TO LIFT HEAVY OBJECT with LIGHT Mr.Piyushkumar V.Upadhyay Chemistry Department Shri R.P.Arts,K.B.Commerce and Smt.B.C.J.Science College.Khambhat,Gujarat,India

Total Page:16

File Type:pdf, Size:1020Kb

TO LIFT HEAVY OBJECT with LIGHT Mr.Piyushkumar V.Upadhyay Chemistry Department Shri R.P.Arts,K.B.Commerce and Smt.B.C.J.Science College.Khambhat,Gujarat,India The International journal of analytical and experimental modal analysis ISSN NO: 0886-9367 TO LIFT HEAVY OBJECT WITH LIGHT Mr.Piyushkumar V.Upadhyay Chemistry department Shri R.P.Arts,K.B.Commerce and Smt.B.C.J.Science college.Khambhat,Gujarat,India. Email id: [email protected] Abstract:- Scientists have designed a way to levitate and propel objects using only light, which means objects of many different shapes and from micrometers to meters could be manipulated with a tight beam. With the new research, published in the journal “ Nature photonics”. The key is to create specific nanoscale patterns on an object‟s surface. This paltering interacts with light in such a way that the object can right it self when perturbed,creating a restoring torque to keep in the light beam.Thus,rather than requiring highly focussed laser beams,the object‟s patterning is designed to „encode ‟their own stability .The light source can also be millions of miles away.Atwater said “ There is an audaciously interesting applications to use this technique as a means for propulsion of a new generation of spacecraft.We were a long way from actually doing that,but we are in the process of testing out the principles”. Key words-: Levitation, Light beam,Manipulated,Micrometers, Nanoscale,Object,Photons, Spacecraft. Introduction:- Scientists have designed a way to levitate and propel object‟s using only light, by creating nanoscale patterns on the object‟s surfaces. Though still theoritical,the work is a step toward developing a spacecraft that could reach the nearest planet outside of our solar system in 20 years,powered and accelerated only by light.This means no fuel needed,just a powerful laser fired at a spacecraft from back on Earth. What is levitation? Levitation is the process by which an object as held aloft, without mechanical support in a stable position. About the research With the new research, published in the journal „Nature photonics‟, objects of many different shapes and sizes from micrometers to meters could be manipulated with a light beam. How will it happen? The key is to create specific nanoscale patterns on an object‟s surface. This patterning interact with light in such a way that the object can right itself when perturbed ,creating a restoring torque to keep it in the light beam.Thus,rather than requiring highly focused laser beam,the object‟s pattering is designed to „encode‟their own stability .The light source can also be millions of miles away.In theory,this spacecraft could be patterned with nanoscale structure and accelerated by Earth- based laser light.Without needling to carry fuel,the spacecraft could reach very high,even relativistic speeds and possibly travel to other stars. Breakthough that laid the ground work for this research.Decades ago,the developments of so-called optical tweezers enabled scientists to move and manipulate tiny objects, tiny objects,like nanoparticles,using the radiative pressure from a sharply focussed beam of laser light. Methods and materials:- Light has been put to work generating the same force that makes airplanes fly,a study appearing online December 5,in Nature protonics shows,with the right design,a uniform steam of light has pushed tiny objects in much the same way that an airplane wing hoists a,747 off the ground.The idea of moving objects with light is not a new one.Solar sails,such as those used by Japan‟s IKARDOS spacecraft,harness the Sun‟s radiation for propulsion,but researchers at the Rochesters Institute of Technology have shown that light can also generate the much more complex force known as lift-the same force that allows airplanes wings to hoist them aloft as they move through the air. Using only light,Australian researchers say they are able to move small particles almost five feet through the air.It‟s more than 100 times the distance achieved by existing optical ‟Tweezers“ the researchers say.The U.S.secreatary of Energy,Steven chu,,won his Nobel prize for work with optical tweezers.But,Anderi Rhode and colleagues at the Australian National University say their new laser device can move glass objects hundreds of times of times bigger than bacteria,and show them a meter and half (5feet) or more . “ One can levitate a ping pong ball using a steady stream of air from a hair dryer ,but it would not work if the ping pong ball was too big ,or if it was too big,or if it was too far away from the hair dryer and so on”. The key to the new research is in creating nano-scale reflection patterns on the