Ablation of Solids by Femtosecond Lasers: Ablation Mechanism and Ablation Thresholds for Metals and Dielectrics
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FY20 National Laser Users' Facility Program
FY20 NATIONAL LASER USERS’ FACILITY PROGRAM FY20 National Laser Users’ Facility Program M. S. Wei Laboratory for Laser Energetics, University of Rochester During FY19, the National Nuclear Security Administration (NNSA) and Office of Science jointly completed a funding opportu- nity announcement (FOA), review, and selection process for National Laser Users’ Facility (NLUF) experiments to be conducted at the Omega Facility during FY20 and FY21. After peer review by an independent proposal review committee for scientific and technical merit and the feasibility review by the Omega Facility team, NNSA selected 11 proposals for funding and Omega shot allocation with a total of 22.5 and 23.5 shot days for experiments in FY20 and FY21, respectively. During the first half of the FY20, LLE completed a one-time solicitation, review, and selection process for Academic and Industrial Basic Science (AIBS) experiments to utilize the remaining NLUF shot allocation in FY20–FY21. Ten new projects were selected for AIBS shot alloca- tion (a total of 11 and 10 shot days) for experiments staring in Q3FY20 and throughout FY21. FY20 was the first of a two-year period of performance for these 21 NLUF including AIBS projects (Table I). Fifteen NLUF and AIBS projects obtained a total of 232 target shots during FY20, which are summarized in this section. A critical part of the NNSA-supported NLUF program and the DOE Office of Fusion Energy Sciences (FES)-supported Laser- NetUS program is the education and training of graduate students in high-energy-density (HED) physics. In addition, graduate students can also access the Omega Laser Facility to conduct their theses research through collaborations with national labora- tories and LLE. -
Ocular Surface Changes Associated with Ophthalmic Surgery
Journal of Clinical Medicine Review Ocular Surface Changes Associated with Ophthalmic Surgery Lina Mikalauskiene 1, Andrzej Grzybowski 2,3 and Reda Zemaitiene 1,* 1 Department of Ophthalmology, Medical Academy, Lithuanian University of Health Sciences, 44037 Kaunas, Lithuania; [email protected] 2 Department of Ophthalmology, University of Warmia and Mazury, 10719 Olsztyn, Poland; [email protected] 3 Institute for Research in Ophthalmology, Foundation for Ophthalmology Development, 61553 Poznan, Poland * Correspondence: [email protected] Abstract: Dry eye disease causes ocular discomfort and visual disturbances. Older adults are at a higher risk of developing dry eye disease as well as needing for ophthalmic surgery. Anterior segment surgery may induce or worsen existing dry eye symptoms usually for a short-term period. Despite good visual outcomes, ocular surface dysfunction can significantly affect quality of life and, therefore, lower a patient’s satisfaction with ophthalmic surgery. Preoperative dry eye disease, factors during surgery and postoperative treatment may all contribute to ocular surface dysfunction and its severity. We reviewed relevant articles from 2010 through to 2021 using keywords “cataract surgery”, ”phacoemulsification”, ”refractive surgery”, ”trabeculectomy”, ”vitrectomy” in combina- tion with ”ocular surface dysfunction”, “dry eye disease”, and analyzed studies on dry eye disease pathophysiology and the impact of anterior segment surgery on the ocular surface. Keywords: dry eye disease; ocular surface dysfunction; cataract surgery; phacoemulsification; refractive surgery; trabeculectomy; vitrectomy Citation: Mikalauskiene, L.; Grzybowski, A.; Zemaitiene, R. Ocular Surface Changes Associated with Ophthalmic Surgery. J. Clin. 1. Introduction Med. 2021, 10, 1642. https://doi.org/ 10.3390/jcm10081642 Dry eye disease (DED) is a common condition, which usually causes discomfort, but it can also be an origin of ocular pain and visual disturbances. -
Formation of Moon Systems Around Giant Planets Capture and Ablation of Planetesimals As Foundation for a Pebble Accretion Scenario T
