Nonlinear Susceptibilities: Quantum Mechanical Treatment

Slides:



Advertisements
Similar presentations
Multi-wave Mixing In this lecture a selection of phenomena based on the mixing of two or more waves to produce a new wave with a different frequency, direction.
Advertisements

Chapter 1 Electromagnetic Fields
Integrals over Operators
METO 621 Lesson 6. Absorption by gaseous species Particles in the atmosphere are absorbers of radiation. Absorption is inherently a quantum process. A.
Molecular Quantum Mechanics
Optimizing SHG Efficiency
The Sum Over States model, although exact, requires a detailed knowledge of many parameters which are not generally available. Experience has shown that.
Light and Matter Tim Freegarde School of Physics & Astronomy University of Southampton The tensor nature of susceptibility.
Limitation of Pulse Basis/Delta Testing Discretization: TE-Wave EFIE difficulties lie in the behavior of fields produced by the pulse expansion functions.
Optical Field Mixing. Oscillating Polarisation Optical polarisation Fundamental polarisation SH Polarisation Constant (dc) polarisation.
Chapter 22: Electromagnetic Waves
No friction. No air resistance. Perfect Spring Two normal modes. Coupled Pendulums Weak spring Time Dependent Two State Problem Copyright – Michael D.
Lecture 3 The Debye theory. Gases and polar molecules in non-polar solvent. The reaction field of a non-polarizable point dipole The internal and the direction.
Lecture 6 The dielectric response functions. Superposition principle.
Narrow transitions induced by broad band pulses  |g> |f> Loss of spectral resolution.
METO 621 Lesson 5. Natural broadening The line width (full width at half maximum) of the Lorentz profile is the damping parameter, . For an isolated.
Fiber-Optic Communications James N. Downing. Chapter 2 Principles of Optics.
P460 - perturbation 21 Time Dependent Perturbation Theory Many possible potentials. Consider one where V’(x,t)=V(x)+v(x,t) V(x) has solutions to the S.E.
Rotational and Vibrational Spectra
LESSON 4 METO 621. The extinction law Consider a small element of an absorbing medium, ds, within the total medium s.
Nonlinear Optics: Phenomena, Materials and Devices -Honors senior undergraduate and graduate level course. -Approximately lecture hours + 3 seminars.
Chapter 21 & 22 Electric Charge Coulomb’s Law This force of repulsion or attraction due to the charge properties of objects is called an electrostatic.
1 Material Electromagnetic Property Material partition under electric field Material partition under magnetic field Lorentzian model Artificial material.
Anharmonic Oscillator Derivation of Second Order Susceptibilities
Vibrational and Rotational Spectroscopy
Vibrational Spectroscopy
Chapter 8. Second-Harmonic Generation and Parametric Oscillation
UNIVERSITI MALAYSIA PERLIS
Density Matrix Density Operator State of a system at time t:
1 ECE 480 Wireless Systems Lecture 3 Propagation and Modulation of RF Waves.
Nanostructures Research Group CENTER FOR SOLID STATE ELECTRONICS RESEARCH Time-Dependent Perturbation Theory David K. Ferry and Dragica Vasileska Arizona.
Average Lifetime Atoms stay in an excited level only for a short time (about 10-8 [sec]), and then they return to a lower energy level by spontaneous emission.