surface of the object to be levitated.By giving the surface of the object the right patterns it will interact with the light beam in such a way that it will continually spin it self back into the light ,creating a feedback loop of sorts with the radiative pressure of light all the way to another star system.If it works,this technology would allow starships to travel at close to the speed of light and would open up a whole new possibilities for the future of sustained interstellar travel,trying to squeeze out the little bit of propulsion.We could from it,when all we really needed was a big flashlight. Though the theory is still untested in the real work,the researchers say that if it pans out ,it could send a spacecraft to the nearest star outside our solar system in just 20 years.As new and better experiments come online over the next few years,it is likely that tiny object being pushed around by light will be testing some big ideas. Volume XI, Issue XI, NOVEMBER/2019 Page No:47 The International journal of analytical and experimental modal analysis ISSN NO: 0886-9367 Results and discussions:- When a blue laser light is sent above an object in a laminar beam,the object under the beam looses the weight .The results seems to indicate that the percentage of weight loss varies directly with the intensity of the amount of lumen of the light beam.Light beam can change the direction of the force of gravity, it follows to show that gravity is caused by something moving at the speed of light,that speed was confirmed by the discovery of gravity by LIGO. The technique allows you to manage an object located many kilometres away from you.This means that the control beam can move spacecraft.The technology has prospects on Earth-for example,it will accelerate the production of printed circuit board and other electronics. Another way to make objects levitate is to act on them with sound waves.A breakthrough in acoustic levitation was made by researchers from the UK.They learned to lift object in the air using ultrasound,bending around obstacles. When a light beam reflects or scatters off an object, the object will recoil.This so-called optical force is used,for example to trap glass beads in optical tweezers.Light can also exert force through the photoelectric effect,where preferential absorption of light on one sight of an object leads to a temperature difference that causes the object to move.The air molecules on the hot side heat up,and their collisions with the object deliever more momentum than those on the colder side,producing motion,as in the rotation of a radiometer (light mill). Experiments in air with an optical fiber that narrows down to a point,like a needle,when light is channelled through this tapered fiber,the amount that leaks out (the evanescent field) increase as you approach the tip.This escaping light generates the optical and photophoretic forces.As their light-interacting object,the team choose a hexagonally –shaped gold plate that was 10 micrometers across and 30 nanometers thick.The team titled their fiber down at a slight angle on top of 90 and placed the plate on top of the fiber,near the end.In multiple trials,the team send a broad spectrum light beam into the fiber and observed the plate sliding up the fiber,about the 20 micrometers or so. Photons have real mass and velocity ,then they have kinetic energy(KE).That KE comes from its linear velocity and its rotational velocity seen.It is the transfer of that kinetic energy,with impact force,that kinetic energy with impact force that allows multitudes of photons of light to heat and to push matter.The ability of light to apply pressure to object is known as radiation processure,which was first postulated in 1619 and proven 1900.This is the principle behind the solarsail,which uses light radiation pressure to move through space.Light is also capable of creating the more complex force of “lift” which is the force generated by air foils that make an airplane rise upwards as it travel forwards.In optical lift,created by a “light foils” the lift is created within the transparent object as light shines through it and is refracted by its inner surfaces.In the light foil rods a greater proportion of light leaves in a direction perpendicular to the beam and this side therefore experiences a larger radiation pressure. Conclusion:- People could lift very heavy objects,such as large stone and some heavy object with light .It can also help people to make other kind of physical work easier by using light beam.The way levers work is by multiplying the effort exerted by the users,specifically,to lift and balance an object,the effort force the user applies multiplied by its distance to the fulcrum must equal the load force multiplies by its distance to the fulcrum.Lifting operations are inherent to many occupations in the constructions industries.
