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1 HIGHPRECISIONMODELINGTOWARDSTHE10−20 LEVEL Author:M.Andres1,L.Banz1,A.Costea1,E.Hackmann2,S.Herrmann2,C.La¨mmerzahl2,L.Nesemann1,B.Rievers2,E.P.Stephan1 1:InstituteforAppliedMathematics,LeibnizUniversityHannover,Germany 2:CenterofAppliedSpaceTechnologyandMicrogravityZARM,UniversityofBremen,Germany Abstract The requirements for accurate numerical simulation are increasing constantly. Modern high precision physics ex- 1 perimentsnowexceedtheachievablenumericalaccuracyofstandardcommercialandscientificsimulationtools. One 1 exampleareopticalresonatorsforwhichchangesintheopticallengtharenowcommonlymeasuredto10−15precision 0 [1].Theachievablemeasurementaccuracyforresonatorsandcavitiesisdirectlyinfluencedbychangesinthedistances 2 betweenthe opticalcomponents. If deformationsin the rangeof 10−15 occur, those effectscannotbe modeledand n analysedanymorewithstandardmethodsbasedondoubleprecisiondatatypes. Newexperimentalapproachespoint a J outthattheachievableexperimentalaccuraciesmayimprovedowntothelevelof10−17inthenearfuture[2]. Forthe developmentandimprovementofhighprecisionresonatorsandtheanalysisofexperimentaldata,newmethodshave 5 to be developedwhich enable the needed level of simulation accuracy. Thereforewe plan the developmentof new ] highprecisionalgorithmsforthesimulationandmodelingofthermo-mechanicaleffectswithanachievableaccuracy h of10−20. Inthispaperweanalyseatestcaseandidentifytheproblemsonthewaytothisgoal. p - p m Motivation soundway. o Todate,thebestcavitystabilizedlasershaveachieved c Optical high-finesse resonators are widely used as a arelativefrequencystabilityontheorderoffewparts . s frequencyreferenceforthestabilizationoflaserse.g. in 1016 [5]. As pointed out by Numata et al. [6, ic in optical atomic clocks, now aiming for the 10−18 7], this precision is limited by fundamental thermal s y levelofprecision [3],orindirecttestsofspecialand noise, mostly affecting the highly reflective mirror h general relativity. For example, [1] and [4] tested coatings. Consequently,low-noise,single-crystalline p the isotropy of the speed of light by comparing the siliconmirrorsarecurrentlybeingdeveloped[2]and [ frequencies of two lasers referenced to crossed res- an improvement of optical cavity stability down to v1 onators witharelativeprecision of10−15 at1sinte- the10−17levelmightbecomefeasiblealreadywithin 1 grationtime. thenextyears. Thesecavities willultimately helpto 8 Typically, an electronic feedback loop is applied to buildopticalclocksofimprovedaccuracyortocarry 9 0 actively stabilize the laser frequency to the optical out fundamental tests at the 10−17 level and below. . resonator. The laser frequency then results directly Thisdevelopment howeverneedstobeparalleled by 1 0 from the geometrical resonator dimensions as given similar advancements in high precision modeling 1 by νL = mc = 2L, where L is the resonator length tools. 1 : and m is the longitudinal mode number. The mea- In order to react to the grown achievable accuracies v surement performance thus depends on the length ofopticalresonatorsandtheneedforimprovedmod- i X stabilityoftheimplementedcavities. Since∆ν/ν = eling methods, we intend to develop a new method r ∆L/L, high precision frequency stabilization at the for the modeling of thermo-mechanical effects in 3 a 10−15 level and below, requires a relative cavity dimensions with an achievable numerical accuracy length stability of the same magnitude. The domi- of 10−20. Inthis paper, weoutline the difficulties to nant effects which cause expansions or contractions overcomebyanalysing acavity testcase. are gravity (in particular if an experiment is assem- bled on earth and conducted in space) and thermal Test case configuration expansion of the components. Therefore high preci- sion modeling of thermo-mechanical effects is a ba- In the following we will present the cavity test case sic requirement for a safe design and verification of which will be used to demonstrate the problems for optical resonators. Only if the models and simula- modeling of thermo-mechanical effects with a nu- tionsofferthesameprecisionwhichcanbeachieved merical accuracy of 10−20. Theanalysis isconfined in experiments, the optimization, design, and eval- to a single mirror within the cavity and performed uation of optical resonators can be performed in a usingtwodifferentapproaches. 