- •Preface
- •Contents
- •1.1 Fundamentals of the semiclassical laser theory
- •1.1.1 The laser oscillator
- •1.1.2.2 Homogeneous, isotropic, linear dielectrics
- •1.1.2.2.1 The plane wave
- •1.1.2.2.2 The spherical wave
- •1.1.2.2.3 The slowly varying envelope (SVE) approximation
- •1.1.2.3 Propagation in doped media
- •1.1.3 Interaction with two-level systems
- •1.1.3.1 The two-level system
- •1.1.3.2 The dipole approximation
- •1.1.3.2.1 Inversion density and polarization
- •1.1.3.3.1 Decay time T1 of the upper level (energy relaxation)
- •1.1.3.3.1.1 Spontaneous emission
- •1.1.3.3.1.2 Interaction with the host material
- •1.1.3.3.1.3 Pumping process
- •1.1.3.3.2 Decay time T2 of the polarization (entropy relaxation)
- •1.1.4 Steady-state solutions
- •1.1.4.1 Inversion density and polarization
- •1.1.4.2 Small-signal solutions
- •1.1.4.3 Strong-signal solutions
- •1.1.5 Adiabatic equations
- •1.1.5.1 Rate equations
- •1.1.5.2 Thermodynamic considerations
- •1.1.5.3 Pumping schemes and complete rate equations
- •1.1.5.3.1 The three-level system
- •1.1.5.3.2 The four-level system
- •1.1.5.5 Rate equations for steady-state laser oscillators
- •1.1.6 Line shape and line broadening
- •1.1.6.1 Normalized shape functions
- •1.1.6.1.1 Lorentzian line shape
- •1.1.6.1.2 Gaussian line shape
- •1.1.6.1.3 Normalization of line shapes
- •1.1.6.2 Mechanisms of line broadening
- •1.1.6.2.1 Spontaneous emission
- •1.1.6.2.2 Doppler broadening
- •1.1.6.2.3 Collision or pressure broadening
- •1.1.6.2.4 Saturation broadening
- •1.1.6.3 Types of broadening
- •1.1.6.3.1 Homogeneous broadening
- •1.1.6.3.2 Inhomogeneous broadening
- •1.1.6.4 Time constants
- •1.1.7 Coherent interaction
- •1.1.7.1 The Feynman representation of interaction
- •1.1.7.3 Propagation of resonant coherent pulses
- •1.1.7.3.2 Superradiance
- •1.1.8 Notations
- •References for 1.1
- •2.1.1 Introduction
- •2.1.3 Radiometric standards
- •2.1.3.1 Primary standards
- •2.1.3.2 Secondary standards
- •References for 2.1
- •2.2 Beam characterization
- •2.2.1 Introduction
- •2.2.2 The Wigner distribution
- •2.2.3 The second-order moments of the Wigner distribution
- •2.2.4 The second-order moments and related physical properties
- •2.2.4.3 Phase paraboloid and twist
- •2.2.4.4 Invariants
- •2.2.4.5 Propagation of beam widths and beam propagation ratios
- •2.2.5.1 Stigmatic beams
- •2.2.5.2 Simple astigmatic beams
- •2.2.5.3 General astigmatic beams
- •2.2.5.4 Pseudo-symmetric beams
- •2.2.5.5 Intrinsic astigmatism and beam conversion
- •2.2.6 Measurement procedures
- •2.2.7 Beam positional stability
- •References for 2.2
- •3 Linear optics
- •3.1 Linear optics
- •3.1.1 Wave equations
- •3.1.2 Polarization
- •3.1.3 Solutions of the wave equation in free space
- •3.1.3.1 Wave equation
- •3.1.3.1.1 Monochromatic plane wave
- •3.1.3.1.2 Cylindrical vector wave
- •3.1.3.1.3 Spherical vector wave
- •3.1.3.2 Helmholtz equation
- •3.1.3.2.1 Plane wave
- •3.1.3.2.2 Cylindrical wave
- •3.1.3.2.3 Spherical wave
- •3.1.3.2.4.2 Real Bessel beams
- •3.1.3.2.4.3 Vectorial Bessel beams
- •3.1.3.3 Solutions of the slowly varying envelope equation
- •3.1.3.3.1 Gauss-Hermite beams (rectangular symmetry)
- •3.1.3.3.2 Gauss-Laguerre beams (circular symmetry)
- •3.1.3.3.3 Cross-sectional shapes of the Gaussian modes
- •3.1.4.4.2 Circular aperture with radius a
- •3.1.4.4.2.1 Applications
- •3.1.4.4.3 Gratings
- •3.1.5 Optical materials
- •3.1.5.1 Dielectric media
- •3.1.5.2 Optical glasses
- •3.1.5.3 Dispersion characteristics for short-pulse propagation
- •3.1.5.4 Optics of metals and semiconductors
- •3.1.5.6 Special cases of refraction
- •3.1.5.6.2 Variation of the angle of incidence
- •3.1.5.7 Crystal optics
- •3.1.5.7.2 Birefringence (example: uniaxial crystals)
- •3.1.5.8 Photonic crystals
- •3.1.5.9 Negative-refractive-index materials
- •3.1.5.10 References to data of linear optics
- •3.1.6 Geometrical optics
- •3.1.6.1 Gaussian imaging (paraxial range)
- •3.1.6.1.1 Single spherical interface
- •3.1.6.1.2 Imaging with a thick lens
- •3.1.6.2.1 Simple interfaces and optical elements with rotational symmetry
- •3.1.6.2.2 Non-symmetrical optical systems
- •3.1.6.2.3 Properties of a system
- •3.1.6.2.4 General parabolic systems without rotational symmetry
- •3.1.6.2.5 General astigmatic system
- •3.1.6.2.6 Symplectic optical system
- •3.1.6.2.7 Misalignments