Recommended publications
  • Frontiers in Optics 2010/Laser Science XXVI
    Frontiers in Optics 2010/Laser Science XXVI FiO/LS 2010 wrapped up in Rochester after a week of cutting- edge optics and photonics research presentations, powerful networking opportunities, quality educational programming and an exhibit hall featuring leading companies in the field. Headlining the popular Plenary Session and Awards Ceremony were Alain Aspect, speaking on quantum optics; Steven Block, who discussed single molecule biophysics; and award winners Joseph Eberly, Henry Kapteyn and Margaret Murnane. Led by general co-chairs Karl Koch of Corning Inc. and Lukas Novotny of the University of Rochester, FiO/LS 2010 showcased the highest quality optics and photonics research—in many cases merging multiple disciplines, including chemistry, biology, quantum mechanics and materials science, to name a few. This year, highlighted research included using LEDs to treat skin cancer, examining energy trends of communications equipment, quantum encryption over longer distances, and improvements to biological and chemical sensors. Select recorded sessions are now available to all OSA members. Members should log in and go to “Recorded Programs” to view available presentations. FiO 2010 also drew together leading laser scientists for one final celebration of LaserFest – the 50th anniversary of the first laser. In honor of the anniversary, the conference’s Industrial Physics Forum brought together speakers to discuss Applications in Laser Technology in areas like biomedicine, environmental technology and metrology. Other special events included the Arthur Ashkin Symposium, commemorating Ashkin's contributions to the understanding and use of light pressure forces on the 40th anniversary of his seminal paper “Acceleration and trapping of particles by radiation pressure,” and the Symposium on Optical Communications, where speakers reviewed the history and physics of optical fiber communication systems, in honor of 2009 Nobel Prize Winner and “Father of Fiber Optics” Charles Kao.
    [Show full text]
  • NIAC Final Report Steering of Solar Sails Using Optical Lift Force
    NIAC Final Report Steering of Solar Sails Using Optical Lift Force Grover A. Swartzlander, Jr. Rochester Institute of Technology Acknowledgements Alexandra Artusio-Glimpse, Rochester Institute of Technology, Rochester, NY Alan Raisanen, Rochester Institute of Technology, Rochester, NY Stephen Simpson, Univ. Bristol, UK Charles (Les) Johnson, NASA Marshall Space Flight Center, Huntsville, AL Andrew Heaton, NASA Marshall Space Flight Center, Huntsville, AL Catherine Faye, NASA Langley, Langley, VA John Dankanich, NASA Glenn, Cleveland, OH Amy Davis, NeXolve Corp., Huntsville, AL SUMMARY Optical wing structures were theoretically and numerically analyzed, and prototype arrays of wings called optical flying carpets were fabricated with solar sail material clear polyimide (CP1). This material was developed at NASA Langley to better withstand damaging ultraviolet radiation found in outer space. Various optical wing sizes and shapes were analyzed to develop design strategies for thrust and torque applications. The developed ray-tracing model has undergone continual advancement, and stands as an effective tool for modeling most types of solar sails. To our understanding, such a model does not exist elsewhere. The distributed forces and torques have been reduced to a simple theoretical whereby the fundamental mechanics may be understood in terms of the numerically determined center of pressure offset from the center of mass. This description applies to any type of solar sail, affording our ray-tracing model a general utility. This research has established a foundation for understanding the force and torque afforded by optical wings. The study began by considering transparent wings and ended by considering wings having a reflecting face. The latter was found to afford the advantages of high thrust and both intrinsic and extrinsic torque.
    [Show full text]
  • Non Conservative Optical Forces for Silicon Nanowires in Optical Traps
    NON CONSERVATIVE OPTICAL FORCES FOR SILICON NANOWIRES IN OPTICAL TRAPS A. MAGAZZU1,2,*, A. IRRERA1, P. ARTONI3, S. H. SIMPSON4, S. HANNA4, P. H. JONES5, F. PRIOLO3, P. G. GUCCIARDI1, and O. M. MARAGÓ1,* 1 CNR-IPCF, Istituto per i Processi Chimico-Fisici, Messina, Italy 2 Dottorato in Fisica, Università di Messina , Messina, Italy 3 Matis CNR-IMM and Dipartimento di Fisica, Università di Catania, Catania, Italy 4 H. H. Wills Physics Laboratory, University of Bristol, Bristol, UK 5 Department of Physics and Astronomy, University College London, London, UK *Corresponding authors: [email protected], [email protected] Abstract For a non-spherical particle the non-conservative forces We measure non-conservative forces in optical can be considered composed by two contributions. A first trapping of ultra-thin Silicon nanowires by photonic force contribution depends on the standard non-homogeneous and torque microscopy. We reveal how the extreme non- radiation pressure due to the gaussian geometry of the spherical shape generates a transverse component of the laser beam that may yield a rotational force in ρ-z plane radiation pressure that results in a thermally activated even for a spherical trapped particle [4,5]. The second non-conservative rotation of the nanowire about the trap contribution, manifest for nonspherical objects, depends axis. We explore the behavior with trapping power and on alignment along the axial direction, that generates a scaling with nanowire length. This has implications for transverse force (optical lift effect) [6] that causes rotations optical force calibration and optomechanics with levitated and precessions in the ρ-z plane.
