Cavity Ringdown Laser Absorption Spectroscopy: History, Development, and Application to Pulsed Molecular Beams
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Self Amplified Lock of a Ultra-Narrow Linewidth Optical Cavity
Self Amplified Lock of a Ultra-narrow Linewidth Optical Cavity Kiwamu Izumi,1, ∗ Daniel Sigg,1 and Lisa Barsotti2 1LIGO Hanford Observatory, PO Box 159 Richland, Washington 99354, USA 2LIGO laboratory, Massachusetts Institute of Technology, Cambridge, Massachussetts 02139, USA compiled: January 8, 2016 High finesse optical cavities are an essential tool in modern precision laser interferometry. The incident laser field is often controlled and stabilized with an active feedback system such that the field resonates in the cavity. The Pound-Drever-Hall reflection locking technique is a convenient way to derive a suitable error signal. However, it only gives a strong signal within the cavity linewidth. This poses a problem for locking a ultra-narrow linewidth cavity. We present a novel technique for acquiring lock by utilizing an additional weak control signal, but with a much larger capture range. We numerically show that this technique can be applied to the laser frequency stabilization system used in the Laser Interferometric Gravitational-wave Observatory (LIGO) which has a linewidth of 0.8 Hz. This new technique will allow us to robustly and repeatedly lock the LIGO laser frequency to the common mode of the interferometer. OCIS codes: (140.3425), (140.3410) http://dx.doi.org/10.1364/XX.99.099999 High finesse optical cavities have been an indispens- nonlinear response [8, 9] dominant and thus hinder the able tool for precision interferometry to conduct rela- linear controller. tivistic experiments such as gravitational wave detection Gravitational wave observatories deploy kilometer [1{3] and optical clocks [4]. The use of a high finesse cav- scale interferometers with extremely narrow linewidth. -
Absorption Spectroscopy and Imaging from the Visible Through Mid-Infrared with 20 Nm Resolution
Absorption spectroscopy and imaging from the visible through mid-infrared with 20 nm resolution. Aaron M. Katzenmeyer,1 Glenn Holland,1 Kevin Kjoller2 and Andrea Centrone1* 1Center for Nanoscale Science and Technology, National Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, Maryland 20899, United States. *E-mail: [email protected] 2Anasys Instruments, Inc., 325 Chapala Street, Santa Barbara, California 93101, United States. Abstract Absorption spectroscopy and mapping from visible through mid-IR wavelengths has been achieved with spatial resolution exceeding the limit imposed by diffraction, via the photothermal induced resonance technique. Correlated vibrational (chemical), and electronic properties are obtained simultaneously with topography with a wavelength-independent resolution of ≈ 20 nm using a single laboratory-scale instrument. This marks the highest resolution reported for PTIR, as determined by comparing height and PTIR images, and its first extension to near-IR and visible wavelengths. Light-matter interaction enables scientists to characterize materials and biological samples across a large range of energies. Visible (VIS) and near-infrared (NIR) light (from 400 nm to 2.5 µm) probes electronic transitions in materials [1], providing information regarding band gap, defects, and energy transfer which is crucial for the semiconductor and optoelectronic industries and for understanding processes such as photosynthesis. Mid-infrared (mid-IR) light (from 2.5 µm to 15 µm) probes vibrational transitions and provides rich chemical and structural information enabling materials identification [2]. Spectral maps can be obtained by coupling a light source and a spectrometer with an optical microscope [3]. However, light diffraction limits the lateral resolution achievable with conventional microscopic techniques to approximately half the wavelength of light [4]. -
Power Build-Up Cavity Coupled to a Laser Diode
I POWER BUILD-UP CAVITY COUPLED I TO A LASER DIODE Daniel J. Evans I Center of Excellence for Raman Technology University of Utah I Abstract combination of these elements will emit photons at different frequencies. The ends of these semiconductor In many Raman applications there is a need to devices are cleaved to form mirrors that bounce the I detect gases in the low ppb range. The desired photons back and forth within the cavity. The photons sensitivity can be achieved by using a high power laser excite more electrons, which form more photons source in the range of tens of watts. A system (referred to as optical pumping). 2 A certain portion of I combining a build-up cavity to enhance the power and the photons emit through the front and back cleaved an external cavity laser diode setup to narrow the surfaces of the laser diode. The amount of photons that bandwidth can give the needed power to the Raman get through the cleaved surfaces can be adjusted by I spectroscopy system. coating the surface or installing other mirrors. Introduction to Laser Diodes The planar cleaved surfaces of the laser diode form a Fabry-Perot cavity with set resonance frequencies I An important characteristic of all lasers is the (vp).3 The typical laser diode has a spacing of 150 f.1I11 mode structure. The mode structure refers to both the with an index of refraction of 3.5, yielding a resonance lasing frequency and the spatial characteristics of the frequency of 285 GHz. The wavelength spacing (~A.) I laser. -
