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Predictions from Quantum Cosmology 1 Alexander Vilenkin Institute of Cosmology, Department of Physics and Astronomy Tufts University, Medford, MA 02155, USA Abstract After…

Ψ-Epistemic Quantum Cosmology Peter W Evans∗1 Sean Gryb†2 and Karim P Y Thébault‡3 1School of Historical and Philosophical Inquiry University of Queensland 2Institute…

Martin Bojowald The Pennsylvania State University General relativity determines dynamics and structure of space-time. 1. Background independence. Space-time structure may

Alpha SYN Εκκρεμές Επένδυση σε Ευρώ ή σε Δολλάριο ΗΠΑ συνδεδεμένη με Καλάθι Μετοχών εκδόσεως 16 Ιουλίου…

Holographic Cosmology and Its Landscape Tom Banks work with W.Fischler, T.J. Torres, C.M. Wainwright May 24, 2013 Introduction Holographic Space-time-HST Dynamics of HST…

21cm cosmology T. Chang, UP, J. Peterson, P. McDonald PRL 100, 091303 (2008) UP, L. Staveley-Smith, J. Peterson, T. Chang, MNRAS, 394, 6 (2009) 21cm: HI hyperfine transition…

* before explosion 31 March 2010 Accelerated expansion : Type Ia SNe, 1998 * MORE REDSHIFT (more expansion since explosion) FAINTER  (further back in time) ~ apparent…

Galaxies and Cosmology 5 points, vt-2007 Teacher: Göran Östlin Lecture 12 Lecture 12 contents Cosmological problems Observational Cosmology: - Galaxy formation and evolution:…

Cosmology with WFMOS Jan 14, 09 @NAOJ Masahiro Takada (IPMU) Precision Cosmology ΛCDM structure formation scenario mh2=0.12770.008 etc ~96% of the Universe is dark,…

Cosmology with WFMOS Jan 14, 09 @NAOJ Masahiro Takada (IPMU) Precision Cosmology ΛCDM structure formation scenario mh2=0.12770.008 etc ~96% of the Universe is dark,…

Decidability and Complexity of Tree Share Formulas Decidability and Complexity of Tree Share Formulas Xuan Bach Le1 Aquinas Hobor1 Anthony W. Lin2 1 National University of…

Introduction Cosmological perturbations Basics of FRW cosmology Scalar-vector-tensor decomposition Evolution of cosmological perturbations Power spectra, r, Ωgw Summary…

Particle Physics and Cosmology cosmological neutrino abundance relic particles examples: neutrinos baryons cold dark matter ( WIMPS ) neutrinos neutrino background radiation…

Neutrinos in Cosmology (I) Sergio Pastor (IFIC Valencia) Universidad de Buenos Aires Febrero 2009 ν Neutrinos in Cosmology 1st lecture Introduction: neutrinos and the History…

MASSIVE NEUTRINOS AND COSMOLOGY Sergio Pastor (IFIC) ν CuTAPP 2005, Ringberg Castle Outline Current bounds and future sensitivities Effect of neutrino mass on cosmological…

Cluster Cosmology at LPPC Illuminating Dark Energy with BCS and PISCO F. William High 2nd Year Grad Student Harvard Univ Dept of Physics Monday, 21 August 2006 F. William…

Scalar Field CosmologyCosmological models with a canonical scalar field Superpotential method in cosmology Scalar Field Cosmology Cosmological models with a canonical scalar

The MHD α2-dynamo ZZ2-graded pseudo-Hermiticity level crossings and exceptional points of branching type ∗ Uwe Günther Frank Stefani Gunter Gerbeth Research Center Rossendorf…

Is cosmology a solved problem? Bepaling van ΩDM met behulp van gravitatie lenzen gevormd door clusters Is cosmology a solved problem? Abell 2218, een cluster lens waarvan…

PHY306 1 Modern cosmology 2: Type Ia supernovae and Λ Distances at z ~1 Type Ia supernovae SNe Ia and cosmology Results from the Supernova Cosmology Project, the High z…