A&A 633, A93 (2020) Astronomy https://doi.org/10.1051/0004-6361/201936804 & © ESO 2020 Astrophysics Formation of moon systems around giant planets Capture and ablation of planetesimals as foundation for a pebble accretion scenario T. Ronnet and A. Johansen Department of Astronomy and Theoretical Physics, Lund Observatory, Lund University, Box 43, 22100 Lund, Sweden e-mail: [email protected] Received 28 September 2019 / Accepted 10 December 2019 ABSTRACT The four major satellites of Jupiter, known as the Galilean moons, and Saturn’s most massive satellite, Titan, are believed to have formed in a predominantly gaseous circum-planetary disk during the last stages of formation of their parent planet. Pebbles from the protoplanetary disk are blocked from flowing into the circumplanetary disk by the positive pressure gradient at the outer edge of the planetary gap, so the gas drag assisted capture of planetesimals should be the main contributor to the delivery of solids onto circum- planetary disks. However, a consistent framework for the subsequent accretion of the moons remains to be built. Here, we use numerical integrations to show that most planetesimals that are captured within a circum-planetary disk are strongly ablated due to the frictional heating they experience, thus supplying the disk with small dust grains, whereas only a small fraction “survives” their capture. We then constructed a simple model of a circum-planetary disk supplied by ablation, where the flux of solids through the disk is at equilibrium with the ablation supply rate, and we investigate the formation of moons in such disks. We show that the growth of satellites is mainly driven by accretion of the pebbles that coagulate from the ablated material. -
A Programmable Mode-Locked Fiber Laser Using Phase-Only Pulse Shaping and the Genetic Algorithm
hv photonics Article A Programmable Mode-Locked Fiber Laser Using Phase-Only Pulse Shaping and the Genetic Algorithm Abdullah S. Karar 1,* , Raymond Ghandour 1 , Ibrahim Mahariq 1 , Shadi A. Alboon 1,2, Issam Maaz 1, Bilel Neji 1 and Julien Moussa H. Barakat 1 1 College of Engineering and Technology, American University of the Middle East, Kuwait; [email protected] (R.G.); [email protected] (I.M.); [email protected] (S.A.A.); [email protected] (I.M.); [email protected] (B.N.); [email protected] (J.M.H.B.) 2 Electronics Engineering Department, Hijjawi Faculty for Engineering Technology, Yarmouk University, Irbid 21163, Jordan * Correspondence: [email protected] Received: 24 July 2020; Accepted: 2 September 2020; Published: 4 September 2020 Abstract: A novel, programmable, mode-locked fiber laser design is presented and numerically demonstrated. The laser programmability is enabled by an intracavity optical phase-only pulse shaper, which utilizes the same linearly chirped fiber Bragg grating (LC-FBG) from its two opposite ends to perform real-time optical Fourier transformation. A binary bit-pattern generator (BPG) operating at 20-Gb/s and producing a periodic sequence of 32 bits every 1.6 ns, is subsequently used to drive an optical phase modulator inside the laser cavity. Simulation results indicate stable programmable intensity profiles for each optimized user defined 32 code words. The laser operated in the self-similar mode-locking regime, enabling wave-breaking free operation. The programmable 32 bit code word targeting a specific intensity profile was determined using 100 generations of the genetic algorithm. -
MRI-Guided Laser Ablation Surgery of Hypothalamic Hamartomas
NEUROSURGERY MRI-Guided Laser Ablation Surgery of Hypothalamic Hamartomas HOW DOES THE TEAM DECIDE IF A PATIENT IS A CANDIDATE FOR MRI-GUIDED LASER ABLATION? A careful review of each patient’s medical records is the first step, including MR imaging of the brain and any applicable neurology or neurosurgery records. Patients with Hypothalamic Hamartomas (HH) typically have gelastic seizures, which are characterized by emotionless laughing, although variations including abnormal movements or staring spells are also common. Every patient’s case is handled individually, and it may be necessary for a patient to come to Texas Children’s Hospital for further testing to determine if they are a candidate for MRI-guided laser ablation surgery. WHAT HAPPENS DURING MRI-GUIDED LASER ABLATION SURGERY? After being placed under general anesthesia, a head frame, or a set of markers, is fitted to the patient’s skull. A CT scan is completed to orient the brain to the frame in 3 dimensions. With the help of computer software, a safe pathway that goes through the brain to the HH is calculated for the laser. The neurosurgeon then makes a small incision and drills a small hole through the skull (3.2 mm wide). The laser applicator, a small tube about the width of a strand of spaghetti, is inserted and guided through the brain into the HH. Once the laser applicator is inserted into the brain, the head frame is removed, and the patient is transported to the MRI scanner. After confirming proper placement of the laser applicator and setting safety markers, the surgeon performs a small test firing using the laser. -
