Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe

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    L1: The Cosmic Microwave Background& the Thermal History of the Universe

    Dick Bond

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    Inflation fluctuationsform: quantum jitter

    Helium forms

    Cosmic backgroundradiation released frommattercarries imprint of

    fluctuations in matter whichgrow to generate galaxies etc.

    NOWPythagoras formed

    Carbon/oxygen/etc

    form

    Galaxies form

    IT from BIT

    Solar system

    earth form

    The Meaning may changeBut the facts will remain

    14 Gyr 1

    9 Gyr 1.4

    2 Gyr 4

    100 sec 109

    0.4 Myr 1100

    10-37sec1029

    Galaxies ClusterCosmic web of

    vast filaments +

    membranes

    Life forms onearth

    Protons/Neutronsform

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    Inflation fluctuationsform: quantum jitter

    Helium forms

    Cosmic backgroundradiation released frommattercarries imprint of

    fluctuations in matter whichgrow to generate galaxies etc.

    NOWPythagoras formed

    Carbon/oxygen/etc

    form

    Galaxies form

    IT from BIT

    Solar system

    earth form

    The Meaning may changeBut the facts will remain

    14 Gyr 1

    9 Gyr 1.4

    2 Gyr 4

    100 sec 109

    0.4 Myr 1100

    10-37sec1029

    Galaxies ClusterCosmic web of

    vast filaments +

    membranes

    Life forms onearth

    Protons/Neutronsform

    fate & dark energyfate & dark energy

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    EGYPT TIMES Mar 31 2006

    Canadians make it easy to say sorry

    Legislation to allow Canadians to admit mistakes

    without litigation

    EGYPT TIMES Mar 31 2006

    Canadians make it easy to say sorry

    Legislation to allow Canadians to admit mistakes

    without litigation

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    CMB/LSS PhenomenologyCITA/CIAR here

    Bond

    Contaldi

    Lewis

    Sievers

    Pen

    McDonald

    Majumdar

    Nolta

    Iliev Kofman

    Vaudrevange

    Shirokov

    El Zant

    UofT here

    Netterfield

    MacTavish

    Carlberg

    Yee

    & Exptal/Analysis/Phenomenology

    Teams here & there

    Boomerang03

    Cosmic Background Imager

    Acbar

    WMAP (Nolta, Dore)

    CFHTLS WeakLens

    CFHTLS - Supernovae

    R S2 R S1 Virmos

    CITA/CIAR there

    Mivelle-Deschenes (IAS) Pogosyan (U of Alberta)

    Prunet (IAP)

    Myers (NRAO)

    Holder (McGill)

    Hoekstra (UVictoria)

    van Waerbeke (UBC)

    Parameter datasets: CMBall_pol

    SDSS P(k), 2dF P(k)Weak lens (Virmos/RCS1;

    CFHTLS, RCS2)

    Lya forest (SDSS)

    SN1a gold (157, 9 z>1), CFHT

    futures: SZ/opt, 21(1+z)cm

    Dalal Dore

    Kesden

    MacTavish

    Pfrommer

    Dalal

    Dore

    Kesden

    MacTavish

    Pfrommer

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    Boomerang@150GHz is

    (nearly)Gaussian:Simulated

    vsReal

    Boomerang@150GHz is

    (nearly)Gaussian:SimulatedvsReal

    thermodynamic

    CMB

    temperature

    fluctuations2.9% of sky

    ~ 30 ppm

    thermodynamic

    CMB

    temperature

    fluctuations

    2.9% of sky

    ~ 30 ppm

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    Sorry CITAzens: real seems to be simulated

    Boomerang, Cosmic Background Imager, WMAP3,

    No wonder the LCDM concordance model looks so

    good

    Sorry CITAzens: real seems to be simulated

    Boomerang, Cosmic Background Imager, WMAP3,

    No wonder the LCDM concordance model looks so

    good

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    Real is a mock: march 29, 2006

    a BLACK DAY for some CITAzens

    Real is a mock: march 29, 2006

    a BLACK DAY for some CITAzens

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    new deeply embedded analysis march 31, 2006

    The wrinkled lightcone may not be LCDM

    but a statistically anisotropic but well-known shape

    new deeply embedded analysis march 31, 2006

    The wrinkled lightcone may not be LCDM

    but a statistically anisotropic but well-known shape

    i i i f

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    The anisotropic lightcone led to a new model for the

    power defining the current universe

    The anisotropic lightcone led to a new model for the

    power defining the current universe

    Acknowledgment:

    realization

    Occurred at Khufus

    place in Giza, the

    chamber in the centreof the great pyramid

    March 31, 2006

    Acknowledgment:

    realizationOccurred at Khufus

    place in Giza, the

    chamber in the centreof the great pyramid

    March 31, 2006

    Pyramid powerPyramid power

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    But new realization now I am on Egyptian time and

    APRIL FOOLs ends at noon April 1

    real is in fact real, for

    Boomerang, Cosmic Background Imager, WMAP3,

    the LCDM concordance model does indeed look good

    & the structure of the universe seems to beunderstandable in terms of a handful of basic

    cosmological parameters,

    Baryon, dark matter, dark energy densities

    Power spectra for primordial fluctuations

    But new realization now I am on Egyptian time and

    APRIL FOOLs ends at noon April 1real is in fact real, for

    Boomerang, Cosmic Background Imager, WMAP3,

    the LCDM concordance model does indeed look good

    & the structure of the universe seems to beunderstandable in terms of a handful of basic

    cosmological parameters,

    Baryon, dark matter, dark energy densities

    Power spectra for primordial fluctuations

    Th Parameters of Cosmic Structure Formation

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    The Parameters of Cosmic Structure FormationThe Parameters of Cosmic Structure Formation

