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REVIEW 4 major objections 3 minor 33 references

All-polarisation beamsplitters for interferometer applications

T0 review · 4 major / 3 minor · reviewed 2026-08-06 · deepseek-v4-flash

Pith's one-line read Two industrially fabricated beamsplitter coatings approach the polarisation-symmetric reflection and phase needed for polarisation-based speedmeters in gravitational-wave detectors.

desk verdict A careful, useful coating characterization whose headline numbers are not yet consistent between abstract and body — fix the numbers and release data, and it's a solid contribution. read the letter →

arxiv 2507.22866 v1 pith:YS4P42PO submitted 2025-07-30 physics.optics astro-ph.IM

classification physics.opticsastro-ph.IM PACS 42.79.Fm07.60.Ly04.80.Nn
keywords all-polarisationbeamsplitterpolarisation-basedspeedmetergravitational-waveinterferometerdifferentialphaseshiftmultilayerdielectriccoatingTa2O5/SiO2SiO2/SiOxscanningMichelson
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper tries to establish that commercially obtainable dielectric beamsplitter coatings can come close to treating s- and p-polarised light identically, the property a polarisation-based speedmeter needs to reduce back-action noise in gravitational-wave interferometers. It characterises two best-effort coatings, one from Laseroptik and one from Optoman, at 1550 nm. The Laseroptik coating, a 22-layer Ta2O5/SiO2 stack, reaches equal power reflectivity of 51% at 46 degrees incidence and zero differential phase at 44.25 degrees. The Optoman coating, a 5-layer SiO2/SiOx stack, holds reflectivity near 49%/51% and a differential phase of about 5 degrees across the measured angle range. If the results hold, the remaining task is to re-optimise the designs so that equal splitting and zero phase occur together at the 45-degree working angle.

What carries the argument

The argument is carried by two multilayer coating stacks and two optical setups. The Laseroptik stack is 22 alternating Ta2O5/SiO2 layers about 5 micrometres thick; the Optoman stack is 5 layers of SiO2 and SiOx about 0.4 to 0.5 micrometres thick. Power splitting is measured from reflected and transmitted powers at 1550 nm over a +-2 degree range around 45 degrees incidence, using R = PR/(PR+PT) to remove sensitivity to power fluctuations. Differential phase is measured in a scanning Michelson interferometer: the p- and s-polarisation outputs form fringe signals, and the phase between them is recovered by Pearson correlation and Lissajous-ellipse fitting. A -1.75 degree offset, measured with single-polarisation light, is subtracted as a common-mode phase from all datasets.

What would settle it

Measure the differential phase of a Laseroptik sample at 44.25 degrees incidence with an independent technique that does not rely on subtracting the common-mode offset, for example spectroscopic ellipsometry or a dual-wavelength interferometer; if the zero-crossing angle moves by more than the roughly 1.5 degree sample-to-sample variation, the common-mode offset assumption is wrong.

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Extended reading notes

Core claim

The paper reports the characterisation of two best-effort all-polarisation beamsplitter coatings. A 22-layer Ta2O5/SiO2 coating from Laseroptik achieves equal power reflectivity of 51% for s- and p-polarisation at 46 degrees angle of incidence and zero differential phase shift at 44.25 degrees. A 5-layer SiO2/SiOx coating from Optoman achieves power reflectivities of 49% for s-polarisation and 51% for p-polarisation, with a differential phase shift of about 5 degrees that is largely independent of angle of incidence. Both are measured at 1550 nm and compared with an off-the-shelf s-optimised beamsplitter, and the layer structures are reconstructed with SEM and EDX. The paper concludes that the two design goals for all-polarisation beamsplitters, polarisation-independent power splitting and polarisation-independent phase, are approachable with existing industrial coating technology, although neither coating meets both goals at the target 45-degree angle.

Load-bearing premise

A -1.75 degree phase offset, measured once with only p- or s-polarised light, is assumed to be the same for every sample and every angle and is subtracted from all phase measurements; if it changes with sample or angle, the reported zero-crossing and residual phases shift accordingly.