Potential of Laser-Induced Ablation for Future Space Applications
Space Policy 28 (2012) 149e153 Contents lists available at SciVerse ScienceDirect Space Policy journal homepage: www.elsevier.com/locate/spacepol Viewpoint Potential of laser-induced ablation for future space applications Alison Gibbings a,c,*, Massimiliano Vasile a, John-Mark Hopkins b, David Burns b, Ian Watson c a Advanced Space Concepts Laboratory, Department of Mechanical and Aerospace Engineering, University of Strathclyde, 75 Montrose Street, Glasgow G1 1X1, UK b Institute of Photonics, University of Strathclyde, Wolfson Centre, 106 Rottenrow, Glasgow, UK c Systems, Power and Energy Research Division, University of Glasgow, School of Engineering, James Watt (South) Building, University of Glasgow, University Avenue, Glasgow, UK article info abstract Article history: This paper surveys recent and current advancements of laser-induced ablation technology for space- Received 24 February 2012 based applications and discusses ways of bringing such applications to fruition. Laser ablation is ach- Received in revised form ieved by illuminating a given material with a laser light source. The high surface power densities 21 May 2012 provided by the laser enable the illuminated material to sublimate and ablate. Possible applications Accepted 22 May 2012 include the deflection of Near Earth Objects e asteroids and comets e from an Earth-impacting event, Available online 16 June 2012 the vaporisation of space structures and debris, the mineral and material extraction of asteroids and/or as an energy source for future propulsion systems. This paper will discuss each application and the tech- nological advancements that are required to make laser-induced ablation a practical process for use within the space arena. Particular improvements include the efficiency of high power lasers, the colli- mation of the laser beam (including beam quality) and the power conversion process. -
Formation of Redback Pulsars
Formation of Redback Pulsars Sarah L. Smedley 10th June 2015 Supervisor: Chris Tout Collaborators: Lilia Ferrario and Dayal Wickramasinghe Talk outline Define redbacks (RBs). Describe the current RB population. Introduce our possible formation pathway for RBs which includes the accretion-induced collapse of an ONeMg white dwarf. Show the results of modelling this formation pathway with the Cambridge STARS code. Draw conclusions on the viability of this formation pathway. Millisecond Pulsars (MSPs) magnetic spin axis axis P < 30ms spin Weaker magnetic fields NS Typically Old Binary What is a Redback Pulsar? A redback pulsar is a millisecond pulsar with a non-degenerate companion. The radio signal of a RB is eclipsed for a large portion of the orbit which suggests the companion is ablated. Ablated Companion Radio MSP There are 16 RBs known. Most of them were found in follow up surveys of gamma-ray sources. They have circular orbits. Observed redback population Median masses of companions of known RBs with main-sequence companions. Median mass of companion to PSR J1816+4510. Median masses of companions for known RBs with unknown companions. Binary mass fuction calculated from measurement of the doppler shift of the pulsar and the orbital period. 3 And BMF = (Mc sin i) 2 (MNS + Mc) Minimum comp. mass: i = 90 degrees. Median comp. mass: i = 60 degrees. Upper comp. mass: i = 25.8 degrees. MNS = 1.25 M for post-AIC NS mass. Observed redback population Median masses of companions of known RBs with main-sequence companions. Median mass of companion to PSR J1816+4510. Median masses of companions for known RBs with unknown companions. -
NEW ACTIVE REMOTE-SENSING CAPABILITIES: LASER ABLATION SPECTROMETER and LIDAR ATMOSPHERIC SPECIES PROFILE MEASUREMENTS. R. J. De Young and J
