Gradient Refractive Index Gradient Refractive Index The refractive index of a particular point of a lens with a gradient refractive index The refractive.

Slides:



Advertisements
Similar presentations
Building a Mock Universe Cosmological nbody dark matter simulations + Galaxy surveys (SDSS, UKIDSS, 2dF) Access to mock catalogues through VO Provide analysis.
Advertisements

Stochastic Gravitational Lensing and the Nature of Dark Matter Chuck Keeton Rutgers University Gravitational lens database --
Outline Brief, non-technical introduction to strong (multiple image) lensing Bayesian approach to the reconstruction of lens mass distribution Overview.
The Large Scale Structure of the Universe Clusters of galaxies X-rays from clusters of galaxies Sheets and voids.
1© Manhattan Press (H.K.) Ltd. Final image at infinity Eye-ring Eye-ring 12.6 Refracting telescope.
Analysis of a New Gravitational Lens FLS Yoon Chan Taak Feb Survey Science Group Workshop
X-Ray Measurements of the Mass of M87 D. Fabricant, M. Lecar, and P. Gorenstein Astrophysical Journal, 241: , 15 October 1980 Image:
Astrophysical applications of gravitational microlensing By Shude Mao Ziang Yan Department of Physics,Tsinghua.
H.-W. Rix, Vatican 2003 Gravitational Lensing as a Tool in Cosmology A Brief History of Lensing 1704 Newton (in Optics): „Do not bodies act upon light.
Color Anomaly in Multiple Quasars - Dust Inhomogeneity or Quasar Microlensing - Atsunori Yonehara (Univ. Tsukuba) with Hiroyuki Hirashita (Nagoya Univ.)
Optical Scalar Approach to Weak Gravitational Lensing by Thick Lenses Louis Bianchini Mentor: Dr. Thomas Kling Department of Physics, Bridgewater State.
Gravitational Lenses The First Discoveries. Summary: - first detections of gravitational deflection of light - some early theoretical developments - discovery.
PRESENTATION TOPIC  DARK MATTER &DARK ENERGY.  We know about only normal matter which is only 5% of the composition of universe and the rest is  DARK.
General Relativity Physics Honours 2006 A/Prof. Geraint F. Lewis Rm 557, A29 Lecture Notes 6.
Strong Lensing in RCS-2 Clusters Matt Bayliss University of Chicago Department of Astronomy & Astrophysics Great Lakes Cosmology Workshop 8 – June 2, 2007.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 12; February
General Relativity Physics Honours 2006 A/Prof. Geraint F. Lewis Rm 557, A29 Lecture Notes 5.
Dark matter and black holes over cosmic time TOMMASO TREU.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 13; February
What’s new here? The accuracy of the thin lens approximation has been assessed through convergence of statistics by increasing the number of lens planes.
14 Black Holes and General Relativity Stuff that warps your mind.
Lenses Physics 202 Professor Lee Carkner Lecture 21.
Einstein’s Lens Presented by: Kevin McLin, SSU NASA E/PO 2008 EA Training, SSU Einstein’s Lens.
Ge/Ay133 What (exo)-planetary science can be done with microlensing?
Phy 212: General Physics II Chapter : Topic Lecture Notes.
Probing Small-Scale Structure in Galaxies with Strong Gravitational Lensing Arthur Congdon Rutgers University.
PX437 EXOPLANETS Horne PX437 EXOPLANETS Gravitational microlensing Paczynski 1996, ARA&A 34, 419 Observer Lensing mass Background source.
Astronomía Extragaláctica y Cosmología ObservacionalDepto. de Astronomía (UGto) Lecture 11 Groups and Clusters of Galaxies – III (DM) Virial Mass Estimates.
Refraction Physics Department, New York City College of Technology.
What is the Dark Matter? What about “ordinary” non-luminous matter (basically, made from proton, neutrons and electrons)? “Dead stars” (White Dwarfs,
Physics 7C SS1 Lecture 6: Electricity Analogies with Gravity: Electric Force, Electric Field, Electric Potential Energy, Electric Potential, As you wait.
Astro 101 Slide Set: Multiple Views of an Extremely Distant Galaxy 0 Topic: Distant galaxies Concepts: Galaxy development, Gravitational lensing Missions:
Gravitational lensing in plasma O.Yu. Tsupko 1,2 and G.S. Bisnovatyi-Kogan 1,2 1 Space Research Institute of Russian Academy of Science, Profsoyuznaya.
LIGHT: Geometric Optics. The Ray Model of Light Light travels in straight lines under a wide variety of circumstances Light travels in straight line paths.
Eric V. Linder (arXiv: v1). Contents I. Introduction II. Measuring time delay distances III. Optimizing Spectroscopic followup IV. Influence.
1 Galaxies at Cosmic Dawn Revealed in the First Year of the Hubble Frontier Fields Initiative Dr. Gabriel Brammer (ESA/AURA, STScI) Hubble Science Briefing.
Gravitational lensing of the CMB Richard Lieu Jonathan Mittaz University of Alabama in Huntsville Tom Kibble Blackett Laboratory, Imperial College London.
Einstein’s Lens Presented by: Name, Affiliation Location and Date here Einstein’s Lens.
Searches for exoplanets
GRAVITATIONAL LENSING
A Short Talk on… Gravitational Lensing Presented by: Anthony L, James J, and Vince V.
PREDRAG JOVANOVIĆ AND LUKA Č. POPOVIĆ ASTRONOMICAL OBSERVATORY BELGRADE, SERBIA Gravitational Lensing Statistics and Cosmology.
Today’s agenda: Death Rays. You must know when to run from Death Rays. Refraction at Spherical Surfaces. You must be able to calculate properties of images.
Gravitational Lensing
Exploring Dark Matter through Gravitational Lensing Exploring the Dark Universe Indiana University June 2007.
Dark Matter and Dark Energy By: Matt Tanaka And Bryent Kaneshiro.
Einstein’s Lens Presented by: Name, Affiliation Location and Date here Einstein’s Lens.
Michael Doran Institute for Theoretical Physics Universität Heidelberg Time Evolution of Dark Energy (if any …)
Studying cool planets around distant low-mass stars Planet detection by gravitational microlensing Martin Dominik Royal Society University Research Fellow.
Wide-field Weak Lensing Mass Reconstructions of Merging Galaxy Clusters Brett Ragozzine, Douglas Clowe Ohio University, Department of Physics & Astronomy,
Space Warps. Light is believed to travel the shortest distance between two points But…… the path of light is curved in the presence of a gravitational.
Constraining Cosmography with Cluster Lenses Jean-Paul Kneib Laboratoire d’Astrophysique de Marseille.
The effects of the complex mass distribution of clusters on weak lensing cluster surveys Zuhui Fan Dept. of Astronomy, Peking University.
10/5/2004New Windows on the Universe Jan Kuijpers Part 1: Gravitation & relativityPart 1: Gravitation & relativity J.A. Peacock, Cosmological Physics,
How did the universe begin?. How do we know? Doppler Shift Lower pitched, longer wavelength Higher pitched, shorter wavelength.
H8: Evidence for general relativity
Dark Matter Facts Only 20% of all known matter is the matter we can see, or “normal matter.” The other 80% is Dark Matter, which is also around us just.
Refraction.
Lecture 16 Interference Chapter 24.1  24.4 Outline Conditions for Interference Experiments Showing Interference Interference in Thin Films.
Metamaterials Andrew Houck, Dave Kong, Matt Reynolds, Peter Eckley, J. Kong, Ike Chuang, Joe Jacobson.
A systematic analysis of caustic methods for galaxy clsuter masses
Probing Dark Energy with Cosmological Observations Fan, Zuhui ( 范祖辉 ) Dept. of Astronomy Peking University.
March 7, 2016March 7, 2016March 7, 2016Yerevan, Armenia1 GRAVITATIONAL LENSING GRAVITATIONAL LENSING History, Discovery and Future Measuring Mass of Dark.
Geometric Optics: Mirrors and Lenses. Mirrors with convex and concave spherical surfaces. Note that θ r = θ i for each ray.
N-body Simulations and Gravitational Lensing with Dark Energy Beyond Einstein Meeting, May 13, 2004.
Thomas Collett Institute of Astronomy, Cambridge
Cosmology with gravitational lensing
Chapter 16 Active Galaxy.
What (exo)-planetary science can be done with microlensing?
The invisibles of the Universe
Presentation transcript:

