'Gravitational lensing' presentation slideshows

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Klopsteg Memorial Lecture Barry Barish Caltech 125th AAPT National Meeting Boise, Idaho 6-Aug-02

Klopsteg Memorial Lecture Barry Barish Caltech 125th AAPT National Meeting Boise, Idaho 6-Aug-02

Klopsteg Memorial Lecture Barry Barish Caltech 125th AAPT National Meeting Boise, Idaho 6-Aug-02. “Catching the Waves with LIGO”. Sir Isaac Newton. Perhaps the most important scientist of all time! Invented the scientific method in Principia

By Thomas
(553 views)

The Search for Gravitational Waves Barry Barish Caltech University of Iowa 16-Sept-02

The Search for Gravitational Waves Barry Barish Caltech University of Iowa 16-Sept-02

The Search for Gravitational Waves Barry Barish Caltech University of Iowa 16-Sept-02. Newton Universal Gravitation. Three laws of motion and law of gravitation (centripetal force) disparate phenomena eccentric orbits of comets cause of tides and their variations

By adamdaniel
(289 views)

พิทยุทธ วงศัจนทร์ วิทยาลัยเพื่อการค้นคว้าระดับรากฐาน

พิทยุทธ วงศัจนทร์ วิทยาลัยเพื่อการค้นคว้าระดับรากฐาน

General Relativity and Black Holes (Overview). 17 th มิถุนายน 2562. พิทยุทธ วงศัจนทร์ วิทยาลัยเพื่อการค้นคว้าระดับรากฐาน. SHEAP2019, IF Naresuan University. Outline. General Relativity. Cosmology. Black Holes. Introduction.

By melosa
(105 views)

Supermassive Black Holes

Supermassive Black Holes

Supermassive Black Holes. Course 689 Presentation by Yan Shi Nov 5, 2009. A Fundamental Relation Between Supermassive Black Holes and their host Galaxies 1 Laura Ferrarese, David Merritt (Published August 2000) Beyond the Bulge: A Fundamental Relation Between

By ziazan
(343 views)

Mini Review: Ocam’s Razor: Start out with simplest assumptions

Mini Review: Ocam’s Razor: Start out with simplest assumptions

Mini Review: Ocam’s Razor: Start out with simplest assumptions Hot Big Bang, Expanding Universe: Only baryonic matter => CMB existence, universe old and large and expanding. CMB too smooth Add non-baryonic matter Galaxies seen early (high 1+z) => CDM

By flavian
(197 views)

Modern Cosmology

Modern Cosmology

Modern Cosmology. Prof Geraint Lewis Sydney Institute for Astronomy University of Sydney. Historically, “cosmology” was the realm of philosophers. Isaac Newton. First mathematical laws of gravity and motion. Thought that an isolated group of stars would collapse in on itself.

By leal
(155 views)

Your next test will be November 14

Your next test will be November 14

Your next test will be November 14. Review session: Friday, Nov. 10, 5:30-7:30 pm Room 205 ENPH-Teaching wing. Summary of Post Main-Sequence Evolution of Stars. Supernova. Fusion proceeds; formation of Fe core. Evolution of 4 - 8 M sun stars is still uncertain.

By carlynda
(251 views)

Astro 101 Test #4 Review

Astro 101 Test #4 Review

Astro 101 Test #4 Review. When: Friday, May 9 at 2pm Where: Regener 103 . Clusters of Galaxies and Large Scale Structure. Outline. Classifying Clusters Morphology-Density Relation Intracluster Gas Dark Matter and Gravitational Lensing Superclusters.

By kimball
(146 views)

General Relativity Physics Honours 2006

General Relativity Physics Honours 2006

General Relativity Physics Honours 2006. A/Prof. Geraint F. Lewis Rm 557, A29 gfl@physics.usyd.edu.au Lecture Notes 6. Gravitational Lensing.

By wanda
(99 views)

Gravity

Gravity

Gravity. Written by: ABDEL DAYEM AL KAHEEL www.kaheel7.com Prepared by: Ahmed Adham ahmed.adham.eg@gmail.com Dina Shawky dinashawkyeg@gmail.com. Our Agenda. In this presentation we will demonstrate the following points: The aim of the presentation. What is gravity?

