'Cosmological models' diaporamas de présentation

GRB

GRB. Useful reviews: Waxman astro-ph/0103186 Ghisellini astro-ph/0111584 Piran astro-ph/0405503 Meszaros astro-ph/0605208 Gehrels 2009 ariv:0909.1531 Useful links: http://qso.lanl.gov/~clf/papers (Chris Fryer lectures). Theory and observations.

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Cosmological Models with No Big Bang

Cosmological Models with No Big Bang. ??? Wun-Yi Shu Institute of Statistics National Tsing Hua University. Presentation at Institute of Physics National Chiao Tung University 2011/04/07.

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Cosmology

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COSMIC POLARIZATION ROTATION & COSMOLOGICAL MODELS AND Detectability of Primordial G-Waves

COSMIC POLARIZATION ROTATION & COSMOLOGICAL MODELS AND Detectability of Primordial G-Waves. Wei-Tou Ni

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High-Z Supernovae: The Evidence for An Accelerating Universe

High-Z Supernovae: The Evidence for An Accelerating Universe. R. Mutel Departmental Astrophysics Seminar February 19, 2003. Outline. Synopsis of 20 th Century Cosmology (Chronology) High-z Supernovae and the Accelerating Universe Potential problems: evolution, dust, lensing

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Cosmological N-Body Simulation - Topology of Large scale Structure

Cosmological N-Body Simulation - Topology of Large scale Structure. CCP 2006. 8. 29. Changbom Park with Juhan Kim (Korea Institute for Advanced Study) & J. R. Gott (Princeton) , J. Dubinski (CITA). History of Universe. Theme: Origin & Formation Mechanism of Cosmic Structures.

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METHODS OF COSMOLOGICAL MODELS SELECTION

METHODS OF COSMOLOGICAL MODELS SELECTION. W?odzimierz God?owski Marek Biesiada Zong-Hong Zhu Institute of Physics UO Institute of Physics U? Department of Astronomy Beijing Normal University. Chongqing 2013.

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Testing cosmological models with the Integrated Sachs-Wolfe effect

Testing cosmological models with the Integrated Sachs-Wolfe effect. Alvise Raccanelli,. Institute of Cosmology and Gravitation, Portsmouth. Outline:. The standard model of cosmology CMB anisotropies The ISW effect Why the ISW is a good test for cosmological models

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Testing cosmological models with the Integrated Sachs-Wolfe effect

Testing cosmological models with the Integrated Sachs-Wolfe effect. Alvise Raccanelli,. Institute of Cosmology and Gravitation, Portsmouth. Outline:. The standard model of cosmology CMB anisotropies The ISW effect Why the ISW is a good test for cosmological models

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Integrated Sachs-Wolfe effect with LOFAR

Integrated Sachs-Wolfe effect with LOFAR. Alvise Raccanelli Institute of Cosmology and Gravitaton. LOFAR Cosmology workgroup: M. Jarvis, W. Percival, D. Bacon, S. Rawlings, F. Abdalla. Outline:. The ISW effect Why the ISW is a good test for cosmological models Recent Results

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Today in Astronomy 102: the Big Bang

Today in Astronomy 102: the Big Bang. General relativistic Universes: dynamic and static. The Universe expands: no use for static models. Cosmological models: Big Bang and steady state. Observational tests of the models, and the direct observation of the Big Bang.

453 views • 26 slides

Today in Astronomy 102: the Big Bang

Today in Astronomy 102: the Big Bang. General relativistic Universes: dynamic and static. The Universe expands: no use for static models. Cosmological models: Big Bang and steady state. Observational tests of the models, and the direct observation of the Big Bang.

401 views • 26 slides

Today in Astronomy 102: the Big Bang

Today in Astronomy 102: the Big Bang. General relativistic Universes: dynamic and static. The Universe expands: no use for static models. Cosmological models: Big Bang and steady state. Observational tests of the models, and the direct observation of the Big Bang.

269 views • 26 slides

radical geography

radical geography. part six: breaking out of grid-consciousness. the grid.

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1B11 Foundations of Astronomy Cosmic distance scale

1B11 Foundations of Astronomy Cosmic distance scale. Liz Puchnarewicz emp@mssl.ucl.ac.uk www.ucl.ac.uk/webct www.mssl.ucl.ac.uk/. 1B11 Cosmic distance scale. Why is it so important to establish a cosmic distance scale?

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Using the Halo Occupation Distribution to Constrain Cosmological Models

Using the Halo Occupation Distribution to Constrain Cosmological Models Oral Section of the Ph.D. General Exam, November 8, 2002. Current Issues in Cosmology:. Current Issues in Cosmology:. Determining the density of the universe, W M .

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The merging history of dark halos dominates galaxy formation .

Cosmological Galaxy Formation. The merging history of dark halos dominates galaxy formation . Spiral galaxies: merging of small, gas-rich substructures. Elliptical Galaxies: merging of equal-mass substructures (Toomre & Toomre 1972).

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Stable cosmological solutions and superpotential method in two-field models

Stable cosmological solutions and superpotential method in two-field models. Nikolay Bulatov Moscow State University

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Sept. 9, 2011: 10am Class

Sept. 9, 2011: 10am Class. Please complete Quiz #3 on d2l before Friday, Sept. 16 Will talk about quizzes at beginning of class 21inch Telescope will open for telescope lab Sept. 19. New homework: Starry Night Lab due Sept. 21 Section 2: STAR PARTIES at Saguaro Nat. Monument

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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

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