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1 Nanophotonics Femius Koenderink Center for Nanophotonics AMOLF, Amsterdam [email protected] Nanoscale: 10 -9 meter Photonics: science of controlling propagation, absorption & emission of light (beyond mirrors & lenses)

Nanophotonics · Course slides & information available at: ... Plasmonics & guiding light 3. Scattering by small particles 4. Metamaterials 5. Microcavities 6. Photonic crystals 7

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  • 1

    Nanophotonics

    Femius Koenderink Center for Nanophotonics AMOLF, Amsterdam [email protected]

    Nanoscale: 10-9 meter Photonics: science of controlling propagation, absorption & emission of light (beyond mirrors & lenses)

  • About length scales

    2

    1 m you and your labtable 100 µm thickness of a hair 10 µm smallest you can see 1 µm size of a cell 300 nm smallest you can see with microscope 0.3 nm Si lattice spacing small molecules 0.05 nm Hydrogen atom 1s orbital

    Geometrical optics

    Domain of e-, not ħω

    Range around and just below the wavelength of light Well above the length scales of atomic & solid state physics

  • Nanoscopy

    Nobel chemistry 2014

    Blue LED Nobel Physics

    2014

  • Information processing THz bandwidth & no loss Lighting & photovoltaics Efficiency Nanoscopy, spectroscopy Fast & noninvasive Quantum information Low loss & decoherence …

  • This course

    5

    1. Tuesdays 13-17: Lecture course (2h), 2h exercises 2. Thursdays 13-17: Lecture 2h, exercises (2h) 3. Labtour AMOLF: provisional April 14th

    Presentations & homework exercises count for final mark Me: [email protected] Exercise help: TA indicated per week (rotates) Course slides & information available at: http://www.amolf.nl/research/resonant-nanophotonics/ http://tinyurl.com/p3eep65

    mailto:[email protected]://www.amolf.nl/research/resonant-nanophotonics/http://www.amolf.nl/research/resonant-nanophotonics/http://www.amolf.nl/research/resonant-nanophotonics/

  • Topics

    1. What do you know about light, matter & optics ? 2. Plasmonics & guiding light 3. Scattering by small particles 4. Metamaterials 5. Microcavities 6. Photonic crystals 7. Emission of light, LDOS 8. Microscopy and Near field optics

  • What do you know about light, matter & optics ?

  • - Light is a wave - Light travels as rays in straight lines - Wavelengths from 450 to 750 nm are recorded by your eye

    - Optics: Light as characterized by color, refraction & reflection - To first order: mirrors, lenses, prisms - Matter enters as refractive index, scattering & absorption -Molecules & atoms as sources -Complicated stuff: interference, diffraction

  • 9

    Maxwell equations I – divergence

    Electric field lines emanate from charge

    Gauss’s law

    If you stick bound charges in a new field D, D-field lines emanate from free charge

    Also

  • Maxwell equations II – curl

    Ampere’s law Current generates magnetic field Separate free current, and bound current in D

    Faraday’s law (and Lenz’s law) A time-changing magnetic flux induces E-field across enclosing curve (electromotively induced voltage).

  • Maxwell together

    Optics is charge-neutral

    Current: only used to describe light sources

  • Optical materials

    Maxwell’s equations Material properties

    +

    Matter enters only via the constitutive relation Nanophotonics controls light via matter

  • Wave equation

    Source free Maxwell - curl one of the curl equations

  • Simple matter

    Plane waves solve Maxwell in free infinite space

    Obviously divergence free if

    Means that

    Transverse wave, with perpendicular, righthanded set

  • Simple matter

    Plane waves solve Maxwell in free infinite space

    Means that

    Dispersion relation:

    Refractive index:

  • Plane wave

    righthanded, perpendicular set Transverse wave Propagation speed , with the refractive index

  • Energy density and Poynting vector

    Subtracting Maxwell curl equations after dotting with complement

    Integrate over volume, use Gauss theorem

  • Poynting’s theorem

    Charge x velocity x force/charge Work done, or work delivered by a source or sink

    Poynting vector – flux integral Energy density in the field

  • Plane wave

    k

    B

    E

    Poynting vector S = E x H along k

  • Photonics

    Dispersion relation:

    Refractive index: I use only relative and

    Homogeneous media

    Photonics Use spatial distribution of to - create confined modes in 0D, 1D and 2D - control dispersion & propagation - control emission & absorption of light

  • What ’s does nature give us ? Why ?