    [Show full text]
  • Poster Presentations
    POSTER PRESENTATIONS Optics, Photonics, and Imaging 1 Terahertz Techniques Based on Laser-Induced Microplasmas Fabrizio Buccheri, Institute of Optics, University of Rochester 2 HapTech - Haptic Enabled VR for a Developing Market Lucian Copeland, Computer Science Department, University of Rochester / HapTech 3 Thickness Estimation with Optical Coherence Tomography and Statistical Decision Theory Jinxin Huang1, Patrice Tankam1, Cristina Canvesi2, and Jannick P. Rolland1,2, 1Institute of Optics, University of Rochester, 2LighTopTech Corporation 4 Further THz Array Development and Characterization Craig McMurtry1, Judith L. Pipher1, Zeljko Ignjatovic1, Mark Bocko1, Jagannath Dayalu1, Zoran Ninkov2, Katherine Seery2, Sahil Bhandari2, Kenneth D. Fourspring3, Dan Newman3, Andrew P. Sacco3, Frank Ryan3, Paul Lee4, 1University of Rochester, 2Rochester Institute of Technology, 3Exelis, 4Consultant 5 Lensless measurements of spatial coherence in the Fresnel region Katelynn A. Sharma, Amber C. Betzold, Miguel A. Alonso, Thomas G. Brown, Institute of Optics, University of Rochester 6 Fiber Pump-Delivery System for Spectral Narrowing and Wavelength Stabilization of Broad- Area Lasers Jordan P. Leidner, John R. Marciante, Institute of Optics, University of Rochester 7 Cerium Oxide Polishing Slurry Reclamation Project: Characterization Techniques and Results Kameron Tinkham1,4, Tess Jacobs1,4, Mark Mayton2, Zachary Hobbs3 , Stephen Jacobs1,4 1Institute of Optics, University of Rochester, 2Flint Creek Resources, Inc., Gorham, NY, 3Sydor Optics, Rochester, NY, 4Laboratory for Laser Energetics, University of Rochester 8 Eikonal+: Optical Design and Visualization Platform for Freeform Optical Instrumentation Daniel Nikolov1, Adam Hayes1, Robert Gray1, Miguel A. Alonso1, Jon Petruccelli2, Jannick P. Rolland1, 1Institute of Optics, University of Rochester, 2Department of Physics, University of Albany 9 Off-null measurements applied to process monitoring using focused beam scatterometry Anthony Vella, Michael J.
    [Show full text]
  • Measurements of Radiation Pressure Owing to the Grating Momentum
    Measurements of Radiation Pressure owing to the Grating Momentum Ying-Ju Lucy Chu1, Eric M. Jansson2, and Grover A. Swartzlander, Jr.1∗ 1Chester F. Carlson Center for Imaging Science, Rochester Institute of Technology 2Charter School of Wilmington, Wilmington, Delaware April 16, 2018 Abstract The force from radiation pressure owing to the grating momentum was measured for a thin transmissive fused silica grating near the Littrow angles at wavelengths of 808 nm and 447 nm. A significant magnitude of force was measured in the direction parallel to the grating surface. We also confirmed that the component of force normal to the grating surface may vanish. This forcing law is characteristically different from radia- tion pressure on a reflective surface, and thus, opens new opportunities for light-driven applications such as solar or laser driven sailcraft, or the transport of objects in liquids. Since Maxwell first predicted radiation pressure in 1873 [1], it has helped to de- scribe phenomena ranging from the astronomical to the quantum realm. For ex- ample the gravitational collapse of stars and accretion dynamics are governed by radiation pressure [2,3]. Experimental evidence of Kepler's 1619 explanation of comet tails [4,5] was later extended to the general distribution of interplanetary dust [6, 7]. Terrestial applications have found uses in biology as optical tweez- ers [8], laser cooling of atoms [9,10] and macroscopic objects [11,12]. The detec- tion of gravitational waves by means of laser interferometers requires an account- ing of radiation pressure [13]. Micro-structures such as optical wings [14] and slot waveguides have promising photonic applications [15, 16].
