'Cosmological model' presentation slideshows

I Neutrini in Cosmologia

1.08k views • 98 slides

Recent results on measurements and interpretation of CMB fluctuations

Recent results on measurements and interpretation of CMB fluctuations. A. Doroshkevich Astro Space Center of the Physical Institute RAS Moscow, Russia. List of the problems. Observations of the CMB Separation of the CMB and galactic foregrounds Power spectrum of the CMB

563 views • 44 slides

Angelica de Oliveira-Costa

The Cosmic Microwave Background:. New Challenges. Angelica de Oliveira-Costa. University of Pennsylvania. XI Advanced School of Astrophysics. Campos do Jordao, September 2002. The Importance of CMB Polarization:.

616 views • 40 slides

The Planck Mission: Scientific expectations

Scientific Expectations. The Planck Mission: Scientific expectations. Lucia A. Popa. ISS I nstitute for S pace S ciences, Bucharest. Lucia Popa ISS I nstitute for S pace S ciences, Bucharest.

391 views • 34 slides

Cosmology : Cosmic Microwave Background & Large scale structure

Cosmology : Cosmic Microwave Background & Large scale structure. Lec . 1: Background universe. Cosmology IUCAA VSP program ( May 18-22, 2012). Tarun Souradeep. I.U.C.A.A . The Realm of Cosmology. Basic unit: Galaxy. Size : 10-100 kilo parsec (kpc.)

493 views • 32 slides

UN/ESA/NASA/JAXA Workshop on Basic Space Science and IHY 2007, Daejeon, Korea

472 views • 30 slides

Hot topics in Modern Cosmology

456 views • 30 slides

Using Spectroscopic Data of Galaxies within and around Galaxy Clusters to Test Structure Formation

Using Spectroscopic Data of Galaxies within and around Galaxy Clusters to Test Structure Formation. Doron Lemze (Johns Hopkins University)

433 views • 28 slides

??? ( ????? ) & ??? ( ????? ), J. R. Gott (Princeton, USA), J. Dubinski (CITA, Canada)

Cosmological N-Body Simulation of Cosmic Structure Formation. ????????? ?????? 2009. 9. 12. ??? ( ????? ) & ??? ( ????? ), J. R. Gott (Princeton, USA), J. Dubinski (CITA, Canada). Simulation of Cosmic Structure Formation 1. Purpose of cosmological simulations 2. Structure

459 views • 27 slides

ISLAM

342 views • 17 slides

Lagrangian Perturbation Theory : 3 rd order solutions for general dark energy models

Lagrangian Perturbation Theory : 3 rd order solutions for general dark energy models. Seokcheon Lee ( ??? ) Korea Institute for Advanced Study ( ????? ) Feb. 12 th . 2014 b ased on : arXiv /1401.2226. Outline. Why do we need LPT? Analytic Perturbation Theories

239 views • 14 slides

What is galaxy and how many different kinds are there?

What is galaxy and how many different kinds are there?. By : Flavio Gutierrez. What is a Galaxy?. Massive Consists of: Stars Dust Dark matter Contains Planets Stars Moon. en.wikipedia.org. Big Bang Theory. Cosmological Model 13.8 billion years ago How the universe started.

233 views • 10 slides

Astronomy 123

Astronomy 123. Cosmology and the Origin of Life. Cosmology. Cosmology is the empirical study of the organization, structure and evolution of the Universe At any given time we always think our Cosmology is correct: Ancient: Earth is at center of Universe

198 views • 4 slides