Technology of terahertz quantum dot detectors and their applications V Antonov Moscow Institute of Physics and Technology, Russia Royal Holloway University.

Slides:



Advertisements
Similar presentations
Astronomy Notes to Accompany the Text Astronomy Today, Chaisson, McMillan Jim Mims.
Advertisements

The Amazing Spectral Line Begin. Table of Contents A light review Introduction to spectral lines What spectral lines can tell us.
Optical sources Lecture 5.
Molecular Bonds Molecular Spectra Molecules and Solids CHAPTER 10 Molecules and Solids Johannes Diderik van der Waals (1837 – 1923) “You little molecule!”
Cphys351 c4:1 Chapter 4: Atomic Structure The Nuclear Atom The Atom as the smallest division of an element quantization of electric charge oil drop experiments.
Gamma-Ray Spectra _ + The photomultiplier records the (UV) light emitted during electronic recombination in the scintillator. Therefore, the spectrum collected.
METO 621 Lesson 6. Absorption by gaseous species Particles in the atmosphere are absorbers of radiation. Absorption is inherently a quantum process. A.
Light. Photons The photon is the gauge boson of the electromagnetic force. –Massless –Stable –Interacts with charged particles. Photon velocity depends.
Chapter 5 Light and Matter: Reading Messages from the Cosmos
School of Physics and Astronomy, University of Nottingham, Nottingham, NG7 2RD, UK. Electrically pumped terahertz SASER device using a weakly coupled AlAs/GaAs.
Superconducting THz Transmission Spectrometer Comprising Josephson Oscillator and Cold-Electron Bolometer M.Tarasov, L.Kuzmin, E.Stepantsov, I.Agulo, A.Kalabukhov,
Alexey Belyanin Texas A&M University A. Wojcik TAMU
Spectroscopy. Atoms and Light  Atomic electron energy levels are a source of discrete photon energies.  Change from a high to low energy state produces.
Atoms and Starlight Chapter 6. Color and Temperature Orion Betelgeuze Rigel Stars appear in different colors, from blue (like Rigel) via green / yellow.
Physics for Scientists and Engineers, 6e Chapter 43 - Molecules and Solids.
Dr. Jie ZouPHY Chapter 43 Molecules and Solids.
9. Semiconductors Optics Absorption and gain in semiconductors Principle of semiconductor lasers (diode lasers) Low dimensional materials: Quantum wells,
Royal Holloway University of London
Laser Physics I Dr. Salah Hassab Elnaby Lecture(2)
Lecture 3 INFRARED SPECTROMETRY
Spectral Regions and Transitions
Quantum Dots. Optical and Photoelectrical properties of QD of III-V Compounds. Alexander Senichev Physics Faculty Department of Solid State Physics
Common types of spectroscopy
Chapter 4 Spectroscopy Chapter 4 opener. Spectroscopy is a powerful observational technique enabling scientists to infer the nature of matter by the way.
Spectroscopic Analysis Part 4 – Molecular Energy Levels and IR Spectroscopy Chulalongkorn University, Bangkok, Thailand January 2012 Dr Ron Beckett Water.
Vibrational and Rotational Spectroscopy
© 2010 Pearson Education, Inc. Light and Matter: Reading Messages from the Cosmos.
Properties of Matter Our goals for learning: What is the structure of matter? What are the phases of matter How is energy stored in atoms?
Learning from Light Our goals for learning What are the three basic types of spectra? How does light tell us what things are made of? How does light tell.
Electrons, phonons, and photons in solids Optoelectronics Group Alex L Ivanov Department of Physics and Astronomy, Cardiff University Wales, United Kingdom.
Nuclear Magnetic Resonance Spectroscopy (NMR) Dr AKM Shafiqul Islam School of Bioprocess Engineering.
ABSORPTION AND DIFFUSION MEASUREMENT OF BIOLOGICAL SAMPLES USING A FREE ELECTRON LASER M. D’Arienzo, A. Doria, G.P. Gallerano, E. Giovenale, A. Lai, G.
INTRODUCTION Characteristics of Thermal Radiation Thermal Radiation Spectrum Two Points of View Two Distinctive Modes of Radiation Physical Mechanism of.
Superradiance, Amplification, and Lasing of Terahertz Radiation in an Array of Graphene Plasmonic Nanocavities V. V. Popov, 1 O. V. Polischuk, 1 A. R.
Electron-Phonon Interaction and Disorder: Nanoscale Interference in Transport Phenomena Andrei Sergeyev, SUNY at Buffalo, DMR Thermomagnetic vortex.
Rotation and vibration spectra. Rotational States Molecular spectroscopy: We can learn about molecules by studying how molecules absorb, emit, and scatter.
441 Chem Introduction to Spectroscopy CH-1 1. Introduction to Spectroscopy Set of methods where interaction of electromagnetic radiation with chemical.
Starlight and Atoms Chapter 6. The Amazing Power of Starlight Just by analyzing the light received from a star, astronomers can retrieve information about.
© 2010 Pearson Education, Inc. Chapter 5 Light and Matter: Reading Messages from the Cosmos.
Surface Plasmon Resonance
Chapter 1 Introduction 1.1 Classification of optical processes Reflection Propagation Transmission Optical medium refractive index n( ) = c / v ( )
Single photon counting detector for THz radioastronomy. D.Morozov 1,2, M.Tarkhov 1, P.Mauskopf 2, N.Kaurova 1, O.Minaeva 1, V.Seleznev 1, B.Voronov 1 and.
Chapter 4 Spectroscopy The beautiful visible spectrum of the star Procyon is shown here from red to blue, interrupted by hundreds of dark lines caused.
IR Spectroscopy Wave length ~ 100 mm to 1 mm
Chapter 4.
1.1 What’s electromagnetic radiation
Chapter 14 The Interstellar Medium. All of the material other than stars, planets, and degenerate objects Composed of gas and dust ~1% of the mass of.
Spectroscopy and Atoms
Simulations of turbulent plasma heating by powerful electron beams Timofeev I.V., Terekhov A.V.
Lecture 8: Volume Interactions Thursday, 28 January 2010 Ch 1.8 Major spectral features of minerals (p. xiii-xv), from Infrared.
Rotation and vibration spectra. Rotational States Molecular spectroscopy: We can learn about molecules by studying how molecules absorb, emit, and scatter.
Conclusion QDs embedded in micropillars are fabricated by MOCVD and FIB post milling processes with the final quality factor about Coupling of single.
MOLECULAR SPECTROSCOPY
PHYS 172: Modern Mechanics Lecture 14 – Energy Quantization Read Summer 2012.
Optical Emitters and Receivers
Electromagnetic Radiation, Cont….
CHAPTER 9 Molecules Rotations Spectra Complex planar molecules
Spectroscopy and Atoms
Light Sources for Optical Communications
PAN-2013: Radiation detectors
CHAPTER 9 Molecules Rotations Spectra Complex planar molecules
Diatomic molecules
Sections 6.1 – 6.3 Electromagnetic Radiation and its Interaction with Atoms Bill Vining SUNY College at Oneonta.
Lecture 8: Volume Interactions
Raman Scattering ——CCl4 molecular Raman Spectrum 崔婧
Chapter 3 Review Worksheet
5.4 Learning from Light Our goals for learning
Lecture 8: Volume Interactions
Mr.Halavath Ramesh 16-MCH-001 Department of Chemistry Loyola College-Chennai University of Madras.
PLASMONICS AND ITS APPLICATIONS BY RENJITH MATHEW ROY. From classical fountations to its modern applications
Presentation transcript:

Technology of terahertz quantum dot detectors and their applications V Antonov Moscow Institute of Physics and Technology, Russia Royal Holloway University of London, UK THz radiation is a fundamental frequency range having origin in rotational and vibrational modes of molecules THz (FIR ) RHUL, EGHAM, UK

Rotational modes of molecules A diatomic molecule rotating about the common centre of mass of its two atoms Transition between rotational modes with angular momentum l - 1 and l The rotational energy spectrum of HCl measured by absorption Typical energy scale of THz photons corresponds to few meV or K ~ few meV

Identification of materials LIQUIDS Divin,2008 methanol acetone Spectral features are broad because of interaction SOLIDS RDX molecule Kemp,2011 Features of THz technology: -paper, plastics, wood, textiles are transparent for THz radiation -brightness of THz radiation emitted by materials is extremely small -Water/water vapor is strong absorber of THz radiation

Terahertz radiation in nanoscale low temperature systems Komiyama, 2011 Cyclotron radiation emitted by Hall bar in Quantum Hall regime Relaxation of injected electrons at the edge states

Terahertz radiation of HTS Josepson Junction JJ radiation of individual Josephson Junction The upper limit of  JJ  is limited by  /e. It can be up to 7THz Only small part is emitted as coherent JJ radiation (pW out of  W dissipated) Coupling of JJ radiation to the planar metallic antennae is weak. A heating of the JJ becomes strong at high bias (when V=1 mV T m exceeds T B by 3K) Line width of radiation is ~1 GHz Josephson Junction is formed in 200nm thick YBa 2 Cu 3 O 7 film at bi-crystal boundary of sapphire substrate.

QD-SET detector Shift of CBO pattern when one electron is excited Switches of SET current due to electron excitations

Spectral sensitivity of Quantum Dot detector Plasma oscillations in QD Plasma resonance in QD n – sheet carrier concentration m – effective electron mass, 0.07m e in GaAs, 0.014m e in InSb  – dielectric constant, ~13 in GaAs R – radius of the QD,  m For 1.4  m dot  ~ 0.25 THz Plasma resonance in QD At B=0T Plasma resonance in QD At B~3T

QD-SET detector

Detection of JJ radiation Counting of the QD excitations without radiation Suppression of thermal counts is described by: with a=12meV/V Counting of the QD excitations due to JJ radiation Detected power corresponds to 2x W Coherent JJ radiation emitted by JJ is 30 aW out of 80 nW dissipated. Conversion factor is 4x

Detection of JJ radiation Direction of switches of the SET current indicates at the excitations of electrons in/out of the QD Decryption of excitations of the QD

Coherent terahertz radiation of stack of HTS JJ Resonances are determined by geometrical design of resonator. Line width of the radiation is down to 50MHz Power emitted out of substrate ~ 1  W

-We detected a coherent radiation of individual HTS JJ -Radiation of individual HTS JJ is weak, conversion factor is ~ 4x The radiation can be used to study/calibrate sensitive spectral detectors Conclusions

R Shaikhaidarov, A Casey, Royal Holloway University of London, UK Y Harada, K Omitsu, NTT Basic Research labs, Japan A Tzalenchuk, National Physical Laboratory, United Kingdom A Kalaboukhov, S Kubatkin, Chalmers University, Sweden Credits