Gradient Refractive Index Gradient Refractive Index The refractive index of a particular point of a lens with a gradient refractive index The refractive index of a particular point of in a lens with a radial gradient refractive index The effects of gravitational potential as related to the effects of a refractive index G.R.I.N. LENS

In reality we have multiple masses… Vector superposition! “The total deflection angle is the vector superposition of the deflections due to all the mass elements of the lens.” (Blandford et al. 825) Angle of deflection: One ray. One Mass. Surface density must exceed critical mass density somewhere within the gravitational lens. For multiple images, the object must lie within the cusp.

Ray Tracing: Multiple images Caustic cusp due to the gravitational lens is shown in ray tracing using the angle of deflection for individual rays in superposition. Einstein Ring First complete ring observed Hubble Telescope (1998)

Angular Deflection

Density Perturbations, Image to source mapping, Time delay R (Image)  S (Source) Time delay calculation is composed of the geometrical delay and the potential time delay

References Blandford, R., et al. Gravitational Lens Optics..JSTOR. Science. 245: Web. Nov Blandford, R., et al. Gravitational Lens Optics..JSTOR. Science. 245: Web. Nov Bradac, M., et al. Revealing The Properties of Dark Matter in the Merging Cluster Macs J arXiv: v2 [astro-ph] Web. Nov Bradac, M., et al. Revealing The Properties of Dark Matter in the Merging Cluster Macs J arXiv: v2 [astro-ph] Web. Nov Levine, H., A. Petters, J.Wambsganss. Singularity Theory and Gravitational Lensing. Boston: Birkhauser, Levine, H., A. Petters, J.Wambsganss. Singularity Theory and Gravitational Lensing. Boston: Birkhauser, Mellier, Y., et al. Lecture Notes in Physics: Gravitational lensing. Berlin: Springer-Verlag, Mellier, Y., et al. Lecture Notes in Physics: Gravitational lensing. Berlin: Springer-Verlag, 1990.

Images King, L. U. Manchester. NICMOS,HST, NASA King, L. U. Manchester. NICMOS,HST, NASA Tsioulia, Andrew,. Gradient Index (GRIN) Lens ~db=all~dumptype=rss Tsioulia, Andrew,. Gradient Index (GRIN) Lens ~db=all~dumptype=rss Solar Eclipses Overview &fbodylongid=1786 Solar Eclipses Overview &fbodylongid= &fbodylongid= &fbodylongid=1786 Grin Micro Lens. 20/Lens.htm Grin Micro Lens. 20/Lens.htm 20/Lens.htm 20/Lens.htm Optica Software. Optica Software.