'Cosmic microwave background radiation' presentation slideshows

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Microwave

Microwave

Microwave. Telescopes. Parvaneh, Shelby & Marleena. Visit www.worldofteaching.com For 100’s of free powerpoints. Discovery (domestic use). Microwaves have wavelengths range from centimeters to those closer to a foot in length. Longer are for heating food. Shorter waves Doppler radar

By jacob
(498 views)

Cosmology and Collider Physics 中科院高能所 张新民 2006.10.28

Cosmology and Collider Physics 中科院高能所 张新民 2006.10.28

Cosmology and Collider Physics 中科院高能所 张新民 2006.10.28. John C. Mather NASA Goddard Space Flight Center, Greenbelt, MD, USA, George F. Smoot University of California, Berkeley, CA, USA. "for their discovery of the blackbody form and

By infinity
(203 views)

Cosmic Microwave Background Radiation (CMBR)

Cosmic Microwave Background Radiation (CMBR)

Cosmic Microwave Background Radiation (CMBR). Relic of the Big Bang ( “afterglow” of initial fireball) predicted in late 1940s Discovered by Penzias & Wilson in 1965 — they won the Nobel Prize for this discovery CMBR studied in detail by satellites (COBE, WMAP)

By rachel
(439 views)

Cosmological Structure Formation A Short Course

Cosmological Structure Formation A Short Course

Cosmological Structure Formation A Short Course. I. Why Dark Matter, and why Cold? Chris Power. Zwicky (1933) measured the radial velocities for eight galaxies in the Coma cluster and found an unexpectedly large velocity dispersion of ~1000 km/s.

By kyna
(170 views)

Lecture 27. Debye Model of Solids, Phonon Gas

Lecture 27. Debye Model of Solids, Phonon Gas

ħ . 1. 3. 2. 3 N. In 1907, Einstein developed the first quantum-mechanical model of solids that was able to qualitatively describe the low- T heat capacity of the crystal lattice. Although this was a crucial step in the right direction, the model was too crude.

By bikita
(719 views)

Cosmology from the Cosmic Microwave Background

Cosmology from the Cosmic Microwave Background

Cosmology from the Cosmic Microwave Background. Katy Lancaster 08/02/08. About Me…. About Me…. ‘Postdoc’ in the Astrophysics group at Bristol working with Professor Mark Birkinshaw, world expert in our field Various projects, OCRA, AMiBA Previously – PhD in Cambridge, working on the VSA

By jacob
(161 views)

Lecture 7

Lecture 7

Demos: U-tube manomoter, Archimedes principle, const fluid height, venturi flowmeter. . Lecture 7. Mechanical sensors: motivations. How do we predict materials failure? . Strength is the ability to withstand force or stress. Predict cracks and collapse in bridges and buildings.

By zack
(139 views)

Cosmology in the 21 st Century

Cosmology in the 21 st Century

Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). Cosmology in the 21 st Century. Chapter 18. Guidepost.

By iram
(110 views)

Spectral Distortions of CMB

Spectral Distortions of CMB

Spectral Distortions of CMB. C. Burigana, A. De Rosa, L. Valenziano, G. Morgante, F. Villa, R. Salvaterra, P. Procopio and N. Mandolesi. Anisotropies. Angular power spectrum. Example:. Polarization. Scattering Thomson of radiation with quadrupole anisotropy generates linear polarization.

By theta
(143 views)

Astronomy

Astronomy

Astronomy. Chapter Nineteen: Galaxies and the Universe. 19.1 Tools of Astronomers 19.2 Stars 19.3 Galaxies and the Universe. 19.3 Galaxies. A galaxy is a huge group of stars, dust, gas, and other objects bound together by gravitational forces.

By karis
(209 views)

International Year of Astronomy 2009 (IYA)

International Year of Astronomy 2009 (IYA)

International Year of Astronomy 2009 (IYA). World-wide celebration of astronomy, its contribution to society and culture 400 th anniversary of first use of astronomical telescope by Galileo. NASA IYA objectives include: strengthen interest in science and science education

By quasar
(99 views)

16.1	Evidence of the Big Bang 16.2	The Big Bang 16.3	Stellar Evolution 16.4	Astronomical Objects 16.5	Problems with the

16.1 Evidence of the Big Bang 16.2 The Big Bang 16.3 Stellar Evolution 16.4 Astronomical Objects 16.5 Problems with the

CHAPTER 16 Cosmology—The Beginning and the End. 16.1 Evidence of the Big Bang 16.2 The Big Bang 16.3 Stellar Evolution 16.4 Astronomical Objects 16.5 Problems with the Big Bang 16.6 The Age of the Universe 16.7 The Future.

By rimona
(279 views)

Unit 11, Chapter 32

Unit 11, Chapter 32

Unit 11, Chapter 32. Integrated Science. Unit Eleven: Astronomy. Chapter 32 The Universe. 32.1 Stars 32.2 Galaxies and the Universe. Chapter 32 Learning Goals. Identify the conditions necessary for fusion to occur inside a star.

By sebastien
(93 views)

UCL Graduate Lectures An Introduction to Cosmology Sarah Bridle A18 2 October 2004

UCL Graduate Lectures An Introduction to Cosmology Sarah Bridle A18 2 October 2004

UCL Graduate Lectures An Introduction to Cosmology Sarah Bridle A18 2 October 2004. Lect 1: Global contents and dynamics of the Universe Lect 2: Dark matter clustering and galaxy surveys Lect 3: The cosmic microwave background radiation Lect 4: Gravitational lensing.

By seamus
(182 views)

Expansion of the Universe

Expansion of the Universe

Expansion of the Universe. Natural consequence of the basic field equations of the General Theory of Relativity (GTR) When GTR was first developed in the 1920s, everyone thought the Universe was static

By vian
(156 views)

Chapter 5: Cosmic foundations for origins of life

Chapter 5: Cosmic foundations for origins of life

Chapter 5: Cosmic foundations for origins of life. Is life a natural consequence of cosmology?. - Evidence for origin of evolution by Big Bang becoming very secure… - expansion of the universe, - cosmic microwave background radiation,

By rafal
(114 views)

Origin of solar system

Origin of solar system

Origin of solar system. “Big Bang’ theory Broadly accepted theory for the origin and evolution of our universe Postulates that the observable universe started from an instantaneously expanding point 13 to 14 billion years ago Since then, the universe has continued to expand

By lore
(220 views)

Cosmology – The Origin and Evolution of the Universe

Cosmology – The Origin and Evolution of the Universe

Cosmology – The Origin and Evolution of the Universe. Expanding Universe – consistent w/ a Big Bang? Olber’s Paradox Large Scale Structure and relation to Dark Matter Evidence for the Big Bang The Cosmic Microwave Background The abundances of the elements

By booker
(146 views)

Exam

Exam

Exam. Final Exam: * Saturday Dec 14 th @ 9am University College Great Hall seats 1-49 * 2 hours Covers material starting with planetary system formation (refer back to previous sections). ~68 questions in 2 hours About a half dozen math questions

By chassidy
(107 views)

Faith, Science and the Human Person

Faith, Science and the Human Person

Faith, Science and the Human Person. Rev. Dr Andrew Pinsent Research Director Ian Ramsey Centre, Faculty of Theology and Religion University of Oxford. Faith, Science and the Human Person. DISTINCTIONS: God, philosophy, religion and faith

By reina
(134 views)

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