Editorial extensions

If this is right

  • The Laseroptik 22-layer design has enough free parameters that a re-optimisation could bring the equal-reflectivity and zero-phase points together at 45 degrees, provided deposition tolerances are controlled.
  • The Optoman design's angle-insensitive phase means that, once the residual roughly 5-degree shift is compensated, the coating could tolerate larger alignment errors than the Laseroptik design.
  • Residual differential phase can be handled at the interferometer level by a phase plate or temperature control, or by operating away from 45 degrees and compensating with intermediate telescopes planned for future detectors.
  • The characterisation method, power-ratio measurement plus scanning Michelson with Lissajous phase readout, applies directly to other beamsplitter coatings for polarisation-symmetric interferometry.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the -1.75 degree common-mode offset is not truly constant across samples and angles, the reported zero-crossing angle of 44.25 degrees for Laseroptik and the roughly 5-degree residual for Optoman could shift by more than the stated uncertainties; an independent phase measurement that avoids this subtraction would settle it.
  • A natural next step is to use the reconstructed layer thicknesses to simulate both coatings and invert the design problem, asking which thickness changes would put equal reflectivity and zero phase at 45 degrees; the Laseroptik stack's 22 layers make this a plausible optimisation.
  • The angle-independent phase of the Optoman coating suggests a single birefringent phase plate placed after the beamsplitter could null the 5-degree shift over the whole angular range, a cheap fix worth testing.
  • The paper's approach could also qualify coatings for space-based or optical-communication polarisation-symmetric beamsplitters where angular tolerance matters.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

4 major / 3 minor

Summary. The paper characterizes two commercial beamsplitter coatings, from Laseroptik and Optoman, that were ordered on a best-effort basis to have similar optical properties for s- and p-polarised light, as required for polarisation-based speedmeter interferometers. The authors use SEM/EDX to determine coating structure, a photodiode-based setup to measure power reflectance versus angle of incidence, and a scanning Michelson interferometer with multiple phase-estimation methods to measure the differential phase shift between polarisations. They report that the Laseroptik 22-layer Ta2O5/SiO2 coating achieves equal power reflectivity near 51% and a zero differential phase, while the thinner 5-layer Optoman SiO2/SiOx coating achieves near-50/50 reflectance with a small, angle-insensitive phase shift. The qualitative conclusion is that industrial coatings can approach the all-polarisation beamsplitter specification, but the quantitative claims are currently inconsistent between the abstract and the body.

Significance. If the quantitative claims survive revision, this is a useful and timely experimental contribution: there are few published characterisations of industrially fabricated coatings that approach polarisation-symmetric beam-splitting behaviour, and the connection to polarisation-based speedmeters is relevant for future gravitational-wave detectors. The measurement methodology is a strong point: the paper describes multiple independent phase-estimation methods (Pearson correlation, cross-correlation, Lissajous ellipse fitting), cross-checks statistical uncertainties with Monte Carlo and bootstrap resampling, and uses repeated measurements and sample-to-sample scatter to estimate systematic errors. The SEM/EDX structural analysis is also clearly presented and supports the claimed difference in coating design strategies. However, the paper in its current form does not support the specific headline numbers because the abstract and the body disagree on several of them.