Lecture 20: More on the deuteron 18/11/ Analysis so far: (N.B., see Krane, Chapter 4) Quantum numbers: (J , T) = (1 +, 0) favor a 3 S 1 configuration.
1 Chapter 3 Electromagnetic Theory, Photons and Light September 5,8 Electromagnetic waves 3.1 Basic laws of electromagnetic theory Lights are electromagnetic.
Absorption and Emission of Radiation:
Ch ; Lecture 26 – Quantum description of absorption.
Hanjo Lim School of Electrical & Computer Engineering Lecture 2. Basic Theory of PhCs : EM waves in mixed dielectric.
MODULE 1 In classical mechanics we define a STATE as “The specification of the position and velocity of all the particles present, at some time, and the.
Linear optical properties of dielectrics
Simple Harmonic Oscillator (SHO) Quantum Physics II Recommended Reading: Harris: chapter 4 section 8.
Nonlinear Optics Lab. Hanyang Univ. Chapter 6. Time-Dependent Schrodinger Equation 6.1 Introduction Energy can be imparted or taken from a quantum system.
1 Introduction to Atomic Spectroscopy Lecture 10.
MODELING MATTER AT NANOSCALES 6.The theory of molecular orbitals for the description of nanosystems (part II) The density matrix.
Laser physics and its application Introductory Concept The word LASER is an acronym for Light Amplification by Stimulated Emission of Radiation Lasers,
Wave Dispersion EM radiation Maxwell’s Equations 1.
MS310 Quantum Physical Chemistry
Förster Resonance Energy Transfer (FRET)
Ch 10 Pages ; Lecture 24 – Introduction to Spectroscopy.
Electromagnetism Around 1800 classical physics knew: - 1/r 2 Force law of attraction between positive & negative charges. - v ×B Force law for a moving.
Chapter 7 Electro-optics Lecture 1 Linear electro-optic effect 7.1 The electro-optic effect We have seen that light propagating in an anisotropic medium.
Conductor, insulator and ground. Force between two point charges:
Time Dependent Perturbation Theory
Quantum Two 1. 2 Time-Dependent Perturbations 3.
Introduction to Coherence Spectroscopy Lecture 1 Coherence: “A term that's applied to electromagnetic waves. When they "wiggle" up and down together they.
MODULE 13 Time-independent Perturbation Theory Let us suppose that we have a system of interest for which the Schrödinger equation is We know that we can.
Electrostatic field in dielectric media When a material has no free charge carriers or very few charge carriers, it is known as dielectric. For example.
MOLECULAR SPECTROSCOPY
7. Electromagnetic Waves 7A. Plane Waves Consider Maxwell’s Equations with no sources We are going to search for waves of the form To make things as general.
Einstein’s coefficients represent a phenomenological description of the matter-radiation interaction Prescription for computing the values of the A and.
Raman Effect The Scattering of electromagnetic radiation by matter with a change of frequency.
Quantum Theory of Hydrogen Atom
Chapter 1 Electromagnetic Fields
Quantum optics Eyal Freiberg.
Density Matrix Density Operator State of a system at time t:
Time Dependent Perturbation Theory
ENE/EIE 325 Electromagnetic Fields and Waves
Quantum Theory of Hydrogen Atom
Handout 4 : Electron-Positron Annihilation
Presentation transcript:

Nonlinear Susceptibilities: Quantum Mechanical Treatment The nonlinear harmonic oscillator model used earlier for calculating (2) did not capture the essential physics of the nonlinear interaction of radiation with molecules. It was useful because knowledge of the sign of (2) is not usually important and because normally experimentally measured nonlinear susceptibilities are used in calculations. BUT, there is no reliable way to evaluate the required nonlinear force constant . In contrast to the nonlinear harmonic oscillator model, the quantum treatment uses first order perturbation theory for allowed electric dipole transitions to derive formulas for the second and third order nonlinear susceptibilities of a single isolated molecule with a given set of energy levels. The results, called the “some over states (SOS)”, will be expressed in terms of the energy separations between the excited state energy levels m and the ground state g, , between excited states m and n, , the photon energy of the incident light and the transition electric dipole moments and between the states. The average electron lifetime in the excited state is . All of these parameters can either be calculated from first principles or can be obtained from linear and nonlinear spectroscopy. The electrons are assumed to be initially in the ground state. This theory can be extended to electrons already in excited states when the optical field is incident. This the density matrix approach which deals with state populations in addition to the parameters stated above.