    [Show full text]
  • Steering of Solar Sails Using Optical Lift Force
    NIAC Final Report – Summary of Research NASA Award NNX11AR40G Steering of Solar Sails Using Optical Lift Force Grover A. Swartzlander, Jr. Rochester Institute of Technology Acknowledgements Alexandra Artusio-Glimpse, Rochester Institute of Technology, Rochester, NY Alan Raisanen, Rochester Institute of Technology, Rochester, NY Stephen Simpson, Univ. Bristol, UK Charles (Les) Johnson, NASA Marshall Space Flight Center, Huntsville, AL Andrew Heaton, NASA Marshall Space Flight Center, Huntsville, AL Catherine Faye, NASA Langley, Langley, VA John Dankanich, NASA Glenn, Cleveland, OH Amy Davis, NeXolve Corp., Huntsville, AL SUMMARY Optical wing structures were theoretically and numerically analyzed, and prototype arrays of wings called optical flying carpets were fabricated with solar sail material clear polyimide (CP1). This material was developed at NASA Langley to better withstand damaging ultraviolet radiation found in outer space. Various optical wing sizes and shapes were analyzed to develop design strategies for thrust and torque applications. The developed ray-tracing model has undergone continual advancement, and stands as an effective tool for modeling most types of solar sails. To our understanding, such a model does not exist elsewhere. The distributed forces and torques have been reduced to a simple theoretical whereby the fundamental mechanics may be understood in terms of the numerically determined center of pressure offset from the center of mass. This description applies to any type of solar sail, affording our ray-tracing model a general utility. This research has established a foundation for understanding the force and torque afforded by optical wings. The study began by considering transparent wings and ended by considering wings having a reflecting face.
    [Show full text]
  • Lateral Optical Force on Chiral Particles Near a Surface
    Lateral Optical Force on Chiral Particles Near a Surface S. B. Wang and C. T. Chan* Department of Physics and Institute for Advanced Study, The Hong Kong University of Science and Technology, Clear Water Bay, Hong Kong, P. R. China * Email: [email protected] Abstract Light can exert radiation pressure on any object it encounters and that resulting optical force can be used to manipulate particles. It is commonly assumed that light should move a particle forward and indeed an incident plane wave with a photon momentum k can only push any particle, independent of its properties, in the direction of k . Here we demonstrate using full- wave simulations that an anomalous lateral force can be induced in a direction perpendicular to that of the incident photon momentum if a chiral particle is placed above a substrate that does not break any left-right symmetry. Analytical theory shows that the lateral force emerges from the coupling between structural chirality (the handedness of the chiral particle) and the light reflected from the substrate surface. Such coupling induces a sideway force that pushes chiral particles with opposite handedness in opposite directions. 1 Electromagnetic (EM) waves carry linear momentum as each photon has a linear momentum of k in the direction of propagation. Circularly polarized light carries angular momentum due to the intrinsic spin angular momentum (SAM) of photons1-6. When light is scattered or absorbed by a particle, the transfer of momentum can cause the particle to move. Thus light can be used to manipulate particles7-25. Light will push a particle in the direction of light propagation (as illustrated in Fig.