    What happens with fields at interfaces ?

  • Boundary conditions

    Take a very thin loop

  • Boundary conditions

    for a thin pillbox

    (so jumps by )

  • Refraction

    Archetypical problem Fresnel reflection & refraction Let’s see if we can retrace how to solve this problem

  • Snell’s law

    Generic solution steps: Step 1: Whenever translation invariance: Use conservation to find allowed refracted wave vectors

  • Sketch of k|| conservation

    k|| conservation: The only way for the Phase fronts to match everywhere, any time on the interface

  • Amplitudes

    Symmetry does not specify amplitudes Step 2: Once you have identified the solutions per domain Tie them together via boundary conditions

  • Amplitude s-polarization

    Remember

    Now eliminate t to obtain reflection coefficient r (equal µ)

  • Amplitude s-polarization

    Shorthand

  • Amplitude p-polarization

    Suppose now that is coming out of the screen. The rules are the same: is conserved, and are continuous

    exercise

  • Fresnel reflection

    From air to glass From glass to air

  • What you see from this problem

    Scattering: incident field (plane wave) is split by object Reflections: are specular whenever translation invariance rules Refraction: Snell’s law is just wave vector conservation Total internal reflection: if wave vector is too long to be conserved across the interface Boundary conditions determine everything to do with amplitude

  • How could you engineer stuff ?

    Break translation invariance: - random stuff creates a diffuse impression (paint) - periodicity creates diffraction orders (gratings) Confine light by internal reflection Boundary conditions control local field strength…

  • What ’s does nature give us ? Why ?

    What happens with fields at interfaces ?

  • 35

    Optical materials

    Optics deal with plane waves of speed with

    Insulators: transparent Metals: reflective

  • Insulators

    0.4 0.7 1.0 1.3 1.6 1.9-101

    2

    3

    4

    Metamaterial(Nature (2008))

    GaAsSi

    TiO2 (pigment)

    glass SiO2 Silicon nitride Si3N4

    Refra

    ctive

    inde

    x

    Wavelength (micron)

    B

    Water

    Density raises Semiconductors help All ’s between 1 and 4 Vacuum = 1 Spoof (later class)

  • How comes about

    The wave is slowed down by polarization induced in the matter

  • Dielectrics

    Dielectric materials: All charges are attached to specific atoms or molecules

    Response to an electric field : Microscopic displacement of charges

    Macroscopic material properties: electric susceptibility , dielectric constant (or relative dielectric permittivity)

  • Wave in a medium

    In vacuum , so

    In a medium consider response of electrons bound to atom nuclei:

  • Atomic polarization

    Equation of motion of electron:

    : damping coefficient for given material : restoring-force constant resonance frequency Assume is varying harmonically, and also

  • Back to waves

    Inserting in wave equation gives

    solution: with complex propagation constant with :

  • So that we find the refractive index of the dielectric:

    - Number density helps - Number of bound electron resonances per atom helps - Free electrons ?

  • Typical solids

    multiple resonances for electrons per molecule:

    Where is the oscillator strength or (quantum mechanically) the transition probability

    is a complex number:

  • Typical solids

    Absorption bands close to intrinsic resonances Real n to the red also outside absorption Most materials have ’normal dispersion’, i.e.,

    goes up with energy is higher towards the blue is higher towards short

    Until you go through an absorption resonance

  • Quartz prism

    goes up with energy is higher towards the blue is higher towards short

    Stronger refraction towards the blue (bad news for microscopy, photography, people with glasses)

  • Transparent media refractive index Scattering Confining, guiding,...

