V + VIPER:

Page 30: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

All65_nucleo 1d

CMB

Page 31: Max Tegmark University of Pennsylvania Max Tegmark University of Pennsylvania NEW CMB CONSTRAINTS ON THE DENSITIES OF HOT AND COLD DARK MATTER FROM THE

Max TegmarkUniv. of Pennsylvania

[email protected] 2K, Marina del Rey

February 24, 2000

sz

CMB