By kamaria
(449 views)

Dark energy and the CMB

Dark energy and the CMB

Dark energy and the CMB. Robert Crittenden. Work with S. Boughn, T. Giannantonio, L. Pogosian , N. Turok, R. Nichol, P.S. Corasaniti, C. Stephan-Otto. Measurements of CMB anisotropies. Beautiful new data from WMAP and smaller angle experiments What do they tell us about dark energy? .

By clove
(0 views)

Cosmology Final Report: Dark energy and the mass of galaxy clusters C. Bambi, Phys . Rev. D 75 : 083003,2007, arXiv:

Cosmology Final Report: Dark energy and the mass of galaxy clusters C. Bambi, Phys . Rev. D 75 : 083003,2007, arXiv:

Cosmology Final Report: Dark energy and the mass of galaxy clusters C. Bambi, Phys . Rev. D 75 : 083003,2007, arXiv:0703645. R98222063 Pao -Yu Wang 王寶瑜. Outline. Introduction of the idea of this paper The role of cosmological constant Different proposals for accelerating universe

By agatha
(106 views)

Searching for Dark Matter

Searching for Dark Matter

Searching for Dark Matter. Ron-Chou Hsieh CYCU. Outline. It seems to have something there! What are they? Link with physics beyond the SM. DM searches. Constructing a DM model Summary. It seems to have something there!. Galactic rotation curves: In 1932, Dutch astronomer Jan Oort

By udell
(113 views)

Intensity interferometry for imaging dark objects

Intensity interferometry for imaging dark objects

Intensity interferometry for imaging dark objects. Dmitry Strekalov , Baris Erkmen , Igor Kulikov , Nan Yu. Jet Propulsion Laboratory, California Institute of Technology Quantum Sciences and Technology group. Ghost Imaging with thermal light. Theory: Experiment:. Object. Image.

By lamya
(161 views)

Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe

Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe

Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe . Unseen Influences. Dark Matter: An undetected form of mass that emits little or no light but whose existence we infer from its gravitational influence

By shayla
(191 views)

On the Possibility of Gravitational Lensing of Terra Electron-volt Gamma Ray Sources

On the Possibility of Gravitational Lensing of Terra Electron-volt Gamma Ray Sources

On the Possibility of Gravitational Lensing of Terra Electron-volt Gamma Ray Sources . Sean Gellenbeck Mentor: Professor Ann Zabludoff, Steward Observatory 21 st Annual Arizona/NASA Statewide Space Grant Undergraduate Research Internship Program Symposium

By thora
(137 views)

Clusters and Superclusters

Clusters and Superclusters

Clusters and Superclusters. Clusters. Galaxies are not distributed randomly through space Concentrated in groups called Clusters Clusters range from about 10 13 M Sun to about 10 15 M Sun Range in size from 2 Mpc to 10 Mpc across

By lars
(225 views)

The Life Cycle of a Star

The Life Cycle of a Star

The Life Cycle of a Star. Nebula. Giant clouds of gas and dust The birthplace of stars!. Eagle Nebula: 9.5 Light Years Tall!. http://hubblesite.org/gallery/tours/tour-m16/. Creation of a Star.

By xuxa
(131 views)

Detector Mosaic Design Considerations for a Wide FOV Drift-Scan Survey Telescope

Detector Mosaic Design Considerations for a Wide FOV Drift-Scan Survey Telescope

Detector Mosaic Design Considerations for a Wide FOV Drift-Scan Survey Telescope. John T. McGraw Mark R. Ackermann Peter C. Zimmer University of New Mexico and Lt. Eric Golden AFRL. The Near Earth Space Surveillance Initiative (NESSI).

By malia
(144 views)

Members of the IC 342 / Maffei Group

Members of the IC 342 / Maffei Group

Members of the IC 342 / Maffei Group. IC 342. The IC 342 / Maffei Group. Hickson Compact Groups. Hot X-ray Emitting Gas in a Group of Galaxies. NGC 2300 Group of Galaxies. The Virgo Cluster of Galaxies. The Coma Cluster of Galaxies. The Hercules Cluster of Galaxies.

By aderes
(169 views)

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