Perturbation Theory of Field Interaction with Molecules is the electron wave function and is the probability of finding an electron in volume at time t with the normalization . The stationary discrete states are solutions of Schrödinger’s equation . The wave function for the m’th eigenstate is written as where is the spatial distribution of the wave function and is a complex quantity with usually which reduces to for the ground state which does not decay. The eigenstates are “orthogonal” in the sense that The ground state wave function is . The superscript s =0 identifies the case that no interaction has yet occurred and s>0 identifies the number of interactions between the electron and an electromagnetic field. An incident field distorts the molecular (atomic) electron cloud and mixes the states via the induced electric dipole interaction for the duration of the field. The probability of the electron in the m’th excited state is proportional to . The total wavefunction becomes

A second and third interaction with the same or different electromagnetic fields lead to For example Interactions in quantum mechanics are governed by the interaction potentials V(t) in which is the induced or permanent dipole moment.

Thus the total wave function can be written in terms of the number of interactions as Permanent dipole moment Linear polarizability First hyperpolarizability Second hyperpolarizability Susceptibilities are calculated via successive applications of first order perturbation theory Equating terms with the same power of  gives

Defining and integrating from t=- to t, After N interactions , Multiplying by , integrating over all space and applying the orthogonality relations Defining and integrating from t=- to t, The total electromagnetic field present at the site of a molecule, is written as Aside: and that in nonlinear optics, and can be considered to be separate input modes for operational purposes.

Interaction of the Molecules With the Field . Interaction of the Molecules With the Field Integrating the first interaction from t’= - to t Redefine the summation over pʹ to a summation over p with p going from -pmax  pmax where pmax is the total number of fields present, and for negative p, .. Second Interaction: Third Interaction:

The summations over n and m are both over all the states The summations over n and m are both over all the states. Also summations over p, q and r are each over all of the fields present. Note that states m and n can be the same state, m and  can be same state etc. Finally, note that there appears to be a time sequence for the interactions with fields which is p, q, r. However, since each of p, q, r is over the total field, all the possible permutations of p, q, r approximate an “instantaneous interaction”. For example, assume there are 2 optical fields present, . Therefore for a(2), p and q each run from -2 to +2, excluding 0, and there are 4x4=16 different contributing field combinations, each defining a time sequence! For each field combination, there are multiple possible “intermediate” states (pathways to state v), denoted by “m” and “n” which can be identical, different etc. For example if there is the ground state “g” and 3 excited states, one of which is the state “v=2”, then the “pathways” to “v=2” could be g 2 1 2, g 3 1 2, g 2 g 2 etc. The probability for each step in the pathway, for example state ”n” to state “m” is given by the transition dipole matrix element . Normally, there are only a few states linked by strong transition moments in a given molecule which simplifies the “sum over states, SOS” calculation. The probability of exciting state “m” also depends, via the resonant denominators, on how close the energy difference is between the ground state (initial electronic state before any interaction) and the state “m”, i.e. whether it matches the energy obtained from the EM fields in reaching state “m” via state “n” and the other states in that particular pathway.

Optical Susceptibilities Recall: Linear Susceptibility

The two denominator terms are referred to as “resonant” and “anti-resonant”. The former has the form and is enhanced when , hence the name “resonant”. For the term , the denominator always remains large and hence the name “anti-resonant” is appropriate. Note that although the resonant contribution is dominant when the photon energy is comparable to , in the zero frequency limit the two terms are comparable. Perhaps a more physical interpretation can be given in terms of the time that the field interacts with the molecule as interpreted by the uncertainty principle. When an EM field interacts with the electron cloud, there can be energy exchange between molecule and field. The uncertainty principle can interpreted in terms of E being the allowed “uncertainty” in energy and t as the maximum time over which it can occur. Within this constraint, a photon can be absorbed and re-emitted, OR emitted and then re-absorbed.

