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Improved multipass second harmonic generation (SHG) is provided by the use of an inverting, self-imaging telescope which ensures parallelism of all passes of all beams within the nonlinear medium. Improved multipass SHG is also provided by the use of a wedged phasor which provides a simple adjustme

Improved multipass second harmonic generation (SHG) is provided by the use of an inverting, self-imaging telescope which ensures parallelism of all passes of all beams within the nonlinear medium. Improved multipass SHG is also provided by the use of a wedged phasor which provides a simple adjustment of the relative phase of the pump beam and second harmonic beam between passes. Improved multipass SHG is provided by the use of an inverting self-imaging telescope in combination with a wedged phasor which provides a simple adjustment of the relative phase of the pump beam and second harmonic beam between passes, ensures parallelism of all passes of all beams within the nonlinear medium. A further embodiment includes an OPO and at least one phasor and preferably first and second telescope assemblies.

대표청구항 ▼

What is claimed is: 1. Apparatus for the nonlinear frequency conversion of optical radiation, the apparatus comprising: a) an optically nonlinear medium that receives at least one input beam wherein each of said at least one beam makes N passes through the nonlinear medium, wherein each pass is spa

What is claimed is: 1. Apparatus for the nonlinear frequency conversion of optical radiation, the apparatus comprising: a) an optically nonlinear medium that receives at least one input beam wherein each of said at least one beam makes N passes through the nonlinear medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate at least one additional beam wherein the sum of the input and additional beams is M, wherein for each nonlinear frequency conversion process m, wherein i denotes a particular beam of the M beams, ωi denotes the frequency of a beam i, wherein Smi is +1, 0 or-1; and b) a telescope subassembly having an ABCD matrix with matrix coefficients substantially A=-1, B has any real value, substantially C=0 and substantially D=-1, for receiving and coupling the input and additional beams emitted from the nonlinear medium after a pass number J, back into the medium for a pass number J+1, where 1≦J<N, and wherein the additional beam issues from the nonlinear medium after pass number J+1. 2. Apparatus for the nonlinear frequency conversion of optical radiation, the apparatus comprising: a) an optically nonlinear medium that receives at least one input beam wherein each of said at least one beam makes N passes through the nonlinear medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate at least one additional beam wherein the sum of the input and additional beams is M wherein for each nonlinear frequency conversion process m, wherein I denotes a particular beam of the M beams, ωi denotes the frequency of a beam I, wherein Smi is +1, 0 or-1, and b) at least one phasor for receiving and adjusting a relative phase of the M beams before a pass number K of the beams through the medium, where 2≦K≦N. 3. The apparatus of claim 2 wherein the optical dispersion of at least one phasor is adjustable. 4. Apparatus for the nonlinear conversion of optical radiation, the apparatus comprising: a) an optically nonlinear medium that receives at least one input beam wherein each of said at least one beam makes N passes through the nonlinear medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate at least one additional beam wherein the sum of the input and additional beams is M, wherein for each nonlinear frequency conversion process m, wherein I denotes a particular beam of the M beams, ωi denotes the frequency of a beam i, wherein Smi is +1, 0 or-1, and b) a telescope subassembly having an ABCD matrix with matrix coefficients substantially A=-1, B has any real value, substantially C=0 and substantially D=-1, for receiving and coupling the input and additional beams, emitted from the nonlinear medium after a pass number J, back into the medium for a pass number J+1, where 1≦J<N and wherein the additional beam issues from the nonlinear medium after pass number J+1; and c) at least one phasor for receiving and adjusting a relative phase of the M beams before a pass number K of the beams though the medium, where 2≦K≦N, where the phasor is positioned between the nonlinear medium and the telescope subassembly. 5. The apparatus of claim 4, wherein the optical dispersion of at least one phasor is adjustable. 