22 Wmap5 PPTs View free & download

Testing CPT with CMB PowerPoint PPT Presentation

Testing CPT with CMB - Interacting dark energy induces cosmological CPT violation, ... CPT is conserved The rolling of dark energy scalar field breaks Lorentz covariance It provides a ...

Interacting dark energy induces cosmological CPT violation, ... CPT is conserved The rolling of dark energy scalar field breaks Lorentz covariance It provides a ...

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Cosmological Constraints from the SDSS maxBCG Cluster Sample PowerPoint PPT Presentation

Cosmological Constraints from the SDSS maxBCG Cluster Sample - Tim McKay. Ben Koester. Jim Annis. Matthew Becker. Jiangang-Hao. Joshua ... mean velocity dispersion of galaxies as a function of richness (Becker, McKay) ...

Tim McKay. Ben Koester. Jim Annis. Matthew Becker. Jiangang-Hao. Joshua ... mean velocity dispersion of galaxies as a function of richness (Becker, McKay) ...

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Cosmological Constant as a Manifestation of the Hierarchy PowerPoint PPT Presentation

Cosmological Constant as a Manifestation of the Hierarchy - DE likely a bone fide CC: w = 1. Observations ~ 10-15 ! ?DE1/4. MSM. If DE never ... and the SM-DE hierarchies suggests a deeper. connection between the two. ...

DE likely a bone fide CC: w = 1. Observations ~ 10-15 ! ?DE1/4. MSM. If DE never ... and the SM-DE hierarchies suggests a deeper. connection between the two. ...

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Weak Lensing and Dark Energy Cosmology PowerPoint PPT Presentation

Weak Lensing and Dark Energy Cosmology - 1. Dark Energy and Neutrino Mass Constraints. from WL, SN Ia and RGA ... The existence of non-zero neutrino masses ... The massive neutrinos could suppress the ...

1. Dark Energy and Neutrino Mass Constraints. from WL, SN Ia and RGA ... The existence of non-zero neutrino masses ... The massive neutrinos could suppress the ...

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Probing Dark Energy with Cosmological Observations PowerPoint PPT Presentation

Probing Dark Energy with Cosmological Observations - Outline Introduction Current Status Discussion Future Introduction The development of cosmology is largely driven by observations The accelerating expansion of the ...

Outline Introduction Current Status Discussion Future Introduction The development of cosmology is largely driven by observations The accelerating expansion of the ...

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Anisotropic non-Gaussianity PowerPoint PPT Presentation

Anisotropic non-Gaussianity - Anisotropic non-Gaussianity arXiv:0812.0264 Mindaugas Kar iauskas work done with Konstantinos Dimopoulos David H. Lyth

Anisotropic non-Gaussianity arXiv:0812.0264 Mindaugas Kar iauskas work done with Konstantinos Dimopoulos David H. Lyth

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Foreground removal forecasts for future CMB experiments : PowerPoint PPT Presentation

Foreground removal forecasts for future CMB experiments : - CMB polarization B modes are a distinct signature of a Gravitational Wave Background ... a deep coverage might help to measure at l=100, BICEPS might ...

CMB polarization B modes are a distinct signature of a Gravitational Wave Background ... a deep coverage might help to measure at l=100, BICEPS might ...

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Baryon Acoustic Oscillations PowerPoint PPT Presentation

Baryon Acoustic Oscillations - After the decoupling, acoustic patterns of photon and baryon density fields were ... There's no significant disturbances that erase acoustic patterns ...

After the decoupling, acoustic patterns of photon and baryon density fields were ... There's no significant disturbances that erase acoustic patterns ...

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Towards the Standard Cosmological Model PowerPoint PPT Presentation

Towards the Standard Cosmological Model - Towards the Standard Cosmological Model. Andrei Linde. Cosmology: A general outlook ... String Cosmology and the Gravitino Mass. Kallosh, A.L. 2004. VAdS. uplifting ...

Towards the Standard Cosmological Model. Andrei Linde. Cosmology: A general outlook ... String Cosmology and the Gravitino Mass. Kallosh, A.L. 2004. VAdS. uplifting ...