2 Fig.1: Designofcavitytestcaseconfiguration. Cavity test case space and cannot be deformed. As the mirrors are bondedtothespacer, adeformation ofthemirrorsat An optical cavity is typically axially symmetric and the contact areas is also not allowed. However, heat composed of two highly reflective concave lenses conduction atthecontactareaistakenintoaccount. whicharebondedtoaspacer. Thedimensionsofthe ULEisdesigned tohaveaminimum thermal expan- test cavity analyzed here are adapted from Webster sioncoefficientatsometemperatureTULEnearroom et al. [8], for the design see Figure 1. The mir- temperature,whoseexactvaluehastobedetermined ror substrates, the mirror coatings, and the spacer experimentally for each cavity. Even if TULE is ex- areassumedtobemadeofultra-lowexpansionglass actly known, in practice it is not possible to achieve (ULE) provided by Corning with the relevant mate- a stable temperature of TULE over the whole cav- rial parameters listed in Tab. 1. Although ULE is ity, and a small temperature gradient is inevitable. knownforanisotropicthermalexpansion,weassume However, by careful thermal control a temperature as an approximation that all materials are homoge- stability of a few mK can be obtained if operating nousandisotropicandthatthespacearoundthecav- near TULE and even about 100µK for temperatures ityisavacuumatroomtemperature. Further,wetake around 300K [9]. Here we assume the mirrors sub- only thermo-elastic effects into account and neglect stratesandcoatingstohaveastabletemperaturecor- othererrorsources likevibration ormateriallosses. responding to a coefficient of thermal expansion of Materialparameter value 30 × 10−9K−1. For more rigorous treatments than thistestcasethethermalexpansioncoefficientshould Thermalconductivity [W/mK] 1.31 be varied in time to reflect the small disturbances of Specificheat[J/kgK] 767 Mean coefficient of thermal ex- 0±30×10−9 thetemperature. Also, weassume thatthis testcavity hasafinesse of pansion [1/K] Elasticmodulus[Pa] 67.6×109 F = 106 andatransmission coefficientoftheincou- pling mirror of T = 10−6. For an input power of Poisson’s ratio 0.17 Massdensity[kg/m3] 2.21×103 Pin = 50µW thisresultswiththegainfactorof F2 Tab.1: MaterialparametersofULECorningcode7972. T ≈ 105 (1) π2 inaneffectivepowerofaboutP = 5W storedinthe Modeled effects, boundaries, and loads cavity. ThelossesAduetoabsorptioncorresponding π to the chosen values for F ≈ and T can be T+A Regarding the setup of the test cavity, the relevant assumedtoA≈ 10−6resultinginadissipatedpower thermal physical effects are heat conduction and ra- ofabout 5µW permirror. Thelaser isassumed here diation as well as the thermal expansion of the ma- to have a diameter of 200µm and to hit the mirror terial. Due to the assumed room temperature, heat perfectly atitscenter. radiation may be neglected as a first simplification. Once an equilibrium state is reached, the tempera- Thespacermayradiatetothewholesurroundingspace tureisconstant intimebutmayvaryoverthecavity. and, thus, we assume it as a heat sink with a con- However, due to the changed temperature the cavity stant temperature of 300K as a second simplifica- willdeform,whatinturnchangestheboundary con- tion. Third, we assume that the spacer is fixed in ditions for the heat conduction. Therefore, the final 3 static state has to be determined iteratively. For this maximal cavity temperature 300.014 test case, we neglect the influence of the changes of uniform mesh adaptive mesh 300.013 boundaryconditionsandperformonestaticanalysis, 300.012 only. mperature [K]30300.00.1011 FE models and results maximal te300.009 Thetestcasedescribedabovewasmodeledusingthe 300.008 Finite Element (FE) approach. Two independ pro- 300.007 grams were used for this task: the academic version 300.006 0 0.5 1 1.5 2 2.5 ofthecommercialANSYSsoftwareandthesoftware DOF x 105 packageMaiProgsdeveloped attheIfAM. Fig.2: Max.tempvs.DOFusingANSYS ANSYS model x 10−11 axial displacement at front of cavity 2 Asafirstapproach,onehalfoftheaxiallysymmetric 0 cavity was modeled in