Primordial fluctuations

Results: 25



#Item
1Neutrino mass limits from galaxy surveys and implications for particle physics Viviana Niro UAM and IFT UAM/CSIC InvisiblesPlus and Elusives network

Neutrino mass limits from galaxy surveys and implications for particle physics Viviana Niro UAM and IFT UAM/CSIC InvisiblesPlus and Elusives network

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Source URL: theory.fnal.gov

Language: English - Date: 2016-05-13 16:16:17
219. Cosmic background radiationCOSMIC BACKGROUND RADIATION Revised February 2000 by G.F. Smoot (LBNL) and D. Scott (University of British Columbia).

19. Cosmic background radiationCOSMIC BACKGROUND RADIATION Revised February 2000 by G.F. Smoot (LBNL) and D. Scott (University of British Columbia).

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Source URL: davidwoolsey.com

Language: English - Date: 2005-08-07 23:31:20
3Lecture V: Primordial fluctuations Jes´ us Torrado — Julien Lesgourgues Instituut-Lorentz — EPFL & CERN London,

Lecture V: Primordial fluctuations Jes´ us Torrado — Julien Lesgourgues Instituut-Lorentz — EPFL & CERN London,

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Source URL: lesgourg.web.cern.ch

Language: English - Date: 2014-05-17 12:25:03
    4CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu, Max-Planck-Institut für Astrophysik The 18th Paris Cosmology Colloquium, Observatoire de Paris July 23, 2014

    CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu, Max-Planck-Institut für Astrophysik The 18th Paris Cosmology Colloquium, Observatoire de Paris July 23, 2014

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    Source URL: chalonge.obspm.fr

    Language: English - Date: 2014-07-28 03:26:11
    5Neutrino physics from future weak lensing surveys R. Ali Vanderveld1 and Wayne Hu1, 2 arXiv:1212.3608v1 [astro-ph.CO] 14 Dec

    Neutrino physics from future weak lensing surveys R. Ali Vanderveld1 and Wayne Hu1, 2 arXiv:1212.3608v1 [astro-ph.CO] 14 Dec

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    Source URL: background.uchicago.edu

    Language: English - Date: 2015-01-06 12:05:31
    6Astro 321 Set 5: CMB & LSS Wayne Hu From Inflation to Horizon Entry • Inflation provides a source of nearly scale invariant comoving

    Astro 321 Set 5: CMB & LSS Wayne Hu From Inflation to Horizon Entry • Inflation provides a source of nearly scale invariant comoving

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    Source URL: background.uchicago.edu

    Language: English - Date: 2011-08-15 18:34:55
    7

    PDF Document

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    Source URL: www.physics.ucdavis.edu

    Language: English - Date: 2011-05-07 09:30:54
    8Accepted by the Astrophysical Journal FIRST YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: TESTS OF GAUSSIANITY E. Komatsu 2 , A. Kogut 3 , M. R. Nolta 4 , C. L. Bennett 3 , M. Halpern 5 , G. Hinshaw 3 ,

    Accepted by the Astrophysical Journal FIRST YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: TESTS OF GAUSSIANITY E. Komatsu 2 , A. Kogut 3 , M. R. Nolta 4 , C. L. Bennett 3 , M. Halpern 5 , G. Hinshaw 3 ,

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    Source URL: lambda.gsfc.nasa.gov

    Language: English - Date: 2008-04-18 17:22:15
    9Microsoft Word - Cosmology Week in Review #1(2).docx

    Microsoft Word - Cosmology Week in Review #1(2).docx

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    Source URL: cfcp.uchicago.edu

    Language: English - Date: 2015-05-04 11:43:41
    10What Energy Drives the Universe? Andrei Linde Department of Physics, Stanford University, Stanford, CA 94305, USA What energy drives the universe? Where did this energy come from? Before trying to answer these questions,

    What Energy Drives the Universe? Andrei Linde Department of Physics, Stanford University, Stanford, CA 94305, USA What energy drives the universe? Where did this energy come from? Before trying to answer these questions,

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    Source URL: energy.nobelprize.org

    Language: English - Date: 2005-06-17 02:46:20