- •3.1.6.3 Lens aberrations
- •3.1.7 Beam propagation in optical systems
- •3.1.7.2.1 Stigmatic and simple astigmatic beams
- •3.1.7.2.1.1 Fundamental Mode
- •3.1.7.2.1.2 Higher-order Hermite-Gaussian beams in simple astigmatic beams
- •3.1.7.2.2 General astigmatic beam
- •3.1.7.3 Waist transformation
- •3.1.7.3.1 General system (fundamental mode)
- •3.1.7.3.2 Thin lens (fundamental mode)
- •3.1.7.4 Collins integral
- •3.1.7.4.1 Two-dimensional propagation
- •3.1.7.4.2 Three-dimensional propagation
- •3.1.7.5 Gaussian beams in optical systems with stops, aberrations, and waveguide coupling
- •3.1.7.5.1 Field distributions in the waist region of Gaussian beams including stops and wave aberrations by optical system
- •3.1.7.5.2 Mode matching for beam coupling into waveguides
- •3.1.7.5.3 Free-space coupling of Gaussian modes
- •References for 3.1
- •4.1 Frequency conversion in crystals
- •4.1.1 Introduction
- •4.1.1.1 Symbols and abbreviations
- •4.1.1.1.1 Symbols
- •4.1.1.1.2 Abbreviations
- •4.1.1.1.3 Crystals
- •4.1.1.2 Historical layout
- •4.1.2 Fundamentals
- •4.1.2.1 Three-wave interactions
- •4.1.2.2 Uniaxial crystals
- •4.1.2.3 Biaxial crystals
- •4.1.2.5.1 General approach
- •4.1.3 Selection of data
- •4.1.5 Sum frequency generation
- •4.1.7 Optical parametric oscillation
- •4.1.8 Picosecond continuum generation
- •References for 4.1
- •4.2 Frequency conversion in gases and liquids
- •4.2.1 Fundamentals of nonlinear optics in gases and liquids
- •4.2.1.1 Linear and nonlinear susceptibilities
- •4.2.1.2 Third-order nonlinear susceptibilities
- •4.2.1.3 Fundamental equations of nonlinear optics
- •4.2.1.4 Small-signal limit
- •4.2.1.5 Phase-matching condition
- •4.2.2 Frequency conversion in gases
- •4.2.2.1 Metal-vapor inert gas mixtures
- •4.2.2.3 Mixtures of gaseous media
- •References for 4.2
- •4.3 Stimulated scattering
- •4.3.1 Introduction
- •4.3.1.1 Spontaneous scattering processes
- •4.3.1.2 Relationship between stimulated Stokes scattering and spontaneous scattering
- •4.3.2 General properties of stimulated scattering
- •4.3.2.1 Exponential gain by stimulated Stokes scattering
- •4.3.2.2 Experimental observation
- •4.3.2.2.1 Generator setup
- •4.3.2.2.2 Oscillator setup
- •4.3.2.3 Four-wave interactions
- •4.3.2.3.1 Third-order nonlinear susceptibility
- •4.3.2.3.3 Higher-order Stokes and anti-Stokes emission
- •4.3.2.4 Transient stimulated scattering
- •4.3.3 Individual scattering processes
- •4.3.3.1 Stimulated Raman scattering (SRS)
- •4.3.3.2 Stimulated Brillouin scattering (SBS) and stimulated thermal Brillouin scattering (STBS)
- •4.3.3.3 Stimulated Rayleigh scattering processes, SRLS, STRS, and SRWS
- •References for 4.3
- •4.4 Phase conjugation
- •4.4.1 Introduction
- •4.4.2 Basic mathematical description
- •4.4.3 Phase conjugation by degenerate four-wave mixing
- •4.4.4 Self-pumped phase conjugation
- •4.4.5 Applications of SBS phase conjugation
- •4.4.6 Photorefraction
- •References for 4.4
22 1.1.5 Adiabatic equations [Ref. p. 40
derived by thermodynamical considerations. The quantum-mechanical equation (1.1.67) delivers in steady state, replacing ∆n by n2 − n1 and n0 by n1 + n2, and furthermore taking into account that for steady state without interaction holds ∆n0 = −n0:
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This equation has the same structure as the Einstein equation. If the monochromatic intensity J (ω) is replaced by the spectral density ρω and integration over the full spectral range is performed, a relation between the Einstein coe cients and the atomic parameters is obtained. These relations read in general for degenerated levels with weighting factors g1, g2 (degeneracies) [92Koe, 81Ver, 00Dav]:
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The above relations were derived for isotropic media. Anisotropic media are discussed in [86Sie]. Equation (1.1.80) holds for all dipole transitions, as long as the quantum system is coupled to a large number of modes (free space or a resonator with dimensions large compared with the wavelength). With these equations the gain coe cient can be related to the Einstein coe cient of spontaneous emission [92Koe]:
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1.1.5.3 Pumping schemes and complete rate equations
The fundamental methods to obtain inversion are presented, discussing the idealized 3- and 4-level system.