Quantum Illumination at the Microwave Wavelengths
Quantum Illumination at the Microwave Wavelengths 1 2 3 4 5 6, Shabir Barzanjeh, Saikat Guha, Christian Weedbrook, David Vitali, Jeffrey H. Shapiro, and Stefano Pirandola ∗ 1Institute for Quantum Information, RWTH Aachen University, 52056 Aachen, Germany 2Quantum Information Processing Group, Raytheon BBN Technologies, Cambridge, Massachusetts 02138, USA 3QKD Corp., 60 St. George St., Toronto, M5S 3G4, Canada 4School of Science and Technology, University of Camerino, Camerino, Macerata 62032, Italy 5Research Laboratory of Electronics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 6Department of Computer Science & York Centre for Quantum Technologies, University of York, York YO10 5GH, United Kingdom Quantum illumination is a quantum-optical sensing technique in which an entangled source is exploited to improve the detection of a low-reflectivity object that is immersed in a bright thermal background. Here we describe and analyze a system for applying this technique at microwave frequencies, a more appropriate spectral region for target detection than the optical, due to the naturally-occurring bright thermal background in the microwave regime. We use an electro-opto- mechanical converter to entangle microwave signal and optical idler fields, with the former being sent to probe the target region and the latter being retained at the source. The microwave radiation collected from the target region is then phase conjugated and upconverted into an optical field that is combined with the retained idler in a joint-detection -
Construction of a Flashlamp-Pumped Dye Laser and an Acousto-Optic
; UNITED STATES APARTMENT OF COMMERCE oUBLICATION NBS TECHNICAL NOTE 603 / v \ f ''ttis oi Construction of a Flashlamp-Pumped Dye Laser U.S. EPARTMENT OF COMMERCE and an Acousto-Optic Modulator National Bureau of for Mode-Locking Iandards — NATIONAL BUREAU OF STANDARDS 1 The National Bureau of Standards was established by an act of Congress March 3, 1901. The Bureau's overall goal is to strengthen and advance the Nation's science and technology and facilitate their effective application for public benefit. To this end, the Bureau conducts research and provides: (1) a basis for the Nation's physical measure- ment system, (2) scientific and technological services for industry and government, (3) a technical basis for equity in trade, and (4) technical services to promote public safety. The Bureau consists of the Institute for Basic Standards, the Institute for Materials Research, the Institute for Applied Technology, the Center for Computer Sciences and Technology, and the Office for Information Programs. THE INSTITUTE FOR BASIC STANDARDS provides the central basis within the United States of a complete and consistent system of physical measurement; coordinates that system with measurement systems of other nations; and furnishes essential services leading to accurate and uniform physical measurements throughout the Nation's scien- tific community, industry, and commerce. The Institute consists of a Center for Radia- tion Research, an Office of Measurement Services and the following divisions: Applied Mathematics—Electricity—Heat—Mechanics—Optical Physics—Linac Radiation 2—Nuclear Radiation 2—Applied Radiation 2—Quantum Electronics 3— Electromagnetics 3—Time and Frequency 3 —Laboratory Astrophysics3—Cryo- 3 genics . -
Absorption Spectroscopy
World Bank & Government of The Netherlands funded Training module # WQ - 34 Absorption Spectroscopy New Delhi, February 2000 CSMRS Building, 4th Floor, Olof Palme Marg, Hauz Khas, DHV Consultants BV & DELFT HYDRAULICS New Delhi – 11 00 16 India Tel: 68 61 681 / 84 Fax: (+ 91 11) 68 61 685 with E-Mail: [email protected] HALCROW, TAHAL, CES, ORG & JPS Table of contents Page 1 Module context 2 2 Module profile 3 3 Session plan 4 4 Overhead/flipchart master 5 5 Evaluation sheets 22 6 Handout 24 7 Additional handout 29 8 Main text 31 Hydrology Project Training Module File: “ 34 Absorption Spectroscopy.doc” Version 06/11/02 Page 1 1. Module context This module introduces the principles of absorption spectroscopy and its applications in chemical analyses. Other related modules are listed below. While designing a training course, the relationship between this module and the others, would be maintained by keeping them close together in the syllabus and place them in a logical sequence. The actual selection of the topics and the depth of training would, of course, depend on the training needs of the participants, i.e. their knowledge level and skills performance upon the start of the course. No. Module title Code Objectives 1. Basic chemistry concepts WQ - 02 • Convert units from one to another • Discuss the basic concepts of quantitative chemistry • Report analytical results with the correct number of significant digits. 2. Basic aquatic chemistry WQ - 24 • Understand equilibrium chemistry and concepts ionisation constants. • Understand basis of pH and buffers • Calculate different types of alkalinity. -
