Sky Scholar | The CMB, Angular Power Spectrum, & Mathemagics! @SkyScholar | Uploaded November 2020 | Updated October 2024, 3 hours ago.
Real Physics Talk, Munich, Germany, 2019: Pierre-Marie Robitaille youtube.com/watch?v=MH9h6eXyMcQ
Have Astronomers Assigned a Signal Produced by the Oceans to the Cosmos? - Sophia, Bulgaria
youtube.com/watch?v=7QVm_50-BDg
The Cosmic Microwave Background | EU2014 youtube.com/watch?v=i8ijbu3bSqI
P.M. Robitaille, WMAP: A Radiological Analysis, Progr. Phys. 2007, v. 3, no. 1, 3-18. ptep-online.com/2007/PP-08-01.PDF
One can find all the NASA/WMAP Team papers here: lambda.gsfc.nasa.gov/product/map/current/map_bibliography.cfm
One can find all the PLANCK Images here (Second Data Release): https://irsa.ipac.caltech.edu/data/Planck/release_2/all-sky-maps/
Planck image gallery: https://www.cosmos.esa.int/web/planck/picture-gallery
Robert D. Klauber, Student Friendly Guide to the Cosmic Microwave Background, May 15, 2019.
quantumfieldtheory.info/cmb_vers_2.pdf
Univeristy of Utah Physics and Spherical Harmonic Analysis
http://www.physics.utah.edu/~sommers/faq/b3.html (accessed on 10/30/2020)
WMAP Angular Power Spectrum (3 year)
iopscience.iop.org/article/10.1086/513698/pdf
WMAP FINAL ANGULAR POWER SPECTRUM (9 year)
iopscience.iop.org/article/10.1088/0067-0049/208/2/20/pdf
WMAP Final Angular Power Spectrum Model Estimates (9 year)
iopscience.iop.org/article/10.1088/0067-0049/208/2/19/pdf
PLANCK FINAL ANGULAR POWER SPECTRUM (2018)
https://www.cosmos.esa.int/documents/387566/387653/Planck_2018_results_L01.pdf
The Pseudo-Cl method: journals.aps.org/prd/abstract/10.1103/PhysRevD.64.083003
arxiv.org/pdf/astro-ph/0008111.pdf
M. Plionis, The Quest for the Cosmological Parameters,
link.springer.com/chapter/10.1007/3-540-48025-0_7
D. Samtleben, S. Staggs, and B. Winstein, The Cosmic Microwave Background for Pedestrians: A Review for Particle and Nuclear Physicists
arxiv.org/pdf/0803.0834.pdf
M. White, CMB Anisotropy, http://w.astro.berkeley.edu/~mwhite/rosetta/node2.html
O.V. Verkhodanov, Searching for non-Gaussianity in observational cosmic microwave background data,
iopscience.iop.org/article/10.3367/UFNe.0182.201211d.1177/pdf
R. Tojeiro, Understanding the Cosmic Microwave Background Temperature Power Spectrum, 2006.
roe.ac.uk/ifa/postgrad/pedagogy/2006_tojeiro.pdf
A. Repp, et al. The Impact of non-Gaussianity upon Cosmological Forecasts.
academic.oup.com/mnras/article/454/4/3533/997798
M. Cruz, et al. The non-gaussian Cold Spot in the 3 Year Wilkinson Microwave Anisotropy Probe Data,
iopscience.iop.org/article/10.1086/509703/pdf
A. Bernui, et al., North-South non-Guassian Asymmetry in the Planck CMB Maps,
arxiv.org/pdf/1404.2936.pdf
V. Desjacques and U. Seljak, Primordial Non-Gaussianity in the Large-Scale Structure of the Universe,
downloads.hindawi.com/journals/aa/2010/908640.pdf
C.H., Lineweaver, Gold in the Doppler Hills: Cosmological Parameters in the Microwave Background
http://articles.adsabs.harvard.edu/full/1997ASPC..126..185L
M. Bucher, Physics of the cosmic microwave background anisotropy, One Hundred Years of General Relativity, pp. 43-149 (2017). (see p. 86ff)
worldscientific.com/doi/pdf/10.1142/9789814678506_0003
C.J. Copi, et al. On the large-angle anomalies of the microwave sky,
academic.oup.com/mnras/article/367/1/79/1020698
C.J. Copi, et al., Large-Angle Anomalies in the CMB Advances in Astronomy, 2010, Article ID 847541,17pages
downloads.hindawi.com/journals/aa/2010/847541.pdf
O. V. Verkhodanov, Low Multipoles Anomalies of CMB Maps,
in "Radiative Mechanisms of Astrophysical Objects (V. Grining et al., eds.). Yerevan, 2017, 363-370.
