# Fused silica Fused silica (silica glass, `SiO2`) has linear and nonlinear models. This page covers: - its complex refractive index from the extreme ultraviolet to the far infrared; - its nonlinear index n2 with the Raman part; - how well both are known, and how they compare with the published alternatives. The manual for solids is {doc}`solid`; the register entries are TC-321 to TC-324 and TC-399 (the linear index) and TC-393 (n2). ```python from optmat.solid.models.registry import default_model, models from optmat.solid.kerr import kerr_models silica = default_model("SiO2") # fit/SiO2, at 20 degrees C n = silica.refractive_index(800e-9) # complex n + ik beta2 = silica.gvd(800e-9) # s^2/m deps = silica.dpermittivity_domega(120e-9) # exact d eps / d omega cold = models("SiO2")["leviton_2008/sellmeier"].at_temperature(120.0) # 30-300 K kerr = kerr_models()["kerr/SiO2"] kerr.n2(1030e-9) # long-pulse n2, m^2/W kerr.n2_effective(1030e-9, 50e-15) # what a 50 fs pulse measures ``` ## The complex index **The recommended model** is `fit/SiO2` (TC-399). It starts from Franta et al.'s universal dispersion model of bulk Schott Lithosil Q2 (`franta_2016/udm_lithosil_q2`), refitted to the absolute refractometry of the transparent window. - **Range:** 24.8 nm to 125 µm, at 20 degrees C. - **Physics:** it is causal, passive and normalised to its transition strengths, with an exact d eps/d omega. - **What it rests on:** - in the window, the absolute indices of Leviton & Frey (Corning 7980, 2008) and Malitson's three prisms (1965), which agree with each other to 1e-5; - Franta's measured absorption at the band edge (146-225 nm) and in the infrared, and his infrared n; - in the vacuum ultraviolet, Franta's model, which above 8.5 eV was fitted to Philipp's tables in Palik's handbook. - **What it changed:** - the interband strength (-2 %) and the higher-energy term (-6 %, and 16.1 eV against 17.0 eV); - the band edge (8.355 against 8.363 eV) and the Urbach width (0.188 against 0.189 eV); - one factor each on the excitons (x1.59), the phonon bands (x1.0006 and x1.003) and the multiphonon bands (x1.12). - **What it keeps** of Franta's model (rms): - the band-edge k to 1.7 %; - the vacuum-ultraviolet n and k to 0.008 and 1.7 %; - in the infrared, k to 6-9 % and n to 2e-3. **In the vacuum ultraviolet** the band edge (E_g = 8.36 eV, 148 nm, with an Urbach tail) and the excitonic structure near 10-12 eV dominate: | lambda (nm) | n | k | |---|---|---| | 50 | 0.8080 | 0.300 | | 80 | 1.1935 | 0.650 | | 100 | 1.4305 | 0.767 | | 110 | 1.8046 | 0.739 | | 120 | 2.2399 | 0.969 | | 130 | 2.0202 | 0.0684 | | 150 | 1.7061 | 0.000880 | | 160 | 1.6490 | 6.68e-05 | | 180 | 1.5859 | 9.12e-07 | | 200 | 1.5511 | 2.98e-08 | Extrapolating a Sellmeier formula through a pole does not describe absorption. For example, evaluating Malitson's printed formula at vacuum wavelengths with a complex square root, outside its stated range, gives Re n = 0.000 at 110 nm and 2.94 at 120 nm, where the recommended complex model gives 1.80 and 2.24. The discrepancy is not an uncertainty estimate for either model. **In the transparent window** the absolute refractometry agrees to 1e-5, once each measurement is referred to vacuum: | At 800 nm | Leviton 2008 (20 C) | Malitson 1965 | Arosa 2020 | Franta 2016 | fit/SiO2 | |---|---|---|---|---|---| | n | 1.45371 | 1.45371 | 1.45337 | 1.45355 | 1.45371 | | group index | 1.46757 | 1.46756 | 1.46727 | 1.46726 | 1.46755 | | GVD (fs^2/mm) | 36.31 | 36.23 | 35.86 | 35.76 | 36.20 | - **Relative to air or to vacuum.