    [Show full text]
  • Measurements of Radiation Pressure on Diffractive Films
    Rochester Institute of Technology RIT Scholar Works Theses 8-2021 Measurements of Radiation Pressure on Diffractive Films Ying-Ju Lucy Chu Follow this and additional works at: https://scholarworks.rit.edu/theses Measurements of Radiation Pressure on Diffractive Films by Ying-Ju Lucy Chu B.S. National Cheng Kung University, Taiwan, 2013 M.S. Biomedical Engineering, 2015 A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Chester F. Carlson Center for Imaging Science College of Science Rochester Institute of Technology [August, 2021] Signature of the Author Accepted by Coordinator, Ph.D. Degree Program Date CHESTER F. CARLSON CENTER FOR IMAGING SCIENCE COLLEGE OF SCIENCE ROCHESTER INSTITUTE OF TECHNOLOGY ROCHESTER, NEW YORK CERTIFICATE OF APPROVAL Ph.D. DEGREE DISSERTATION The Ph.D. Degree Dissertation of Ying-Ju Lucy Chu has been examined and approved by the dissertation committee as satisfactory for the dissertation required for the Ph.D. degree in Imaging Science [Dr. Grover Swartzlander], Dissertation Advisor [Dr. Karl Hirshman], External Chair [Dr. Zoran Ninkov] [Dr. Mihail Barbosu] Date ii Measurements of Radiation Pressure on Diffractive Films by Ying-Ju Lucy Chu Submitted to the Chester F. Carlson Center for Imaging Science in partial fulfillment of the requirements for the Doctor of Philosophy Degree at the Rochester Institute of Technology Abstract One of the few ways to reach distant stars is by radiation pressure, in which photon mo- mentum is harnessed from free sunlight or extraordinarily powerful laser systems. Large but low mass light-driven sails reflect photons and transfer momentum to the sailcraft, providing large velocity from continuous acceleration.
    [Show full text]
  • POLLARD-DISSERTATION-2016.Pdf (4.640Mb)
    GAS PHASE SWITCHING FOR PULSED POWER APPLICATIONS A Dissertation by WILLIAM NICHOLS POLLARD Submitted to the Office of Graduate and Professional Studies of Texas A&M University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Chair of Committee, David Staack Committee Members, Gerald Morrison Sy-Bor Wen Edward White Head of Department, Andreas Polycarpou May 2016 Major Subject: Mechanical Engineering Copyright 2016 William Nichols Pollard ABSTRACT This dissertation serves to increase the understanding of applied pulsed plasma. Pulsed plasmas are experimentally studied in three contexts 1) fundamentally as switches, 2) applied in a dense plasma focus (DPF), and 3) applied as flow actuators. In these contexts the systems were studied with voltage, repetition frequency, energy, and pulse duration, ranges from 10 – 100 kV, 1 to 20 kHz, 1 mJ to 1 J, and 5 to 100 ns respectively depending on the requirements of ultimate application. These high voltages at high frequency push the current limits of spark switches. Attaining desired conditions required an understanding of the plasma switching characteristics, electrical coupling with the load, and the ultimate application. In the first experimental study plasma pulsing limitation were determined. In these experiments a DC pulsed plasma is pushed to its limits (within constraints) to determine maximum pulsing frequency while maintaining 10 kV available to drive novel applications. In these experiments 137 mJ of energy were pulsed at a frequency of 20 kHz with full-width half-max of 8 ns. Similar pulsing at 42 kHz was observed while maintaining roughly 5 kV. Operating performance was governed by electrode material, discharge gas/flow, chamber pressure, and circuit elements, both intentional and parasitic.