three dimensions. However, due to the limited node number of 256000 nodes of m] −2 m the academic version of ANSYS, this turned out to ment [ −4 be nonsufficient for reaching a high modeling ac- displace curacy. Therefore, the axial symmetry of the prob- −6 lem was used to reduce the model to two dimen- −8 sions. For the computation of heat conduction and mechanical deformation, the eight nodes PLANE77 −1−015 −10 −5 0 5 10 15 position on diameter [mm] and PLANE183 element types were used. On the spacer a fixed temperature and no displacement are Fig.3: NodalsolutionplotusingANSYS prescribed and, therefore, we modeled it in ANSYS with a uniform mesh with a large maximal element ofthecavityatthefrontandthebackisplottedusing size of 1mm. On the lens we started with the same thedataofthecomputations withMaiProgs. element size and reduced it step by step. However, Topointoutthesensitivityofthemathematicalmodel the best results could be obtained by using a mesh ontheaccuracyofthesolution,computationsontwo adapted to the problem with maximal element sizes different mesheswereperformed attheIfAM.Inthe of approximatly 0.002mm in the regions of interest firstcasetheusualh-versiononaquasiuniformmesh andatotal nodenumberofabout247000. Themax- was computed. The geometry is modeled via two imum temperatures for the various degrees of free- cylinders where the ring of the outer cylinder fits dom are shown in figure 2. After solving the ther- withtheringofthecavitythatisbondedtothespacer. mal problem the resulting temperature distribution Thetetrahedralelementshavenearlythesameshape was applied as a body load for the following struc- and size. Since the laser is striking the cavitiy in tural analysis. From a preliminary analysis the dis- placementswereexpectedintherangeof10−12mm. Therefore, as the structural analysis isalinear prob- x 10−11 axial displacement at back of cavity 3 lem,wedecidedtorescalethethermalexpansionco- efficientforabetter numerical performance. There- 2.5 sulting displacements atfront and back ofthe cavity 2 areshowninfigures3and4. mm] ment [1.5 MaiProgs model displace 1 At the IfAM computations were made for linear el- 0.5 ements on tetrahedral meshes with up to seven mil- 0 −15 −10 −5 0 5 10 15 lion nodes. For the computations the self developed position on diameter [mm] FE/BE-softwareMaiProgs[10]wasused. InFigures Fig.4: NodalsolutionplotusingANSYS 5 and 6 the axial displacements on the cross section 4 x 10−11 axial displacement at front of cavity maximal cavity temperature 2 10−2 0 −2 displacement −4 θmax −6 10−3 extrapolated −8 h−version h−adaptive version −1−015 −10 −5 0 5 10 15 103 104 105 106 107 position on diameter DOF Fig.5: NodalsolutionplotusingMaiProgs Fig.7: Max.tempvs.elementsize x 10−11 axial displacement at back of cavity seemsreasonable toassumethatanadaptivecompu- 3 tationusingsomekindofaposteriorierrorestimator 2.5 (residual, hierarchical, etc.) [13, 14] would exceed- inglyimprovetheaccuracyofthesolution. 2 ment displace1.5 Comparison of results 1 Thetwodifferentsoftwaresandapproachesdescribed inthissection leadtoresultscomparing welltoeach 0.5 other. However,acloserinspectionofthetworesults 0 reveal significant differences: the maximal tempera- −15 −10 −5 0 5 10 15 position on diameter turesforthetworesultsdifferby Fig.6: NodalsolutionplotusingMaiProgs −05 ∆T = 1.904041846501059 ×10 K. Giventhisquitelargediscrepancyitisalmostsupris- its midpoint with a radius of 0.1mm it is obvious ingthatthemaximaldisplacementsforbothapproaches thatthe temperature willhavealarge gradient there. differbyonly This is also emphasized by the axial displacement in Figure 5 where the displacement seems to have −12 ∆D = 1.447725122807002 ×10 mm. a singularity in the midpoint of the cavity. Using this information the IfAM modeled a second mesh These differences are caused ontheone hand bythe consisting of three cylinders where the inner cylin- discretizationerrorsconnectedtothedifferentmeshes, der has the radius of the laser such that the coars- and ontheother hand bythelimited accuracy ofthe est mesh has 400 more points in the neighborhood numerical procedures involved in the solution pro- of the midpoint than the first version. The tetrahe- cess. Whereas