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Springel, Frenk & White 2006, Nature, 440, 11

Springel, Frenk & White 2006, Nature, 440, 11. de Lapparent, Geller & Huchra 1986. LSS. LSS. LSS. Cmbgg OmOl. How flat is space?. Somewhat. Cmbgg OmOl. How flat is space?.  tot =1.003 . Cmbgg OmOl. CMB+SN Ia. CMB+LRG. Beth Reid et al, arXiv 0907.1559. Cmbgg OmOl.

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Springel, Frenk & White 2006, Nature, 440, 11

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  1. Springel, Frenk & White 2006, Nature, 440, 11

  2. de Lapparent, Geller & Huchra 1986 LSS

  3. LSS

  4. LSS

  5. Cmbgg OmOl How flat is space? Somewhat.

  6. Cmbgg OmOl How flat is space? tot=1.003

  7. Cmbgg OmOl CMB+SN Ia CMB+LRG Beth Reid et al, arXiv 0907.1559

  8. Cmbgg OmOl Two embarrassing problems: Inflation String theory V()  Mark Hertzberg, MT, Shamit Kachru, Wati Taylor, Jessie Shelton, Onur Özcan 2007: arXiv:0709.0002 [astro-ph] arXiv:0711.2512 [hep-ph]

  9. Cmbgg OmOl Jargon dictionary: Stringlish English

  10. Cmbgg OmOl (14 fields)

  11. Cmbgg OmOl Slow-roll inflation is forbidden in themost clearly understood class of compactifications: in the large volume and small string couplinglimit of all Calabi-Yau orientifold compactifications when only standard NS-NS three-form flux, R-Rfluxes, D6-branes and O6-planes are included. With these ingredients, the first slow-roll parametersatisfiesϵ≥27/13wheneverV >0..

  12. New clues about dark matter

  13. Four roads to dark matter: catch it, infer it, make it, weigh it Production: Direct: Gravitational: Indirect: Planck launched May 14 2009 21 cm tomography happening

  14. 000619 Upcoming lensing measurements: Ongoing Within a year Not yet guaranteed Compilation from Masahiro Takada 2010

  15. SOME SURVEYS TO LOOK FORWARD TO: (Table from Natalie Roe)

  16. LAMOST: The Large Sky Area Multi-Object Fibre Spectroscopic Telescope Chinese Academy of Science

  17. (Image courtesy of Yongheng Zhao)

  18. Physics with 21 cm tomography

  19. 75% 21% 4% ? Cosmological data Cosmological Parameters Why these particular values? Nature of dark matter? Map our universe! Fundamental theory Nature of dark energy? Nature of early Universe?

  20. History Our observable universe CMB Foreground-cleaned WMAP map from Tegmark, de Oliveira-Costa & Hamilton, astro-ph/0302496 Last scattering surface

  21. Our observable universe LSS Last scattering surface 21cm tomography

  22. The time frontier LSS Last scattering surface 21cm tomography

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