Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
Transcript of Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
1/35
L1: The Cosmic Microwave Background& the Thermal History of the Universe
Dick Bond
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
2/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
3/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
4/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
5/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
6/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
7/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
8/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
9/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
10/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
11/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
12/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
13/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
14/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
15/35
Cosmic topologyCosmic topology
Multiply connected universe ?Multiply connected universe ?
Simple Torus
(Euclidean)
Compact hyperbolicspace
MC spherical space
(soccer ball)
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
16/35
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
17/35
WMAP3 thermodynamic CMB temperature fluctuationsWMAP3 thermodynamic CMB temperature fluctuations
Co(s)mic Topology
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
18/35
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:
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
19/35
COBE satellite 1989-1994
Picked up as TV snow a few %
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
20/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
21/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
22/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
23/35
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)
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
24/35
Thermodynamic temperature T(q)e ody c e pe u e (q)
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
25/35
Sources, sinks, scattering processesSources, sinks, scattering processesTime derivative along the
photon direction
the Boltzmann transport equation for photonsthe Boltzmann transport equation for photons
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
26/35
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
-
8/3/2019 Dick Bond- The Cosmic Microwave Background & the Thermal History of the Universe
27/35
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