major comments (4)
  1. [Abstract; Section II B] The central Laseroptik result is internally inconsistent: the abstract states 'equal power reflectivity of 51% at 46 deg angle of incidence', while Section II B states that for the plane beamsplitter samples (LO-P) the equal-reflectance condition is met 'close to 47 deg at 51% reflectance'. The measurement grid in Section II B uses 0.5° steps, so 46° and 47° are not interchangeable without showing the data or the interpolation procedure. No raw data or per-sample tables are provided, so a reader cannot determine which number is correct. Please harmonise the abstract with the body and provide the underlying data or an explicit statement of how the equality angle was obtained.
  2. [Abstract; Section II B] The Optoman reflectivity values are reversed between abstract and body. The abstract reports '49% for s-polarisation and 51% for p-polarisation', whereas Section II B states that the averaged reflectance is '~51% for s-polarised light and ~49% for p-polarised light'. Since the paper's key claim concerns the magnitude and sign of |Rp - Rs|, this is a material discrepancy that must be corrected before the results can be cited.
  3. [Abstract; Section III] The reported differential phase values for the two coatings are not consistent within the manuscript. The abstract quotes the Optoman differential phase as 'around 5 deg', while Section III states a 'dark fringe offset of Δφbs ∼ 7°'; given the quoted measurement-to-measurement standard deviation of less than 1.5° (Section II C), these values are not compatible at the stated precision. In addition, the Laseroptik zero-phase crossing at 44.25° appears only in the abstract; the body (Section III) states only that the zero-phase condition is reached 'for a smaller angle of incidence compared to the target 45°'. Please make the reported values consistent and specify which samples and data sets produce each headline number.
  4. [Section II C] The common-mode phase offset of -1.75°, measured with only p- or s-polarised light, is subtracted from all phase-shift data, but its uncertainty and any possible dependence on sample or angle are not propagated into the reported zero-crossing angle or residual phase values. The text says there were 'no large variations' but gives no quantitative bound. Given that the quoted systematic uncertainty from repeated measurements is already 1.5°, this offset should be treated as a systematic error and propagated before the headline phase results are considered established.
minor comments (3)
  1. [Section II A] The definition of SiOx is internally inconsistent: the introduction and Section II A define the material as SiOx with 0 < x < 2, but the text later says 'SiO_x is either amorphous silicon (x = 0) or substoichiometric silicon oxide (0 < x < 2)'. Since x = 0 falls outside the earlier range, please reconcile the definition.
  2. [Fig. 7 caption] The word 'introcuded' in the caption of Fig. 7 should be 'introduced'.
  3. [Section II B] Equation (1) defines reflectance as R = PR/(PR + PT), which assumes negligible absorption and scattering. A sentence stating whether losses were checked to be negligible would strengthen the interpretation of the reported reflectance values.

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity: the paper's central claims are direct external measurements, not derivations from their own inputs.

full rationale

The load-bearing claims — power reflectivity vs angle of incidence and differential phase shift vs angle for the Laseroptik and Optoman coatings — are obtained from two independent optical setups (Figs. 5 and 7) using standard calibrated photodiodes, fringe analysis, Pearson correlation, cross-correlation, and Lissajous ellipse fitting. The only data-derived correction applied to the phase results is the measured −1.75° common-mode offset, which was obtained separately with only p- or s-polarised light and then subtracted uniformly; it is not a fitted parameter chosen to force a desired outcome. No coating parameter is fitted to a subset of the reported data and then presented as a prediction. Self-citations (e.g., refs. [6,13]) appear only as background motivation for why polarisation-symmetric beamsplitters are relevant to speedmeters; they do not provide the measured coating performance or the analysis methods. The manuscript's internal inconsistency between abstract values (46°, 49%/51%, ~5°) and body values (47°, ~51%/~49%, ~7°) is a correctness and reproducibility concern, not a circularity. Accordingly, no circular step can be exhibited, and the circularity score is 0.

Assumptions & free parameters 3 free parameters · 4 assumptions · 0 invented entities

The paper is measurement-driven and introduces no new physical entities. Its claims rest on standard thin-film optics, identification of coating materials by SEM/EDX, calibration of photodiodes and piezo, and the assumption that a measured phase offset is common-mode. These are not free postulates in the theory sense, but the calibration constants and the phase-offset correction are parameters the final numbers depend on.

