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11 - 20 of 21 search results for Economics test |u:people.ast.cam.ac.uk where 0 match all words and 21 match some words.

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  2. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture07.pdf
    23 Oct 2023: Referring to Figure 7.1, the gravitational force acting on a test particle ofmass dmi at a distance r from the centre of a spherically symmetric massdistribution is. ... The corresponding gravitational potential energy ofthe test mass is:. dUg,i = GMr dmi

  3. MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: potential test for. ... order of magnitude.This is plausibly an important test of whether large planetes-imals.

  4. Draft version March 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: We performour averaging tests using different sections (e.g., quarters,thirds, halves) of a box that is slightly longer than theone used for the full-disk averaging described above. ... from the outer regions of the disk, our second test is toanalyze the

  5. MNRAS 000, 1–24 (2023) Preprint 9 November 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/pksj23.pdf
    22 Mar 2024: so we can test different initial surface-density profiles; weconsider initial surface-density profiles between 𝑟0 and 𝑟1.5.

  6. Cosmic dust fertilization of glacial prebiotic chemistry on early ...

    https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf
    22 Mar 2024: This minimises sources of uncertainty thatwould otherwise be difficult or impossible to constrain, i.e., allowing us to test theprebiotic relevance of dust supply in one well constrained early Earth scenario.

  7. MNRAS 000, 1–22 (2021) Preprint 29 September 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/yw23.pdf
    29 Sep 2023: observations. This paper aims to test how often the action of the Kozai-Lidovmechanism on a belt of planetesimals due to a wide binary compan-ion can excite the largest planetesimals ... Figure 3. Evolution of a test particle in the eccentric Kozai-Lidov

  8. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: 1. Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. Corresponding author: Sascha P. Quanz, ETH Zurich, Institute for Particle Physics and Astrophysics, Zurich, Switzerland Contact

  9. Draft version July 18, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 Mar 2024: Withthese assumptions, we can test if the same evolutionary model is consistent with observations of the Pleiades.

  10. Inner edges of planetesimal belts: collisionally eroded or truncated?

    https://people.ast.cam.ac.uk/~wyatt/immb23.pdf
    20 Feb 2024: We use both parametric and non-parametric modelling to test if their inner edges are shallow and consistent with collisional evolution.

  11. Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: The PSO framework was chosen as it showed, during tests,a higher convergence rate than Bayesian optimisation and al-lowed multi-core estimation7, reducing the computation time.More standard minimisation frameworks

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