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Gaussianity, Flatness, Tilt, Running, and Gravity Waves: WMAP and Some Future Prospects

Gaussianity, Flatness, Tilt, Running, and Gravity Waves: WMAP and Some Future Prospects. Eiichiro Komatsu University of Texas at Austin July 11, 2007. Cosmology and Strings: 6 Numbers. Successful early-universe models must produce: The universe that is nearly flat, | ? K |<O(0.02)

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556 views • 46 slides

Primordial non- Gaussianity from inflation

ICGC, Goa 19 th December 2011. Primordial non- Gaussianity from inflation. David Wands Institute of Cosmology and Gravitation University of Portsmouth

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605 views • 45 slides

Primordial non- Gaussianity from inflation

Cosmo-12, Beijing 13 th September 2012. Primordial non- Gaussianity from inflation. David Wands Institute of Cosmology and Gravitation University of Portsmouth

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422 views • 27 slides

Primordial non- Gaussianity from inflation

Cosmo-12, Beijing 13 th September 2012. Primordial non- Gaussianity from inflation. David Wands Institute of Cosmology and Gravitation University of Portsmouth

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482 views • 27 slides

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Nl 10 - PowerPoint PPT Presentation

Gaussianity, Flatness, Tilt, Running, and Gravity Waves: WMAP and Some Future Prospects

Primordial non- Gaussianity from inflation

Primordial non- Gaussianity from inflation

Primordial non- Gaussianity from inflation