Till now a two-level system was discussed, assuming a steady-state inversion ∆ n0, which is always negative. To obtain positive inversion ∆ n = n2 − n1 > 0 and gain, additional levels are necessary.
Landolt-B¨ornstein
New Series VIII/1A1
Ref. p. 40] |
1.1 Fundamentals of the semiclassical laser theory |
23 |
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∆ n > 0 is a state of non-equilibrium. To support this state, energy has to be pumped into the system. This pumping energy can be incoherent light, kinetic energy of electrons/ions, chemical energy or electric energy. The pumping schemes can become very complicated, and in most cases many energy levels are involved. To understand the principal process for the generation of inversion, two idealized pumping schemes will be discussed.
1.1.5.3.1 The three-level system
The simplified diagram of the three-level system is shown in Fig. 1.1.8. The level E3 is excited by absorption of light or by electron collisions, depending on the specific system. The decay from E3 to E2, the upper laser level, is very fast. Nearly all excited atoms are transferred into this level, which has a very long life time. If the pumping power is su ciently high to overcome the decay of level E2, atoms will be accumulated and finally n2 is larger than n1. The adiabatic rate equations give for the upper-level population without induced emission between the two levels (J = 0):
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The relation between the inversion density and the pump rate is shown in Fig. 1.1.9. Inversion occurs for W T1 > 1. With increasing pump rate the inversion increases also and approaches finally one, all atoms are in the upper level. To obtain ∆ nsteady,3 > 0 requires at least 50 % of the active atoms to be pumped into the upper level, high pump rates are necessary and the e ciency is low. Equation (1.1.82) has to be completed by the coherent interaction term of (1.1.67). The complete rate equation for the three-level system with pump rate W , interacting with a monochromatic field of intensity J is given in (1.1.84). For the intensity (1.1.48c), (1.1.48d) hold, depending on the type of line-broadening (Sect. 1.1.6).
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Landolt-B¨ornstein
New Series VIII/1A1
24 |
1.1.5 Adiabatic equations |
[Ref. p. 40 |
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1.1.5.3.2 The four-level system
Fig. 1.1.9. Inversion density vs. pump rate for a threeand four-level system.
(1.1.84)
The commonly used pump scheme, due to its high e ciency, is the four-level system as shown in Fig. 1.1.8. The two laser levels are E2 and E1, where the lower level E1 has a very short lifetime and its population n1 is nearly zero. This requires that the energy E1 − E0 is much larger than the thermal energy κT . The pump level E3 decays very rapidly to the upper laser level E2 and its population is again nearly zero. The inversion density now is ∆ n = n2 − n1 ≈ n2. Then the rate equation for the pump process reads:
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Landolt-B¨ornstein
New Series VIII/1A1
Ref. p. 40] |
1.1 Fundamentals of the semiclassical laser theory |
25 |
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1.1.5.4 Adiabatic pulse amplification
The amplification and shaping of light pulses by saturable two-level systems is presented.
The pulse is adiabatic if its width τ is small compared with T1 and large compared with T2. Then the variation of the upper-level population due to spontaneous emission and pump can be neglected and this term can be neglected. If such a pulse travels through an active medium of length , it depletes the upper level, is amplified and shaped as depicted in Fig. 1.1.10. The initial conditions at t = −∞ are:
Inversion density: |
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Input intensity: |
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Input energy: |
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The equations (1.1.67)/(1.1.68) can be solved for a loss-free-medium (α = 0) with a four-level system and yield for the output intensity [63Fra]:
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Es = Js,4T1 : saturation energy density,
Ein,out : input/output energy density.
Equations (1.1.88)–(1.1.90) also hold for saturable absorbers with G0 < 1. The pulse will be shaped in any case and the peak velocity will di er from the phaseand group velocities.
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Landolt-B¨ornstein
New Series VIII/1A1