O. V. Verkhodanov, Series of Anomalies of low multipoles of WMAP and Planck Missions: What are They?
https://www1.jinr.ru/publish/Pepan/v-46-2/18_verk.pdf
H. Liu and T.P. Li, New Evidence for Lack of CMB Power on Large Scales,
arxiv.org/pdf/0911.4063.pdf
H. Liu and T.P. Li, Missing Completely of the CMB Quadrupole in WMAP Data,
arxiv.org/pdf/1203.5720.pdf
C.L. Bennett et al., Seven-Year Wilikinson Microwave Anisotropy Probe (WMAP) Observations:
Are There Cosmic Microwave Background Anomalies,
iopscience.iop.org/article/10.1088/0067-0049/192/2/17/pdf
Pierre-Marie Robitaille, Ph.D., was a professor of Radiology at The Ohio State University from 1989-2019, and also held an appointment in the Chemical Physics Program. In 1998, he led the design and assembly of the world’s first Ultra High Field MRI System. Readings from this equipment brought into question fundamental aspects of modern thermal physics, such as Kirchhoff’s Law of thermal emission.
This channel is educational in nature.
Link to Professor Robitaille’s papers on Vixra:
vixra.org/author/pierre-marie_robitaille
Outro Music:
Foria: Break Away
soundcloud.com/foria
youtube.com/watch?v=UkUweq5FAcE
Real Physics Talk, Munich, Germany, 2019: Pierre-Marie Robitaille youtube.com/watch?v=MH9h6eXyMcQ
Have Astronomers Assigned a Signal Produced by the Oceans to the Cosmos? - Sophia, Bulgaria
youtube.com/watch?v=7QVm_50-BDg
The Cosmic Microwave Background | EU2014 youtube.com/watch?v=i8ijbu3bSqI
P.M. Robitaille, WMAP: A Radiological Analysis, Progr. Phys. 2007, v. 3, no. 1, 3-18. ptep-online.com/2007/PP-08-01.PDF
One can find all the NASA/WMAP Team papers here: lambda.gsfc.nasa.gov/product/map/current/map_bibliography.cfm
One can find all the PLANCK Images here (Second Data Release): https://irsa.ipac.caltech.edu/data/Planck/release_2/all-sky-maps/
Planck image gallery: https://www.cosmos.esa.int/web/planck/picture-gallery
Robert D. Klauber, Student Friendly Guide to the Cosmic Microwave Background, May 15, 2019.