Lunar and Planetary Science XXXVI (2005) 1196.pdf NEW ACTIVE REMOTE-SENSING CAPABILITIES: LASER ABLATION SPECTROMETER AND LIDAR ATMOSPHERIC SPECIES PROFILE MEASUREMENTS. R. J. De Young and J. T. Bergstralh, Science Directorate, NASA Langley Research Center, MS 401A, Hampton, VA 23681, [email protected], [email protected] Introduction: With the quality (M2 = 1.5). As tested, this anticipated development of high- system occupies a volume of 114 x 152 capacity fission power and electric x 45 cm, but it could be made propulsion for deep-space missions, it substantially smaller for space will become possible to propose applications. This laser could be the experiments that demand higher power pump source for the following than current technologies (e.g. instruments. radioisotope power sources) provide. Laser Ablation Mass Jupiter Icy Moons Orbiter (JIMO), the Spectrometer: High-energy pulses from first mission in the Project Prometheus the Yb:YAG laser, focused by a 2 meter program, will explore the icy moons of diameter transmission mirror, would Jupiter with a suite of high-capability produce energy densities of the order of experiments that take advantage of the 109 Watts cm-2 on a surface at a distance high power levels (and indirectly, the of 100 km. The resulting plasma would high data rates) that fission power generate ions of sufficient energy and affords. This abstract describes two quantity to be detected with a mass high-capability active-remote-sensing spectrometer on the spacecraft [1,2]. experiments that will be logical This would make it possible to map with candidates for subsequent Prometheus- very high spatial resolution the class missions. -
Volume Estimation of Excimer Laser Tissue Ablation for Correction of Spherical Myopia and Hyperopia
Volume Estimation of Excimer Laser Tissue Ablation for Correction of Spherical Myopia and Hyperopia Damien Gatinel,1 Thanh Hoang-Xuan,1 and Dimitri T. Azar1,2 PURPOSE. To determine the theoretical volumes of ablation for stromal bed have been implicated as determinants of corneal the laser treatment of spherical refractive errors in myopia and stability, further studies are necessary to evaluate their exact hyperopia. significance. New models estimating the volume of the corneal METHODS. The cornea was modeled as a spherical shell. The tissue ablated by a laser refractive procedure may also be ablation profiles for myopia and hyperopia were based on an necessary to determine the influence of ablated volumes on established paraxial formula. The theoretical volumes of the corneal stability and the procedure’s outcome. ablated corneal lenticules for the correction of myopia and The primary focus of this work is to provide a formula to hyperopia were calculated by two methods: (1) mathematical approximate the volume of tissue ablation for spherical cor- approximation based on a simplified geometric model and (2) rection in myopia and hyperopia. In this study, we approached finite integration. These results were then compared for opti- the volume calculation by two approaches: finite integration cal zone diameters of 0.5 to 11.00 mm and for initial radii of and mathematical approximation. We compared the theoreti- curvature of 7.5, 7.8, and 8.1 mm. cal values of volumes of tissue removal in the treatment of spherical refractive errors predicted by our geometric approx- RESULTS. Referring to a simplified geometrical model, the vol- imation with the values given by finite integration. -
Formation of Moon Systems Around Giant Planets: Capture and Ablation of Planetesimals As Foundation for a Pebble Accretion Scenario
Astronomy & Astrophysics manuscript no. draft c ESO 2019 December 11, 2019 Formation of moon systems around giant planets Capture and ablation of planetesimals as foundation for a pebble accretion scenario T. Ronnet and A. Johansen Department of Astronomy and Theoretical Physics, Lund Observatory, Lund University, Box 43, 22100 Lund, Sweden e-mail: [email protected] Received ; accepted ABSTRACT The four major satellites of Jupiter, known as the Galilean moons, and Saturn’s most massive satellite, Titan, are believed to have formed in a predominantly gaseous circum-planetary disk, during the last stages of formation of their parent planet. Pebbles