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Conceptual Issues in Inflation PowerPoint PPT Presentation

Conceptual Issues in Inflation - * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * More observers live in the inflationary (part of the) universe because there are more stars and ...

* * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * More observers live in the inflationary (part of the) universe because there are more stars and ...

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Constraining Dark Energy: First Results from the SDSSII Supernova Survey - Constraining Dark Energy: First Results from the SDSSII Supernova Survey

Constraining Dark Energy: First Results from the SDSSII Supernova Survey

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Dick Bond - ... ppt/s/_rels/6.xml.rels ppt/s/_rels/16.xml.rels ppt/s ... jpeg ppt/media/image2.png ppt/media/image1.png ppt/media/image5.png ppt/media ...

... ppt/s/_rels/6.xml.rels ppt/s/_rels/16.xml.rels ppt/s ... jpeg ppt/media/image2.png ppt/media/image1.png ppt/media/image5.png ppt/media ...

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Bin Wang Fudan University Shanghai PowerPoint PPT Presentation

Bin Wang Fudan University Shanghai - Interaction between dark energy and dark matter Bin Wang Fudan University Shanghai

Interaction between dark energy and dark matter Bin Wang Fudan University Shanghai

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Cosmological Constraints from the SDSS maxBCG Cluster Sample - However, large numbers of X-ray follow ups are needed (~ 400) ... About Follow Ups. Hao-Yi Wu. The Challenge. For follow ups to be effective, the follow up mass ...

However, large numbers of X-ray follow ups are needed (~ 400) ... About Follow Ups. Hao-Yi Wu. The Challenge. For follow ups to be effective, the follow up mass ...

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JOINT DARK ENERGY MISSION PowerPoint PPT Presentation

JOINT DARK ENERGY MISSION - wp. Have 36 principal components. Errors s (a i) are uncorrelated ... Data models can not be constructed with high degree of certainty ...

wp. Have 36 principal components. Errors s (a i) are uncorrelated ... Data models can not be constructed with high degree of certainty ...

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Measurements of Neutrino Mass Using Cosmological Methods : Future Improvement to Accuracy in H0 - Measurements of Neutrino Mass Using Cosmological Methods : Future Improvement to Accuracy in H0

Measurements of Neutrino Mass Using Cosmological Methods : Future Improvement to Accuracy in H0

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Component Separation - Component Separation

Component Separation

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JOINT DARK ENERGY MISSION - Barocky Kolb, on behalf of the Science Working Group. FoMSWG ... community can exercise the formalism. pre-JDEM Fisher matrices ...

Barocky Kolb, on behalf of the Science Working Group. FoMSWG ... community can exercise the formalism. pre-JDEM Fisher matrices ...

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Wei-Tou NI Department of Physics PowerPoint PPT Presentation

Wei-Tou NI Department of Physics - Title: PowerPoint Presentation Author: granite Last modified by: granite Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3)

Title: PowerPoint Presentation Author: granite Last modified by: granite Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3)

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Diapositiva 1 PowerPoint PPT Presentation

Diapositiva 1 - but untill then we have to work with the best all-sky available data, WMAP. ... M. L pez-Caniego Cavendish Laboratory University of Cambridge ...

but untill then we have to work with the best all-sky available data, WMAP. ... M. L pez-Caniego Cavendish Laboratory University of Cambridge ...

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Nflation: - Nflation: observational predictions from the random matrix mass spectrum ... Adiabatic perturbations. Density perturbations. The tensor-to-scalar ratio. Introduction ...

Nflation: observational predictions from the random matrix mass spectrum ... Adiabatic perturbations. Density perturbations. The tensor-to-scalar ratio. Introduction ...

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GEM Project CrossCorrelations of WMAP5 PowerPoint PPT Presentation

GEM Project CrossCorrelations of WMAP5 - ... similar to above, but uses auto and cross-correlations to use ... sync,dust,ff = syncrotron, dust, and free-free template maps, Vary a/b as above...

... similar to above, but uses auto and cross-correlations to use ... sync,dust,ff = syncrotron, dust, and free-free template maps, Vary a/b as above...

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Wmap5 PowerPoint PPT Presentations