the first error source can be mini- dral elements do not have the same size any longer, mized by using finer meshes, the second one is an sincetheelementsnearthemidpointofthecavityare inert problem of floating point arithmetic. As a rule considerably smaller than the other elements. From of thumb, one can say that for a result with n sig- this point of view the second mesh can be regarded nificant accurate digits anaccuracy of2nsignificant as kind of an adaptive mesh. This leads to a bet- digitsforeachadditionandmultiplication isneeded. ter approximation of the boundary loads and hence Asthe exponent is treated seperatly, for linear prob- to a better approximation of the solution as can be lems with known order of magnitude for displace- seen in Figure 7. Here the red dashed line is the ex- ment or temperature the accurate digits can be con- trapolatedmaximaltemperatureinsidethecavity. On siderablyimprovedbyasuitablerescalingofthema- bothmeshestheIfAMcomputedfourstepsoftheh- terial properties. However, for nonlinear problems version [11, 12] starting with a coarsest mesh with this approach will in general not work. As a con- 2400 points and 2800 points, respectively. Figure 7 sequence, the only way to minimize the numerical showsthatthecomputationsonthesecondmeshlead errorsistousequad(with128bits)orevenarbitrary tomuchbetterapproximations ofthetemperature. It precision arithmetic instead of the usual double pre- cision (with 64 bits). Since there is no appropriate 5 percentage thermal energy error percentage structural energy error 100 35 uniform mesh uniform mesh 90 adaptive mesh adaptive mesh 30 80 25 70 percentage error 456000 percentage error1250 30 10 20 5 10 0 0 0 0.5 1 1.5 2 2.5 0 0.5 1 DOF 1.5 2 x 1025.5 DOF x 105 Fig.9: Structuralenergyerrornormplot Fig.8: Thermalenergyerrornormplot relative errors in energy norm hardwareavailable, thesecomputations mustbeper- formedwithasoftware emulation. Thisslowsdown 100 thecomputation processsignificantly. Accuracy Evaluation or err el. r ANSYS h−version(θ) Within the ANSYS software a posteriori error esti- 10−1 h−version(u) h−adaptive(θ) mator can be used to evaluate the quality of the so- h−adaptive(u) lution. As the exact solution is not known in gen- 103 104 105 106 107 eraland,inparticular, notforourtestcase,thiserror DOF estimator compares the (discountinous) heat flux or Fig.10:Errornormplot stresses, respectively, in each node as computed by ANSYStoanaveraged(continuous)function,which sure to compare different approximations. The aim interpolates thesevalues. IneachelementEi theen- is to derive efficient and reliable a posteriori error ergy norm ei of the difference of the discontinuous estimators for the test case in order to have a better valuesandtheinterpolated function isameasurefor prediction of thetrue error. Ofcourse, these estima- theerrorinthiselement. Forthewholemodelaper- tors can be used within adaptive algorithms leading centaged relative energy norm error can be given by toafasterconvergence [13,14]. the sum of all ei’s divided by Piei and the thermal dissipation energy. ThisisakindofZienkewics/Zhu error estimator [15], which converges to the true er- ror. The percentage error for various degree of free- Conclusion domsareplottedinFigures8and9forboththether- malandstructural computations. We analysed a cavity test case for thermal induced changes in the cavity length, which directly influ- ences the stability of the laser frequency used to in- terrogatethecavity. Weusedtwodifferent andinde- pendentsoftwaresforafiniteelementanalysisofthe thermo-elastic deformation of the cavity lens due to MaiProgs thedissipated powerofthelaser. Since the exact solution of the presented test case is Despitethenumeroussimplificationsassumedforthis not known in advance it is impossible to compute test case the results of the two independently com- the exact error of the computed approximations in puted values forthe maximaldisplacement differ by the energy norm. Therefore Figure in 10 extrapo- an order of magnitude of 10−12, which is consid- latednormsforthetemperatureandthedisplacement erably lower than the corresponding achievable fre- arecompared withthe energy norms ofthe