Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special...
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![Page 1: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/1.jpg)
Anomalies of low multipoles of WMAP and Planck missions: what are they ?
Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences
![Page 2: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/2.jpg)
Wilkinson Microwave Anisotropy Probe (WMAP, NASA)
5 frequencies:23, 33, 41, 61, 94 GHz
Best determination of cosmological parameters in 2011 !
2001-2011
![Page 3: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/3.jpg)
Planck mission, ESA
Low Frequency Instrument: 30,44,70HFI: 100, 143, 217, 353, 545, 857 GHz
Zeldovich-Sunyaev effect
3) Gravitational waves in the B-mode of polarization ?
2010-20131)
2)
![Page 4: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/4.jpg)
Observations
![Page 5: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/5.jpg)
Data analysis of CMB
Registration: time odered data: T(t)=T(l,b) Pixelization: map-making and restoration data in pixels Component separation Multipole analysis Pixel statistics of the CMB map Angular power spectrum analysis and determination of cosmological parameters
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Component separation
![Page 7: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/7.jpg)
WMAP observational bands
![Page 8: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/8.jpg)
Component separation:Signal = (CMB + Synchrotron+dust+FreeFree+radiosouces)*Beam + Noise
![Page 9: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/9.jpg)
Two basic properties of CMB:1) Black body emission — same temperature at all wavelengthes;2) Correlation of CMB and foregrounds should be close to zero: because CMB is a random gaussian process
![Page 10: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/10.jpg)
The maps
WMAP 9, Lmax=150(Hinshaw et al., 2012)
Planck, Lmax=150
Planck collaboration, 2013
Lmax = 150
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Masks
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Angular power spectrum of CMB
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The spectra
WMAP 9,2012
Planck2013
![Page 14: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/14.jpg)
Let us go to data
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Legacy Planck Archive (LPA)http://www.sciops.esa.int/index.php?page=Planck_Legacy_Archive&project=planck
1) 4 CMB maps2) maps at observational bands (30, 44, 70, 100, 143, 217, 353,545, 857 GHz)3) CO emission maps 4) Maps of dust5) Maps of galactic low frequency emission (synchrotron + free-free)6) Zodiac light maps7) Maps of gravitational lensing8) y-comptonization maps9) Masks
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Planck maps
Observational frequency maps
30GHz 44GHz 70GHz
100GHz 143GHz 217GHz
353GHz 545GHz 857GHz
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Planck maps: component separation
![Page 18: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/18.jpg)
Legacy Planck Archive (LPA)http://www.sciops.esa.int/index.php?page=Planck_Legacy_Archive&project=planck
![Page 19: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/19.jpg)
Maps WMAP9 of Planck mission
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Power spectrum
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Cosmological results: WMAP9 and Planck data
http://lambda.gsfc.nasa.gov
No revolution...
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CMB for neutrino parameters
1)
2)
3)
4)
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«Bad» spots...
![Page 24: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/24.jpg)
WMAP CMB anomalies
1) Cold Spot2) Axis of Evil3) Primirdial non-gaussinity (low limit by Planck data)4) Violation of the power spectrum parity5) Asymmetry 'North — South' in galactic coordinate system
6) New anomaly: too low amplitude of low harmonics
![Page 25: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/25.jpg)
Let us look at some anomalies...
![Page 26: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/26.jpg)
Cold Spot
Part of octupole
Cold Spot < -5sigma
1) Huge Sachs-Wolfe effect (Rudnick et al, 2007)2) Anistropic expansion (Jaffe et al., 2005)3) Topological defect [texture] (Cruz et al., 2007,2008, Planck 2013 ?)4) Artifact ?5) Galactic phenomena (M.Hansen et al., 2012)
CMB NVSSRadio sources
(Rudnick et al., 2007)
![Page 27: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/27.jpg)
Axis of Evil
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Problems of WMAP quadrupole
AmplitudeAxis of Evil: planarity + alignment(Land & Magueijo, 2005)
![Page 29: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/29.jpg)
What is the reason ?1) Component separation (Doroshkevich, Verkhodanov, 2010)2) Kouper Belt (Hansen et al. 2011)3) Moving in Local Group of galaxies? (Tegmark et al., 2004)4) Something else...5) It is absent...
![Page 30: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/30.jpg)
Axis of Evil(Planck data)
Copi et al., arXiv:1311.4562: direction of our motion exists
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Primordial non-gaussianity ?
![Page 32: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/32.jpg)
Primordial non-gaussianity ?
