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Introduction to Big Bang Cosmology The Universe is expanding Hubble 1929 redshift-distance relation – but also Lemaitre! z = λobs −λem λem = υem −νobs νobs z…
The expanding universe Lecture 2 Expanding universe : content • part 1 : ΛCDM model ingredients: Hubble flow cosmological principle geometry of universe •…
Slide 1 Dipole leakage and low CMB multi-poles (Indo-UK meeting) 10th August, 2011 by Santanu Das IUCAA, Pune PhD Supervisor : Prof. Tarun Souradeep Problem formulation monopole…
Computational topology of configuration spaces Yoav Kallus Santa Fe Institute Stochastic Topology and Thermodynamic Limits ICERM, Providence October 17, 2016 Y. Kallus (Santa…
Low-dimensional and Symplectic Topology http:dxdoiorg101090pspum082 This page intentionally left blank American Mathematical Society Providence Rhode Island PURE MATHEMATICS…
The dark side of our universe Max Tegmark, MIT Max Tegmark Dept. of Physics, MIT [email protected] Bright Horizons Cruise May 31, 2010 Smorga THE COSMIC SMÖRGÅSBORD Galaxy…
PowerPoint Presentation Postgraduate Diploma in Business Management 2014/15 Dr. M. Ganeshamoorthy, B.A (Hons) PDN, PgDED CMB, M.A CMB, Ph.D The Netherlands 1 MUx = ΔTU/…
Cosmology CMB Set2: Linear Perturbation Theory Davide Maino Covariant Perturbation Theory • Covariant = takes same form in all coordinate systems • Invariant = takes…
Winter conferences: cosmology • CMB • clusters • dark energy • dark matter Jean-Marc Le Goff séminaire SPP 7 avril 2014 CMB 2 PolarBear: lensed B…
[email protected] 2 3 Kirchhoff’ Experiment : “D” Lines in Na D lines darken noticeably when Sodium vapor introduced Between slit and prism
Said Zeidan Topology Optimization Applied Topology Optimization The topology optimization method Topology Optimization (TopOpt) ”is a material distribution method for finding…
1 © D as sa ul t S ys tè m es Ι S G L M ic hi ga n R U M , O ct ob er 12 , 20 11 Topology and Shape Optimization with Abaqus 2 © D as sa ul t S ys tè m es Ι S G L M…
1Institute of high energy physics 1) Brief review on the models of dark energy, especially on Quintom model; 2) Current constraints on the equation of state of dark energy;
CMB as a dark energy probe Carlo Baccigalupi Outline Fighting against a cosmological constant Parametrizing cosmic acceleration The CMB role in the current dark energy bounds…
Slide 1 Postgraduate Diploma in Business and Finance 2015/16 Dr. M. Ganeshamoorthy, B.A (Hons) PDN, PgDED CMB, M.A CMB, Ph.D The Netherlands Slide 2 Slide 3 Slide 4 Slide…
The expanding universe Lecture 1 The early universe chapters 5 to 8chapters 5 to 8 Particle Astrophysics , D. Perkins, 2nd edition, Oxford 5. The expanding universe…
0.5 % Stars and other visible stuff Ay 127 ��� The Contents of the Universe Supernovae alone ⇒ Accelerating expansion ⇒ Λ > 0 CMB alone ⇒ Flat universe ⇒…
1 Other polarimeters • Wave plates can be used to build polarimeters sensitive to linear or to circular polarization • Half-wave plate φ=180o • Quarter-wave plate…
Koichi Funakubo — Baryon Asymmetry of the Universe — 1/30 content¶ ³ §1. Evidence of the BAU §2. Requirements for the baryogenesis §3.
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