'Structure formation' presentation slideshows

Structure formation - PowerPoint PPT Presentation


Data Mining - CSE5230

Data Mining - CSE5230

CSE5230/DMS/2004/8. Data Mining - CSE5230. S elf-Organizing Maps (SOMs). Lecture Outline. Motivation unsupervised learning the cortex topographic feature maps biological self-organizing maps Artificial self-organizing maps Kohonen’s self-organizing network learning algorithm examples

By veata
(188 views)

UNIT 6

UNIT 6

UNIT 6. The Earth ’ s structure. FORMATION OF THE DIFFERENT TYPES OF ROCKS. Natural Science 2. Secondary Education. UNIT 6. Formation of the different types of rocks. TYPES OF ROCKS. MAGMATIC ROCKS. METAMORPHIC ROCKS. SEDIMENTARY ROCKS. Click on each box to find out more.

By suki
(1 views)

Cosmological Structure Formation A Short Course

Cosmological Structure Formation A Short Course

Cosmological Structure Formation A Short Course. III. Structure Formation in the Non-Linear Regime Chris Power. Recap. Cosmological inflation provides mechanism for generating density perturbations … … which grow via gravitational instability

By kiaria
(95 views)

Synthesis and Characterization of Amphiphilic Dendron Coils – Potential Nanomicelle Precursors

Synthesis and Characterization of Amphiphilic Dendron Coils – Potential Nanomicelle Precursors

Synthesis and Characterization of Amphiphilic Dendron Coils – Potential Nanomicelle Precursors. Jeromy T. Bentley University of Illinois at Chicago RET Fellow Department of Biopharmaceutical Sciences Advisor: Dr. Seungpyo Hong Mentor: Ryan Pearson July 28, 2011. Summer Plan.

By rupert
(153 views)

Synthesis and Characterization of Dendron-based Nanomicelles for Targeted Cancer Therapy

Synthesis and Characterization of Dendron-based Nanomicelles for Targeted Cancer Therapy

Synthesis and Characterization of Dendron-based Nanomicelles for Targeted Cancer Therapy. Jeromy T. Bentley University of Illinois at Chicago RET Fellow Department of Biopharmaceutical Sciences Advisor: Dr. Seungpyo Hong Mentor: Ryan Pearson June 30, 2011. Impact and Motivation .

By maire
(372 views)

Seeing the universe through redshifted 21-cm radiation

Seeing the universe through redshifted 21-cm radiation

Somnath Bharadwaj Physics & CTS IIT Kharagpur. Seeing the universe through redshifted 21-cm radiation. Tarun D Saini. Biswajit Pandey. Collaborators. Sanjay Pandey. IISc. RRI. Biman Nath. LBSC,Gonda. BITS,Pilani. RRI. Jayaram Chengalur. Tapomoy Guha Sarkar. Shiv K Sethi.

By gyan
(137 views)

Dark Matter

Dark Matter

Dark Matter. Expect Unexpected outside LHC. Jingsheng Li. Introduction. SM is confirmed precisely? NO! Dark Matter is OUT THERE!! SC=SM+more ∟ (New Phy=ptc+int) +unexpected ∟ astrophy effect? ∟ modify gravity?. Outline. Standard Cosmology Evidence for Dark Matter

By kailey
(149 views)

Irreversible Time and the Big Bang

Irreversible Time and the Big Bang

Irreversible Time and the Big Bang. The Main Point. The expansion of the early universe, that followed the Big Bang, played a major part in creating the “ arrow of time .”. The Arrow of Time. We instinctively know that this movie is wrong!. Statistical Mechanics.

By tannar
(115 views)

2005. 2. 16 - 19 Changbom Park (Korea Institute for Advanced Study)

2005. 2. 16 - 19 Changbom Park (Korea Institute for Advanced Study)

Workshop for Underground Experiments and Astroparticle Physics. Dark Matter and Clustering Motivation and Findings on Dark Matter from the Study of Structure Formation. Dark Matter. 2005. 2. 16 - 19 Changbom Park (Korea Institute for Advanced Study). DM.

