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Paper Review β€” Claim-Level

Inspect each claim in a paper alongside its supporting experiments, exact results, and falsification criteria for rigorous review.Know what the science actually supports before you trust the answer.

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     Long Answer



    Direct answer: No source in the supplied evidence reports survival fractions of Earth-analogue planets in binaries from an N-body grid, so the number cannot be stated from data β€” it must be produced by a new simulation. The literature provided only establishes the ingredients: (1) binaries are dynamically hostile zones whose stability depends on separation and mass ratio (the 1974 premise, now known to be an over-generalization since planets do form and survive in binaries); (2) post-formation N-body evolution over 100 Myr preserves most planets in isolated systems but reshapes eccentricities β€” the same machinery needed for the binary grid; (3) modern N-body/TTV pipelines (jnkepler, SPOCK, exoplanet in JAX) are the validated toolchain for such experiments

    Grid design (BGPT plan, explicitly simulated/inferred β€” not observed data)

    • Grid axes: binary semi-major axis a_bin = 10–1000 AU (log-spaced, 12 points) Γ— binary eccentricity e_bin = 0–0.9 (10 points); fixed solar-type primary (1 Mβ˜‰), mass ratio q = 0.5 and 1.0 sub-grids.
    • Planet: 1 Mβ˜‰ analogue at 1 AU (S-type orbit), 5Β° mutual inclination; 10 random phase seeds per cell for statistics.
    • Integrator: REBOUND WHFast/IAS15 or MERCURY, 10 Gyr (with 100 Myr quick-screen); ejection, stellar collision, or crossing of the Mardling–Aitford-style critical radius counted as death.
    • Expected analytic first-cut (illustrative, computed from the empirical stability boundary, shown below as a simulated curve β€” NOT observational data): survival β‰ˆ 1 for a_bin above a few Γ— the critical periastron ratio (~3:1 outer-to-inner periastron), collapsing sharply as a_bin shrinks or e_bin grows.

    Curve is a BGPT parametrized expectation around the empirical critical periastron boundary; it must be replaced by the actual N-body histogram output of the grid.

    Confidence note: high confidence that the empirical answer is absent from supplied sources and that the toolchain above is the validated route; the plotted fractions are assumptions to be falsified by the run.



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    Updated: September 14, 2026

    BGPT Paper Review



    Study Novelty

    70%

    The follow-up question targets an unexplored quantitative gap relative to the 1974 claim: a systematic binary-separation/eccentricity survival grid, enabled by modern N-body tooling from the 2015/2026 papers.



    Scientific Quality

    80%

    Supplied records are methodologically solid (100-Myr SyMBA synthesis, Nature-level TTV/N-body work), but none directly measure binary survival fractions, so the 1974 basis remains qualitative and detection-biased.



    Study Generality

    80%

    Binary survival of habitable-zone planets generalizes to exoplanet occurrence, habitable-planet counts, and SETI priors across stellar multiplicity.



    Study Usefulness

    80%

    A quantified survival map would replace qualitative 1974-era claims with testable occurrence-rate corrections for roughly half of all stellar systems.



    Study Reproducibility

    90%

    All needed code (exoplanet, SPOCK, jnkepler, SyMBA-style integrators) is open-source with public archives; the grid is fully reproducible by design.



    Explanatory Depth

    70%

    Mechanism (three-body perturbation scaling with periastron) is understood, but quantitative survival curves require the proposed simulation; supplied sources give no direct mechanistic numbers for binaries.

     Analysis Wizard



    Building an N-body simulation grid that measures how Earth-analogue planets survive around one star of a binary across binary separations and eccentricities, producing survival-fraction maps.



     Hypothesis Graveyard



    'Binaries suppress all Earth-like planets' (Kumar 1974): falsified by modern detection of S-type and circumbinary planets and by 2015 synthesis showing dynamics rarely erases formed planets.


    'Eccentricity pumping destroys binaries' habitability uniformly': unsupported; supplied 2015 data show eccentricity evolution without wholesale loss, suggesting survival depends on periastron geometry, not e_bin alone.

     Science Art


    What is the survival fraction of Earth-analogue planets in binaries as a function of binary separation and eccentricity (quantify with N-body grid)?

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