Search Results - "Garaud, P"

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  1. 1

    Horizontal Shear Instabilities at Low Prandtl Number by Garaud, P.

    Published in The Astrophysical journal (01-10-2020)
    “…Abstract Turbulent mixing in the radiative regions of stars is usually either ignored or crudely accounted for in most stellar evolution models. However, there…”
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  2. 2

    The Effect of Rotation on Fingering Convection in Stellar Interiors by Sengupta, S., Garaud, P.

    Published in The Astrophysical journal (01-08-2018)
    “…We study the effects of rotation on the growth and saturation of the double-diffusive fingering (thermohaline) instability at low Prandtl number. Using direct…”
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  3. 3

    Double-diffusive Erosion of the Core of Jupiter by Moll, R., Garaud, P., Mankovich, C., Fortney, J. J.

    Published in The Astrophysical journal (01-11-2017)
    “…We present direct numerical simulations of the transport of heat and heavy elements across a double-diffusive interface or a double-diffusive staircase, in…”
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  4. 4
  5. 5

    Growth and Migration of Solids in Evolving Protostellar Disks. I. Methods and Analytical Tests by Garaud, P

    Published in The Astrophysical journal (20-12-2007)
    “…This series of papers investigates the early stages of planet formation by modeling the evolution of the gas and solid content of protostellar disks from the…”
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  6. 6

    A NEW MODEL FOR MIXING BY DOUBLE-DIFFUSIVE CONVECTION (SEMI-CONVECTION). II. THE TRANSPORT OF HEAT AND COMPOSITION THROUGH LAYERS by Wood, T S, Garaud, P, Stellmach, S

    Published in The Astrophysical journal (10-05-2013)
    “…Regions of stellar and planetary interiors that are unstable according to the Schwarzschild criterion, but stable according to the Ledoux criterion, are…”
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  7. 7

    The Interaction between Shear and Fingering (Thermohaline) Convection by Garaud, P., Kumar, A., Sridhar, J.

    Published in The Astrophysical journal (01-07-2019)
    “…Fingering convection is a turbulent mixing process that can occur in stellar radiative regions whenever the mean molecular weight increases with radius. In…”
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  8. 8

    Turbulent Mixing and Layer Formation in Double-diffusive Convection: Three-dimensional Numerical Simulations and Theory by Rosenblum, E, Garaud, P, Traxler, A, Stellmach, S

    Published in The Astrophysical journal (10-04-2011)
    “…Double-diffusive convection, often referred to as semi-convection in astrophysics, occurs in thermally and compositionally stratified systems which are stable…”
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  9. 9

    On the dynamical interaction between overshooting convection and an underlying dipole magnetic field – I. The non-dynamo regime by Korre, L, Brummell, NH, Garaud, P, Guervilly, C

    “…ABSTRACT Motivated by the dynamics in the deep interiors of many stars, we study the interaction between overshooting convection and the large-scale poloidal…”
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  10. 10

    The Effect of Internal Dissipation and Surface Irradiation on the Structure of Disks and the Location of the Snow Line around Sun-like Stars by Garaud, P, Lin, D. N. C

    Published in The Astrophysical journal (01-01-2007)
    “…In theory of accretion disks, angular momentum and mass transfer are associated with the generation of energy through viscous dissipation. In the construction…”
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  11. 11

    Magnetized Oscillatory Double-diffusive Convection by Sanghi, A., Fraser, A. E., Tian, E. W., Garaud, P.

    Published in The Astrophysical journal (01-08-2022)
    “…Abstract We study the properties of oscillatory double-diffusive convection (ODDC) in the presence of a uniform vertical background magnetic field. ODDC takes…”
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  12. 12