Raman Spectroscopy for In-Line Water Quality Monitoring — Instrumentation and Potential
Sensors 2014, 14, 17275-17303; doi:10.3390/s140917275 OPEN ACCESS sensors ISSN 1424-8220 www.mdpi.com/journal/sensors Review Raman Spectroscopy for In-Line Water Quality Monitoring — Instrumentation and Potential Zhiyun Li 1, M. Jamal Deen 1,2,4,*, Shiva Kumar 2 and P. Ravi Selvaganapathy 1,3 1 School of Biomedical Engineering, McMaster University, Hamilton, ON L8S 4K1, Canada; E-Mails: [email protected] (Z.L.); [email protected] (P.R.S.) 2 Electrical and Computer Engineering, McMaster University, Hamilton, ON L8S 4K1 Canada; E-Mail: [email protected] 3 Mechanical Engineering, McMaster University, Hamilton, ON L8S 4K1, Canada 4 Electronic and Computer Engineering, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, China * Author to whom correspondence should be addressed; E-Mail: [email protected] or [email protected]; Tel.: +1-905-525-9140 (ext. 27137); Fax: +1-905-521-2922. Received: 1 July 2014; in revised form: 7 September 2014 / Accepted: 9 September 2014 / Published: 16 September 2014 Abstract: Worldwide, the access to safe drinking water is a huge problem. In fact, the number of persons without safe drinking water is increasing, even though it is an essential ingredient for human health and development. The enormity of the problem also makes it a critical environmental and public health issue. Therefore, there is a critical need for easy-to-use, compact and sensitive techniques for water quality monitoring. Raman spectroscopy has been a very powerful technique to characterize chemical composition and has been applied to many areas, including chemistry, food, material science or pharmaceuticals. -
Basics of Plasma Spectroscopy
Home Search Collections Journals About Contact us My IOPscience Basics of plasma spectroscopy This content has been downloaded from IOPscience. Please scroll down to see the full text. 2006 Plasma Sources Sci. Technol. 15 S137 (http://iopscience.iop.org/0963-0252/15/4/S01) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 198.35.1.48 This content was downloaded on 20/06/2014 at 16:07 Please note that terms and conditions apply. INSTITUTE OF PHYSICS PUBLISHING PLASMA SOURCES SCIENCE AND TECHNOLOGY Plasma Sources Sci. Technol. 15 (2006) S137–S147 doi:10.1088/0963-0252/15/4/S01 Basics of plasma spectroscopy U Fantz Max-Planck-Institut fur¨ Plasmaphysik, EURATOM Association Boltzmannstr. 2, D-85748 Garching, Germany E-mail: [email protected] Received 11 November 2005, in final form 23 March 2006 Published 6 October 2006 Online at stacks.iop.org/PSST/15/S137 Abstract These lecture notes are intended to give an introductory course on plasma spectroscopy. Focusing on emission spectroscopy, the underlying principles of atomic and molecular spectroscopy in low temperature plasmas are explained. This includes choice of the proper equipment and the calibration procedure. Based on population models, the evaluation of spectra and their information content is described. Several common diagnostic methods are presented, ready for direct application by the reader, to obtain a multitude of plasma parameters by plasma spectroscopy. 1. Introduction spectroscopy for purposes of chemical analysis are described in [11–14]. Plasma spectroscopy is one of the most established and oldest diagnostic tools in astrophysics and plasma physics 2. -
Ophthalmic Laser Therapy: Mechanisms and Applications
1 Ophthalmic Laser Therapy: Mechanisms and Applications Daniel Palanker Department of Ophthalmology and Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA Definition The term LASER is an abbreviation which stands for Light Amplification by Stimulated Emission of Radiation. The laser is a source of coherent, directional, monochromatic light that can be precisely focused into a small spot. The laser is a very useful tool for a wide variety of clinical diagnostic and therapeutic procedures. Principles of Light Emission by Lasers Molecules are made up of atoms, which are composed of a positively charged nucleus and negatively charged electrons orbiting it at various energy levels. Light is composed of individual packets of energy, called photons. Electrons can jump from one orbit to another by either, absorbing energy and moving to a higher level (excited state), or emitting energy and transitioning to a lower level. Such transitions can be accompanied by absorption or spontaneous emission of a photon. “Stimulated Emission” is a process in which photon emission is stimulated by interaction of an atom in excited state with a passing photon. The photon emitted by the atom in this process will have the same phase, direction of propagation and wavelength as the “stimulating photon”. The “stimulating photon” does not lose energy during this interaction- it simply causes the emission and continues on, as illustrated in Figure 1. Figure 1: LASER: Light Amplification by Stimulated Emission of Radiation For such stimulated emission to occur more frequently than absorption (and hence result in light amplification), the optical material should have more atoms in excited state than in a lower state. -