free parameters (3)
  • Photodiode calibration factors (V/W) = not stated in paper
    Linear least-squares fits of photodiode voltage versus input power are used to convert measured powers in Eq. (1); any error in the relative calibration directly biases the reported reflectances.
  • Common-mode phase offset = -1.75 deg
    Measured with p- or s-only light and subtracted from all phase-shift data in Sec. II C; the central zero-crossing angle and the residual phase values depend on this correction.
  • Piezo length coupling cpz = calibrated to lambda = 1550 nm
    Enters the fringe model in Eq. (2), but phase estimates were cross-checked with methods that do not require absolute length calibration, so the impact on the reported phase is limited.
assumptions (4)
  • standard math Fresnel equations govern polarisation-dependent reflectance and phase at dielectric interfaces.
    Used in the introduction and Sec. II B to motivate why equal s/p performance is nontrivial.
  • domain assumption EDX and BSE contrast identify the coating materials as Ta2O5/SiO2 for Laseroptik and SiOx/SiO2 for Optoman.
    Sec. II A infers composition from electron microscopy and X-ray spectra; no manufacturer confirmation or independent refractive-index measurement is provided.
  • domain assumption The fringe signals are single-frequency cos^2 fringes away from piezo ramp turning points.
    Sec. II C uses Eq. (2) through Eq. (4) and tests consistency across three phase-estimation methods, but no independent interferometric reference is given.
  • domain assumption The measured -1.75 deg phase offset is common-mode and independent of sample and angle.
    Sec. II C states it is subtracted from all measurements and was found to have no large variations, but this is assumed rather than proven for every sample and angle.

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Cite this review

Pith. "Pith review of All-polarisation beamsplitters for interferometer applications." pith.science (2026). https://pith.science/paper/YS4P42PO

@misc{pith2026250722866,
  author       = {Pith},
  title        = {Pith review of: All-polarisation beamsplitters for interferometer applications},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/YS4P42PO}},
  note         = {Machine review of arXiv:2507.22866}
}
read the original abstract

Optical beamsplitters with similar properties for orthogonal, linear polarisation modes are required for realising polarisation-based speedmeter schemes to reduce back-action noise in gravitational-wave interferometers. In this paper, we investigate two beamsplitter coatings obtained from Laseroptik GmbH and Optoman on a best-effort basis that aim for a 50/50 power splitting ratio and equal overall phase shift for two orthogonal, linear polarisation modes interacting with the optic. We show that while Laseroptik GmbH opted for coating stack with 22 alternating layers of Ta2O5 and SiO2, Optoman produced a much thinner coating made of 5 SiO2 and SiOx (0 < x < 2) layers. With these strategies, the Laseroptik coating achieves an equal power reflectivity of 51% at 46 deg angle of incidence, and zero phase shift between both polarisations at 44.25 deg angle of incidence. The Optoman coating achieves power reflectivities of 49% for s-polarisation and 51% for p-polarisation with a differential phase shift around 5 deg largely independent of the angle of incidence.

Figures

Figures reproduced from arXiv: 2507.22866 by the authors.

Figure 1
Figure 1. FIG. 1: (a) BSE image of the Laseroptik coating [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. FIG. 2: SE image of the Optoman coating, acquired in [PITH_FULL_IMAGE:figures/full_fig_p003_2.png] view at source ↗
Figure 3
Figure 3. FIG. 3: EDX spectra measured on cross-sections of the [PITH_FULL_IMAGE:figures/full_fig_p003_3.png] view at source ↗
Figures from the paper (7 more)
Figure 4
Figure 4. Figure 4: FIG. 4: Visual representation of the beamsplitter coating composition and structure (with estimated layer [PITH_FULL_IMAGE:figures/full_fig_p004_4.png]
Figure 6
Figure 6. Figure 6: FIG. 6: Average reflectance of the all-polarisation [PITH_FULL_IMAGE:figures/full_fig_p005_6.png]
Figure 5
Figure 5. Figure 5: FIG. 5: Schematic of the setup used to measure the [PITH_FULL_IMAGE:figures/full_fig_p005_5.png]
Figure 7
Figure 7. Figure 7: FIG. 7: Schematic of the scanning Michelson [PITH_FULL_IMAGE:figures/full_fig_p006_7.png]
Figure 8
Figure 8. Figure 8: FIG. 8: Signals from the scanning Michelson [PITH_FULL_IMAGE:figures/full_fig_p006_8.png]
Figure 9
Figure 9. Figure 9: FIG. 9: Example of a Lissajous figure from an Optoman [PITH_FULL_IMAGE:figures/full_fig_p007_9.png]
Figure 10
Figure 10. Figure 10: FIG. 10: Summary of results from phase shift [PITH_FULL_IMAGE:figures/full_fig_p008_10.png]