** Refractometry by minimum deviation in room air gives the index relative to that air, 2.7e-4 below the absolute index at room conditions (TC-398). - **Leviton & Frey** measured in vacuum (the CHARMS refractometer), from 30 to 310 K, to +-1e-5 (`leviton_2008`). - **Malitson's** 1965 indices are relative to air. The paper does not say so, but Leviton & Frey read them so, and converted to vacuum they agree with Leviton's to 4.5e-6 rms from 0.4 to 2 µm. `malitson_1965/sellmeier` now returns the absolute index, through Edlen's air at 20 degrees C (TC-399). - **Rodney & Spindler's** 1954 indices, from the same apparatus, are relative to air too (`rodney_1954`). - **Arosa & de la Fuente's** formula (2020) is levelled by an Abbe refractometer, which also reads relative to air. Taken to vacuum it agrees with Leviton's to 5e-5 from 0.4 to 2 µm; the table shows it as published. - **Franta's published model** lies 3.4e-4 below Leviton's at 400 nm and 0.8e-4 below at 2 µm, and its GVD is 1.5 % low at 800 nm. It was the recommended model until this comparison (TC-324); the refit keeps everything else about it. - **Uncertainty of the recommended model in the window (0.21-2.6 µm):** - n to about 2e-5: the fit's residuals against Malitson and Leviton are 1-2e-5, and Malitson's twelve specimens of three grades scatter by 1-3e-5 about it; - the group index to about 3e-5 (the refit is 2.3e-5 below Leviton's formula and 0.6e-5 below Malitson's at 800 nm); - GVD to about 0.3 %: Leviton's formula gives 36.31 fs^2/mm and Malitson's 36.23 at 800 nm, against the fit's 36.20. - **Near the 2.73 µm OH band and beyond** grades differ: the fit, with Lithosil Q2's OH band and Franta's infrared, departs from Malitson's glasses by up to 5e-5 at 3.3 µm. - **The dispersion near 2 µm carries Lithosil Q2's OH bands.** The fit keeps Franta's bands of the plate unscaled (Nph36-52; TC-399), and their Kramers-Kronig partners shape the dispersion well before the bands themselves: - the 2.73 µm fundamental (Nph36-41); - a narrow group at 2.21-2.25 µm, 51-293 cm⁻¹ wide, with k up to 1.0e-5 (0.6 cm⁻¹) at 2212 nm (Nph45-47); - weaker bands at 1.90-2.59 µm and 1.38 µm. At 2 µm the fit's GVD is 1.7 % above Malitson's formula's. The bands account for +2.1 % of that (the fundamental 1.3 %, the 2.2 µm group 0.8 %); the refit alone would be 0.3 % below. The 2.2 µm group alone changes β3 by 7 % at 2 µm, and near 2.2 µm the GVD swings through +700 fs²/mm. A finite-difference stencil a few nm wide resolves this. It is not an artefact of the fit. It is the dispersion of absorption measured in one sample: - Franta et al. do not assign the 2.2 µm bands; - their n swing, 1.2e-5 peak to peak, is about the precision of the absolute refractometry, whose wavelengths are 0.1-0.2 µm apart; - Malitson's three grades and Leviton's Corning 7980 agree with the fit to 1e-5 from 1.5 to 2.44 µm. They neither confirm nor exclude bands of this strength in their glasses. A grade with less OH has weaker bands. Malitson's and Leviton's Sellmeier formulas have none (TC-841). - **Evaluation noise:** the UDM's closed forms lose digits to cancellation below a term's characteristic energy (TC-321). n carries 1e-15 to 6e-15 of relative rounding noise from 0.8 to 3.5 µm, and dn/dω (a complex step, exact) 1e-13 to 6e-13. That is far below any physical effect, but it bounds a derivative differenced from them (TC-841). - **Temperature:** Leviton & Frey's temperature-dependent formula (Corning 7980, 30-300 K, 0.4-2.6 µm) is the model `leviton_2008/sellmeier`; `at_temperature` evaluates it at any temperature in that range. Their dn/dT (Table 6) is curated as datasets: 8.6e-6 per K at 800 nm and 295 K. **In the infrared** the model's phonon bands are Franta's measurement of Lithosil Q2. Philipp's older tables (Kramers-Kronig of reflectance) differ by up to 0.5 in n on the reststrahlen bands (TC-324). ## The nonlinear index The model (`kerr/SiO2`; TC-393) gives the long-pulse n2 and its Raman fraction f_R: $$ n_{2,\mathrm{meas}}(\lambda, \tau) = n_2(\lambda)\left[(1 - f_R) + f_R\,\eta(\tau)\right], \qquad n_2(\lambda) = N\left(1 + a E^2\right), $$ - E is the photon energy (eV); - eta(tau) is the share of the delayed Raman response a Gaussian pulse of duration tau sees, from Hollenbeck & Cantrell's 13-mode response; - eta is 0.96 at 100 fs, 0.86 at 47 fs, and 1 for picosecond and longer pulses. It is fitted to eleven sources' measured self coefficients, each with its own calibration