Adding in the approximate local field correction term from lecture 1, and writing which is almost identical to the SHO result, with physical quantities for the oscillator strength. Second Order Susceptibility Sum frequency Difference frequency

Nonlinear polarization at Local Field Corrections in Nonlinear Optics (not just for !) A Maxwell polarization exists throughout the medium at the nonlinearly generated frequency ʹ=pq Maxwell field (spatial average) The total dipole moment induced at the molecule is Maxwell polarization (induced on walls of spherical cavity) Nonlinear polarization at molecule due to mixing of fields Extra term

Examples of Second Order Processes e.g. Type 2 Sum Frequency Generation [ input; generated Note that order of polarization subscripts must match order of frequencies in susceptibility! e.g. nonlinear DC field generation by mixing of Since the summations are over all states, n and m include the ground state which produces divergences as marked by red circles – unphysical divergences!

These divergences can be removed, see B. J. Orr and J. F These divergences can be removed, see B. J. Orr and J. F. Ward, “Perturbation Theory of the Nonlinear Optical Polarization of an Isolated System”, Molecular Physics 20, (3), 513-26 (1971). The prime in the ground state is excluded from the summation over the states, i.e. the summation is taken over only the excited states. Note that the summation includes contributions from permanent dipole moments in the ground state and excited states (case n=m). Non-resonant Limit (ω0) The same susceptibility is obtained for SHG, sum frequency and difference frequency generation, as expected for Kleinman symmetry.

Third Order Susceptibility (Corrected for Divergences) In general for   0 (Kleinman limit) In the limit   0, all the third order are equal!

Symmetry Properties of : Isotropic Media Isotropic media: simplest case of relationships between elements In an isotropic medium, all co-ordinate systems are equivalent, i.e. any rotation of axes must yield the same results! xxxx  yyyy  zzzz; in general for , yyzz  yyxx  xxzz  xxyy  zzxx zzyy; in general for xyyx  xzzx  yxxy  yzzy  zxxz  zyyz; in general for xyxy  xzxz  yxyx  yzyz  zxzx  zyzy. in general for Assume the general case of three, parallel, co-polarized (along, for example, the x-axis) input fields with arbitrary frequencies . x y x y The axis system (x', y') is rotated 450 from the original x-axis in the x-y plane. arbitrary choice of axes 

x y x y Valid for any arbitrary set of frequencies Kleinman (0) limit There is a maximum of 34=81 terms in the tensor. The symmetry properties of the medium reduce this number and the number of independent terms for different symmetry classes was given in lecture 4. The inter-relationships between the non-zero terms are given in the Appendix. All materials have some non-zero elements.

Appendix: Symmetry Properties For Different Crystal Classes Triclinic For both classes (1 and ) there are 81 independent non-zero elements.   Monoclinic For all three classes (2, m and 2/m) there are 41 independent non-zero elements: 3 elements with suffixes all equal, 18 elements with suffixes equal in pairs, 12 elements with suffixes having two y’s, one x and one z, 4 elements with suffixes having three x’s and one z, 4 elements with suffixes having three z’s and one x. Orthorhombic For all three classes (222, mm2 and mmm) there are 21 independent nonzero elements, 3 elements with all suffixes equal, 18 elements with suffixes equal in pairs Tetragonal For the three classes 4, and 4/m, there are 41 nonzero elements of which only 21 are independent. They are: xxxx=yyyy zzzz zzxx=zzyy xyzz=-yxzz xxyy=yyxx xxxy=-yyyx xxzz=yyzz zzxy=-zzyx xyxy=yxyx xxyx=-yyxy zxzx=zyzy xzyz=-yzxz xyyx=yxxy xyxx=-yxyy xzxz=yzyz zxzy=-zyzx yxxx=-xyyy zxxz=zyyz zxyz=-zyxz xzzx=yzzy xzzy=-yzzx