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Works this paper leans on

33 extracted references · 28 canonical work pages

  1. [1]

    J. Aasi, B. Abbott, R. Abbott, T. Abbott, M. Abernathy, K. Ackley, C. Adams, T. Adams, P. Addesso, R. Ad- hikari, et al., Classical and Quantum Gravity 32, 074001 (2015)

  2. [2]

    Acernese et al

    F. Acernese et al. (Virgo Scientific Collaboration), Clas- sical and Quantum Gravity 32, 024001 (2015)

  3. [3]

    Abbott, R

    B. Abbott, R. Abbott, T. Abbott, S. Abraham, F. Ac- ernese, K. Ackley, C. Adams, R. Adhikari, V. e. a. L. S. C. Adya, and V. Collaboration, Physical Review X 9, 031040 (2019)

  4. [4]

    Abbott et al

    R. Abbott et al. (LIGO and Virgo Scientific Collabora- tions), Physical Review D 109, 022001 (2024)

  5. [5]

    Abbott et al., Physical Review X 13, 041039 (2023)

    R. Abbott et al., Physical Review X 13, 041039 (2023)

  6. [6]

    Danilishin, F

    S. Danilishin, F. Khalili, and H. Miao, Living Reviews in Relativity 22 (2019)

  7. [7]

    Braginsky and F

    V. Braginsky and F. Khalili, Physics Letters A 147, 251 (1990)

  8. [8]

    Braginsky, M

    V. Braginsky, M. Gorodetsky, F. Khalili, and K. Thorne, Physical Review D 61, 044002 (2000)

Show all 33 references
  1. [9]

    Purdue and Y

    P. Purdue and Y. Chen, Physical Review D 66, 122004 (2002)

  2. [10]

    Chen, Physical Review D 67, 122004 (2003)

    Y. Chen, Physical Review D 67, 122004 (2003)

  3. [11]

    A. Wade, K. McKenzie, Y. Chen, D. Shaddock, J. Chow, and D. McClelland, Physical Review D 86, 062001 (2012)

  4. [12]

    M. Wang, C. Bond, D. Brown, F. Br¨ uckner, L. Carbone, R. Palmer, and A. Freise, Physical Review D 87, 096008 (2013)

  5. [13]

    Knyazev, S

    E. Knyazev, S. Danilishin, S. Hild, and F. Khalili, Physics Letters A 382, 2219 (2018)

  6. [14]

    Zukic, K

    M. Zukic, K. Guenther, and R. Chipman, in Polarization Considerations for Optical Systems(1988), vol. 891, pp. 238–241

  7. [15]

    Mordechai, Applied Optics 31, 5345 (1992)

    G. Mordechai, Applied Optics 31, 5345 (1992)

  8. [16]

    J. Feng, C. Zou, J. Zheng, H. Cao, and P. Lv, Applied Optics 48, 5636 (2009)

  9. [17]

    Shen and D

    Z. Shen and D. Huang, Nanomanufacturing 2, 194 (2022)

  10. [18]

    R. M. A. Azzam and A. De, Journal of the Optical So- ciety of America A 20, 955 (2003), URL https://doi. org/10.1364/JOSAA.20.000955

  11. [19]

    Zhang and A

    K. Zhang and A. Smajkiewicz, in Proc. SPIE 6105, Free- Space Laser Communication Technologies XVIII(2006), vol. 6105, p. 61050I, published 1 March 2006, URL https://doi.org/10.1117/12.644885

  12. [20]

    Rothhardt, P

    C. Rothhardt, P. Birckigt, K. Grabowski, S. Risse, R. Schlegel, S. Shestaeva, S. Schwinde, S. Schmidl, and S. Klose, in Proc. SPIE 12777, International Conference on Space Optics — ICSO 2022 (2023), vol. 12777, p. 1277719, presented at the International Conference on Space Opt...