from the protoplanetary disk are blocked from flowing into the circumplanetary disk by the positive pressure gradient at the outer edge of the planetary gap, so the gas drag assisted capture of planetesimals should be the main contributor to the delivery of solids onto circum-planetary disks. However, a consistent framework for the subsequent accretion of the moons remains to be built. Here we use numerical integrations to show that most planetesimals being captured within a circum-planetary disk are strongly ablated due to the frictional heating they experience, thus supplying the disk with small dust grains, whereas only a small fraction ’survives’ their capture. We then construct a simple model of a circum-planetary disk supplied by ablation, where the flux of solids through the disk is at equilibrium with the ablation supply rate, and investigate the formation of moons in such disks. We show that the growth of satellites is driven mainly by accretion of the pebbles that coagulate from the ablated material. -
Laser Threshold
Main Requirements of the Laser • Optical Resonator Cavity • Laser Gain Medium of 2, 3 or 4 level types in the Cavity • Sufficient means of Excitation (called pumping) eg. light, current, chemical reaction • Population Inversion in the Gain Medium due to pumping Laser Types • Two main types depending on time operation • Continuous Wave (CW) • Pulsed operation • Pulsed is easier, CW more useful Optical Resonator Cavity • In laser want to confine light: have it bounce back and forth • Then it will gain most energy from gain medium • Need several passes to obtain maximum energy from gain medium • Confine light between two mirrors (Resonator Cavity) Also called Fabry Perot Etalon • Have mirror (M1) at back end highly reflective • Front end (M2) not fully transparent • Place pumped medium between two mirrors: in a resonator • Needs very careful alignment of the mirrors (arc seconds) • Only small error and cavity will not resonate • Curved mirror will focus beam approximately at radius • However is the resonator stable? • Stability given by g parameters: g1 back mirror, g2 front mirror: L gi = 1 − ri • For two mirrors resonator stable if 0 < g1g2 < 1 • Unstable if g1g2 < 0 g1g2 > 1 • At the boundary (g1g2 = 0 or 1) marginally stable Stability of Different Resonators • If plot g1 vs g2 and 0 < g1g2 < 1 then get a stability plot • Now convert the g’s also into the mirror shapes Polarization of Light • Polarization is where the E and B fields aligned in one direction • All the light has E field in same direction • Black Body light is not polarized -
Experimental Studies and Simulation of Laser Ablation of High-Density Polyethylene Films by Sandeep Ravi Kumar a Thesis Submitte
Experimental studies and simulation of laser ablation of high-density polyethylene films by Sandeep Ravi Kumar A thesis submitted to the graduate faculty in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Major: Industrial Engineering Program of Study Committee: Hantang Qin, Major Professor Beiwen Li Matthew Frank The student author, whose presentation of the scholarship herein was approved by the program of study committee, is solely responsible for the content of this thesis. The Graduate College will ensure this thesis is globally accessible and will not permit alterations after a degree is conferred. Iowa State University Ames, Iowa 2020 Copyright © Sandeep Ravi Kumar, 2020. All rights reserved. ii DEDICATION I dedicate my thesis work to my family and many friends. A special feeling of gratitude to my loving parents Ravi Kumar and Vasanthi, whose words of encouragement have made me what I am today. iii TABLE OF CONTENTS Page LIST OF FIGURES .................................................................................................................... v LIST OF TABLES ....................................................................................................................vii NOMENCLATURE ................................................................................................................ viii ACKNOWLEDGMENTS .......................................................................................................... ix ABSTRACT ..............................................................................................................................