For the four classes 422, 4mm, 4/mmm and 2m, there are 21 nonzero elements of which only 11 are independent. They are: xxxx=yyyy zzzz yyzz=xxzz yzzy=xzzx xxyy=yyxx zzyy=zzxx yzyz=xzzx xyxy=yxyx zyyz=zxxz zyzy=zxzx xyyx=yxxy   Cubic For the two classes 23 and m3, there are 21 nonzero elements of which only 7 are independent. They are: xxxx=yyyy=zzzz yyzz=zzxx=xxyy zzyy=xxzz=yyxx yzyz=zxzx=xyxy zyzy=xzxz=yxyx yzzy=zxxz=xyyx zyyz=xzzx=yxxy For the three classes 432, 3m and m3m, there are 21 nonzero elements of which only 4 are independent. They are: xxxx=yyyy=zzzz yyzz=zzxx=xxyy=zzyy=xxzz=yyxx yzyz=zxzx=xyxy=zyzy=xzxz=yxyx yzzy=zxxz=xyyx=zyyz=xzzx=yxxy Trigonal For the two classes 3 and , there are 73 nonzero elements of which only 27 are zzzz xxxx=yyyy=xxyy+xyyx+xyxy xxyy=yyxx xyyx=yxxy xyxy=yxyx yyzz=zzxx xyzz=-yxzz zzyy=zzxx zzxy=-zzyx zyyz=zxxz zxyz=-zyxz yzzy=xzzx xzzy=-yzzx xxyy=-yyyx=yyxy+yxyy+xyyy yyxy=-xxyx yxyy=-xyxx xyyy=-yxxx

yyyz=-yxxz=-xyxz=-xxyz yyzy=-yxzx=-xyxz=-xxzy yzyy=-yzxx=-zxyx=-xxzy zyyy=-zyxx=-zxyx=-zxxy xxxz=-xyyz=-yxyz=-zzxz xxzx=-xyzy=-xyzy=-yyzx xzxx=-yzxy=-yzyx=-xzyy zxxx=-zxyy=-zyxy=-zyyx For the three classes 3m, m and 3,2 there are 37 nonzero elements of which only 14 are independent. They are: zzzz xxxx=yyyy=xxyy+xyyx+xyxy xxyy=yyxx xyyx=yxxy xyxy=yxyx yyzz=xxzz zzyy=zzxx zyyz=zxxz yzzy=xzzx yzyz=xzxz zyzy=zxzx xxxz=-xyyz=-yxyz=-yyxz xxzx=-xyzy=-yxzy=-yyzx zxxx=-zxyy=-zyxy=-zyyx Hexagonal For the three classes 6, and 6/m there are 41 non-zero elements of which only 19 are independent. They are: xxxx=yyyy=xxyy+xyyx+xyxy xxyy=yyxx xyyx=yxxy xyxy=yxyx yyzz=zzxx xyzz=-yxzz zzyy=zzxx zzxy=-zzyx zyyz=zxxz zxyz=-zyxz yzzy=xzzx xzzy=-yzzx yzyz=xzxz xzyz=-yzxz zyzy=zxzx zxzy=-zyzx xxyy=-yyyx=yyxy+yxyy+xyyy yyxy=-xxyx yxyy=-xyxx xyyy=-yxxx For the four classes 622, 6mm, 6/mmm and m2, there are 21 nonzero elements of which only 10 are independent. They are: xxxx=yyyy=xxyy+xyyx+xyxy xxyy=yyxx xyyx=yxxy xyxy=yxyx yyzz=xxzz zzyy=zzxx zyyz=zxxz yzzy=xzzx yzyz=xzxz zyzy=zxzx

Common Third Order Nonlinear Phenomena Most general expression for the nonlinear polarization in the frequency domain is Each is the total field! Consider just isotropic media, more complicated but same physics for anisotropic media Single Incident Beam Third Harmonic Generation Intensity-Dependent Refraction and Absorption

Two Coherent Input Beams Case I Equal Frequencies, Orthogonal Polarization Third Harmonic Generation Cross Intensity-Dependent Refraction and Absorption (also known as cross-phase modulation) for example

4-Wave-Mixing Case II Unequal Frequencies, Parallel Polarization Cross Intensity-Dependent Refraction and Absorption (also known as cross-phase modulation) Most common is effect of strong beam on a weak beam

Coherent Anti-Stokes Raman Scattering CARS) 2a-b, a > b Case III Incoherent Beams Cross Intensity-Dependent Refraction and Absorption (also known as cross-phase modulation) Most common is effect of strong beam on a weak beam