    [Show full text]
  • Interplay of Optical Force and Ray-Optic Behavior Between Luneburg Lenses † ‡ ‡ § ‡ ‡ Alireza Akbarzadeh,*, J
    Article pubs.acs.org/journal/apchd5 Interplay of Optical Force and Ray-Optic Behavior between Luneburg Lenses † ‡ ‡ § ‡ ‡ Alireza Akbarzadeh,*, J. A. Crosse, Mohammad Danesh, , Cheng-Wei Qiu, Aaron J. Danner, † ∥ and Costas M. Soukoulis , † Institute of Electronic Structure and Laser, Foundation for Research and Technology-Hellas, Heraklion, Crete, Greece 71110 ‡ Department of Electrical and Computer Engineering, National University of Singapore, 4 Engineering Drive 3, Singapore 117576 § Electronics and Photonics Department, Institute of High Performance Computing, 1 Fusionopolis Way, Singapore 138632 ∥ Ames Laboratory and Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, United States ABSTRACT: The method of force tracing is employed to examine the optomechanical interaction between two and four Luneburg lenses. Using a simplified analytical model, as well as a realistic numerical model, the dynamics of elastic and fully inelastic collisions between the lenses under the illumination of collimated beams are studied. It is shown that elastic collisions cause a pair of Luneburg lenses to exhibit oscillatory and translational motion simultaneously. The combination of these two forms of motion can be used to optomechanically manipulate small particles. Additionally, it is addressed how fully inelastic collisions of four Luneburg lenses can help us achieve full transparency as well as isolating space to trap particles. KEYWORDS: optical force, geometrical optics, optical manipulation, graded-index media, metamaterials
    [Show full text]
  • NIAC Final Report Steering of Solar Sails Using Optical Lift Force
    NIAC Final Report Steering of Solar Sails Using Optical Lift Force Grover A. Swartzlander, Jr. Rochester Institute of Technology Acknowledgements Alexandra Artusio-Glimpse, Rochester Institute of Technology, Rochester, NY Alan Raisanen, Rochester Institute of Technology, Rochester, NY Stephen Simpson, Univ. Bristol, UK Charles (Les) Johnson, NASA Marshall Space Flight Center, Huntsville, AL Andrew Heaton, NASA Marshall Space Flight Center, Huntsville, AL Catherine Faye, NASA Langley, Langley, VA John Dankanich, NASA Glenn, Cleveland, OH Amy Davis, NeXolve Corp., Huntsville, AL SUMMARY Optical wing structures were theoretically and numerically analyzed, and prototype arrays of wings called optical flying carpets were fabricated with solar sail material clear polyimide (CP1). This material was developed at NASA Langley to better withstand damaging ultraviolet radiation found in outer space. Various optical wing sizes and shapes were analyzed to develop design strategies for thrust and torque applications. The developed ray-tracing model has undergone continual advancement, and stands as an effective tool for modeling most types of solar sails. To our understanding, such a model does not exist elsewhere. The distributed forces and torques have been reduced to a simple theoretical whereby the fundamental mechanics may be understood in terms of the numerically determined center of pressure offset from the center of mass. This description applies to any type of solar sail, affording our ray-tracing model a general utility. This research has established a foundation for understanding the force and torque afforded by optical wings. The study began by considering transparent wings and ended by considering wings having a reflecting face. The latter was found to afford the advantages of high thrust and both intrinsic and extrinsic torque.
    [Show full text]
  • Ray-Traced Simulation of Radiation Pressure for Optical Lift Timothy Peterson
    Rochester Institute of Technology RIT Scholar Works Theses Thesis/Dissertation Collections 2011 Ray-traced simulation of radiation pressure for optical lift Timothy Peterson Follow this and additional works at: http://scholarworks.rit.edu/theses Recommended Citation Peterson, Timothy, "Ray-traced simulation of radiation pressure for optical lift" (2011). Thesis. Rochester Institute of Technology. Accessed from This Thesis is brought to you for free and open access by the Thesis/Dissertation Collections at RIT Scholar Works. It has been accepted for inclusion in Theses by an authorized administrator of RIT Scholar Works. For more information, please contact [email protected]. Ray-Traced Simulation of Radiation Pressure for Optical Lift by Timothy J. Peterson A Thesis Submitted in Partial Fulfillment of the Requirements for the Degree of Master of Science in Computer Science Supervised by Associate Professor Dr. Grover Swartzlander Center for Imaging Science, Department of Physics Rochester Institute of Technology Rochester, New York November 8, 2011 Approved by: Dr. Joe Geigel, Associate Professor Thesis Advisor, Department of Computer Science Dr. Grover Swartzlander, Associate Professor Reader, Center for Imaging Science, Department of Physics Dr. Hans-Peter Bischof, Professor Observer, Department of Computer Science ii Abstract Ray-Traced Simulation of Radiation Pressure for Optical Lift Timothy J. Peterson Advisor: Dr. Joe Geigel When light refracts at a surface, it changes the direction and intensity of the light rays. By Newton’s 3rd law, this process imparts a small momentum to the object. This effect can be exploited to manipulate very small objects, by carefully selecting the shape and optical properties of the object.
    [Show full text]