1) Obtained with bispectrum2) Low multimoples anomalies exist
![Page 33: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/33.jpg)
Low multipoles in Planck
L=2 L=3 L=4
L=5 L=6 L=7
L=8 L=9 L=10
![Page 34: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/34.jpg)
Low multipoles in WMAP
L=2 L=3 L=4
L=5 L=6 L=7
L=8 L=9 L=10
![Page 35: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/35.jpg)
Asimmetry North-South
Planck CMB CMB and Bianchi 7h anisotropy model ?
![Page 36: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/36.jpg)
Violation of power spectrum parity
![Page 37: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/37.jpg)
Power spectrum and separate multipoles
![Page 38: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/38.jpg)
SMICA
SEVEM
NILC
WMAP9
Maps, L<=100
![Page 39: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/39.jpg)
Power spectrum C(l), l<=50
Planck, WMAP
![Page 40: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/40.jpg)
-
=
Planck, SMICAWMAP
L=5
![Page 41: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/41.jpg)
-
=
Planck, SMICAWMAP
L=7
![Page 42: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/42.jpg)
-
=
Planck, SMICAWMAP
L=11
![Page 43: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/43.jpg)
Planck, SMICA
WMAP
L=70
NILC
SEVEM
![Page 44: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/44.jpg)
Cosmology with Suynaev-Zeldovich effect ?
Problem with cluster parameters ?Planck: optic and mm/submm centers differ from X-ray.
![Page 45: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/45.jpg)
Missed sources in the Planck data: radio sources at sigma level < 3 sigma
Awaited source of the secondary anistropy: >20000 radio galaxies ?
0015+0501
0225+0506
0226+0512
0302+0456
0311+0507, z=4.514
0427+0457 1113+0436RG in cluster ?
![Page 46: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/46.jpg)
SZ-effect
![Page 47: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/47.jpg)
30 44 70 100 143 217 353 545 CMB
0702+0440
0748+0452
0756+0506
0924+0508
1022+0450
![Page 48: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/48.jpg)
Observational channel of 217 GHz: what is unusual ?
![Page 49: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/49.jpg)
Data of 217 GHz: what is unusual ?
1) Very close to CMB map outside the Galactic plane, but let us remember WMAP bands:
![Page 50: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/50.jpg)
Data of 217 GHz: what is unusual ?
1) Close to the CMB map
2) Calibration problem ? (Spergel et al., arXiv:1312.3313)
If remove the 217 GHz channel, then it can be obtained accurate restoration of the WMAP cosmology
![Page 51: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/51.jpg)
Stephen Hawking «stamp» :)
WMAP
Planck,SMICA
![Page 52: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/52.jpg)
What have we wait for ? and what to do ?
1) WMAP and Planck data have practically the same low multipole anomalies
2) The difference of power spectra looks like one due to systematic effects of maps prepartion
3) We are waiting for a new release in June 2014: Maps of temperature anisotropy and polarization
4) Data are comparatively good (in resolution and sensetivity) when we take into account strangeness
Summary
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Корреляция: (Chаnnel — CMB) * CMB
![Page 55: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/55.jpg)
Карты(и их характеристика)
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Карты
SMICA
SEVEM
NILC
![Page 57: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/57.jpg)
Фазы
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Фазы
SEVEM
NILC
SMICA
![Page 59: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/59.jpg)
Фазы, L<=4096
SEVEMSMICA
![Page 60: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/60.jpg)
Фазы, L<=256
SEVEMSMICA
![Page 61: Anomalies of low multipoles of WMAP and Planck missions: what are they ? Oleg Verkhodanov Special astrophysical observatory of Russian Academy of Sciences.](https://reader035.fdocuments.in/reader035/viewer/2022081519/56649f335503460f94c500ed/html5/thumbnails/61.jpg)
Чтобы не забыть...
(Chiang et al. 2003)
WMAP:2 картыТегмарка
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Космологические результаты WMAP9 и Planck
http://lambda.gsfc.nasa.gov
Революции нет ... Так это прекрасно !
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Приложения
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Мультипольное разложение
Приложение 1.
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Multipole expansion
L = 2 (quadrupole) L =3 (octupole)
L = 4 L = 5
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L=2 (2,0)
(2,1) (2,2)
=
+ +
+
Квадруполь
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Октуполь
= +
+ +
(3,0)
(3,1) (3,2) (3,3)
L=3
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Для простейшей инфляционной модели
Возмущения плотности -> возмущения CMB:
Первичная негауссовость
Приложение 2: негауссовость