scale (a 10 % prior), from 350 nm to 3.5 µm, and to Stolen & Ippen's measured Raman gain of fused quartz, which sets f_R (TC-696): | lambda (nm) | n2 (1e-20 m^2/W) | sigma | electronic | |---|---|---|---| | 400 | 3.05 | 0.18 | 2.39 | | 532 | 2.78 | 0.13 | 2.17 | | 800 | 2.59 | 0.11 | 2.02 | | 1030 | 2.53 | 0.11 | 1.97 | | 1550 | 2.47 | 0.11 | 1.93 | | 2000 | 2.46 | 0.11 | 1.92 | The Raman fraction is f_R = 0.22 +- 0.03, set by Stolen & Ippen's gain, 1.5e-11 cm/W at 330 cm⁻¹ for a 526 nm pump, predicted as 2 omega_s n2 f_R Im H_R / c with Hollenbeck & Cantrell's response (TC-695, TC-696). It agrees with Hellwarth et al.'s nuclear share of n2 from Raman spectra, 0.21 +- 0.03, which is compared, not fitted. Stolen et al.'s 0.18, the prior until then, is left out: it was derived from these two measurements. The electronic part is 0.78 of n2; a 50 fs pulse measures 0.97 of it. The Raman response itself, with this f_R and two literature forms, is on {doc}`raman_response`. - **Compared with the literature:** - Milam's much-used recommended values (2.74e-20 m^2/W at 1053 nm) are 8-11 % higher. His assessment rests largely on nanosecond measurements, which may include electrostriction. - Santran et al.'s ten grades are 37 % higher, beyond their stated absolute accuracy (10-28 %). Their pump-probe isolates the electronic part, which the larger f_R lowers. - The other nine sources lie within -13 % and +4 % of the fit. Milam & Weber's 1976 interferometric value at 1064 nm (125 ps) is 4 % above it (TC-594). - **Below 350 nm** two-photon absorption sets in (2 hbar omega above the 8.4 eV gap). DeSalvo et al.'s 266 nm value is twice this dispersion's extrapolation, and the model warns there. - **Two-photon absorption, multiphoton and field ionisation, and laser damage:** their data are curated (TC-325 onwards). Their models are next. ## The nonlinear bundle A propagation code in the $n_0 = 1$ convention of the nonlinear Schrödinger equation takes the response $R(t) = (1 - f_R)\,\delta(t) + f_R\,h_R(t)$, with $\int h_R\,dt = 1$ and the total $n_2$: the triple $(n_2, f_R, h_R)$. `optmat.solid.bundle.silica_bundle` gives it as one object whose parts cannot be mismatched (OEP 1, sections 4.7 and 6.9). Every bundle holds the Kerr fit's **total** long-pulse $n_2(\lambda)$, the quantity the data measure, and its shape's own $f_R$. Its electronic part is $(1 - f_R)\,n_2$, so a scalar and a vector run agree in the long-pulse limit. - `"default"`: Hollenbeck and Cantrell's shape with the Kerr fit's $f_R = 0.219$, `paired`, copolarised only. - `"tensor"`: Lin and Agrawal's shape with its own $f_R = 0.245$ (TC-734), which has isotropic and anisotropic parts. Its electronic part is 3.3 % smaller than the default's, and its Raman part 12 % larger. - One bundle for each silica response, under the response's name. The silica response's `raman_coefficient` and `electronic_susceptibility` include $n_0^2$; a code in the $n_0 = 1$ convention takes the bundle's parts instead. Each bundle carries its gain check against Stolen and Ippen's measured gain, $1.5 \times 10^{-11}$ cm/W ± 10 % at 330 cm⁻¹ for a 526 nm pump (`gain_check`). The Kerr fit's $f_R$ was set by this gain through Hollenbeck's shape, so for another shape it is a consistency check, not an independent validation: | Bundle | $f_R$ | Gain at 330 cm⁻¹ (10⁻¹¹ cm/W) | Against the measurement | |---|---:|---:|---:| | `default` (Hollenbeck, paired) | 0.219 | 1.35 | −9.7 % | | `tensor` (Lin and Agrawal, their $f_R$) | 0.245 | 1.38 | −7.9 % | | `blow_1989` (Blow and Wood, their $f_R$) | 0.222 | 1.46 | −2.5 % | ```python import numpy as np from optmat.solid.bundle import silica_bundle bundle = silica_bundle("tensor") n2 = bundle.n2(1030e-9) # m^2/W, the Kerr fit's total fraction = bundle.raman_fraction t = np.linspace(0.0, 1e-12, 2001) h = bundle.h_r(t, "b") # 1/s, the anisotropic part assert abs(float(bundle.n2_electronic(1030e-9)) - (1 - fraction) * float(n2)) < 1e-30 assert abs(bundle.gain_check.deviation) < 0.1 ```