quantumfieldtheory.info/cmb_vers_2.pdf
Univeristy of Utah Physics and Spherical Harmonic Analysis
http://www.physics.utah.edu/~sommers/faq/b3.html (accessed on 10/30/2020)
WMAP Angular Power Spectrum (3 year)
iopscience.iop.org/article/10.1086/513698/pdf
WMAP FINAL ANGULAR POWER SPECTRUM (9 year)
iopscience.iop.org/article/10.1088/0067-0049/208/2/20/pdf
WMAP Final Angular Power Spectrum Model Estimates (9 year)
iopscience.iop.org/article/10.1088/0067-0049/208/2/19/pdf
PLANCK FINAL ANGULAR POWER SPECTRUM (2018)
https://www.cosmos.esa.int/documents/387566/387653/Planck_2018_results_L01.pdf
The Pseudo-Cl method: journals.aps.org/prd/abstract/10.1103/PhysRevD.64.083003
arxiv.org/pdf/astro-ph/0008111.pdf
M. Plionis, The Quest for the Cosmological Parameters,
link.springer.com/chapter/10.1007/3-540-48025-0_7
D. Samtleben, S. Staggs, and B. Winstein, The Cosmic Microwave Background for Pedestrians: A Review for Particle and Nuclear Physicists
arxiv.org/pdf/0803.0834.pdf
M. White, CMB Anisotropy, http://w.astro.berkeley.edu/~mwhite/rosetta/node2.html
O.V. Verkhodanov, Searching for non-Gaussianity in observational cosmic microwave background data,
iopscience.iop.org/article/10.3367/UFNe.0182.201211d.1177/pdf
R. Tojeiro, Understanding the Cosmic Microwave Background Temperature Power Spectrum, 2006.
roe.ac.uk/ifa/postgrad/pedagogy/2006_tojeiro.pdf
A. Repp, et al. The Impact of non-Gaussianity upon Cosmological Forecasts.
academic.oup.com/mnras/article/454/4/3533/997798
M. Cruz, et al. The non-gaussian Cold Spot in the 3 Year Wilkinson Microwave Anisotropy Probe Data,
iopscience.iop.org/article/10.1086/509703/pdf
A. Bernui, et al., North-South non-Guassian Asymmetry in the Planck CMB Maps,
arxiv.org/pdf/1404.2936.pdf
V. Desjacques and U. Seljak, Primordial Non-Gaussianity in the Large-Scale Structure of the Universe,
downloads.hindawi.com/journals/aa/2010/908640.pdf
C.H., Lineweaver, Gold in the Doppler Hills: Cosmological Parameters in the Microwave Background
http://articles.adsabs.harvard.edu/full/1997ASPC..126..185L
M. Bucher, Physics of the cosmic microwave background anisotropy, One Hundred Years of General Relativity, pp. 43-149 (2017). (see p. 86ff)
worldscientific.com/doi/pdf/10.1142/9789814678506_0003
C.J. Copi, et al. On the large-angle anomalies of the microwave sky,
academic.oup.com/mnras/article/367/1/79/1020698
C.J. Copi, et al., Large-Angle Anomalies in the CMB Advances in Astronomy, 2010, Article ID 847541,17pages
downloads.hindawi.com/journals/aa/2010/847541.pdf
O. V. Verkhodanov, Low Multipoles Anomalies of CMB Maps,
in "Radiative Mechanisms of Astrophysical Objects (V. Grining et al., eds.). Yerevan, 2017, 363-370.
O. V. Verkhodanov, Series of Anomalies of low multipoles of WMAP and Planck Missions: What are They?
https://www1.jinr.ru/publish/Pepan/v-46-2/18_verk.pdf
H. Liu and T.P. Li, New Evidence for Lack of CMB Power on Large Scales,
arxiv.org/pdf/0911.4063.pdf
H. Liu and T.P. Li, Missing Completely of the CMB Quadrupole in WMAP Data,
arxiv.org/pdf/1203.5720.pdf
C.L. Bennett et al., Seven-Year Wilikinson Microwave Anisotropy Probe (WMAP) Observations:
Are There Cosmic Microwave Background Anomalies,
iopscience.iop.org/article/10.1088/0067-0049/192/2/17/pdf
Pierre-Marie Robitaille, Ph.D., was a professor of Radiology at The Ohio State University from 1989-2019, and also held an appointment in the Chemical Physics Program. In 1998, he led the design and assembly of the world’s first Ultra High Field MRI System. Readings from this equipment brought into question fundamental aspects of modern thermal physics, such as Kirchhoff’s Law of thermal emission.
This channel is educational in nature.
Link to Professor Robitaille’s papers on Vixra:
vixra.org/author/pierre-marie_robitaille
Outro Music:
Foria: Break Away
soundcloud.com/foria
youtube.com/watch?v=UkUweq5FAcE