Generation of a Flat-Top Laser Beam for Gravitational Wave Detectors By
Generation of a flat-top laser beam for gravitational wave detectors by means of a nonspherical Fabry–Perot resonator Marco G. Tarallo,1,2,* John Miller,2,3 J. Agresti,1,2 E. D’Ambrosio,2 R. DeSalvo,2 D. Forest,4 B. Lagrange,4 J. M. Mackowsky,4 C. Michel,4 J. L. Montorio,4 N. Morgado,4 L. Pinard,4 A. Remilleux,4 B. Simoni,1,2 and P. Willems2 1Dipartimento di Fisica, Università di Pisa, Largo Pontecorvo 3, 56100 Pisa, Italy 2LIGO Laboratory, California Institute of Technology, 1200 E. California Boulevard, Pasadena, California, USA 3Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK 4Laboratoire des Matèriaux Avancès, 22 Boulevard Niels Bohr, Villeurbanne, France *Corresponding author: [email protected] Received 23 February 2007; revised 6 July 2007; accepted 11 July 2007; posted 13 July 2007 (Doc. ID 80265); published 7 September 2007 We have tested a new kind of Fabry–Perot long-baseline optical resonator proposed to reduce the thermal noise sensitivity of gravitational wave interferometric detectors—the “mesa beam” cavity—whose flat top beam shape is achieved by means of an aspherical end mirror. We present the fundamental mode intensity pattern for this cavity and its distortion due to surface imperfections and tilt misalignments, and contrast the higher order mode patterns to the Gauss–Laguerre modes of a spherical mirror cavity. We discuss the effects of mirror tilts on cavity alignment and locking and present measurements of the mesa beam tilt sensitivity. © 2007 Optical Society of America OCIS codes: 140.4780, 120.2230, 230.0040. -
Atomic Spectroscopy 008044D 01 a Guide to Selecting The
PerkinElmer has been at the forefront of The Most Trusted inorganic analytical technology for over 50 years. With a comprehensive product Name in Elemental line that includes Flame AA systems, high-performance Graphite Furnace AA Analysis systems, flexible ICP-OES systems and the most powerful ICP-MS systems, we can provide the ideal solution no matter what the specifics of your application. We understand the unique and varied needs of the customers and markets we serve. And we provide integrated solutions that streamline and simplify the entire process from sample handling and analysis to the communication of test results. With tens of thousands of installations worldwide, PerkinElmer systems are performing WORLD LEADER IN inorganic analyses every hour of every day. Behind that extensive network of products stands the industry’s largest and most-responsive technical service and support staff. Factory-trained and located in 150 countries, they have earned a reputation for consistently AA, ICP-OES delivering the highest levels of personalized, responsive service in the industry. AND ICP-MS PerkinElmer, Inc. 940 Winter Street Waltham, MA 02451 USA P: (800) 762-4000 or (+1) 203-925-4602 www.perkinelmer.com For a complete listing of our global offices, visit www.perkinelmer.com/ContactUs Copyright ©2008-2013, PerkinElmer, Inc. All rights reserved. PerkinElmer® is a registered trademark of PerkinElmer, Inc. All other trademarks are the property of their respective owners. Atomic Spectroscopy 008044D_01 A Guide to Selecting the Appropriate -
3-5 Development of an Ultra-Narrow Line-Width Clock Laser
3-5 Development of an Ultra-Narrow Line-Width Clock Laser LI Ying, NAGANO Shigeo, MATSUBARA Kensuke, KOJIMA Reiko, KUMAGAI Motohiro, ITO Hiroyuki, KOYAMA Yasuhiro, and HOSOKAWA Mizuhiko An optical lattice clock and a single ion optical clock are being developed in National Institute of Information and Communications Technology (NICT). Diode lasers are used for the develop- ment of extremely narrow linewidth clock lasers for optical frequency standards. Using the Pound- Drever-Hall technique, the required reduction of linewidth was achieved by locking the laser to an ultrahigh-fi nesse ultralow-expansion glass (ULE) reference cavity, which is set in the high vacuum chamber with a constant temperature and isolated against environmental noise and vibration. As a result, the laser linewidth is decreased down to several Hz. The Allan deviation is less than 4×10−15 at an averaging time over 100 s. A vibration-insensitive optical cavity has been designed, aiming the linewidth below 1 Hz. In this chapter, we report the present status of development of the clock lasers at NICT. Keywords Laser frequency stabilization, Diode laser, Optical reference cavity, Optical clock, Optical frequency standard 1 Introduction an uncertainty of 10−17 or less is divided into two types. The fi rst is the “optical lattice The second, the current time and frequency clock” [4] [5], neutral atoms are trap in the opti- standard unit, is defi ned according to the hy- cal lattice “magic wave length” and the second perfi ne structure transition of cesium atoms by is the “single ion clock” [6], single ion is con- the General Conference of Weights and Mea- fi ned to the Lamb-Dick regime.