    WMAP3 WMAP3+CBIcombinedTT+CBIpol

    CMBall = Boom03pol+DASIpol +VSA+Maxima+WMAP3+CBIcombinedTT+CBIpol

    bh2 = .0222 +- .0007ch2 = .107 +- .007 = .75 +- .03

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    Parameters of Cosmic Structure Formation

    k

    What is the Background

    curvature of the universe?

    k > 0k = 0

    k < 0

    closed

    flat

    open

    bh2 nsdmh

    2

    Density of

    Baryonic MatterDensity of non-

    interacting Dark

    Matter

    Cosmological

    Constant

    Spectral index of

    primordial scalar

    (compressional)perturbations

    P(k)

    k

    ns1

    nt

    Spectral index of

    primordial tensor

    (Gravity Waves)perturbations

    Ph(k

    ) k

    nt

    As 8

    Scalar Amplitude

    At

    Tensor Amplitude

    Period of inflationary expansion,

    quantum noise metric perturb.

    Inflationpredicts nearly scale invariant scalar perturbations

    and background of gravitational waves

    Passive/adiabatic/coherent/gaussian perturbations

    Nice linear regime

    Boltzman equation + Einstein equations to describe the LSS

    c

    Optical Depth to

    Last Scattering

    SurfaceWhen did stars

    reionize the

    universe?

    P t f C i St t F tiThe Parameters of Cosmic Structure Formation

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    The Parameters of Cosmic Structure FormationThe Parameters of Cosmic Structure Formation

    WMAP3 WMAP3+CBIcombinedTT+CBIpol

    CMBall = Boom03pol+DASIpol +VSA+Maxima+WMAP3+CBIcombinedTT+CBIpol

    bh2 = .0222 +- .0007ch2 = .107 +- .007 = .75 +- .03

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    Cosmic topologyCosmic topology

    Multiply connected universe ?Multiply connected universe ?

    Simple Torus

    (Euclidean)

    Compact hyperbolicspace

    MC spherical space

    (soccer ball)

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    WMAP3 thermodynamic CMB temperature fluctuationsWMAP3 thermodynamic CMB temperature fluctuations

    Co(s)mic Topology

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    No?

    Co(s)mic Topology

    Non april fool

    Is the universe like a

    soccer ball?

    The CMB data

    decides:

    Non april fool

    Is the universe like a

    soccer ball?

    The CMB data

    decides:

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    COBE satellite 1989-1994

    Picked up as TV snow a few %

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    Hot

    BigBang

    Picked up as TV snow - a few %

    2.725 .001 degrees above absolute zero

    410 photons per cubic centimetre

    Isotropic (smooth) to one part in 100,000

    released as redlight 400,000

    yrs after theBig Bang,expansion of

    spacestretched thewavelengths

    to microwave

    Perfect

    Planck

    Curve

    (almost)

    Di f th Mi

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    Discovery of the Microwave

    Background Discovered accidentally as a source of noise in aradio receiver

    1965 Bell Telephone Laboratories Penzias and Wilson share Nobel prize in 1978

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    Planck distribution function

    f = 1/(exp[q/(aT)] -1)

    Planck distribution function

    f = 1/(exp[q/(aT)] -1)

    d Number of photons = f d Phase Space Volume

    = f 2 d3q/(2)3 d3xd Number of photons = f d Phase Space Volume

    = f 2 d3q/(2)3 d3x

    Thermodynamic temperature T(q) from f(q)Thermodynamic temperature T(q) from f(q)

    Sources, sinks, scattering processesSources, sinks, scattering processesTime derivative along thephoton direction

    d E/V = f q3 /2 dq Planck energy curved E/V = f q3 /2 dq Planck energy curve

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    when was the entropy generated in the U?when was the entropy generated in the U?

    dE + p dV = T dS ( - d N )dE + p dV = T dS ( - d N )

    (when was the baryon number generated? dB=0 after)(when was the baryon number generated? dB=0 after)

    Answer: earlier than redshift z ~ 106.8Answer: earlier than redshift z ~ 106.8

    or distortions in the CMB spectrumor distortions in the CMB spectrum

    s*/nb* =0.65 x 1010 (.02/bh2)[1+(7/8)(4/11)N x 1.04] total entropys*/nb* =0.65 x 1010 (.02/bh2)[1+(7/8)(4/11)N x 1.04] total entropy

    cf. entropy per baryon in the centre of the sun ~19

    In a pre-supernova core about to implode ~1

    n*

    = 410/cc,

    * = 0.26 ev/cc1+(7/8)(4/11)N4/3 x

    1.04]

    total energy

    *h2 =2.45x10-5Lev Kofman lecturesLev Kofman lectures

    Thermodynamic temperature T(q)Thermodynamic temperature T(q)

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    Thermodynamic temperature T(q)e ody c e pe u e (q)

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    Sources, sinks, scattering processesSources, sinks, scattering processesTime derivative along the

    photon direction

    the Boltzmann transport equation for photonsthe Boltzmann transport equation for photons

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    Z ~ 1100, z~100,t~400000 yr, lightcrossing 300 Mpc

    Distortions inenergy

    < .0001 (Comptoncooling ofelectrons)

    Starlight+

    (EBL): .06-.12

    (>400 microns) ~.001

    Planck dist fnPlanck dist fn

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    Planck dist fn

    max entropy

    for fixed

    energy

    max entropy

    for fixedenergy

    Bose-Einsteindist fn

    max entropyfor fixed

    energy and

    number

    Bose-Einsteindist fn

    max entropy

    for fixed

    energy and

    numberz >~

    10

    5.4

    (.02/bh2)1/2z >~

    105.4

    (.02/bh2)1/2but