  • …Waves Can Scatter

    here: a little circular speck of silicon

    scattering by spheres: solved by Gustav Mie (1908)

    small particles: Lord Rayleigh (1871) why the sky is blue

    checkerboard pattern: interference of waves traveling in different directions

  • Multiple Scattering is Just Messier?

    here: scattering off three specks of silicon

  • Not so messy, very different

    the light seems to form several coherent beams that propagate without scattering (or diffraction)

  • Shrink λ by 20%

    light cannot penetrate the structure at this wavelength! all of the scattering destructively interferes

  • 3µm

    Photonic Crystals in Nature

    wing scale:

    Morpho rhetenor butterfly

    [ P. Vukosic et al., Proc. Roy. Soc:

    Bio. Sci. 266, 1403 (1999) ]

    Peacock feather

    [J. Zi et al, Proc. Nat. Acad. Sci. USA, 100, 12576 (2003) ]

    [figs: Blau, Physics Today 57, 18 (2004)]

    http://www.bugguy012002.com/MORPHIDAE.html

    [ also: B. Gralak et al., Opt. Express 9, 567 (2001) ]

  • Example

    Periodically perforated Si confines light to within λ/4 or so How strong is the ‘potential’ set by ? (Si: =3.5) How slow or fast does the wave travel ?

  • Snell’s law with negative index

    Does ‘negative index’ mean negative refraction of rays ?

    S1 S2

    Povray raytrace of Snell’s law

  • 54

    Squeezing plasmons in a nanowire

    Mode width 150 nm SPP-λ < 1 µm At λ = 1.550 µm

    Verhagen et al. 2008

  • Microcavity examples • Whispering gallery mode resonators (e.g. Vahala, Caltech) • Silica microspheres Q ≈ 109

    • Silica microtoroids on Si chip Q ≈ 108, V ≈ 10-11 - 10-10 cm3 fabricated by CO2 laser

    melting of silica disk

    30 µm

  • Cheating the diffraction limit

    PALM, STORM: beat Abbe limit by seeing a single molecule at a time Using a stochastic on/off switch to keep most molecules dark

    Resolution: how discernible are two objects ? If you have a single object, you can fit the center of a Gaussian with arbitrary precision (depends on noise)

  • Measurement of guiding & bending

    57

    Sample: AIST Japan Meas: AMOLF

  • Single photons from single emitters

    Single emitter Quantum dot, molecule

    photon photon

    Challenges: (1) Surely catching each photon in a single beam (2) Surely absorbing each photon from a beam

    Addressing and seeing single molecules with unit efficiency

  • 59

    Motivation

    Single photon sources: Quantum information in 1 photon can not be eavesdropped

    Microscopy: Single molecules at a time can circumvent the diffraction limit Information from fluctuations

  • Information processing THz bandwidth & no loss Lighting & photovoltaics Efficiency Nanoscopy, spectroscopy Fast & noninvasive Quantum information Low loss & decoherence …

  • Controlling single molecules

  • What it is all about

    - Guiding light on scales of a integrated circuit - Seeing ultrasmall things efficiently, such as a single molecule - Controlling transitions in matter by confining light around it emission, absorption, lasing, switching of light Our tools - Light is not a ray - Light is a wave - Control interference by clever placing of materials is to control light at a scale of λ/20 to , and even smaller

    Slide Number 1About length scalesSlide Number 3Slide Number 4This courseTopicsSlide Number 7Slide Number 8Maxwell equations I – divergenceMaxwell equations II – curlMaxwell togetherOptical materialsWave equationSimple matterSimple matterPlane waveEnergy density and Poynting vectorPoynting’s theoremPlane wavePhotonicsSlide Number 21Boundary conditionsBoundary conditionsRefractionSnell’s lawSketch of k|| conservationAmplitudesAmplitude s-polarizationAmplitude s-polarizationAmplitude p-polarizationFresnel reflectionWhat you see from this problemHow could you engineer stuff ?Slide Number 34Optical materialsInsulatorsHow comes aboutDielectricsWave in a mediumAtomic polarizationBack to wavesSlide Number 42Typical solidsTypical solidsQuartz prismSlide Number 46…Waves Can ScatterMultiple Scattering is Just Messier?Not so messy, very differentShrink l by 20% Photonic Crystals in NatureExampleSnell’s law with negative indexSqueezing plasmons in a nanowireMicrocavity examplesCheating the diffraction limitMeasurement of guiding & bendingSingle photons from single emittersSlide Number 59Slide Number 60Controlling single moleculesWhat it is all about