6. Apparatus for the nonlinear conversion of optical radiation, the apparatus comprising: a) an optically nonlinear medium that receives at least one input beam wherein each of said at least one beam makes N passes through the nonlinear medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate at least one additional beam wherein the sum of the input and additional beams is M, wherein for each nonlinear frequency conversion process m, wherein i denotes a particular beam of the M beams, ωi denotes the frequency of a beam i, wherein Smi is +1, 0 or-1, wherein M> 3 and b) a telescope subassembly having an ABCD matrix with matrix coefficients substantially A=-1, B has any real value, substantially C=0 and substantially D=-1, for receiving and coupling the input and additional beams, emitted from the nonlinear medium after a pass number J, back into the medium for a pass number J+1, where 1≦J<N and wherein the additional beam issues from the nonlinear medium after pass number J+1. 7. Apparatus for frequency-doubling optical radiation, the apparatus comprising: a) an optically nonlinear medium that receives a first beam of optical radiation having a first frequency, wherein the first beam makes N passes through the nonlinear medium, wherein the each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate a second beam having a second frequency substantially equal to twice the first frequency; and b) a wedged phasor for adjusting a relative phase of the first and second beams before a pass number K of the beams through the medium, where 2≦K≦N. 8. Apparatus for frequency-doubling optical radiation, the apparatus comprising: a) an optically nonlinear medium that receives a first beam of optical radiation having a first frequency, wherein the first beam makes N passes through the nonlinear medium between a first face and a second face of the medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate a second beam having a second frequency substantially equal to twice the first frequency; b) a first telescope subassembly having a first ABCD matrix with matrix coefficients substantially A=-1, substantially C=0 and substantially D=-1, for receiving and coupling the first and second beams, emitted from the medium after a pass number J, back into the medium for a pass number J+1, where 1≦J<N, wherein the second beam issues from the nonlinear medium after pass number J+1; and c) a wedged phasor for adjusting a relative phase of the first and second beams before a pass number K of the beams though the medium, where 2≦K≦N, where the phasor is positioned between the nonlinear medium and the telescope subassembly. 9. The apparatus of claim 8, wherein a reference plane within said nonlinear medium is substantially re-imaged onto itself with negative unity magnification by said telescope subassembly, and wherein the reference plane is substantially perpendicular to a direction of propagation of said first and second beams. 10. The apparatus of claim 9, wherein said first beam is substantially a Gaussian beam having a beam waist with a 1/e amplitude radius w that is related to a distance L between said first and second faces according to Lopt/3<L<3 Lopt, where L opt=5.687πw2nω/λ, n107 is an index of refraction of said nonlinear medium at said first frequency, and λ is a free space wavelength of said first beam, and wherein the beam waist is substantially located on said reference plane and said reference plane is substantially centered between said first and second faces. 11. The apparatus of claim 10, wherein said distance L is substantially equal to Lopt. 12. The apparatus of claim 8, wherein said nonlinear medium is birefringently phase-matched. 13. The apparatus of claim 8, wherein said nonlinear medium is quasi-phase-matched. 14. The apparatus of claim 13, wherein said nonlinear medium comprises periodically-poled Potassium Titanyl Phosphate (KTiOPO4 ), periodically-poled Lithium Niobate (LiNbO3), or periodically-poled Lithium Tantalate (LiTaO3). 15. The apparatus of claim 8, wherein said first and second beams pass through said wedged phasor at an angle substantially equal to Brewster's angle and wherein said beams are incident on a face of said wedged phasor with substantially p polarization. 16. The apparatus of claim 8, wherein said nonlinear medium is substantially a parallelepiped having a center line intersecting centers of said first and second medium faces, the apparatus further comprising a second telescope subassembly having a second ABCD matrix with matrix coefficients substantially A=-1, B has any real value, substantially C=0 and substantially D=-1, wherein said first telescope subassembly has a first axis which is substantially collinear with the center line, wherein the second telescope subassembly has a second axis which is parallel to and spaced apart from the center line, and wherein a plane containing the first axis and the second axis is substantially parallel to a face of the parallelepiped. 17. The apparatus of claim 8, further comprising means for astigmatism compensation for at least one of said first telescope subassembly and said phasor. 18. The apparatus of claim 8, further comprising means for ensuring collinearity of said second beam with said first beam for at least one of said passes through said nonlinear medium. 