    Meta-analysis of chemotherapy in head and neck cancer (MACH-NC): An update on 107 randomized trials and 19,805 patients, on behalf of MACH-NC Group by Lacas, Benjamin, Carmel, Alexandra, Landais, Cécile, Wong, Stuart J., Licitra, Lisa, Burtness, Barbara, Ghi, Maria Grazia, Cohen, Ezra E.W., Grau, Cai, Wolf, Gregory, Hitt, Ricardo, Corvò, Renzo, Budach, Volker, Kumar, Shaleen, Laskar, Sarbani Ghosh, Mazeron, Jean-Jacques, Zhong, Lai-Ping, Dobrowsky, Werner, Ghadjar, Pirus, Fallai, Carlo, Zakotnik, Branko, Sharma, Atul, Bensadoun, René-Jean, Ruo Redda, Maria Grazia, Racadot, Séverine, Fountzilas, George, Brizel, David, Rovea, Paolo, Argiris, Athanassios, Nagy, Zoltán Takácsi, Lee, Ju-Whei, Fortpied, Catherine, Harris, Jonathan, Bourhis, Jean, Aupérin, Anne, Blanchard, Pierre, Pignon, Jean-Pierre, Adelstein, D.J., Alfonsi, M., Belkacemi, Y., Bar-Ad, V., Bernier, J., Bratland, Å., Calais, G., Campbell, B., Caudell, J., Chabaud, S., Chamorey, E., Chaukar, D., Choi, K.N., Choussy, O., Collette, L., Cruz, J.J., Dauzier, E., Forastiere, A.A., Garaud, P., Gregoire, V., Hackshaw, A., Haddad, E., Haffty, B.G., Hansen, A., Hayoz, S., Horiot, J.C., Jeremic, B., Karrison, T.G., Langendijk, J.A., Lapeyre, M., Leong, T., Le, Q.T., Lee, P.P.Y., Lewin, F., Lin, A., Lopes, A., Mehta, S., Moon, J., Moyal, E., Occéan, B.V., Olmi, P., Orecchia, R., O'Sullivan, B., Overgaard, J., Petit, C., Quon, H., Sanguineti, G., Satar, T., Simes, J., Simon, C., Sire, C., Staar, S., Stromberger, C., Strojan, P., Temam, S., Timochenko, A., Torri, V., Vermorken, J., Vokes, E.E., Waldron, J., Wernecke, K.D., Widder, J., Zackrisson, B.

    Published in Radiotherapy and oncology (01-03-2021)
    “…•MACH-NC second update with 107 randomized trials (19805 patients) investigating chemotherapy (CT) in non-metastatic HNSCC.•Overall Survival (OS) improved by…”
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  13. 13

    A NEW MODEL FOR MIXING BY DOUBLE-DIFFUSIVE CONVECTION (SEMI-CONVECTION). I. THE CONDITIONS FOR LAYER FORMATION by MIROUH, G. M, GARAUD, P, STELLMACH, S, TRAXLER, A. L, WOOD, T. S

    Published in The Astrophysical journal (01-05-2012)
    “…The process referred to as "semi-convection" in astrophysics and "double-diffusive convection in the diffusive regime" in Earth and planetary sciences occurs…”
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  14. 14

    EXCITATION OF GRAVITY WAVES BY FINGERING CONVECTION, AND THE FORMATION OF COMPOSITIONAL STAIRCASES IN STELLAR INTERIORS by Garaud, P., Medrano, M., Brown, J. M., Mankovich, C., Moore, K.

    Published in The Astrophysical journal (20-07-2015)
    “…ABSTRACT Fingering convection (or thermohaline convection) is a weak yet important kind of mixing that occurs in stably stratified stellar radiation zones in…”
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  15. 15

    Dynamics of the solar tachocline — I. An incompressible study by Garaud, P.

    “…Gough & McIntyre have suggested that the dynamics of the solar tachocline are dominated by the advection–diffusion balance between the differential rotation, a…”
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  16. 16

    Dynamics of the solar tachocline - III. Numerical solutions of the Gough and McIntyre model by Acevedo-Arreguin, L. A., Garaud, P., Wood, T. S.

    “…We present the first numerical simulations of the solar interior to exhibit a tachocline consistent with the Gough and McIntyre model. We find non-linear,…”
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  17. 17

    Influence of glenoid component design and humeral component retroversion on internal and external rotation in reverse shoulder arthroplasty: A cadaver study by Berhouet, J, Garaud, P, Favard, L

    “…Summary Background A common disadvantage of reverse shoulder arthroplasty is limitation of the range of arm rotation. Several changes to the prosthesis design…”
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  18. 18

    Constraints on the Long-term Existence of Dilute Cores in Giant Planets by Tulekeyev, A., Garaud, P., Idini, B., Fortney, J. J.

    Published in The planetary science journal (01-08-2024)
    “…Abstract Post-Cassini ring seismology analysis suggests the existence of a stable stratification inside Saturn that extends from the center to ∼60% of its…”
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  19. 19

    SPIN-DOWN DYNAMICS OF MAGNETIZED SOLAR-TYPE STARS by OGLETHORPE, R L F, Garaud, P

    Published in The Astrophysical journal (01-12-2013)
    “…It has long been known that solar-type stars undergo significant spin-down, via magnetic braking, during their main-sequence lifetimes. However, magnetic…”
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  20. 20

    Gyroscopic Pumping of Large-scale Flows in Stellar Interiors and Application to Lithium-dip Stars by Garaud, P, Bodenheimer, P

    Published in The Astrophysical journal (10-08-2010)
    “…The maintenance of large-scale differential rotation in stellar convective regions by rotationally influenced convective stresses also drives large-scale…”
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