By pegeen
(105 views)

Topology of Large Scale Structures Introduction, Theory and Progress Report

Topology of Large Scale Structures Introduction, Theory and Progress Report

KIAS Workshop on Cosmology and Structure Formation. Topology of Large Scale Structures Introduction, Theory and Progress Report. 2004. 10. 28-29 Changbom Park (Korea Institute for Advanced Study). 1. Genus – A Measure of Topology. Definition G = # of holes - # of isolated regions

By jayden
(124 views)

cosmological computing

cosmological computing

cosmological computing. computing is central to all major science components of the Center. analyses of large data sets (e.g., CMB data, SDSS, DES) data modeling (air shower simulations, mock galaxy catalogs, Monte Carlo simulations of experiments, etc.)

By yamal
(102 views)

Dark energy fluctuations and structure formation

Dark energy fluctuations and structure formation

Dark energy fluctuations and structure formation. Rogério Rosenfeld Instituto de Física Teórica/UNESP. I Workshop "Challenges of New Physics in Space" Campos do Jordão, Brazil 26/04/2009. Standard Model of Cosmology. + homogeneity and isotropy. FLRW model.

By lavender
(89 views)

Radio astronomy: Probing the Cosmic Reionization Manchester, Oct 2007 Chris Carilli (NRAO)

Radio astronomy: Probing the Cosmic Reionization Manchester, Oct 2007 Chris Carilli (NRAO)

Radio astronomy: Probing the Cosmic Reionization Manchester, Oct 2007 Chris Carilli (NRAO). Ionized. Neutral. Reionized. Chris Carilli (NRAO) Berlin June 29, 2005. WMAP – structure from the big bang. Hubble Space Telescope Realm of the Galaxies.

By joben
(133 views)

Neutrino hot dark matter and hydrodynamics of structure formation: Two “new” features of matter

Neutrino hot dark matter and hydrodynamics of structure formation: Two “new” features of matter

Neutrino hot dark matter and hydrodynamics of structure formation: Two “new” features of matter. Dr. Theo M. Nieuwenhuizen Institute for Theoretical Physics University of Amsterdam. Harvard Smithsonian Center for Astrophysics 22 Jan 2010. Outline. Two types of dark matter.

By hasad
(164 views)

Cosmological Fluid Dynamics with AMR

Cosmological Fluid Dynamics with AMR

Cosmological Fluid Dynamics with AMR. Michael L. Norman Laboratory for Computational Astrophysics, UCSD. Baryons + Radiation + Magnetic fields. Under the gravitational influence of dark matter. Interacting galaxies. Coma cluster in X-ray. Cosmological Fluid Dynamics. Definition

By piera
(177 views)

Cosmological structure formation: models confront observations

Cosmological structure formation: models confront observations

Cosmological structure formation: models confront observations. Andrea V. Maccio’ Max Planck Institute for Astronomy Heidelberg. A. Boyarsky (EPFL), A. Dutton (Univ. Victoria), B. Moore (Zurich), H.W. Rix (MPIA) , O. Ruchayskiy (EPFL), F. van den Bosch (Yale). Is (L)CDM the right model?.

By artie
(141 views)

Cosmological Aspects of Neutrino Physics (II)

Cosmological Aspects of Neutrino Physics (II)

Cosmological Aspects of Neutrino Physics (II). ν. Sergio Pastor (IFIC) 61st SUSSP St Andrews, August 2006. Cosmological Aspects of Neutrino Physics. 2nd lecture. Degenerate relic neutrinos (Neutrino asymmetries). Massive neutrinos as Dark Matter.

By kairos
(157 views)

N-body Simulations and Gravitational Lensing with Dark Energy

N-body Simulations and Gravitational Lensing with Dark Energy

N-body Simulations and Gravitational Lensing with Dark Energy. Beyond Einstein Meeting, May 13, 2004. Outline. Why Structure Formation and Dark Energy? Studying Dark Energy with Structure Formation: achievements and plans

By mandell
(112 views)

Cosmic reionization and the history of the neutral intergalactic medium

Cosmic reionization and the history of the neutral intergalactic medium

Cosmic reionization and the history of the neutral intergalactic medium MAGPOP Summer School, Kloster Seeon Chris Carilli, NRAO, August 10, 2007. Introduction: What is Cosmic Reionization? Current constraints on the IGM neutral fraction with cosmic epoch

By ronli
(134 views)

Large-scale Structure: Theory & Observations

Large-scale Structure: Theory & Observations

Large-scale Structure: Theory & Observations. Josh Frieman. Structure Formation & Evolution, Santiago, October 2002. The Structure Formation Cookbook. 1. Initial Conditions: A Theory for the Origin of Density Perturbations in the Early Universe

By lynley
(124 views)

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