19. A method for frequency-doubling optical radiation, the method comprising: a) transmitting a first beam of optical radiation having a first frequency of through an optically nonlinear medium so that the first beam makes N passes through the nonlinear medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate a second beam having a second frequency ω2 substantially equal to twice the first frequency; and b) passing the first and second beams, emitted from the medium after a pass number J, through a telescope subassembly having an ABCD matrix with matrix coefficients substantially A=-1, B has any real value, substantially C=0 and substantially D=-1, whereby the first and second beams are coupled back into the medium for a pass number J+1, where 1≦J<N and wherein the second beam issues from the nonlinear medium after pass number J+1. 20. A method for frequency-doubling optical radiation, the method comprising: a) transmitting a first beam of optical radiation having a first frequency ω1 through an optically nonlinear medium so that the first beam makes N passes through the nonlinear medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate a second beam having a second frequency ω2 substantially equal to twice the first frequency; and b) passing the first and second beams through a wedged phasor for adjusting a relative phase of the first and second beams before a pass number K of the beams through the nonlinear medium, where 2≦K≦N. 21. A method for frequency-doubling optical radiation, the method comprising: a) transmitting a first beam of optical radiation having a first frequency ω1 through an optically nonlinear medium so that the first beam makes N passes through the nonlinear medium between a first face and a second face of the medium, wherein each pass is spatially separate from all preceding passes, where N is an integer≧2, to thereby generate a second beam having a second frequency ω2 substantially equal to twice the first frequency; b) passing the first and second beams, emitted from the medium after a pass number J, through a first telescope subassembly having a first ABCD matrix with matrix coefficients substantially A=-1, B has any real value, substantially C=0 and substantially D=-1, whereby the first and second beams are coupled back into the medium for a pass number J+1, where 1≦J<N; and c) passing the first and second beams through a wedged phasor for adjusting a relative phase of the first and second beams before a pass number K of the beams through the nonlinear medium, where 2≦K≦N, where the phasor is positioned between the nonlinear medium and the telescope subassembly where the second beam issues from the. nonlinear medium after pass number J+1. 22. The method of claim 21, wherein a reference plane within the nonlinear medium is substantially re-imaged onto itself with negative unity magnification by said telescope subassembly, and wherein the reference plane is substantially perpendicular to a direction of propagation of said first and second beams. 23. The method of claim 22, wherein said first beam is substantially a Gaussian beam having a beam waist with a 1/e amplitude radius w that is related to a distance L between said first and second faces according to Lopt/3<L<3 Lopt, where L opt=5.687πw2nω/λ, nω is an index of refraction of said nonlinear medium at said first frequency, and λ is a free space wavelength of said first beam, and wherein the beam waist is substantially located on said reference plane. 24. The method of claim 23, wherein said distance L is substantially equal to Lopt. 25. The method of claim 21, wherein said nonlinear medium is birefringently phase-matched. 26. The method of claim 21, wherein said nonlinear medium is quasi-phase-matched. 27. The method of claim 26, wherein said nonlinear medium comprises periodically-poled Potassium Titanyl Phosphate (KTiOPO4 ), periodically-poled Lithium Niobate (LiNbO3) or periodically-poled Lithium Tantalate (LiTaO3). 28. The method of claim 21, wherein said first and second beams pass through said wedged phasor at an angle substantially equal to Brewster's angle and wherein said beams are incident on a face of said wedged phasor with substantially p polarization. 29. The method of claim 21, wherein said nonlinear medium is substantially a parallelepiped having a center line intersecting centers of said first and second medium faces, the method further comprising passing said first and second beams through a second telescope subassembly having a second ABCD matrix with matrix coefficients substantially A=-1, B has any real value, substantially C=0 and substantially D=-1, wherein said first telescope subassembly has a first axis which is substantially collinear with the center line, wherein the second telescope subassembly has a second axis which is parallel to and spaced apart from the center line, and wherein a plane containing the first axis and the second axis is substantially parallel to a face of the parallelepiped. 30. The method of claim 21, further comprising compensating for the astigmatism of at least one of said telescope subassembly and said phasor. 31. The method of claim 21, further comprising ensuring collinearity of said second beam with said first beam for at least one of said passes through said nonlinear medium.