approxi- quencystabilitiesofultrastablecavities. Theindivid- matedsolutions. Theerrordoes notreflecttheaccu- ual analysis have two major error sources: the dis- racy of the solution but can be considered as a mea- cretization errorofthemeshandthenumerical error 6 ofthesolution process. Thefirsterrorcan beshown J. C. Bergquist. Visible Lasers with Subhertz toconvergetozeroforaninfinitlyfinemesh. Succes- Linewidths,Phys.Rev.Lett.82,3799-3802. sively finer meshes can be produced with any com- [6] K. Numata, A. Kemery, and J. Camp. Thermal- mercialFEsoftwareandadequatecomputingpower. Noise Limit in the Frequency Stabilization of Therefore, this error source can be minimized with- Lasers with Rigid Cavities, Phys. Rev. Lett. 93, out principle problems. The second error source is 250602 (2004). inerttofloatingpointarithmeticandcanonlybemin- imized if data types with more bits are used. For [7] M.Notcutt, L-S.Ma,A.D.Ludlow,S.M.Fore- the present hardware, these data types have in gen- man,J.Ye,andJ.L.Hall.Contributionofthermal eral to be software emulated, which will slow down noise to frequency stability of rigid optical cav- the computation process considerably. Also, to the ity via Hertz-linewidth lasers, Phys. Rev. A 73, knowledge of the authors, a publicly available FE- 031804(R) (2006). solver using quad or arbitrary precision arithmetics doesnotexist. [8] S.A. Webster, M. Oxborrow, and P.Gill. Vibra- Thetestcase presented hereisprocessed taking into tion insensitive optical cavity, Phys.Rev. A75, account only thermo-elastic effects. For the design 011801, 2007. of high precision cavities, this is of course not suffi- [9] J. Alnis, A. Matveev, N. Kolachevsky, Th. cient. However, the principle problems for the FE- Udem, and T. W. Ha¨nsch. Subhertz linewidth modelling will remain the same. Therefore, cavi- tieswithlengthstabilities onthe10−17 leveloreven diode lasers by stabilization to vibrationally and thermally compensated ultralow-expansion glass higher can only be simulated if the problem of nu- Fabry-Pe´rot cavities, Phys. Rev. A 77, 053809 merical errors can be solved. We plan to solve this (2008). problem with the development of a stand-alone FE- solverusingarbitrary precision arithmetics, whichis [10] M. Maischak. Webpage of basedonthesolveralreadyimplementedinMaiProgs, the Software package Maiprogs, together with an interface to ANSYS or other pre- http://www.ifam.uni-hannover.de/∼maiprogs. pocessors. [11] E.P. Stephan. The h-p version of the boundary element method for solving 2- and 3-dimensional References problems, Comp. Meth. Appl. Mech. Eng. 133 [1] Ch.Eisele,A.Yu.Nevsky,andS.Schiller.Labo- (1996)183-208. ratoryTestoftheIsotropyofLightPropagationat [12] E.P. Stephan. Hp-Finite Element Methoden, the 10−17 Level, Phys. Rev. Letters 103, 090401 Vorlesungsskript 2009, Leibniz Universita¨t Han- (2009). nover. [2] F. Bru¨ckner, D. Friedrich, T. Clausnitzer, M. [13] E.P. Stephan. Coupling of Boundary Element Britzger,O.Burmeister,K.Danzmann,E-B.Kley, MethodsandFiniteElementMethods,Encyclope- A. Tu¨nnermann, and R. Schnabel. Realization of diaofComputationalMechanics,EditedbyErwin aMonolithicHigh-ReflectivityCavityMirrorfrom Stein,RenA˜(cid:13)c deBorstandThomasJ.R.Hughes. a Single Silicon Crystal, Phys. Rev. Lett. 104, Vol.1,Chapter13: Fundamentals. 2004JohnWi- 163903(2010). ley&Sons. [3] T. Rosenband et al. Frequency Ratio ofAl+ and [14] R. Araya, A.H. Poza, and E.P. Stephan. Hg+Single-Ion Optical Clocks; Metrology atthe A hierarchical a posteriori error estimate for 17th Decimal Place, Science 319, 1808 – 1812 an advection-diffusion-reaction problem, Math. (2008). Models Methods Appl. Sci. 15 (2005), no. 7, [4] S. Herrmann, A. Senger, K. Mo¨hle, M. Nagel, 1119-1139. E.V. Kovalchuk, and A. Peters. Rotating optical [15] 0.C. Zienkiewics and J.Z. Zhu. A simple error cavity experiment testing Lorentz invariance at estimator and adaptive procedure for practical the 10 − 17 level, Phys. Rev. D 80, pp. 105011 engineering analysis, Int. J. Numer. Meth. Eng. (2009). 24,337-357 (1987). [5] B. C. Young, F. C. Cruz, W. M. Itano, and 7 [16] R. W. Fox. Temperature analysis of low- expansion Fabry-Perot cavities, Optics Express 17,15023(2009).

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