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CMB, CMB lensing, non-Gaussianity

Cross correlation between the CMB lensing potential measured by Planck and high z submillimeter galaxies detected by the Herschel ATLAS survey

Cross correlation between the CMB lensing potential measured by Planck and high z submillimeter galaxies detected by the Herschel ATLAS survey

... the lensing reconstruction noise power spectrum N ℓ kk , which was estimated from the set of 100 simulated lensing maps 16 recently released by the Planck team that account for the inhomogeneous noise ...

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Exploring cosmic origins with CORE: Gravitational lensing of the CMB

Exploring cosmic origins with CORE: Gravitational lensing of the CMB

... (including CMB, foregrounds and noise), which can be approximated by smoothed versions of the measured spectra, and fiducial lensed CMB power ...the lensing power spectrum or derived ...the ...

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To the horizon and beyond: weak lensing of the CMB and binary inspirals into horizonless objects

To the horizon and beyond: weak lensing of the CMB and binary inspirals into horizonless objects

... a non-Gaussian deflection field and contamination from the kinetic Sunyaev-Zel’dovich (kSZ) ...to non-Gaussianity in the deflection field, so Amblard et ...resulting non-Gaussian deflection ...

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CMB—A Geometric, Lorentz Invariant Model in Non Expanding Lobachevskian Universe with a Black Body Spectral Distribution Function

CMB—A Geometric, Lorentz Invariant Model in Non Expanding Lobachevskian Universe with a Black Body Spectral Distribution Function

... It is well known that the Big Bang based space inflation hypothesis requires a flat Euclidean geometry of space . Both Euclidean space and Lobachevskian space are non-compact/locally compact spaces. The difficulty ...

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Signatures of Self-Interacting Dark Matter in the Matter Power Spectrum and the CMB

Signatures of Self-Interacting Dark Matter in the Matter Power Spectrum and the CMB

... V. Conclusions. SIDM is a compelling alternative to CDM. It keeps all the success of CDM on large scales, while modifying the inner halo structure in accord with observa- tions. Using a simplified particle physics ...

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Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum

Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum

... from non-relativistic quantum mechanics to field theories, the formal definition of integrals requires the introduction of a lattice, in order to properly account for, the known fact that quantum paths are nowhere ...

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Experiments on the CMB Spectrum, Big Jets Model and Their Implications for the Missing Half of the Universe

Experiments on the CMB Spectrum, Big Jets Model and Their Implications for the Missing Half of the Universe

... According to the Big Jets model[16, 18], the presence of an extremely distant ‘antimatter-galaxies blackbody’ could contribute to the observed dipole anisotropy in CMB. The Big Jets model suggests that the ...

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Adapted Method for Separating Kinetic SZ Signal from Primary CMB Fluctuations

Adapted Method for Separating Kinetic SZ Signal from Primary CMB Fluctuations

... the CMB signal on masked pixels by interpolation, and then we deduce the best estimate of the KSZ map by minimisa- ...underlying CMB (sensitive to our knowledge of the CMB through the confidence ...

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Thermodynamics of SU(2) quantum Yang-Mills theory and CMB anomalies

Thermodynamics of SU(2) quantum Yang-Mills theory and CMB anomalies

... is, non-selfintersecting center-vortex loops 6 (zero selfintersection number, N = 0) in the confining phases of pure SU(2) gauge theories whose Yang-Mills scales match the masses of charged ...the CMB, over ...

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Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum

Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum

... these non-Gaussian amplitudes are expected to be rather small, with very significant suppressions by extra factors of 1/ξ ...a non-trivial gravitational scaling dimensions scenario as described ...

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Imprints on CMB Angular Power Spectrum Modes from Cosmological Reionization

Imprints on CMB Angular Power Spectrum Modes from Cosmological Reionization

... current CMB data, a great attention has been recently posed on the accurate compu- tation of the reionization signatures in the CMB for a large variety of astrophysical scenarios and physical ...the ...

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Calculation of the Universal Gravitational Constant, of the Hubble Constant, and of the Average CMB Temperature

Calculation of the Universal Gravitational Constant, of the Hubble Constant, and of the Average CMB Temperature

... We call its value “apparent” because the equation giving Ru assumes a speed of light that is constant over time and equal to c, for a time equal to the apparent age of the universe Tu = [r] ...

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Hartle-Hawking wave function and large-scale power suppression of CMB

Hartle-Hawking wave function and large-scale power suppression of CMB

... Up to now, the observed CMB data has a tension with the theoretical expectations (based single field inflation and the ΛCDM model), especially for large length scales [9]. It is not clear whether this tension will ...

5

An SU(2) gauge principle for the CMB: Perspectives on Dark Sector of the Cosmological Model

An SU(2) gauge principle for the CMB: Perspectives on Dark Sector of the Cosmological Model

... seed non-linear structure formation and whether their role in galactic halo formation and baryon accretion meets the observational constraints (Tully-Fisher relation, ...the CMB large-angle anomalies, see ...

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Rossmanith, Gregor
  

(2011):


	Concepts of non-linear data analysis applied to the search of non-Gaussianities in the CMB.


Dissertation, LMU München: Fakultät für Physik

Rossmanith, Gregor (2011): Concepts of non-linear data analysis applied to the search of non-Gaussianities in the CMB. Dissertation, LMU München: Fakultät für Physik

... the CMB is a rather young story: The existence of a relic radiation was first proposed by George Gamov in 1946 [195], and the evaluation of its temperature was done by Ralph Alpher and Robert Herman in 1950 ...the ...

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The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing

The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing

... The latest CMB measurements from Boomerang (Net- terfield et al. 2001, de Bernardis et al. 2002), Maxima (Lee et al. 2001; Stomper et al. 2001) and DASI (Halverson et al. 2002; Pryke et al. 2002) suggest three ...

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PARTICIPATORY NATURAL RESOURCES MANAGEMENT IN THE TONLE SAP REGION GCP/CMB/002/BEL

PARTICIPATORY NATURAL RESOURCES MANAGEMENT IN THE TONLE SAP REGION GCP/CMB/002/BEL

... Finally, a GIS component was officially included in Phase 2 project document, including specific GIS-related expected outputs, recruitment of a GIS associate professional officer, and option for another GIS consultancy. ...

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Studying Heavy Ion Collisions Using Methods From Cosmic Microwave Background (CMB) Analysis

Studying Heavy Ion Collisions Using Methods From Cosmic Microwave Background (CMB) Analysis

... Abstract. We present and discuss a framework for studying the morphology of high- multiplicity events from relativistic heavy ion collisions using methods commonly em- ployed in the analysis of the photons from the ...

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Revisiting non-Gaussianity from non-attractor inflation models

Revisiting non-Gaussianity from non-attractor inflation models

... Abstract. Non-attractor inflation is known as the only single field inflationary scenario that can violate non-Gaussianity consistency relation with the Bunch-Davies vacuum state and generate large ...

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CORPORATE GOVERNANCE PRINCIPLES CAPITAL MARKETS BOARD OF TURKEY (CMB)

CORPORATE GOVERNANCE PRINCIPLES CAPITAL MARKETS BOARD OF TURKEY (CMB)

... T he Principles mainly address publicly held joint stock companies. However, it is considered that other joint stock companies and institutions, active in private and public sector, may also implement these Principles. ...

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