Lateral Optical Force on Chiral Particles Near a Surface
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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. -
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. -
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. -
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. -
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. -
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]. -
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. -
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. -
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. -
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 -
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. -
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.