  13. [21]

    J. I. Goldstein, D. E. Newbury, J. R. Michael, N. W. Ritchie, J. H. J. Scott, and D. C. Joy, Scanning electron microscopy and X-ray microanalysis(springer, 2017)

  14. [22]

    Q. Song, F. Huang, M. Li, B. Xie, H. Wang, Y. Jiang, and Y. Song, Journal of Vacuum Science & Technology A 26, 265 (2008), URL https://doi.org/10.1116/1.2837836

  15. [23]

    J. L. Rodgers and W. A. Nicewander, The American Statistician 42, 59 (1988), ISSN 00031305, URL http: //www.jstor.org/stable/2685263

  16. [24]

    Halir and J

    R. Halir and J. Flusser, In Proc. 6th International Con- ference in Central Europe on Computer Graphics and Visualization 98, 125 (1998)

  17. [25]

    L.-W. Wei, H. Hollis, B. Willke, A. D. Spector, and G. Mueller, Applied Optics 63, 3406 (2024), URL https: //doi.org/10.1364/AO.519987

  18. [26]

    L.-W. Wei, J. H. Pold, D. Schmelzer, K. Karan, and B. Willke, Applied Optics 63, 3445 (2024), URL https: //doi.org/10.1364/AO.519988

  19. [27]

    Rowlinson, A

    S. Rowlinson, A. Dmitriev, A. W. Jones, T. Zhang, and A. Freise, Phys. Rev. D 103, 023004 (2021), URL https: //link.aps.org/doi/10.1103/PhysRevD.103.023004

  20. [28]

    Srivastava, D

    V. Srivastava, D. Davis, K. Kuns, P. Landry, S. Ballmer, M. Evans, E. D. Hall, J. Read, and B. S. Sathyaprakash, The Astrophysical Journal 931, 22 (2022), URL https: //dx.doi.org/10.3847/1538-4357/ac5f04

  21. [29]

    Reitze, R

    D. Reitze, R. X. Adhikari, S. Ballmer, B. Barish, L. Bar- sotti, G. Billingsley, D. A. Brown, Y. Chen, D. Coyne, R. Eisenstein, et al., Cosmic explorer: The u.s. contribu- tion to gravitational-wave astronomy beyond ligo(2019), 1907.04833, URL https://arxiv.org/abs/1907.04833

  22. [30]

    Evans, R

    M. Evans, R. X. Adhikari, C. Afle, S. W. Ballmer, S. Bis- coveanu, S. Borhanian, D. A. Brown, Y. Chen, R. Eisen- stein, A. Gruson, et al., A horizon study for cosmic ex- plorer: Science, observatories, and community (2021), 2109.09882, URL https://arxiv.org/abs/2109.09882

  23. [31]

    Punturo et al., Classical and Quantum Gravity 27, 194002 (2010), URL https://doi.org/10.1088/ 0264-9381/27/19/194002

    M. Punturo et al., Classical and Quantum Gravity 27, 194002 (2010), URL https://doi.org/10.1088/ 0264-9381/27/19/194002

  24. [32]

    Maggiore et al., Journal of Cosmology and Astroparti- cle Physics 2020, 050–050 (2020), ISSN 1475-7516, URL http://dx.doi.org/10.1088/1475-7516/2020/03/050

    M. Maggiore et al., Journal of Cosmology and Astroparti- cle Physics 2020, 050–050 (2020), ISSN 1475-7516, URL http://dx.doi.org/10.1088/1475-7516/2020/03/050

  25. [33]

    Abac et al., The science of the einstein tele- scope (2025), 2503.12263, URL https://arxiv.org/ abs/2503.12263

    A. Abac et al., The science of the einstein tele- scope (2025), 2503.12263, URL https://arxiv.org/ abs/2503.12263

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